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Rambling through space ...
August 06

Astroprof's Page is Moving!!!!!

Hello, everyone!  Astroprof has blasted off into space.

Astroprof's Page has Moved!
Please reset your bookmarks and pointers.

My new little corner of the internet is
http://astroprofspage.com

I hope to see you there!
-Astroprof
August 05

Astroprof's Page is about to move.

Well, I finally did it.  I got my own domain name.  I've staked out my little piece of the internet.  Now, I just have to build something there.  I will be moving astroprof's page there.  I'll try to bring the postings already here over to the new site.  Now, this will likely take a while for me to get things over there like I want them.  So, I may not be doing much posting this next week or so.

When things are fully running, I'll post a note here with a link here telling you where to find me.  I am looking forward to this.  It ought to be fun.  If anyone has any suggestions about what might be good to have for the new location, let me know.  I don't know if I'll be able to work out everything (or even if I want to!), but I'll gladly consider any suggestions.

-Astroprof
August 04

Ares Rockets: More Blogging

Not too long ago, I posted an entry about the new Ares Rockets that NASA is designing. I mentioned that portions of the new rockets are based on Shuttle technology, in particular the exteranal tank. Well, that includes the problamatic foam. There was an article in the local paper here today about just that. As with most of the news in the local paper, local reporters didn't come up with it. This was an AP story. The reporter pointed out that this is the same foam that keeps flaking off, and that a piece of foam falling off on liftoff was what did the damage to the Columbia that ultimately proved fatal to that craft. However, the report also goes on to say that this should not be a problem. Well, I thought that I might expand on that.

Foam has been flaking off of the Shuttle external tank since the early days of the Space Shuttle in the 1980's. At first, engineers correcty were concerned. However, as time passed without a major incident relating to the foam problems, their concerns were put on the back burner. Then, in the 1990's, the manufacturing process for the external tanks changed to use a new, more environmentally friendly way of applying foam to the tanks. I am all for saving the environment. But, folks, we need to be reasonable. The problem with the new method was that the foam was even more likely to flake off than before. Concerns about this went unheeded. Even when a particularly large chunk of foam fell off and seriously damaged a support brace holding the solid rocket boosters to the external tank on the STS-112 mission, higher ups didn't take the matter seriously. Not, until the loss of the Columbia on mission STS-107, that is.

So, can foam flaking be dangerous with this new design? Well, yes. But, not nearly as dangerous as with the Shuttle program. First of all, the biggest concern that NASA has with foam flaking is that the foam flaking off might damage the orbiter's heat shield. The heat shield is composed of rather delicate porous ceramic tiles that are easy to damage. Hitting them hard enough can break or scour them. Even more fragile are the tiles on certain parts of the orbiter, like on the leading surfaces of the wings, where the heat load is greatest. These tiles are much more brittle, and they are easier to damage. A foam strike on the leading edge of the Columbia's port wing is what is believed to have doomed the craft.

However, the new CEV won't have that problem. This new craft rides atop the rockets. So, any foam shedding will not be able to strike the crew vehicle. Furthermore, it is expected that foam shedding should not strike anything important. The Ares I, which will be used to lift the astronauts into space in their CEV will not even have fins to damage. This rocket is steered with gimballed rocket motor nozzles. There is a faring around the base of the rocket, but foam should actually have moved away from the rocket body enough by the time that it reaches the faring that impact is unlikely, and if impact did occur, serious damage is also unlikely. In theory, that is. A worse case scenario would be if foam near the top of the rocket peeled off, and that exposed more foam to aerodynamic stresses that cause it to peel off, and so forth. One could imagine foam breaking away from an entire side of the rocket. This could, in theory, lead to handling problems. I don't think that any problems of this sort would bring down the rocket, but then it would be unwise not to consider every possibility, however remote. And, this is, indeed, an exceedingly remote possibility. Such a cascading foam peeling has never happened, and I don't think that it can even happen without a whole lot of things going wrong with rocket manufacture, foam composition, foam application, rocket handling after fabrication, etc. It would take a remarkable series of failures to even lead to such a foam cascade, which would unlikely have a disastrous result even if it did occur.

