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April 30 Late PapersEvery semester ends the same way. Students are always trying to turn in
late work. Often it isn't a day or two late, rather it is a month
or two late. I just got through grading a mountain of
papers. I still have a mountain to grade. This is normal
end-of-the-semester type of stuff for faculty. However, it is
worse when so many of these things are late work. The students
know the due dates. I put them in the course syllabus. In
case they lose the syllabus, the due dates are also available on my web
page. So, they know from the first day of the semester what is
due and when. Sometimes I have students who download a copy of
the syllabus the week before the semester starts and they turn in the
first assignment the first day of the semester ... weeks ahead of
time. Others try to turn in things weeks late. For my
astronomy class, the students have homework assignments using some
software that comes in a CD that is packaged with their textbook.
In case they don't have a computer at home (and some don't), then they
can use the computers in the labs on campus. The computer lab in
the library has the software loaded and ready to go. So, last
week, a student comes to me asking if he can borrow a CD from me so
that he can install the software to do the homework. The due date
for the LAST assignment was a week ago. This week is the last
week of the semester. I have due dates spread out all semester
long. This isn't just because I am mean. I don't have time
to grade all these papers at the end of the semester. Also, the
students don't have time to do them all at the end. Now is really
too late to start doing the work. Why is that so hard for them to
get? It is particularly hard for me to understand since I've been
telling them for some time that they can't dilly dally and not do the
work. Things have to be turned in on time. Now, I do
understand if once in a while something comes up. That has
happened to me from time to time. However, I can't believe that
half the class has unusual circumstances. This is just poor
planning on their parts. What is worse is that they simply expect
me to accept these late papers without question!!!! Does this
mean that other faculty accept late work? Well, I will accept
late things since I do understand exceptional circumstances. But,
there is absolutely NO reason for turning in an entire semester's worth
of work in the last week. There is NO excuse for turning in work
a month late! So, I penalize the late papers. I explain to
the students that the penalty is assessed after the grade. I also
explain that the penalty is a flat amount, and that the penalty gets
bigger the later the paper. That means that a late paper that is
poorly done, as most are, can get a low grade followed by a big
penalty. I take the numeric value that follows ... even if it is
negative. I explain this to the students, with the warning that I
take off 100% for things that are more than a couple weeks old, and
even more than 100% for things over a certain point. That means
that students who are just now turning in work due in February can
expect a negative grade even if they turn in a paper that has
everything correct. So, it would be best not to turn in anything,
right? Well, in my stack of papers that I'll pass back this week,
I have about a dozen negative grades. And, yes, negative
means negative. In other words, they actually do worse than if I
had not graded it. For some reason they don't really believe me
when I tell them that. You'd think that they'd learn. -Astroprof April 28 Let's think, now.OK, here I am grading a stack of laboratory exercise. I just finished grading an exercise where students measure the expansion rate of the universe. This was first observed in the 1920s by Edwin Hubble. He found that the the farther a galaxy is away from us, the faster it appears to be moving away from us. This led to the realization that the universe is expanding. Erroniously, many took this to be the evidence of a massive explosion in the early universe. Rather, as it turns out, nothing is really moving. Instead, space itself is expanding, and all the galaxies are just along for the ride. It simply appears that things are moving away from us. However, this still implies that the universe must have been far more compact in the distant past. We now realize that the whole universe came from a single point. The galaxies are not hurling off into space, because it is space that is expanding. All of space was at the beginning a single point. This is quite a bit different from LeMaitre's original concept of a primordeal atom. And, as it turns out, calculations of what you should see from such a "hot big bang" as it is called agree quite well with observations. So, the Big Bang was, as it turns out, not very big, nor was it a bang. Other than that, the name is OK. ;)
If y'all are interested, I can do a blog about the Big Bang sometime.
Well, back to my story of grading lab exercises. The students make measurements of the redshifts of distant galaxies and then plot recessional velocities versus distance. They find the best fit line. Next, they measure the distance of a very distant galaxy and measure its redshift. Assuming that the universe expands at a constant rate (which it does not), you can compute how long it would take for a galaxy to get that distance moving at that speed. As I said, this is not what is really happening, but it still gives you a ballpark estimate of the age of the universe (thousands of years, hundreds of thousands, millions of years, billions of years, etc). So, you know the order of magnitude of the age of the universe. It turns out that the gravitational slowing of the expansion makes the real number closer to about 2/3 of the age that you compute in this manner. Then, you add in the complication that for the last few billion years the universe seems to actually have begun to accelerate it expansion, ...
Well, this can get a bit involved. The students do it the simple way and multiply by 2/3, though, to get an estimate of the age of the universe. If they do the exercise right, they get answers in the range of 12 to 15 billion years for the age of the universe. Well, I just found a group of students who obviously copied off of each other. No less than four students tell me that, as of the time that they did their lab, the universe was 0.000000000000000000034 seconds old. Now, it is bad enough that they just copied from one another, but they wrote that down without even thinking!!!!!! How can you even dream of writing a number like that down as the age of the universe?!?!?! Alas, I get things like this every semester.
"But that is what the calculator said, ..."
Then you must have hit the wrong buttons.
-Astroprof April 27 Ending another semesterWell, the semester is about to end around here. We have one more week of classes and then final exams. I have to make up exams to give, I have to grade term papers, I have to grade laboratory reports, and I have to grade homework. The pile is growing exponentially. Wow. I feel so behind. Of course, I always feel behind. Then, on top of it all, we have meetings, forms to fill out, etc due now, as if we had nothing else to do. Students are now looking to turn in extra credit. So, I want to ask them why they didn't just do what they were supposed to do earlier in the semester. They want to know if they can turn in things during finals week. I tell them sure. I just won't grade them. They don't seem to realize that I am as frantic as they are.
Well, that is life in academia, I guess.
-Astroprof April 25 M 82M 82 is the eighty second object on Charles Messier's list of fuzzy things that are not comets. It is located in Ursa Major, forward of the bowl of the Big Dipper. Actually, it is right next to another Messier object, M 81, in the sky. Both M 81 and M 82 are galaxies, and as it turns out they are not just in the same direction, they really are fairly close to one another. In fact, they recently (in galactic terms) passed even closer to one another.
Now, the reason I thought to blog about M 82 is that it turned up in the most recent Astronomy Picture of the Day, here. M 82 has always been interesting to me. Even in amateur telescopes you can see that something isn't quite right about it. With larger telescopes you see that is doesn't quite fit with the normal Hubble classification scheme for galaxies. It isn't a pretty spiral galaxy, and it definitely isn't an elliptical galaxy. Normally, it is simply tagged as an irregular galaxy, in particular an Irregular Type I. You can see in visual light streamers appearing to eminate from M 82. These streamers are giant plumes of gas, mostly hydrogen. When I was a kid, I remember reading a book written by Isaac Asimov about various astronomy topics. He talked about M 82 as an exploding galaxy. It sure looks like that! However, we now realize that galaxies don't really explode. A more modern description would be to describe M 82 as a starburst galaxy. As the name suggests, a starburst galaxy is a galaxy that has undergone a sudden burst of star formation. When all these stars form at once, what happens is that all types of stars form, including a large number of the very massive short-lived stars. These stars die quite violently in supernovae explosions. A supernova is about the most violent explosion that you run into. When a supernova occurs, not only does the star explode, but the interstellar medium in the vicinity of the star is shocked to high temperature and is pushed aside. Supernovae can cause the interstellar medium to get a bit compressed, causing it to exceed a critical density, and it will collapse to form new stars, including more of the massive ones. These in turn go supernova, and the process continues. In addition to creating new stars, supernovae can also create hot thin regions of the interstellar medium. Our own Sun happens to reside in a large region like this called the Local Bubble. Several supernovae in the same general area of the galaxy in fairly short times can even eject interstellar medium from the galaxy. This seems to be what is happening to M 82.
So, why did all these stars form in the first place? Well, it seems that the answer lies with the nearby M 81. When M 82 and the larger M 81 passed one another, the gravity from M 82 caused M 81 to develop a very nice and well defined spiral structure. However, M 81's gravitational effect on M 82 was to compress the interstellar medium throughout the galaxy, creating a massive wave of star formation. This then led to the starburst activity that is in the process of ejecting interstellar medium from the galaxy.
-Astroprof April 24 AlgolIn the constellation Perseus, the star having Bayer designation Beta Persei is called Algol. This is a shortened form of the original Arabic Al Ra’s al Ghul, or “the head of the demon.” Needless to say, this star is often called “the demon star.” Interestingly enough, Pliny regards this star as the head of the Medusa, the Gorgon killed by the Greek hero Perseus. The Hebrews called this star Rosh ha Satan, Satan’s head. It isn’t really surprising that multiple eastern Mediterranean cultures would have similar names for a star, since they all talked to one another. What is surprising, though, is that the Chinese called this star Tseih She, meaning “the piled up corpses.” Hmm. So, what is so terrible about this star that has everyone thinking ill of it?
We don’t really know for sure what the ancients were thinking. However, we do know that this star is one of only a handful of naked-eye variable stars. Normally, Algol is the second brightest star in Perseus, shining with magnitude of 2.1. However, every 2.87 days, Algol dims to be the sixth or seventh brightest star, at magnitude 3.4. This dimming actually takes hours, but it is most obvious to the naked eye about an hour or so before or after the minimum brightness. The actual period between minima is about 68 hours, 48 minutes, and 56 seconds. To the ancients, who regarded the stars as fixed and unchanging, it would have been an ill omen when a star began to fade like this. Hence, it is the eye in the head of the Medusa, or even the eye of the Devil himself.
The variable nature of Algol is not directly reported in ancient texts. By the Middle Ages, people seem to have forgotten it. The first report of Algol’s variable nature seems to be that of Geminiano Montanari of Bologna in 1667. He reported that about every three days, Algol seemed dimmer. John Goodricke, an astronomer noted for his many contributions to the area of variable star astronomy, reported in 1782 that the variation in brightness was regular and always of equal magnitude. He proposed that perhaps Algol was composed of two stars too close together to be seen as a single star that passed in front of one another on a regular basis. This, in fact, is exactly what is happening with Algol. A dimmer star periodically moves in front of a brighter star, making the pair seem to become much dimmer. Midway between the minima, there is a very small dip in brightness as the brighter star passes in front of the dimmer one. This secondary minimum is far too little of change to be reliably observed with the naked eye. Binary stars whose orbits block one another from our view are called eclipsing binaries. Algol is sort of the prototype of this class of variable star.
Algol is about 92 lightyears away from us. The primary star is a spectral type B star. This is an unusually hot and bright star. The dimmer companion was always lost in the light of the primary star. However, in 1978 astronomers at McDonald Observatory, located in the Davis Mountains in west Texas, managed to isolate the spectrum of the dimmer companion. The companion star is a late G type subgiant star. A subgiant star is one that has ended its life on the Main Sequence and is dying. Algol thus consists of a physically large cool star of mass less than the mass of the Sun orbiting a hot main sequence star of several times the mass of the Sun. This is a problem in that the more massive stars are supposed to die before the less massive ones. So, what gives? The famous astronomer Fred Hoyle gave us the answer. He suggested that the two stars are very close together. We know this to be true. When the more massive star began to die, it began to expand. Again, we know this happens with stars. Well, in a binary star system, there exists a point between the two stars where each star’s gravity pulls equally. To one side or the other of this point, and one star will dominate. Well, when the dying star expanded to the point that its outer edges reached this point, then it began to lose mass to the lower mass star. Eventually, the high mass star lost most of its mass. The formerly low mass star then became hotter and brighter. The formerly high mass star was left with less mass than its companion, but it was still dying, so it was still a distended object. We, therefore, call a star like Algol a semi-detached binary star. The dying companion is still losing some mass to what is now the primary star. The orientation of the orbits of these two stars means that the secondary does not completely cover the primary star during eclipse. Rather, about 21% or so of the primary is still visible during maximum eclipse. The secondary star is still a couple times brighter than our Sun, so that gives an idea of just how bright the primary star is.
Algol is obviously a binary star. However, by the middle of the 20th Century, it had become clear that that wasn’t the whole story. As it turns out, there is a third star to Algol! This third star orbits some 50 million miles from the other two, in a different plane. This star, also a star hotter and more massive than our Sun, never blocks our view of the other stars. This is about the only way that a triple star system could be stable: two stars orbiting very close together with one much farther out orbiting the other pair. Another example of a star like this is Alpha Centauri, where there are two stars orbiting close together and one more much farther out.
Interestingly enough, Algol is not the only naked-eye variable in Perseus. Right near Algol in the sky is the star Rho Persei. As it turns out, Rho Persei is also a variable star. Rho Persei is what we call a semi-regular variable, meaning that it varies, but without a clear cut pattern. Also, Rho Persei only varies by 0.7 magnitudes over several months, so it is hard to notice its variation with the naked eye.
For those of you who want to see Algol, you’ll either have to stay up really late, get up really early, or wait until later this summer.
-Astroprof
April 21 Atlas RocketsThe Atlas family or rockets has a long and proud heritage. The Atlas V is a heavy lift booster, and it is often used to launch some of the bigger space probes. There are some interesting peculilarities in the Atlas rockets, so I thought that I might say a few things about them.
The Atlas was designed as America's first Intercontinental Ballistic Missile (ICBM). Sometimes the Redstone Missile is given this designation, but it was more properly a mid range ballistic missile. The Atlas had the lift to launch a nuclear warhead from the United States to the Soviet Union, or pretty much anywhere else for that matter. The Atlas was also the rocket chosen to launch John Glenn into orbit. All orbital Mercury missions used Atlas rockets.
The Atlas was a rather unusual design. First of all, it was made of stainless steel rather than the lighter materials used in earlier rockets. Stainless steel would not corrode, so it would not need to be painted like other rockets. That made Atlas rockets very shiny and futuristic looking. However, stainless steel is heavy. So, to keep the weight down, the skin of the rocket was kept very thin and the rocket framework was kept to a minimum. In fact, the rocket body itself was so lightweight that it could not even hold itself up under its own weight. Rather, what kept the rocket from crushing itself was pressure in the propellant tanks. So, when fueled, the Atlas was said to be "propellant stabalized". Rocket engineers preferred the term "balloon tanks" to indicate that the tanks required pressure to support the rocket. You wonder about the Mercury astronauts who agreed to sit on top of these things! Often, as a missile, the Atlas was kept horizontal in a container until ready to fire. Then it was fueled and raised vertical. Later variants were housed vertically in silos, and then raised to the surface to be fired. One of the major problems with the Atlas being used as a ready ICBM was the thin skin. There are cases where workers accidentally dropped a screwdriver or wrench onto an Atlas, and the tool pierced the skin of the missile, sometimes even causing an explosion. The other problem was the propellant itself. The Atlas rockets were fueled with RP-1 (basically a highly refined kerosine) and liquid oxygen. RP-1 is a common rocket fuel, and even the first stage of the Saturn V used RP-1. The RP-1 fuel can be stored in the missiles fuel tanks if needed. However, the liquid oxygen could only be loaded aboard just before launch. So, an Atlas missile could not be launched with just a moment's notice. This doomed the Atas and its cousin the Titan I missiles as ready nuclear deterent missiles. The Titan II misiles, though, replaced the propellant with hydorzine and nitric oxide, both of which could be stored onboard, making the Titan II capable of being launched with very short notice. Though the Atlas missiles were never used in war, and were soon phased out as ICBMs, they served as boosters to launch spacecraft. Often, the Atlas was coupled with a Centaur upper stage, so the Atlas launched the Centaur to orbit, where the Centaur rocket then propelled the payload where it needed to go. Interestingly, the Centaur (or rather a derivative of the early Centaur) is still used today, and the Centaur rocket also used balloon tanks to stabalize it.
The Atlas used a rather staging unique method to achieve orbit. Early on, rocket scientists realized that much of a rocket's mass is propellant tanks and framework to hold those tanks. When the tanks are empty, then you are just carrying around extra mass. So, it is easier to drop off these tanks when they are empty. This is staging. The classic way to stage is to burn until you exhaust the propellant, and then you drop off the tanks, engine, framework, and so forth, leaving behind another rocket engine and more tanks to push what is left of the rocket. Since there is less to push, the second stage and its rocket engine(s) can be smaller than the first. If needed, you can have a third stage, or even more. In the 1950's though, no one really knew if you could ignite a rocket in space. So, both the Soviets and the Americans developed strategies to overcome this. Sergei Korolev, the Soviet chief rocket designer, built his R-7 missile with a core that fired its engines all the way to orbit. The additional thrust needed for launch was provided by auxilary rockets strapped to the sides of the central core rocket. This gave the R-7, and its direct descendant the Soyuz, their distinctive conical shape. The Atlas, though, had a different design. Instead, it had three main engines that fired at liftoff. In addition to these three engines, a couple of smaller rockets were used for guidance and steering. When sufficently high, the outer two engines quit firing. These outer engines, along with the engine skirt, were then jettisoned. The center engine continued to fire from launch to orbit. There is considerable argument on whether or not this makes the Atas the first Single Stage to Orbit (SSTO) rocket, or not since it jetissoned these engines. Most rocketeers think of the Atlas as a 1.5 stage design.
Though it was retired as a military weapon, the Atlas continued to serve as a launch system. So, it was no wonder that improvements were made. The Atlas II rockets used improved engines having higher thrust than the earlier models, improved electronics, and an improved Cenaur upper stage. Longer propellant tanks were used, adding several feet to the length of the rocket, but also adding to the length of time that it could fire its engines. This permitted the Atlas II to lift much heavier payloads than the earlier model. Later variants of the Atlas II also incorporated small solid rockets strapped to the bottom of the booster. These rockets would fire at liftoff but burn out quickly and be discarded.
More improvements followed with the introduction of the Atlas III system in the late 1990's. One of the biggest changes was the adoption of a new engine for the main rockets. This engine, the RD-180 was built by Pratt and Whitney under a license from it Russian manufacturer. So, the Atlas, once designed as a missile to be pointed at the Soviet Union, now was using a Russian engine! Other changes involved stretching the propellant tanks even more than had been done with the Atlas II and again improving the Centaur upper stage.
The most recent Atlas variant is the Atlas V. It involves a major redesign. In fact, one can argue that it really shouldn't be called an Atlas due to the extensive redesign. The 1.5 staging was dropped, so the Atlas V is now a true multi-stage rocket with its Centaur upper stage. The framework was beefed up, so the balloon tanks are gone. About all that is the same is that the Atlas V still uses RP-1 and LOX propellant, the RD-180 engine, and a Centaur upper stage. However, RP-1 and LOX are used extensively as propellant by many types of rockets. Other rockets have used the RD-180 engines. And the Centaur upper stage is common on other rocket systems, too. Different variants of the Atlas V include changes in the number of engines in the Centaur stage, different size and number of solid rocket boosters, and different options for fairing covers for the payload and the Centaur upper stage. The effect is to make different Atlas V models look quite different from one another.
So, that in a nutshell is the Atlas family of rockets.
-Astroprof
April 19 The five brightest starsWhat is the brightest star in the sky? The answer depends on how you define your terms. Do you mean what star shines with the most light, or do you mean what star looks brightest? The answers differ. When people ask me this question, what they are really asking is, "What star looks brightest as seen from Earth?"
The answer, of course, is the Sun. It is as star, and is by far the brightest thing in the sky other than an occasional unusually large meteor or a nuclear explosion. Of course, neither of the latter are stars, so we'll ignore them. Well, the Sun is not what people want to hear. So, again, rephrasing the question as to what they really, really wanted to hear, we get "What star appears the brightest, seen during the night, as viewed by the naked eye, from the surface of the Earth?" Now, the answer is Sirius. For some reason, people often think that the North Star is the brightest star. Well, it isn't. The North Star isn't even on the list of the top 25 brightest stars. Since people ask me this question a lot, I thought that perhaps I'd give some of the brighter stars and say a few words about each.
We'll define brightness by apparent visual magnitude. The magnitude of a star is a quantitative way of measuring how bright a star appears. It is an archaic system that dates all the way back to ancient Greece. In this system, the bigger the number, the dimmer the star, and the smaller the number, the brighter the star. I know that seems backwards. However, to Hipparchus, who came up with the system, it would make perfect sense. He grouped stars by "importance", with the importance being their brightness. So the first most important stars would be brighter than the second most important, which would be brighter than the third most important, and so forth. The importance became the magnitude. So first magnitude stars are brighter than second magnitude stars and so forth. Eventually, the system was extended, because many first magnitude stars were much brighter than other first magnitude stars, so they became zeroth magnitude stars, or even negative one magnitude stars.
As I said, Sirius appears as the brightest star visible at night. Sirius, also known as the Dog Star, is located in Canis Major, just down and to the left of Orion (as seen from the Northern hemisphere when Orion is high in the sky). Sirius appears magnitude -1.43. I won't go on too much about Sirius here, since I did a blog entry on Sirius back at the beginning of March. You can look at that to see more about Sirius. Sirius is visible in the evenings in the Winter and Spring months (for Northern hemisphere observers).
Canopus is the second brightest night star. Canopus is located almost 33 degrees south of Sirius in the constellation Carina. It's far southern location makes it difficult to see from the Northern Hemisphere, but it readily stands out from the Southern Hemisphere. Being so bright, Canopus is sometimes called the Great Star of the South. It is a white hot giant star. Though at magnitude -0.72, Canopus is second only to Sirius, it is nearly 35 times farther away from us. This gives an idea of how bright this star really is. An interesting thing to note is that the constellation Carina was not a separate constellation until in the 20th Century when the old constellation Argo Navis (the ship Argo in which Jason and the Argonauts sailed) was broken up into the constellations of Carina (the Keel), Puppis (the Stern), and Vela (the Sail). There is a whole story here, but perhaps I'll save that for another blog entry.