However, the Ares V is another story. This is the heavy lift vehicle. It will be the rocket to lift the major heavy components of Lunar and Martian missions into space. It will be used for future major launches of space station components. And, it is more susceptable to damage. This is because it is composed of a central core with two solid rockets strapped to the side. Despite the fact that Atlantis safely completed the STS-112 mission, there was serious damage caused by foam shedding to a strut holding one of the solid rockets onto the external tank. The strut held. However, in only just held. Had the damage happened earlier in the flight, had the damage been slightly more severe, had the damage happened closer to the end of the strut, then the solid rocket might have torn away from the external tank. Well, actually, only part of the solid rocket would have torn away. The other part would have torn off part of the external tank, resulting in a repeat of the sort of even that destroyed the Challenger. This is still a danger. And this danger would still exist with the Ares V rocket. It is a remote possibility, but then so is the possibility of damage such as that which downed Columbia. Again, ignoring it is dumb. However, even a loss of an Ares V, while bad, and disastrous for the completion of a mission, would not result in loss of life (unless, of course, the debris fell on someone). The astronauts will be riding into space aboard an Ares I, which is unlikely to suffer horrible damage from any foam shedding.

So, there you have more on the Ares rockets.

Oh, and I am still looking to move my blog. I'll post a forwarding address when that happens. Interestingly, this new thing that they've put into effect here actually seems to work better with Firefox than it does with Internet Explorer. Imagine that. A Microsoft product that doesn't work well with other Microsoft things. Still, not all features work, and I don't like it. So, I am looking to move.

-Astroprof
August 03

2006 Hurricane Season - Part II

OK.  I am still planning on moving my blog.  This new format is driving me nuts.  Why couldn't they just leave things alone?
 
Hmm.  Here is an interesting development.  If you recall, I predicted just about the same thing back some months ago.  Now, the experts are saying that they are reducing their estimate of how many tropical cyclones are expected to form in the Atlantic basin.  I rather thought that the estimates made last winter were too high. 
 
Now, I don't want to seem like I am boasting, or anything.  Just, the media really got carried away.  For some reason, people think that just because the weather or climate acts one way one year, it will do the same thing the next year, or next decade, or even next century.  It is really a lot more complex than that.  Last year was probably an anomaly, not something that should be expected to be repeated.  People also forget that just because some weather has not happened in the last 20 years doesn't mean that it won't happen again.
 
I'm keeping this post short, because typing this in under the new format is driving me nuts.
 
(Also, I am trying to write this during lab, and students are coming and asking questions every few minutes.  What do we put in this blank?  I ask them what the lab manual says to measure and record.  They say X.  So, I tell them to write X in that blank.   Between silly questions and this new format that MSN Spaces has dumped on me, I am getting really frustrated!  And, it is getting me even more determined to move my space.)
 
-Astroprof
August 02

Am I going to pass this class?

We are getting near the end of the summer.  There are just under three weeks left of summer school.  I've been teaching a summer-long class (not those silly 5 week long classes that so many places do for summer school).  Anyway, now the questions are coming.  A couple of students who had been scoring in the 30's on exams, and not much better on labs and homework have figured out that they are not passing and have dropped.  Some have been in the 80's on exams, and 90's on homework and labs, and they realize that they have a shot at an A if they work hard.  Others are looking at a C, and they feel that they'll be happy with that.  At least one is thinking that a D will be the best that he can hope for, and so he is going to try to get his rear in gear to at least pass the class.  These are students who are figuring it out on their own. 

Then, one comes to me and asks, "Is there any hope of my passing this class?" 

"Well," I say, "There's always hope.  But you need to really concnetrate on the class.  You won't pass if you keep going the way that you are going.  You need to actually show up, do the work, and turn things in to be graded.  You need to spend the time on the class, and you need to decide if passing the class is a priority or not.  What means more, passing the class or the rest of your life?  You clearly are smart enough, and you clearly have the math background, the problem solving skills, and so forth to do well in the class.  However, you are not putting the effort into it that is needed." 

So, he went away to think about that.