The third brightest star is Arcturus, in the constellation Bootes (the Herdsman). Most all of my North American readers know the asterism called the Big Dipper, which is part of the constellation Ursa Major. If you look at the Big Dipper, the handle appears to curve. Imagine that curve as being a portion of a circle. Continue going around that circle, and you'll come to a bright star. That is Arcturus. You could say that you "Arc to Arcturus." Arcturus is a red giant star. That is a star that has run out of hydrogen to fuse in its core and has begun the process of dying. One of the first steps is that it swells up to a size where the outer edges of the star extend out to nearly the distance between the Sun and Venus or Earth. Arcturus is also interesting in that, unlike most other stars that you see in the sky, it is not a star that orbits in the disk of the galaxy. Our galaxy is not just the spiral shape that you often see depicted. Rather, the galaxy also has a large, roughly spherical halo of stars and globular star clusters. These halo objects orbit around the center of the galaxy in orbits that are largely independent of the motion of the disk of the galaxy. Arcturus is one of these halo stars that just happens to be passing through our part of the galaxy. Most of these halo stars are small and rather dim. Normally, we'd never see them with the naked eye. However, when a star becomes a red giant, it gets brighter for a while. Eventually, Arcturus will become unstable, pulsate, and shed its outer layers into space, forming a cloud of gas that we call a planetary nebula. The core will collapse to a body about the size of the Earth called a white dwarf. Not much will then ever again happen with the white dwarf. It will just cool off and get dimmer. The white dwarf will be composed of what is left after all the hydrogen that can fuse into helium has done so, and all the helium that can fuse into carbon has done so. So, it will be largely carbon. As it cools, it will eventually become crystalline --- essentually, a planet sized diamond. Of course, we'll be long gone by the time that happens. Arcturus is magnitude -0.04.
The fourth brightest star, at magnitude -0.01, is Rigel Kentaurus, the foot of the Centaur. This is a far southern star, and it is never visible from North America. :( That is realy a shame, too, because it is also the nearest star, other than the Sun. To avoid confusion with Rigel in Orion, which is the seventh brightest star, Rigel Kentaurus is often referred to by its Bayer designation: Alpha Centauri. This is actually a triple star system, with the brightest component of the three being a star very much like our own Sun. That a star like the Sun, coupled with dimmer stars, still only comes in as fourth brightest in the sky, even though it is the closest of the neighboring stars, tells us that the Sun really isn't all that bright of a star. Virtually every star that you see in the sky is an unusually bright star, which is why you see it. The vast majority of stars are very small and very dim. In fact, most stars, even those very nearby, could never be seen with the naked eye. About a month ago, I did a blog entry on the nearest stars. I sort of envy those of you living in the Southern hemisphere, because you get to see this near neighbor of ours. It will be high in the evening sky from about May to about August for southern observers.
The fifth brightest star in the night sky is Vega, at magnitude +0.03. Vega is often used as a standard star for photometric purposes. It is a nice stable type A0 main sequence star, almost pure white. Vega is located in the constellation Lyra (the Harp). Three stars, Vega, Deneb, and Altair make up a large triangle of very bright stars that rises in the early evenings during the Summer months in the Northern Hemisphere, so these stars are often called the Summer Triangle. Another interesting factoid about Vega is that it will one day be the North Star. Polaris is the current north star because the north pole of the Earth points very near to it. So, an observer on Earth will see Polaris star roughly in the same spot all night, every night: due north. However, the Earth is slowly precessing, like a giant top. It is changing the direction that it points in the sky. In ten thousand years, or so, the Earth will be pointing in the general direction of Vega, so Vega will appear to hover around the north celestial pole all night, every night. That will make for a very impressive North Star. The one that we have is second magnitude, and Vega is much brighter than that.
Well, that marks the five brightest stars in the sky other than the Sun. I could keep going on with this list, telling a few things about each star, if there is any interest in my readers. Just let me know.
-Astroprof
April 18 Finder ScopesLast night was the first decent clear night to set up telescopes with the students in several weeks. We have not had rain, but lots of clouds, haze, etc. So, we set up the telescopes. By this point in the semester, I don't help them all that much. They should KNOW how to do this by now. Well, we get going, and a couple of them are having a terrible time finding anything, so I go over to help them. Well, I center the telescope on the object that they were supposed to look for, look in the eyepiece, and .... it isn't there. So, then I check through the finder scope, and the cross hairs are dead on. So, I ask them if they aligned the finder scope before starting. No, of course they didn't. They said, "We did that last time that we used the telescope a few weeks ago." Yeah, right, like no one has touched it since they last did. Like they didn't bump it putting things away. I remind them that aligning the finder scope is always the first thing that needs to be done.
So, for those of you new to the world of astronomy, what am I talking about?
Most telescopes have enough magnification, and small enough of a field of view that they only see a tiny portion of the sky. That makes them really tough to use to find anything. So, coaxial with the telescope is a smaller telescope that we call the finder scope. This finder scope is low magnification and large field of view, making finding things easier. Good finder scopes have a set of cross hairs visible when you look through them. You center the cross hairs on the object of interest, and then when you look through the main telescope, you can see what you want. This only works, though, if the finder scope is properly aligned with the telescope. The finder scope has a set of set screws that can be adjusted to properly align it with the main instrument. If you do this very carefully, and if the finder is very securely attached to the telescope, and if you don't jar it when you put away the telescope, then the finder should stay pretty well aligned. However, with the student telescopes, this is never the case. They don't treat the equipment as I do mine. My personal telescope rarely needs adjusting because I am always careful. So, I teach the students to always check the finder scope alignment first thing.
Well, this brings up the point about what sort of finder is best. There are lots of opinions here. Often you find that the smaller telescopes, or the telescopes that you buy at discount stores, have very inexpensive (we can call them cheap) small finder scopes. The general opinion is that they are next to worthless. Why? Well, this gets back to how telescopes work. They gather light and they magnify. Really, the gathering light is more important than magnification. The bigger the aperture, then the more light that is gathered. So, you want to have as large an aperture as is reasonable given price, portability, ease of use, etc. This same goes for finder scopes. The typical finder scope is too small and too much magnification for its size. The problem is that the more you magnify, the more you spread out the light, and the dimmer things will be. Usually, you are looking for something too dim to see with the naked eye. So, making it dimmer is bad. The bigger the finder, then brigher it will be, unless you have too much magnification. The typical finder with a small telescope has an aperture not much bigger than your eye's pupil, so any magnification makes things look dimmer than they would with the naked eye!!!! So, I always recommend replacing the small finder with something else. There are a couple of options. One is to replace it with a bigger finder scope. This works if the telescope itself is large enough to support the weight of a larger finder. I normally recommend a finder with no more than 10 times magnification. Any more, and you wind up reproducing the problem of the telescope itself --- seeing too small a part of the sky. Magnification lower than about 5 times magnification, though, and you are not zooming in much better than you see with the naked eye, so why bother magnifying? Also, the larger the aperture of the finder, the dimmer things that you can see through it. If the finder is large enough, and not too high magnification, then it will show things that you normally could not see with the naked eye, making setting the telescope on these objects far easier than just guessing where they are. Binoculars are good for this, and among the best binoculars for astronomical work are 10x50 binoculars. So, I usually suggest a 50mm aperture finder scope. For most amateur telescopes, then, something like a 9x50 finder seen here is quite good. For many of the telescopes that we use at the college, we replaced the stock finder with a 50mm finder scope similar to this. The more that you can see with the finder scope, then the easier it is to use it to point the telescope. Even if the target is still too dim to see through the finder, you can look on a star chart and see, for example, that Object X is about a third of the way between two stars that you can see in the finder scope. Put the cross hairs about a third of the way between, and you should be pointing pretty darn close to the target --- at least close enough to find it with the main telescope. But, the finder needs to be able to see the reference stars.
However, even a finder scope is sometimes hard to use, since even the finder shows a small portion of the sky. I often sight along the barrel of the telescope to line it up with where I want to look. That way, when I look in the finder scope, what I want is often in the field of view, or at least near the field of view, so this makes finding objects easier. Well, if that is the case, then if you could just visually align the telescope more precisely without a magnifying finderscope, it would be much easier to use. A number of years ago, amateur astronomers used a variety of devices to get past this problem. I have seen small plastic pipes tied to the barrel of telescopes that you can look through to point them in the general direction of what you want. Some would install screws at the front and back of the tube adjusted so that lining one up with the other and with the location of the target would do the trick. This was fine for the Moon, Jupiter, certain stars, or other objects visible with the naked eye. For many other objects, you could still look at star charts and see where they are located in relation to brighter naked eye stars. You could then put your sights about a third of the way between two stars if you know that the object is about a third of the way between those two stars. This works better if you are using very low power with the main telescope, so that it sees the largest portion of the sky. Then, someone had the idea of having illuminated finding aids. This eventually took the form of the Telrad sight. The Telrad is basically a sort of heads-up display. You look through a piece of glass at the sky, and a target is projected onto the glass. You adjust the target to center on where the telescope points. Then, you move the telescope to where the target is over the object that you want to look at, and if you did it right the object will appear in the eyepiece when you look through the telescope. The only problem with the Telrad is that it is big and heavy. It is not appropriate for a small telescope. That is OK, though, since there are now several other smaller non-magnifying sights available. They, in fact, are often smaller and lighter that the tiny and nearly useless finder scopes that the smaller telescopes come with, and I think far better as well.
But, of course, it all eventually come down to having the finder, of whatever type, aligned with the telescope. Checking this alignment should always be a first priority when setting up the telescope. But do you need to do this for the goto telescopes? After all, you might think that since they go to the object by themselves, you don't need a finderscope. Well, unless you have a GPS unit that plugs into the goto controls so that the telescope knows immediately how it is oriented, then you will still need to point the telescope at several known stars to help it orient itself. That means using the finder scope.
So, if you plan on getting a telescope, plan on spending more money to get a good finder scope. If you don't, then you will wind up frustrated and not using the telescope much.
-Astroprof
April 17 Financing Public EducationNormally, I blog about astronomy or space exploration topics. Sometimes, I talk about issues related to being a college professor. On rare occasions, I am more personal. And on very rare occasions I do something quite different. This is one of those, though, I suppose, it does relate to being a professor in a round about way. I am going to talk about public schools.
Today, here in Texas, the state legislature meets for a special legislative session to try to deal with public school financing issues. Funding public education is an issue all over the country, of course. Here in Texas, it has become a nightmare. So, let me fill you in on the situation. This session will be the sixth legislative attempt to deal with public school funding in three years. The previous five times met with dismal failure, as have several attempts in previous years. It takes a special session here, because the Texas legislature only meets every two years. Normally, this is a good thing. The less frequently we let them meet, the fewer flakey laws they can come up with. This would normally be an off year, so the governor had to call a special session. Now, I will explain what is going on. For those of you with an interest in law, this might be interesting. For the rest of you, skip to the end, because it is convoluted and a mess.
OK, now for why this is an issue at all. In Texas, all areas of the state are divided up into local school districts. These districts get some state support, but most of their operating money comes from local property taxes. Texas has no state income tax, so we have a high sales tax, and very high property taxes to fund local government. Well, the legislature sets a limit on how much property tax a local school district can charge. It is limited to $1.50 per $100 of valuation. So, a $100,000 dollar home would nominally pay about $1500 in school tax. However, they allow an additional surtax to pay for bonds used for capital expenses. So, the school district can tax at the maximum rate, and then tack on another $0.50 per $100 to pay for new schools, football stadiums, school busses, etc. That means that the $100,000 home might actually be paying $2000 per year in school tax. Add to that the city, county, etc taxes, and you are looking at a $3500 or more property tax bill each year. And it is going up! Since I bought my home almost 7 years ago, my taxes have almost doubled. This is true all over the state, and the taxpayers are demanding some relief.
Ah, but it is more complicated. As it turns out, we are under a court order to fix the school finance situation before June 1 or the courts say that they will shut down the schools. Huh? How did it get to be that big of a mess? It goes back to 1971. In that year, a lawsuit several years in the making was decided by a federal judge declaring the Texas school finance system unconstitutional. According to the ruling, our system of local taxes funding local school districts discriminates against children in poor school districts, many of whom are minorities. Anyway, more court battle ensue, with rulings overturned, more rulings, etc. all the way up to the US Supreme Court. Finally, this culminates by a ruling of the Texas Supreme Court in 1989 that the Texas schools are financed violates the state constitution by not providing substantively equal education for all students in the state. Now, if you've ever seen the Texas constitution, then you might understand my confusion that you could rule that anything is either guaranteed or prohibited by it. That thing is a hideous and completely arcane document filled with inconsistencies and even contradictory provisions. At any rate, in a special session, the legislature passes a bill changing school funding in 1990. It is declared unconstitutional a few months later. The following year, the legislature had to come up with a new plan. That plan lasted one year before being declared unconstitutional. Then, by 1993 another plan came into being called the "Robin Hood Plan" by most people. Under this plan, money is taken from property rich districts and given to property poor districts. There are more court cases. Property rich districts argue that the plan violates the state constitution by taking property tax money collected by a local taxing agency and using outside of the jurisdiciton of that agency --- a prohibited act. A bigger issue is that the property rich districts are often required to give 30% up to even 50% of their tax revenue to the state to be distributed to poor districts. This means that they must raise taxes accordingly. But, they still give away money as a percentage, not a monetary value, so they give even more away if they raise taxes. Eventually, what has happened is that many of these "wealthy" school districts have had to cut teachers, not give teachers raises, cut their talented and gifted programs, drop special academic programs, and charge students to participate in extra-curricular activities, and even make students buy their own band and football uniforms. Some even have the teams pay the cost of going to games themselves. To rub salt into the wound, the poor districts receiving the money are not giving teachers raises or improving classroom education. They are building new administration buildings, hiring new administrators to handle the influx of money, building new football stadiums, and so forth. So, the rich districts brought a new lawsuit to bear. This time they argued successfully that the current system has resulted in nearly 3/4 of the school districts taxing at the maximum allowed rate, thus having a defacto statewide property tax, since much of this money is being redistributed to other districts. The courts agreed, and so the Robin Hood plan was declared unconstitutional.
Well, while the courts were hearing the arguments this last time, the legislature was in session. It was clear that the arguments that Robin Hood was unconstitutional were valid, so they were trying to come up with a new plan to put in place when the court declared it so. They failed when Texas Democrats decided to go en masse to Oklahoma so that there would be no quorom, so no vote could be held on redistricting for Congressional seats. Unfortunately, the school finance plan got lost in the shuffle. The court declared Robin Hood unconstitutional. The governor called a special session and presented his plan to cut property taxes, raise the cigarette tax, alcohol tax, and impose a tax on topless bars and X-rated videos (huh?). Anyway, the legislature rejects his plan, but can't come up with one of their own. A judge declared the current system unconstitutional and gave the legislature one year to come up with a new plan. The following year, 2005, in the regular legislative session, the legislature agrees to reduce property taxes, but can't agree on how to raise money to offset that, so the session ends with a bill passed that did not effectively address property tax relief, and only put a window dressing on the whole constitutional issues. The governor decides to veto the bill rather than just let the law be declared unconstitutional, which surely would have happened. So, the governor declared another special session and charged the legislature with fixing the problem. They argued and could not agree on any solution before the session ended. The governer called another special session, with the same result. The judge ordering a solution within a year gave an extension during all of this, but that has now run out. The state is under a deadline to fix things by June 1 of this year. So, the governor has called yet another special session to deal with school finance. Why did he wait so long? Well, this session is right after runoff elections for the primaries. That way, the incumbants can go ahead and be either heros or asses as they see fit and they won't have to face the consequences of their actions at the polls for a while. My bet is that they will chose to be asses, as usual.
Anyway, there you have it. That is the mess that is Texas school finance. So, what will they do? I dont' know. What should they do? I don't know. I am glad that I don't have to work on this. It will be a mess. I really don't know how public schools should be funded or managed, but I am convinced that how we do it here in Texas doesn't work. I see evidence of that everywhere that I look. The clearest evidence that things are not working is looking at my incoming college students. They are the worst prepared to be in college that I have seen in all the years that I've been teaching. The only thing that they know how to do is to pass the state assessment test, which is pretty poor. That thing is how they rate schools here, and so all the schools have classes on how to pass the test. Forget learning the material. Learn which multiple choice answers not to select. Learn strategies to guess answers. Memorize key words or phrases and their counterparts so that you can match an answer with one word to a phrase or word in the question. Forget critical thinking. That isn't tested. Problem solving? The majority of what they call problem solving on the test is just plug numbers from a word problem into an equation. It isn't really problem solving, so students come to college not knowing how to solve problems. It is really sad.
So, we'll see what the legislature comes up with, or even if they manage to come up with anything at all. I fear that they might not, and then it will be up to the courts to do something. Well, it should be interesting. With luck, my property tax will go down to something more reasonable, but I doubt it.
-Astroprof
April 16 Forbidden Planet at 50Fifty years ago, the award winning classic science fiction movie Forbidden Planet was released. The movie predates me, but I did get to see it on television when I was young.
I have always rather enjoyed science fiction. Growing up, I used to watch scifi movies on TV whenever I got a chance. There was often one showing on Saturday afternoons, and for several years, there was a station that showed a scifi movie every Friday night. There was also a station that showed movies every weekday afternoon, with one day per week set aside as science fiction day. It was one of these afternoons, I think, that I first saw the movie. It made an impression that stuck with me, so when the movie came out on DVD a few years back, I just had to get it.
For those of you who don’t know the movie, the screenplay for Forbidden Planet was written by Cyril Hume, the movie was directed by Fred Wilcox and produced by Nicholas Nayfack. Forbidden Planet had an all star cast (or least a cast that were to be stars) including Walter Pidgeon, Leslie Nielson, Richard Anderson, and Anne Francis.
In the annals of science fiction films, this movie is a giant. It is a well thought out story with several sub-plots running. The movie has the sort of optimistic American ideals of the 1950’s and elements of the sort of fear of technology of that era. The movie also had a fairly sophisticated commentary on the state of humanity. Even the dialogue is good. For the 1950’s, the special effects were stupendous. Personally, I don’t think that any special effects equaled those of Forbidden Planet until Star Wars in the 1977. I showed this movie one night to the students of our astronomy club when it was too cloudy to go outside. The story is still good, and the special effects even hold up today, though they don’t look quite as sophisticated as we are used to seeing now-a-days. Several of the plot devices and ideas formed the basis of much of what we have come to think of as standard ideas in science fiction. You can see the legacy of Forbidden Planet in Star Wars, Star Trek, and all sorts of other stories.
The story of the movie is loosely based on Shakespeare’s The Tempest. The story starts with an interplanetary flying saucer from Earth coming to investigate why an expedition to the planet Alair-IV has apparently vanished. This saucer is part of a galactic space quasi-military space fleet (similar to Star Fleet). The captain and crew land on the planet, ignoring a broadcast warning that to land was to face great danger. Upon landing, a robot named Robby meets them and takes the captain, Commander Adams, and the ship’s doctor to meet the sole surviving member of the expedition, a man named Morbius. There they find Morbius living with his daughter Altaria and their robotic servant, Robby. Morbius claims that the original expedition had been killed by some sort of creature that for some reason has left him and his daughter alone for all these years. Morbius claims to have found knowledge left over from an ancient civilization that used to live on the planet. Commander Adams wants to take them back to Earth, but Morbius refuses, so Adams decides to use parts of his spaceship to fabricate an interstellar communication system to report home and get orders to deal with the situation. Soon, somehow the communicator is sabotaged. Adams suspects Morbius, but there is no proof. Eventually, a crewmember is gruesomely killed, and Adams heads to Morbius’ residence to demand answers. There, he and the doctor find that Morbius has discovered found actual working artifacts of the ancient beings called the Krel. They had a teaching tool that had taught him how to build Robby the robot. Underneath the Morbius residence is a massive Krel facility that goes on for miles and miles. It has been self sustaining and self repairing for millennia, though even Morbius has no idea what it does for sure. He suspects that the Krel were on the verge of developing a technology that would do all their work for them with just a thought. Adams and the doctor are impressed, but this does not help explain the loss of a crewmember. They go back to the spaceship where disintegrator cannon have been set up to protect the ship and crew. That night, a giant invisible monster attacks. The monster seems to resist their every weapon, and then it suddenly disappears. Decades later, I still had an image of the giant creature caught in the disintegrator beams where it became sort of visible. The special effects are obviously animation by hand drawing, but it still gives me a chill when I see it. Adams and the doctor go back to the Morbius residence, where they confront Morbius again. While Adams and Morbius argue, the doctor gets his brain boosted in the Krel machine, and he realizes the monster is actually a creature created by Morbius’ subconscious mind. The giant Krel machine had created it in response to Morbius’ subconscious (the Freudian id) desire to put an end to the people who disagreed with his wishes. Eventually his own daughter disobeys him and challenges him, and his Id Monster attacks. He eventually sacrifices himself to save his daughter. Adams takes Altaria and they leave for Earth. Their last act was to set the self destruct on the giant Krel machine.
Robby the robot is interesting in that he had built in programming that prohibited him from harming any human being. This predates Asimov’s laws of robotics. As I suggested, the Earth saucer is reminiscent of the Star Trek, with an organization like Star Fleet, and an intrepid captain and doctor rushing off into danger (though no Vulcan science officer!). The disintegrator ray guns seem to work a lot like phasers. Scenes of the Krel machine are seen in other science fiction movies and shows that follow, and they bear some resemblance to scenes in the interior of the Death Star in Star Wars. There are even force fields like seen in Lost in Space.
There are a couple of interesting commentaries here, as well. One, of course, which was a common theme in science fiction in the 1950’s and 1960’s was taking a shot at technology. Frequently in these movies some technological advance gets out of control and everyone is in peril. In Forbidden Planet, at least, the technology is rather neutral. It is the use of the technology that gets everyone in trouble. In many of these movies, some technological or scientific advance is made without any regard for its moral consequences. Here, the Krel machine was designed with the high and noble goals of freeing the peaceful Krel from work so that they could concentrate on learning, poetry, art, and such. The problem was their baser instincts that the machine keyed on, and the Krel wound up killing themselves off. Then, when Morbius came to be connected with the machine, anyone crossing him got killed. The commentary here is that we all have a selfish and brutal side to us that we must keep under control. In Star Wars terms, we can all be tempted to the dark side. Again, this is a little different from other movies of the era, where some mad scientist is totally immoral. Here Morbius is essentially a good and caring person who would never consciously harm anyone. His subconscious, though, wishes harm to those who challenge him.