He really can pass.  He does show in class (when he bothers to be there) that he can grasp what we are doing.  When I set up a problem on the blackboard, and then pose a question to the class on what step we should do next, he frequently comes up with a correct approach, especially if the best next step is a derivative, integral, or some other procedure using calculus.  He can do this.  The problem is that he is trying to do too much.  He is trying to work full time this summer and take a difficult class.  He works some distance away, and he has to commute.   That is why he misses class and almost always drags in late, he says.  Working all day and taking an evening class leaves no time to study or do homework, which is why he says that he is doing poorly and not turning things in.  Well, not doing the homework is why he is doing poorly, for sure.  If they will just do the homework problems, then they'll be ready for the exams.  That's how this class works.  I fully sympathize with the whole thing of life interfering with studies.  I've had that problem, too.  You need to work to pay the bills, including tuition.  But, you need time to do the classwork.  In the summer, the students also try to run around with friends who are not taking classes in the summer, and that takes time away from studies.  Taking a physics class, or any other time intensive class in the summer is hard, even with my summer long class.  It is still accelerated from the regular semester.  But, what is the solution?

I honestly don't know.  The system isn't set up to further the aims of non-traditional students.  I went to college after high school.  My parents paid for the university's tuition, with the help of a scholarship and student loans.  I had to pay off the student loans myself.  I did get a small job on campus for a while, but it was working with one of the professors in one of the research labs, so it was directly related to the field.  The same with summer jobs.  I didn't do summer school.  Graduate school, though, I had a teaching assistantship, like most of the other graduate students.  That took more time, but it was still part time, and it was directly related to what I was doing.  Also, there were more student loans. 

Students today, though, try to juggle full time jobs and college.  When I was a student, full time college was full time.  I spent most of my time outside of class studying, doing homework problems, lab write-ups, papers, etc.  I spent untold hours in the library, reading, researching, studying.  Yeah, there was some play time, but it was mostly study.  I didn't have time for a job then!  Yet, almost all of my students work.  Some work part time, but many try to work full time.  They have to.  Tuition is astronomical.  Textbook prices are beyond astronomical.  Most of my students pay far more for textbooks than they do tuition.  I occasionally teach a class over at the big private university across town, and a single semester there costs as much as my entire 4 year degree did.  Parents simply can not afford to foot the bills.  Scholarships and grants don't provide near enough support.  Nearly 75% of the students are on some sort of financial aid.  Most of that is student loans.  Some students are graduating college now with student loan debt that approximates a mortgage.  To keep that down, they work while going to school.  But, they still have to go full time, otherwise they don't qualify for any student loans at all, and worse, they have to start paying back the ones that they already have if they are not full time students.  Many also try to remain full time students so that they can get affordable health insurance.  But, working gives them little time to be students.

Then, even worse, they are programmed by the public schools to think that they don't need to work outside of class.  Most of the schools here give very little homework, and they use class time to work on the homework (isn't that classwork rather than homework?).  So, students get used to the idea that they can learn all that they need in class.  They don't realize that they need to spend hours outside of class each day.  They don't realize that college in-class  time is just setting the stage for them to learn!  So, they try to work and go to school.  Worse, many of my students went and did something else for a few years between high school and college.  Among those other things, all too often, were getting married and having kids.  So, now they try to add family time to a full time college schedule and full time work.  Something has to give.  But what?

Do we assign less work to accomodate these new type of students?  But, wouldn't that mean less learning?  Yeah, I know that some faculty are doing just that.  They are cutting material out of the classes to make them easier.  But doesn't that devalue the class, and ultimately the college degree?  Surely that isn't the answer.  What if students took fewer classes so that they could manage the time?  Well, they can't.  If they took fewer classes, then they don't qualify for financial aid, insurance, and a host of other things.  Here in Texas, there are even penalties for taking longer than four years to get an undergraduate degree, so that is an added incentive to sign up for a full load (and the legislature has been talking of making those penalties far stiffer). 

I just don't know.  I don't really see how my students manage.  It looks like getting through college is just getting tougher and tougher.  I sort of wonder how I'd do it if I were a student today.

-Astroprof

Huh?

..
What the @$&# ?  Does my blog look as different to everyone else as it does to me?  Last night, I logged on to work on an entry while my students were doing a lab exercise, and the entire thing was screwed up.  The format was messed up, the usual options were gone, and it was unbelievably SLOW loading up.  In fact, the panes didn't even fit on the screen!  I couldn't do anything!  Then, aferwards, I tried from my office, and it was still different, but at least things fit on the screen and some options worked.  The same at home.  I guess that this is Microsoft's new "improvement" to their Spaces.  Well, as usual, they took something that worked adequately, though not well, and made it worse in the name of improvement.  I figured out that probably the reason that it is totally unusable from the lab was that the computer there is using an older version of Internet Explorer.  My office uses a newer version, and at home I use a new version of Firefox.  So, in typical microsoft fashion, you have to get the latest product to do anything.  The latest product doesn't always work on older computers.  Also, the lab computers are protected so that students can't download and install things on them, and that means that I also can't do anything.  I have to get someone to do that.  Tell me that this is better?  They are apparently raving about how the new features are so much better.  Well, I don't even see much in the way of new features (other than an icon for the blog owner, is that important?) .  In fact, many of the old things that I used no longer work.  Wow.  I'll have to try to figure out if I can adapt this thing.  If not, I may be moving my blog.  I have thought about that now and then, since this never was something that worked quite like I had wanted.  But, it was here, and this is where I started the blog, and it did work for at least posting stuff, so I just kept it since people had gotten used to finding me here. 

Oh, and as if to make things even more confusing, they changed the URL on me once again.  Why can't they leave things alone?  What about all the pointers to this little spot on the internet?  Yeah, yeah, they apparently went and automatically fixed pointers within their system so that other blogs pointing here were corrected.  That is only blogs pointing here from within their own system.  As usual, they forgot that there is an entire world out there that is not doing everything under microsoft.

So, I will see if I can get the new features (if I can find them) working, see if I like them, and if not ...
It wold just be a hassle to move.  Still, it is a hassle to stay and have everything change every now and then.  That is just like moving.  Does anyone out there have suggestions for favorite places to host a blog?  I realize there are several, and the best one for me might not be the most popular.

-Astroprof

August 01

Maria Mitchell

Astronomy is a heavy male dominated field. Interestingly, over 50% of my students are female, but only 10% of my colleagues. The percentage is slightly higher than that in graduate school, but still few women go into the field. Almost all of my students are majoring in something else and are taking astronomy only to fulfil a science credit. Despite being a heavily male dominated field, women astronomers have made significant contributions. One of the first woman astronomers in America was Maria Mitchell.

She was born August 1, 1818, in Nantucket. She was a distant cousin of Benjamin Franklin. She was always interested in astronomy, and her father would take up onto the roof of the house to look at the stars and constellations. Using her father's telescope, she discovered a comet in 1847. This comet immediately became known in the Americas as Miss Mitchell's Comet. She shared a gold medal prize from the king of Denmark for discovering the comet. She shared the prize because it had already been awarded to European astronomer Francesco de Vico, who had discovered the comet on his own two days later. Though he found the comet later, the king heard of de Vico's discovery first, as the news did not have to cross the ocean.

The following year, Maria Mitchell was admitted as the first woman in any discipline to the American Academy of Sciences. Interestingly, the second woman, nearly a half century later, was also an astronomer. She was the first American woman to receive an advanced degree. When Vassar College was formed, she was the first faculty member selected for the college. She taught women science at a time in American history when most felt that science was too hard for women. In fact, her father had to pull numerous strings to get her to be allowed to study astronomy at Harvard, particularly since Harvard did not admit women at the time. Her degree was actually at Hanover college, though she took the classes at Harvard.

She studied variable stars, and was instrumental in bringing an observatory to Vassar. The Maria Mitchell Observatory was built in 1908 and named in her honor. This observatory focusses its studies on variable stars. Michell Crater, located on the Moon, is named in her honor, as was the USS Mitchell, a World War II Liberty ship. The Mitchell house is maintained as a museum by the Maria Mitchell Association, and is open to the public.