The movie is very interesting and thought provoking, and it deserves to be a classic. I think that even people who don’t normally like science fiction would find something of value here. If you haven’t seen Forbidden Planet, then you should! It is well worth your time.
-Astroprof
April 14 Planetarium StuffI have always liked going to a planetarium. Growing up, trips to the planetarium allowed me to learn the night sky in a way that I could not have otherwise done. A knowledgeable person would point out stars and constellations on the dome of the planetarium, time could be sped up and slowed down to see the motions of the planets, and you could see what the sky would look like without light pollution (something that growing up in Houston, Texas, was hard to fathom). So, I thought that perhaps a planetarium blog entry might be in order.
First of all, since I wanted to talk about more than one planetarium, I figured that it would be useful to know the plural of the word. The word obviously comes from Latin, and having had several years of Latin, I knew that the plural should be “planetaria,” if normal Latin conventions are used. However, I often have also heard “planetariums” used as the plural of the word. So, I naturally decided to look in the dictionary. Much to my consternation, I find that both words are listed as the plural of planetarium! Now, if that isn’t silly. Microsoft Word seems to think that the plural is planetariums, but the majority of people that I personally know who are in the planetarium field (planetarians, they call themselves) use planetaria as the plural. Since planetaria also fits with my own reasoning from knowing the Latin root of the word, that is what I will use.
So, now that we have the grammar down, what exactly is a planetarium? Put simply, a planetarium is a device that shows what the sky looks like. Planetaria in some form have been around since ancient times. We don’t know who came up with the first one, but there are stories that the Arabs used to have tents with small holes punched through the material. Inside, the tent during the daytime, you’d see a representation of the night sky. There were also devices such as astrolabes that could be used to show the relative orientation of stars, the Sun, Moon, etc in the sky at different times of the day. One might think of these as handheld planetaria. A more modern version of this would be software that lets you see on your computer screen what the sky would look like at night. This is universally called “planetarium software.” Interestingly, many modern planetarium projectors use computers to drive them, and the software so used is also called planetarium software, even though it only superficially resembles the planetarium software that shows visualizations of the sky. Personally, I use planetarium software on both my desktop computer and on a laptop that I can take into the field. Also, I have planetarium software on a PDA that has turned into one of the most useful programs that I have ever put on that device. Anyone who plans on going out observing, especially any amateur, should think about putting planetarium software on a PDA (if you’ve got a PDA, that is!). You would not believe how often that you use it if it is available.
Related to a planetarium is an orrery. Most of you have probably seen an orrery, but had no idea what it was called. An orrery is, simply put, a model of the Solar System. It usually has the Sun in the middle, and the planets positioned in their proper positions around the Sun. The planets can then be repositioned to show their motion around the Sun. A mechanical orrery has gears and motors to move the planets about in the proper speed. So, an orrery would be a sort of working model of the Solar System. I have seen some very complex ones that even had moons around the various planets. A few that I’ve seen have even incorporated projectors to shine the relative planetary positions onto a screen. That makes such an orrery very close to a planetarium.
But, what I really wanted to talk about was not planetarium software, but rather what I think of as actual planetaria: i.e. planetarium projectors inside specially built buildings. This is what I think of as a planetarium. There is a certain mystic to the large domed room with the strange machine in its middle. I don’t know how long such planetaria have existed. The first large precision planetaria seem to date to early in the Twentieth Century, with the construction of such a device by Carl Zeiss in 1924. I have heard that less sophisticated devices existed before that, but for now we’ll just attribute the first modern planetarium device to Zeiss. Essentially, such a device is a powerful lamp situated inside a hollow ball. The ball has holes drilled in its surface to represent stars. The larger the stars, the larger the hole is drilled. This star ball is then place inside a room with a domed ceiling. However, the star ball is very expensive to make. It can’t be done on an assembly line, so it must be done one at a time by a craftsman. Also, drilling precision holes in a spherical shape is quite difficult and time consuming. Until the invention of computer controlled machining, even a template was not possible. So, that made construction of the planetarium ball very expensive. Also, you can’t drill holes for planets on a ball like that since they move around. That meant that in addition to the large star ball, the planetarium projector also needed a separate mechanism to show the planets. This usually consists of a light source and a set of individually controlled mirrors. The mirrors are geared to turn together, much in the way that the orrery works, projecting a dot onto the planetarium ceiling at the proper place to represent the planet. But, since the planet projector is not on the star ball itself, the positions of the planets will be slightly off. This effect is minimized by making sure that the ceiling onto which the stars and planets are projected is located many times the diameter of the ball away from the projector itself. Also, the image on the ceiling will be misshapen to an observer sitting far from the star projector. These are known issues, so a well designed planetarium has the seating clustered near the star ball in the center of the room. Planetaria designed as public theaters, though, often cram as many seats as possible into the space, resulting in a poor view for anyone not near the center of the theater.
The Zeiss planetaria were a fantastic success. However, they were quite expensive, so only a few were built. These were associated with major museums in large cities, and even then they could only be built if some generous benefactor donated a large sum of money to the museum to build the planetarium. Armand Spitz, an amateur astronomer and astronomy populizer, decided to design a less expensive planetarium that would be affordable to colleges, schools, and smaller museums. Spitz was convinced that a planetarium could be used as a fantastic tool for education. He developed a design for a planetarium projector consisting of a dodecahedral ball of flat plates. The ball looked sort of funny, but the holes for the stars drilled in the flat plates were easy to produce from a template. This cut down costs. This new planetarium design eventually took off, and these smaller, less expensive, planetaria started popping up all over the country. His company still exists, but they eventually switched production to the more traditional spherical star ball. A college that I used to teach at had a planetarium with a Spitz projector. It was absolutely wonderful to teach astronomy using a planetarium.
Of course, technology has continued to advance. It is now possible to have a computer screen and a fish-eye lens that can project onto the dome of the planetarium anything that is shown on the screen. This has some advantages over the old star ball. For one thing, the star ball is limited to showing what the sky looks like from Earth (Granted, if you know how to use it, then you can show the sky from anywhere on Earth, any day, any time of day, any year, and I have done this.). The computer screen can show the sky from anywhere in the universe that the computer has enough data to generate a sky view. You can even simulate “flying” from one star system to another. You can also highlight and zoom in on certain things, something not possible with the star ball projector. One disadvantage, though, is that for most of the computer generated views, the stars don’t quite look right. For one thing, to make a brighter star, these projectors usually use bigger dots (especially the earlier ones). In the sky, the stars all look the same size, just different brightness. This is more what the sky looks like using a star ball. Still, the more modern computerized projectors seem to be overcoming this limitation.
While I normally think of the planetarium as a place to see the stars, you can do more with it. Basically the planetarium building is a room with a high domed ceiling. The ceiling is reflective so that you can see the stars better, and this makes the entire ceiling basically a giant projection screen. So, you can also show movies and slide shows in the planetarium. It also is a place where you can see laser shows. Sadly, these seem to be more common uses than showing the sky. The last few planetarium shows that I have been to didn’t even really mention the stars on the ceiling one time all during the show! In fact, the shows were little more than fancy slide shows with some cool narration. This misses out on the entire reason for having a planetarium in the first place!!!!
The other problem seems to be that most planetarium shows produced now-a-days seem aimed at elementary school kids. While I have no problem with planetarium shows aimed at young children, and I believe that it is essential to get them interested in science early on, I also think that it is a mistake to only aim at the young ones. We are losing children from the sciences in middle and high school. When asked why they didn’t want to study science, a group of high school students a few years ago replied that it was because they thought that science was boring, irrelevant, and only for kids. Clearly something is horribly wrong here. I can’t imagine anything less boring. I see science involved in all aspects of my life, so it is far from irrelevant. And as for being only for kids, I guess that I am young at heart, but still … . So, perhaps we should have some of these programs aimed at middle and high school, and even some aimed at adults. I think that we are missing out here.
I wish that we had a planetarium at my college so that I could put together some planetarium shows that used the unique capabilities of the planetarium projector and the planetarium experience. Alas, planetaria are still expensive to build and to maintain, so we aren’t likely to get one anytime soon (if ever). -Astroprof Astroprof is HeartlessEarlier today, I had a student come by asking for an incomplete for the course. I looked blankly at her and said "Huh?" She repeated, eplaining that she was having a hard time, had all sorts of things going on, and so forth. I explained that the rules for an incomplete are that they are to be assigned only to those students who have completed at least 85% of the course, and are simply unable to complete the last portion of the course by the deadline to turn in grades due to extenuation circumstances. It isn't for students that are having trouble keeping up. Also, incompletes are assigned here only during the last two weeks of the semester, and we go until the middle of May. Then the tears came. She explained that she was working full time, that her son has been sick, that her husband has been sick, and she has been unable to do the homework, turn in lab exercises, etc, and she needs more time. I said that I was quite sympathetic to her plight, and that I had been there myself, but this is way too early to think about an incomplete. She begged, saying that she wasn't going to do well in the class and that she needed the incomplete. I explained that the institutional policy is that incompletes are to be given only for extraordinary circumstances, and then only at the end if something keeps the student from finishing due to circumstances arising at the end of the semester. They are not for students who have trouble keeping up over the course of the semester, whatever the reason. Also, over the years that I have given incompletes, only one student has ever successfully finished one. This is particulary important here, since we have an institutional policy that the incomplete MUST be finished within three weeks of the next semester starting or else it becomes an F automatically. Other colleges and universities in the area hand out incompletes like candy, and they never enforce completion deadlines. Many studenst sign up for classes, never attend or do any of the work, and then ask for an incomplete. We are far more stringent here, thankfully. I told her that we still have an exam, a term paper, a final exam, and a number of homework and laboratory exercise yet to come. It is way too early to give up. Even if she got an incomplete, it will only get harder to finish as time passes. Also, I am not going to give up my time to come in to meet with her during the break between semesters to do laboratory exercises with her. She went away very unhappy and in tears.
I felt really terrible, but the truth is that she would be better off doing her best and getting the grade that she gets rather than trying to take an incomplete. We also have a ridiculously late drop date around here. She can even still drop the class if she feels like she won't pass. Again, I feel badly for her, and I felt really terrible sending her away like that. I know that she feels that I am heartless and uncaring, but I really think that taking an incomplete, especially at this point, is the wrong move (even if institutional policies allowed it).
Does anyone have any ideas?
-Astroprof
April 13 Of Meatballs and WormsOh, now doesn't that sound like a wonderful title? Well, it's got nothing to do with food and animals. Rather, this has to do with NASA insignia. I thought that it might interest a few of y'all to hear something about them.
During the 1950's, both the United States and the Soviet Union were working to put the first artificial satellite into orbit around the Earth. The Soviet Union beat us with Sputnik. Eventually, the United States joined in with Explorer 1. Part of the delay seems to be that President Eisenhower wanted the American space effort to be civilian in nature rather than military. The Soviet agency that put Sputnik into orbit was the same agency designing and building ballistic missiles to loft thermonuclear warheads at us. However, our best rocket scientists, under the leadership of Werher von Braun, worked at the Army Ballistic Missile Agency in Huntsville, Alabama. The Vanguard rockets, funded by the NSF, kept blowing up when we tried to launch them. Finally, von Braun's team was given the go-ahead to launch a satellite designed by the Army's Jet Propulsion Laboratory in Pasadena, California. It was clear that our best rockets were military, just as in the Soviet Union. It also became clear that we were also in a race to put a man in space. Again, the military had oversight of the Soviet space program, and we wanted to be different. We wanted a civilian space program. So, in 1958, President Eisenhower signed a bill into law creating the National Aeronautics and Space Administration (NASA). This new agency was given the assets of the old National Advisory Committee of Aeronautics (NACA) together with most of the Army Ballistic Missile Agency (which became the Marshall Spaceflight Center) and the Jet Propulsion Laboratory (whose name being less militaristic was kept). NASA also got the Ames Research Center, the Langley Research Center, the Lewis Research Center, and a couple of flight stations.
Now, the only thing needed was a logo for this new civilian space agency. The old seal used by NACA simply wouldn't do. It was really cool, after all, with a picture of the Wright brothers' airplane on it, but a primative biplane was not really the symbol that they wanted for an agency that was going to be sending men into space. So, a new symbol was clearly in order. A formal seal was produced at Lewis showing the Earth and Moon System, with a satellite orbiting the Earth, and a large red chevron around the Earth symbolizing the aeronautics part of NASA (that being the latest thing in high speed aircraft wings at the time). Around the outside of the seal the words "National Aeronatics and Space Administration" and "U.S.A." are written. However, the seal was complicated and quite involved. So, James Modarelli, of Lewis Research Center, was asked to design a somewhat less formal emblem. What he came up with is the most familiar symbol that people associate with NASA. It is a blue sphere (symbolic of Earth) with stars in it (symbolic of space), the letters NASA in the center, with a stylized orbiting body going around the letters. Across the face of the blue ball, in front and back of the "NASA" is the red airfoil from the NASA seal. This is the symbol at the entrance to NASA centers, the symbol of the Apollo days, and the symblol that most associate with NASA. The official seal is only used on formal documents and such.
Following Apollo, though, NASA began to wonder about updating its image. They wanted a more modern symbol. They wanted something with a bit more of a flair to it, and not something that calls to mind engineers with white shirts, narrow black ties, thick glasses, and pocket protectors. So, they came up with a thoroughly 70's symbol: the word NASA written in smooth, curvy red letters. At once the new logo drew criticism and praise. It was modern, sure, but for the more conservative folks it looked silly. The new logo got the nickname "worms" from its appearance. However, the new logo's supporters liked the stylistic flair, and they called the old logo the "meatball." Also, the old round logo was difficult to place letterhead, and block lettering looked out of place too near it. The meatball logo also could not be sized too small. If the size were reduced below about half an inch, then the stars disappeared. Two colors to the logo also made it much more expensive to reproduce. The single colored, somewhat rectangular worms seemed an easier fit. So, for some time, the worms began to displace the meatball. However, in 1992, the then NASA administrator Dan Golden decided that the agency should return to the meatball. NASA had attempted in the 70's to make spaceflight routine with the Space Shuttle. They almost succeeded, too, until the Challenger accident showed that space travel is never routine. Goldin thought that the meatball logo would recall the glory of the early days of spaceflight. So, the worms are now back out. They are not to be any longer used on any NASA equipment or publication. About the only place that you see worms are in the gift shops on NASA related items, or on old hardware that hasn't been repainted.
Now, there were a lot of things that Goldin did that I think could have been done better, and some things that he did that I disagree with. However, I rather like the meatball logo. It is easy to identify, and it instantly is recognizable as NASA. Also, it does bring to mind the heady days of Mercury, Gemini, and Apollo. I can see a place for the worms, too, though. I rather disagree with the decision to ban worms altogether. A mix of the logos might be OK. Individual centers, programs, and projects often have their own logos, too. I also agree that all external correspondance should include the official NASA emblem rather than the local logo. That makes it clear that the program is a NASA program. Since NASA is publically funded, it is important for people to see and immediately recognize NASA's involvement. That way, they can see what NASA is doing for them. However, the worms are pretty unique, too. I don't think that anyone can mistake what they represent.
That's my two cents.
-Astroprof
April 12 45 Years of Manned SpaceflightForty-five years ago, a massive rocket, basically a modified R-7 ballistic missile, roared to life at Bailonur. The R-7 was the Soviet Union's first long range ballistic missile. It consisted of a central tube with four strap on boosters around outside of the bottom of the central tube, giving it a sort of tapered shape, rather like a metallic Christmas tree. Propellant for the R-7 was refined kerosine and liquid oxygen. The R-7 was designed to carry a 5 metric ton thermonuclear warhead. However, on April 12, 1961, this R-7 held a small sphere on top that resembled a bathosphere. Inside this sphere was Yuri Gagarin. The spacecraft was Vostok 1. Gagarin was basically along for the ride. In fact, his controls were locked so that he could not assume control of the spacecraft. In an emergency he could be given a key to enter into the instruments to assume command. However, this would be an extraordinary situation. For all practical purposes, he had as little control of his spacecraft as Laika, the dog that flew on Sputnik 2. The flight was successful, with Gagarin making a complete orbit of the Earth in a little over an hour and a half. The Vostok capsule was not designed to safely land with the cosmonaut on board, so he ejected when the craft was at a safe altitude and floated down by parachute. The R-7 missile was not a good design for an ICBM: it took too long to fuel and prepare for flight. However, it was a fantastic booster to lift payloads into space. With some modifications, the R-7 flies today as the Soyuz rocket. All manned Soviet and Russian space missions, Vostok, Voskhod, and Soyuz, have lifted on some variant of the R-7 rocket. This is a fantastic tribute to Sergei Korolev's rocket design. It is still in use 45 years later supporting missions to the International Space Station.
On can argue that manned spaceflight began some time prior to April 12, 1961, because planning for this flight can be traced as far back as the 1950's. Even Wernher von Braun was thinking of manned spaceflight in the 1940's. However, Gagarin's flight was the first successful manned mission.
The Soviet Union, though, was not the only nation working to put a man in space. On May 5, 1961, Alan Shepard rode a capsule named Freedom 7 on a quarter hour flight from Florida to the Atlantic Ocean in a large parabolic arc to become the first American in space. The Redstone rocket that launched him was nowhere near powerful enough to lift a load as heavy as a capsule into orbit. That required an Atlas rocket. The problem with the Atlas, though, was that it tended to explode when launched. Those bugs had to be worked out before John Glenn could ride Friendship 7 into orbit on February 20, 1962. By this time, both nations had set eyes on the Moon. The Soviet Union began development of the Soyuz spacecraft and the massive N-1 rocket to launch a vehicle to the Moon. The United States began work on Apollo and the Saturn V rocket. The Saturn V, a massive rocket nearly as tall as a 40 story building, was the largest operational rocket ever built. When it launched, all of Florida and Georgia shook. However, as big as the Saturn V was, it still was not large enough to lift a spacecraft large enough to land on the Moon and return to Earth. Instead, a small lander would separate from a mother ship to land. The lander would then lift off and rendezvous with the orbiting mother ship, which would then return to Earth. This meant that spacecraft had to be able to find each other and dock in orbit. Also, no one knew if astronauts could live that long in space, without the feel of the gravitational pull of Earth on their bodies. So, Project Gemini was born. Gemini perfected the skills needed for piloting and docking spacecraft. Gemini provided valuable data on long duration spaceflight. Gemini provided the opportunity for the first spacewalks. So, when Apollo came, NASA had plenty of practice in space. However, budget issues cut Apollo short. The last three missions to the Moon never flew.
The United States had won the space race. Now, what? What was to come next? It would be a shame to shut down NASA, put away all our rockets and spacecraft, and go home. Surely, the justification for going into space was more than just beating the Soviet Union, right? Well, along the way, other reasons for space exploration were soon found. Satellite communications, at first a novelty, grew to become a major fixture of society. The military began to rely on satellite surveillance, communications, and navigation. Scientists and engineers realized that materials behaved differently in low gravity environments, paving the way for space research. It was no surprise that a manned space station should be in the plans.
The Soviet Union beat the United States to orbiting a space station with Salyut 1, launched April 19, 1971. Salyut 1 was a fairly small structure with simple living and work spaces, however it paved the way for later space exploration. Salyut 1 was followed by six more Salyut class stations, with Salyut 7 being launched April 19, 1982. Then, the Soviet Union launched Mir. The Mir space station started as an improved Salyut, but then more sections and modules were added, and numerous spacecraft came to call on Mir over its decade long life, including not only Soyuz craft, but also the American Space Shuttles, making Mir truly into a modular space station. However, we can't overlook the first American space station: Skylab. With the last three Apollo missions cancelled, NASA had three Saturn V rockets left over. The upper stage of one was adapted to become Skylab, the first American space station. Three cycles of astronauts visited Skylab using Apollo capsules launched atop smaller Saturn I-b rockets. Skylab proved the value of space-based research.
With the end of the Apollo program, NASA had to select a new mission. Originally, plans called for a permanently manned Earth orbiting space station, a permanently manned Moon base, and a mission to Mars. All this was to be done by the end of the 20th Century. Given how quickly space exploration had gone from Sputnik to landing a man on the Moon just over a decade later, this seemed a realistic goal. However, the lack of sufficient budget kept this from happening. NASA got a space shuttle. The shuttle that was built was a scaled down version of what they wanted, together with a load of compromises. The Space Shuttle was planned to be a cheap and efficient way into space. The need for inexpensive access to space was obvious. We were increasingly dependent upon satellites, but each satellite launched took a multi-million dollar rocket. Also, several satellites were doomed by very simple failures that could easily be fixed on Earth, but not remotely. Also, plans were still on the books to build a space station. So, the Space Shuttle was supposed to be a bridge between Apollo and the next generation of spacecraft. To cut costs, the Space Shuttle was supposed to be reusable. Originally, all parts were to be reusable multiple times, but soon it was decided to expend the external fuel tank. After the Challenger accident, it was decided that the solid rocket components were not to be reused to the extent that had originally been planned. Also, to make the Shuttle efficient, there had to be one to two shuttle flights per week. This never materialized. Furthermore, the Challenger accident showed that what many had forgotten: the Space Shuttle, as a first generation reusable spacecraft, is an experimental vehicle. All the bugs have not been worked out. Prior to the Challenger accident, the Space Shuttles had begun to be used to deliver satellites to orbit, to retrieve satellites for repair, and to conduct microgravity experiments in orbit. After the accident, though, President Reagan issued a directive that the Space Shuttles were not to be used for missions that did not require manned spaceflight. In other words, if a mission could be performed without risking human life, then do it that way, ignoring cost. So, post Challenger, the Space Shuttles lifted a small backlog of satellites into orbit that had been designed for delivery by space shuttle, but future satellites were delivered by unmanned rockets. The Space Shuttles continued to do science missions, and they did servicing missions to the Hubble Space Telescope. However, the number of missions dropped to about six per year. Furthermore, after each mission, the orbiter was gone through with a fine tooth comb, so turn-around began to be longer and longer. It became impossible for the Shuttle program to make money or be cost effective under such conditions. In fact, as unmanned spacecraft became cheaper and more reliable, then using a Space Shuttle to launch a satellite came to even cost more than using an unmanned rocket! The Space Shuttle continued to fly missions up to two weeks in length to study the effects of microgravity in various experiments. Thus, the shuttles were being used as temporary space stations rather than as "shuttles."