-Astroprof

July 31

The Caesar Months

We are moving from July to August. Both months are named for Roman emperors. How did this come about? Well, we need to go back to the Roman calendar before Julius Caesar. In those days, the calendar was alternating months of 29 and 31 days. As I said in an earlier post, a month started as a cycle of the Moon's phases, about 29.5 days. So, why wouldn't the calendar be alternating 29 and 30 day months? Well, simply, the Romans thought that 30 was an unlucky number. But, alternating 29 and 31 day months don't add up to the right number of days to keep track of the seasons, which repeat about every 365.24 days. So, the Romans would take the last month of the year, February (they started in March), and add some days in the middle of it. How many days do you add? Well, they had people who decided that. The problem was that they didn't use any good reason for their decisions. Sometimes they'd put too many days in, and often too few. So, by the time that Julius Caesar became emperor, the whole thing was so screwed up that they had to add nearly a couple hundred days into the middle of February to fix the calendar so that the first month of the year, March, would be in the spring. After this "year of confusion" Julius Caesar imposed new rules for the calendar. Undoubtedly, he got the idea from Egypt. In Egypt, they knew the length of the year to very high precision. So, to keep the calendar right, they'd run a 365 day year, with an extra day between the years every now and then as needed. Generally that was every four years. It wasn't exactly a rule to do that every four years, but it would work that way for almost a century before they needed to skip a year. Probably Caesar didn't know that, so his rules did not allow for that provision, a problem that would require a major revision to the calendar by Pope Gregory XIII, but that is a different story. Anyway, the new calendar that Julius Caesar implemented had alternating 31 and 30 day months, except for February, which had 29 days, with one extra day every four years. After the new calendar went into effect, the fifth month of the year, the fifth month of the year (remember, starting in March), was renamed from Quintilius (meaning fifth) to Iulius (from which we get July). Eventually, Augustus became Caesar. Well, to honor him, the sixth month, Sextilius, was renamed Augustus (in English, simply August). The seventh, eighth, nineth, and tenth month were left September, October, November, and December. However, there was a problem. August had one fewer days than July. So, a day was moved from February to August, leaving February with 28 days, with one extra every four years. But, that left July, August, and September as three months in a row of 31 days. So, a day was moved from September to October, and from November to December. That left a calendar that looks just like what we have today (with the eventual change of starting the month with January instead of March). This was the Julian Calendar.

The only problem was that the new calendar had an average year of length of 365.25 days. The seasons actually repeat about every 365.24 days. So, after long enough, there was a day's error in the calendar. Over the centuries, this error accumulated, to that by the Sixteenth Century, it was over a week off. Due to the rules for computing Easter (the Sunday following the Full Moon following March 21, which was supposed to be the Vernal Equinox), that holiday was being celebrated a month off about 1/4 of the time. The Catholic Church decided that that was a very bad thing. So after decades of study, Pope Gregory XIII issued a papal bull decreeing a new calendar. The new calendar, to replace the old Julian Calendar, is called the Gregorian Calendar. This calendar has months the same as the Julian calendar months. But, the rules for leap year changed. Now, leap year is every four years, except centennial years (the last year of each century), unless those centenial years are evenly divisible by 400. So, the year 1900, the last year of the Nineteenth Century was not a leap year, even though 1896 and 1904 were leap years. It was one of the ones skipped. But, the year 2000, the last year of the Twentieth Century, was a leap year since it was evenly divisible by 400. This new calendar went into effect in 1582. But the problem with Easter would remain unless the calendar were shifted so that the Vernal Equinox came closer to March 21. So, in the year 1582, October was shortened by ten days. October 4 of that year was followed by October 15, not October 5. That shifted the calendar to make March 21 the Vernal Equinox.

But, of course the Pope is Catholic. Sadly, some Protestant countries went to war with Catholic countries over the calendar. As bizarre as it may seem, some people actually believed that the Pope was trying to steal 10 days out of everyone's life so that he'd live forever. Yep. People fought and died over what the date should be. Some countries did not adopt the new calendar for centuries to come.

Anyway, enjoy these Caesar months!

-Astroprof

July 30

Riding a Sunbeam

Towards the end of my second semester physics classes, we show that light can push on things. Yes, you heard that right. Light can push on things. Light shining on an object exerts a force on that object. Of course, Newton's third law also is at work here, so the think shining the light is also pushed by shining light. Now, it isn't much force involved. You aren't going to have to worry about a flashlight leaping out of your hand due to its recoil. But there are a few really powerful lasers that exist which do experience significant recoil.