After the first few test missions, the Space Shuttle fleet was delivering satellites into orbit, one of its original purposes, but that stopped after the Challenger accident. The science missions were part of the original idea, as well, but one of the biggest plans for the Space Shuttles was to carry astronauts, equipment, and components to a space station. The only problem was that we didn't have a space station. Eventually, however, on June 27, 1995, the Space Shuttle Atlantis blasted off on mission STS-71 to dock with Mir on June 29. This was the first visit of a Space Shuttle to a space station, and it wasn't an American space station. Eight other Space Shuttle missions went to Mir. The original plans for an American space station, Space Station Freedom, never materialized. Freedom was to be the United States response to Mir. However, with the cold war ending, and then the fall of the Soviet Union, plans for Freedom were shelved. Instead, the United States decided to cooperate with the Russians on working with Mir, with a module dedicated to the Americans being added to Mir.
However, Mir had reached the end of its life. The United States, Russia, and several other nations agreed to fund an international venture. This became the International Space Station. Unfortunately, the economy of Russia was collapsing, so funding for the ISS largely fell to the Americans. The first component of the ISS was launced by Russia in November 1998, followed shortly thereafter by the delivery of the first American component by the Space Shuttle Endeavour in December 1998. Ten other space shuttle missions followed, each delivering components, supplies, and crew rotations. Unfortunately, the loss of the Columbia has had a major impact on the completion of the ISS. Without a crew escape vehicle other than a Soyuz, the crew of the ISS is limited to 3, and it takes 2 to run the space station, leaving only one to do science experiments. However, the Progress modules are not sufficent to provide supplies for a crew of three, so the crew has been limited for the last couple years to two. The ISS has been largely in a holding pattern, waiting for the return of the Space Shuttle to active duty. This has been a great disappointment. Many in the space community think of the ISS as a budget black hole for NASA. Keeping it flying is costing other programs, and keeping it flying has produced nowhere near the rewards that we had hoped due to the lack of shuttle support.
We don't have a moon base. We have not had a manned mission to Mars. We barely have a space station, and it doesn't really do much at the moment. We have a lot of satellites, of course. But, manned spaceflight seems to have gotten nowhere as far along as we had hoped when I was young. This is sad.
-Astroprof
April 11 Venus Express ArrivingThe European Space Agency (ESA) is really moving along. On the heals of Mars Express, they now have Venus Express, which is just now arriving at Venus. Mars Express had the ill-fated Beagle 2 along for the ride. However, the orbiter has performed like a champ. We can hope that the same will be true of Venus Express. In case you've noticed the similarity of names, it isn't a coincidence. Both were called "Express" due to the short time taken to plan and build the spacecraft. Both spacecraft share similar designs, too.
Launching only about five months ago, Venus Express didn't waste any time getting to Venus. As with Mars Express, ESA used a Soyuz/Fregat rocket to boost Venus Express to its other worldly rendezvous.
Venus Express will mainly study Venus' astmosphere. Though Venus is very much like the Earth in size and mass, and it is only a little closer to the Sun, getting consequently only somewhat more solar energy, the planet is enveloped by a noxious atmosphere consisting of mostly carbon dioxide. The pressure at the surface is close to 90 times the pressure at Earth's surface, and the temperature is almost 900 degrees Fahrenheit (460 degrees Celsius, for my readers from the rest of the world!). This is even hotter than the surface of Mercury, which is almost half of Venus' distance to the Sun. The planet is surrounded by dense clouds composed of concentrated sulfuric acid. The surface of the planet does not show evidence of the wide scale plate tectonics that Earth has. So, what happened to make a planet so similar to Earth so different? This is part of what Venus Express hopes to help us answer. In the process, we might find that we learn a whole lot about how Earth itself works.
The clouds block our view of the surface of Venus, so previous spacecraft have had to use radar to map the surface of the planet. Venus Express will use infrared to yield some information about the surface of the planet and the lower layers of the atmosphere. Venus' atmosphere permits some wavelengths of infrared light to pass. Venus Express will be the first spacecraft to exploit these atmospheric windows to study the planet. However, some of the most important measurements will be of Venus' atmosphere. Hopefully, Venus Express will help answer questions about how the weather cycles and circulation work on Venus, and why it seems that there is so little difference in day and night temperatures, and how chemistry plays a role in climate of Venus. Though atmospheric studies are such a major component of the mission, Venus Express will also try to nail down whether or not there are active volcanoes on Venus (we are pretty certain that there are, but we have not definite proof). Also, there has been some speculation that Venus periodically undergoes massive and catastropic volcanic activity, completely resurfacing the planet in a geologically short period of time. There is some speculation that this may have happened about 500 million years ago. Venus Express hopes to answer the question of whether or not this may have in fact happened.
Venus Express will orbit for about 1.3 years, with an option to extend the mission to over 2.5 years. We'll know in a few days if the orbital insertion was successful. Already Venus Express has been sending useful data, so there is a promise of far more to come.
-Astroprof
April 10 Breathing VacuumSeveral movies have scenes where the key figures are exposed to a vacuum for some period of time with apparently no ill effects. 2001, A Space Odyssey has our hero doing several seconds of unprotected space walking. The Hitchhiker’s Guide to the Galaxy has our heroes tossed into space without spacesuits, only to be rescued seconds later. And, the lead character in Sudden Recall is suddenly exposed to the Martian atmosphere, which is nearly a vacuum. All survived. How realistic is this? How would we know how the human body really reacts in space?
Well, it turns out that we do have a pretty good idea what happens to a human body in a vacuum. We can get a pretty good estimate of what would occur from looking at divers who suddenly depressurize from depth to one atmosphere. All sorts of bad things can happen. But, we have an even better model. Animals, and humans, actually have been exposed to vacuum conditions, so we have first hand data.
In the earliest days of spaceflight, the space agencies considered the possibility of a breach in the integrity of a spacecraft to be a very real possibility. It still is, but is now thought to be much less likely than it was then. Naturally, there was concern about what would happen to the astronaut. Everyone knew that you’d die without air, but the question was whether or not a human could live long enough to put on a spacesuit’s helmet, or to close the visor if the helmet were already in place. If a spacesuit were punctured on a spacewalk, how long would an astronaut’s companion have to get him to the safety of a pressurized spacecraft? These were questions that animals helped to answer. Personally, while I agree that the answers to the question are important, I don’t think that I could ever purposefully do that to an animal. Nor, would I want to be anywhere around before, during, or after the experiment.
In addition to animal tests, there have been human tests for exposure to very low pressures, such as those experienced by the sudden decompression in a high altitude aircraft. Extrapolation of these test results lets us figure what may happen with no pressure rather than low pressure. And, there have been accidents. Humans have accidentally been exposed to vacuum, or to pressures so low as to be effectively vacuum as far as human physical responses go.
An actual human exposure accident occurred during the early tests for Apollo at the Johnson Space Center in Houston. JSC has several vacuum chambers, with at least two large enough for humans to work and move about in while in a vacuum. These chambers not only operate at a vacuum, but they also have lights, heat lamps, and chilling coils to simulate both thermal and radiation conditions experienced in space. In one space simulation in 1966, a technician at the Manned Spacecraft Center in Houston (later it was renamed the Johnson Space Center) was testing a spacesuit in such a vacuum chamber. The suit tore and rapidly depressurized. An emergency repressurization procedure was initiated and the subject was rescued by medical personnel standing by for just such an emergency. The technician was exposed to vacuum and low pressure conditions for under a minute, and though he has severe problems at the time and shortly after, he eventually fully recovered. Other accidents also occurred, not all of which resulted in survival of the victim. Still other incidents involved ruptures in pressure suits resulting in partial body decompression. And, in 1971, Soyuz 11 had a failure resulting in sudden decompression during reentry. The cosmonauts onboard did not survive. Animal studies coupled with medical accounts (for the accident survivors) or autopsy reports (for those that did not survive) give us a pretty good idea of how the human body responds to vacuum exposure. These incidents, though, were accidental, and were not carefully controlled experiments, so the data is a bit incomplete in places. Needless to say, there are few volunteers for controlled experiments detailing vacuum exposure!
So what does happen? There has been all sorts of speculation by laymen and science fiction writers. Many suggest that the victim will simply explode (after all it is called explosive decompression!). Well, obviously this can’t be right, since some people survive! There is also speculation that the victim’s blood would boil. This, too, did not happen with the technician in Houston, nor with many of the animals. Why would this speculation even occur, though? Doesn’t water boil at 100C? Yes, and no. As pressure drops, the boiling point of water drops. At sufficiently low pressure, the boiling point drops all the way to freezing, and water exists only as a solid or a gas. The atmospheric pressure on Mars is this low! However, remember that you are a fairly sealed system. So, unless something bad happens (which I’ll mention later), even if the pressure outside your body drops, then the pressure inside your body should remain high enough (at least on the arterial side of the circulatory system) to just avoid your blood boiling.
But what does happen? Well, it isn’t really pretty, but here is a synopsis of what I gather is likely to occur, based on studies human and animal vacuum exposure. First, it depends upon how quickly the lungs empty. If the victim is smart enough to quickly exhale, then massive internal injuries can be prevented. On the other hand, if the victim tries to hold his breath, or has some sort of airway obstruction, then the lung tissues can rupture, spilling air into the body cavities. This causes massive system failure, and the victim, if holding his breath, can no longer hold his breath. The rapid reduction in pressure in the lungs now results in reduction of pressure within the body, and bodily fluids do begin to boil. Such an event is always fatal, even if pressure is rapidly returned to normal.
If the victim exhales, though, then several things happen. First to occur is that there is no air for the blood to exchange oxygen and carbon dioxide with. In fact, worse than no air, the blood flow through the lungs can even lose oxygen to space! This can occur only for about 10 to 15 seconds with a human before loss of consciousness. Hypoxia and impaired judgment begin to occur within about 7 or 8 seconds, though. So, anything the victim must do to save himself must be instinctive, and drilled and trained to the point of being nearly automatic, without much thought. Given the surprise factor likely in a sudden accident, there may be only five seconds or so to react. If exposed to sudden explosive decompression, the victim must remember to exhale at once. This must be automatic and drilled into the subject. There are only a couple of seconds before serious, and often irreversible, damage to the lungs occurs. The 1966 accident victim at the Manned Spaceflight Center remembered to exhale. He did report the rather strange feeling that occurred as water in the saliva on his tongue began to boil. A more serious problem is that water on the surface of the eye also begins to boil, drying the eye, resulting in severe pain almost immediately. Hypoxia results in loss of vision after 10 seconds or so. This loss of vision often remains for a while after the victim is returned to atmospheric pressure.
The external pressure on the body is suddenly released, and this causes pressure in the soft tissues to fall, resulting in some water vapor forming in those tissues. This water vapor then presses on the veins, increasing pressure. The water vapor also causes the tissues to distend, swelling to nearly double their normal size. The body appears bloated. Some capillaries can rupture, causing bruising. In an incident on a high altitude balloon flight, a glove lost pressure. The pilot’s hand became bloated and he experienced great pain. After several seconds, the hand became useless. In another incident, a potentially fatal accident occurred during a spacewalk on STS-37. During this mission, the astronaut punched a tiny hole in the hand of his spacesuit. However, the pressure in is spacesuit pressed his hand against the hole. The vacuum at this hole caused tiny ruptures below the skin, and his blood actually clotted to seal the edges of the hole to his flesh. Upon returning to the shuttle, he had a small, very red, and very painful lesion on his hand. He was quite fortunate.
As a response to loss of oxygen in the blood, the heart begins to beat very rapidly, as if the victim were doing heavy exercise. However, there is no oxygen to get. Eventually, the heart beat slows, and with the slowing heart, the blood pressure drops. When the blood pressure on the arterial side of the circulatory system drops to equal that on the venous side, then blood no longer will flow. After about 45 seconds or so, effective circulation stops, even though the heart continues to pump. The body goes into convulsions shortly after cessation of consciousness, then paralysis sets in. Starved for oxygen the heart itself stops after 60 to 90 seconds, though some reports report fibrillation beginning prior to the time that it stops beating, sometimes even during the first minute of exposure. A second set of convulsions hits at the end, then the heart stops. To my knowledge, no subject has ever survived this point, even if oxygen is immediately restored. In some animal studies, sometimes, distension of the stomach can press on the diaphragm, compressing the thoracic cavity, causing heart fibrillation or cardiac arrest prematurely. None survived this event, either.
So, if you are ever in a spacecraft or a spacesuit, and you suddenly experience explosive decompression, then you need to remember at once to exhale, then you need to position yourself for assistance. You’ve only got seconds before you are helpless. Then, you just have to hope and pray that someone gets you back into pressure within a minute or so. Subjects who manage to avoid some of the more unpleasant events above seem to achieve a complete recovery if they get oxygen again within 45 to 60 seconds.
So, that is what happens to a human body in a vacuum.
-Astroprof
April 05 Space Shuttle ChallengerSo, what's so special about April 4, 1983? This was the first flight of the Space Shuttle Challenger.
OK, so this blog entry is a day late. I know. Things have been pretty crazy around here, so I've not been keeping up. Next week should be smoother, I hope. Still, I wanted to go ahead and do this entry about the Challenger.
The Challenger, designation OV-099, was the second space shuttle to fly into space. The shuttle frame used was actually older than the one used for Columbia, the fist shuttle to fly in space. OV-099 was oritinally designed to be a test frame, with plans to outfit the Enterprise, the shuttle used in test atmospheric flights, for space. However, NASA determined that modifications needed to make Enterprise spaceworthy would cost more than what it would take to make Challenger spaceworthy.
Challenger's first mission, STS-6, which began April 4, 1983, was itself the sixth space shuttle mission flown. The launch had been delayed by about two and a half months due to a hydrogen leak discovered prior to the original launch date of January 20 of that year. For this first fligh of Challenger, a crew of only four astronauts flew about the shuttle. Highlights of the mission included deployment of the first Tracking and Data Relay Satellite (TDRS) as well as the first spacewalk of the Shuttle program. This first spacewalk, performed by Donald Peterson and Story Musgrave, lasted a bit over 4 hours. This mission was also the first to fly with the lighter external fuel tank haivng only the foam coating, without the outer coating of protective white paint.
Just two months later, Challenger again blasted into space on mission STS-7, this time with Sally Ride aboard --- NASA's first woman astronaut in space. Two communication satellites were deployed on this mission.
Only about a month after landing from STS-7, Challenger again blasted into space on STS-8 to deploy another satellite. Challenger was the shuttle of another first in space with this mission, as Guion Bluford, Jr., became the first African American in space. Here, we see with the rapid turnaround for Challenger between the STS-7 and STS-8 missions NASA's goal of quick turnarounds that were supposed to make spaceflight routine and inexpensive. STS-8 also marked both the first night launch and the first night landing of the Space Shuttle program.
Challenger's fourth flight was STS-41B, which began February 3, 1984. Two more satellites were deployed, as well as a space pallet flown on STS-7 that was refurbished and flown back into space --- another NASA first. STS-41B also marked the first untethered spacewalk and a test of the foot restraints on the remote manipulator arm that would be used for another NASA first planned for the next shuttle flight --- the retrieval and repair of a satellite in orbit.
That flight, STS-41C, also marked Challenger's fifth flight. Challenger deployed the Long Duration Exposure Facility (LDEF), which was to remain in orbit conducting experiments while the shuttle returned to Earth. The LDEF was to be retrieved on a later mission. This did, in fact occur, however the deployment was far longer than originally planned due to stoppage of shuttle flights after the Challenger explosion on STS-51L. In addition to deployment of LDEF, Challenger rendesvoused with the Solar Max satellite and conducted repairs.
Challenger flew into space a sixth time October 5, 1984, on mission STS-41G. Another satellite was deployed on this mission. STS-41G marked the first time seven astronauts flew aboard a shuttle, as well as marking the first mission with two women aboard, as well as the first spacewalk by a woman of any nationality, Kathryn Sullivan.
On April 29, 1985, Challenger again flew into space carrying a spacelab module in the payload bay. This mission, STS-51B, carrying Spacelab 3, was primarily a science mission, though another satellite was deployed.
Spacelab 2 was carried into space on July 29, 1985, on Challenger's eighth mission, STS-51F. Three communication satellites were also deployed. This mission got off to a rocky start, though, as one of the Shuttle's main engines prematurely shut down. The boost phase of the flight, though, was far enough along that a return to Earth would have not been safe or practical, so an order was given to abort to orbit. This abort scenario puts the Shuttle safely into orbit until a decision can be made as to the fate of the mission, but the orbit is not the one orginally planned for the spacecraft. In this case, controllers decided to continue the mission in this lower orbit, and STS-51F was declared a success.
Challenger's ninth trip into space began October 30, 1985, with the launch of STS-61A, another science mission. In this mission, the first with eight astronauts aboard, the shuttle carried the German Spacelab D-1. This was also the first mission financed primarily by another nationality. A couple of small satellites were deployed, as well.
January 28, 1986, Challenger sat on Pad B of Launch Complex 39 awaiting liftoff for its tenth flight into space. This mission, STS-51L, was the first to use Pad B at the Kennedy Space Center since the days of Apollo. Launch Complex 39 consists of the Vehicle Assembly Building, where the Saturn V rockets were assembled, and which was converted to assemble the Shuttle components for flight, the launch control firing rooms, and two launch pads, Pad A and Pad B, each located several miles from the Vehicle Assembly Building. All previous Space Shuttle Launches had been from the more directly accessible Pad A. However, January 1986 had two flights scheduled only days apart. Pad A was used to launch Columbia on STS-61C just two weeks prior to Challenger's STS-51L mission. So, that meant that Pad A was occupied during the time that Challenger was being rolled out to the launch pad for final launch preparations. Launching from Pad B is not a problem, though, as both launch pads have identical systems. It simply means that the Transporter Crawler has to make an additional turn and carry the orbiter and its mobile launch platform a bit farther. However, it was cold on the morning of the launch. That was a problem. Later investigations showed that the cold caused O-rings on the solid rocket boosters to harden. These O-rings were designed to seal in the hot gasses formed by the burning fuel in the Shuttle's solid rocket boosters. Being hardened, though, meant that the O-rings did not seal properly. The hot gasses escaped, and like a blowtorch cut into the soft and unprotected main fuel tank below the Shuttle's belly. This tank, filled with two parts hydrogen and one part oxygen, ignited in a giant fireball. The orbiter was suddenly thrown sideways, creating enormous atmospheric stresses on the frame of the spacecraft. The fuel tank explosion did not destroy the orbiter. However, the atmospheric stresses did, and the orbiter disintegrated. A tribute to how solid and securely the crew compartment was constructed is that the crew compartment remained largely intact after the disintegration of the orbiter. In fact, the crew compartment remained largely intact all the way until it struck the surface of the Atlantic Ocean several minutes later, at which time all seven astronauts aboard were killed.
The explosion destroying the Challenger put a halt to space shuttle flights until STS-26 on September 29, 1988. During this time, an investigation into the Challenger accident highlighted bad decisions, bad decision chains, bypassed safety protocals, poor communication, and a bureaucratic mentallity that emphasised schedules over safety, all of which doomed the Shuttle. Interestingly enough, after the Apollo 1 accident killing three astronauts on the launch pad, the investigation came to about the same conclusions, as did the one following the Columbia accident.
You may have noticed that the numbering scheme for Space Shuttle missions changed during all of this. The STS stands for Space Transportation System, the official name for the Space Shuttle program. The first missions were simply numbered in order of the mission. Then, in 1984, a new numbering system came into being. Here, the first digit of the number was the federal fiscal year of the mission, with the second number designating the launch side (1 = Kennedy Space Center, 2 = Vandenberg Air Force Base). Vandenberg was never used, though orginal plans called for an eventual shift of military missions to Vandenberg. The letter following the numbers indicated the sheduled mission during the year (A = first mission, B = second mission, C = third mission, etc). When Space Shuttle missions returned to flight after the Challenger explosion, then NASA returned to a sequential numbering scheme. However, now the numbers were the scheduled mission, not necessarily the flight order. So, if a mission were delayed or rescheduled, then the flight order might not match the number.
So, yesterday got me to thinking about the shuttle Challenger, and I decided to blog about it. I just didn't have time until today. So, you got a NASA history lesson today. I hope that it didn't bore you too much!
-Astroprof
PS: I'll be at the Johnson Space Center for the next few days, so I don't know if I'll get a chance to add to my blog. I'll try if I get the time, but I'll be working pretty hard the whole time.
April 03 Busy, busy, busyJust in case my loyal readers were wondering what is up with me. I have been sort of snowed under. I am giving three exams this week that I am writing (I think that I spend more time on them than do my students). Also, I spent the weekend catching up on grading from the time that I missed going to the conference. Then, later this week, I am going to the Johnson Space Center, and, of course, students are coming to me with last minute panic over their projects. Oh, and since I am taking students with me to the space center, there is a MOUNTAIN of paperwork to fill out. Egad. I sort of wonder if they don't come up with all of the paperwork to discourage faculty from doing anything with students outside of the classroom. So, when I get a chance, I'll make an entry or two. Until then, I am just trying to keep my head above water.
gurgle, gurgle, gurgle April 02 DSTWell, another spring rite for the US has come: resetting the
clock. This spring change really gets me, as it means losing an
hour of sleep each morning. I can't really get to bed much
earlier (an astronomy thing), but I have to get up earlier because
things are tied to the clock. Now, I do see where it is useful to
get up earlier in the summer. After all, the sun has already been
rising quite a bit before I do. In the summer, it is so hot
around here that the only time of the day that is really nice to be
outside doing yard work is early in the morning. Still, suddenly
getting up an hour each day takes some getting used to. Why can't
we just phase this in? After all, set the clock ahead 15 minutes,
then another 15 minutes, and so forth. |
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