So, how much does light push on things? Well, normally we derive the pressure, of the force per area in terms of light intensity. And, it is really simple. To find the pressure, just divide the intensity (measured in power per area) by the speed of light. Now, the speed of light is a huge number, so unless you've got a ridiculously large intensity, then you get a really small number when you divide. So, light has very low pressure. Low pressure normally means low force. This is for light being absorbed. If light is reflected, then you get double the pressure, and hence double the force.

Now, another interesting thing is that there are two ways to derive the light pressure. For my calculus based class (physics and engineering majors, mostly) you can derive the light pressure quite easily using Maxwell's Equations. James Clerk Maxwell put four equations together (that other people came up with) and got a set of equations that can then be solved for the wave properties of light. But, Maxwell's equations are calculus equations. And manipulating them to yield light pressure involves calculus. That is perfectly appropriate for that class. However, I also sometimes teach a non-calculus based class (life science majors, architecture majors, and pretty much all the rest that need physics). In this class, we can't really do Maxwell's Equations right. But, interestingly there is an entirely different way to derive light pressure. Special Relativity only requires high school algebra to derive the basic equations. And, from special relativity, you can show that light must carry momentum. A change in momentum is associated with a force, so when light is absorbed or reflected, you get a force.

Both approaches yield the same answers. It sure is nice when things work out that way! For a long time, this light pressure result was an interesting mathematical curiosity. After all, the pressure was always such a small number that it would never really matter, right? But, astrophysics is a realm of extremes. Three cases immediately come to my mind in astrophysics where the light pressure really matters.

The first case is comet tails. Comets, are made of collections of dust and frozen gasses. The gasses sublimate and spew out from the nucleus along with dust grains. Light pressure from the Sun acts on some of these dust particles to push them away from the nucleus of the comet to form a tail. Gas molecules are caught in the solar wind and pushed away to form another tail.

A second place where light pressure shows up in the Solar System is with rotating asteroids. As asteroids rotate, the side towards the Sun heats up, and the side away from the Sun cools off. This means that the side of asteroid where the Sun is setting is warmer than where the Sun is rising. Warmer means a tiny bit greater intensity of infrared light emited. This means that there is a slight push on the asteroid due to this assymetry, and this push can over millions of years alter the course of an asteroid. This effect on asteroids is called the Yarkovsky effect.

A third place in astrophysics to see the effects of light pressure is with very bright objects. For example very high mass stars are very hot and very bright. If they are too bright, the light pressure starts to push away their outer layers. In effect, they tear themselves apart. But, it isn't just stars. The accretion disks of black holes or neutorn stars also get hot and bright. If they are too bright, then they too push material away. Sir Arthur Eddington first showed that there is a maximum brightness that something can be before it tears itself apart due to light pressure. So, we call this maximum brightness the Eddington limit.

But, now that we know about light pressure, can we use it for anything? Let's look at these cases that I 've mentioned. One (the comet) involves sunlight pushing on very tiny things, dust particles. Another (the Eddington limit) involves exceedingly bright objects. The Yarkovsky effect is a tiny effect, but it adds up over sufficiently long time periods. Space scientists proposed several decades ago that perhaps we could use light pressure from the Sun to push spacecraft around the Solar System. Rockets have severe limitations. They push hard for a while, but only for a short while until they use up their propellant. Light pressure would not push hard, but it adds up. You'd have low acceleration, but if you keep it up, then that would still yield high speeds. So, if you had a big enough mirror to catch and reflect sunlight (remember, reflecting gives twice the effect of absorbing), then you could push a spacecraft around. The problem is making a spacecraft light enough. Remember, the dust particles in a comet's tail are tiny. But, if you have a big enough mirror, they you get a pretty decent force. As long as the spacecraft, and mirror, are light enough, then you could use this as a propulsion source. NASA is in fact working on this concept. Or at least they have been. There's no telling with all the budget cuts going on. But, comet tails are always pushed away from the Sun. Light pressure could push a spacecraft away from the Sun, but what if you wanted to come back? No problem! Remember the Yarkovsky effect pushes the asteroids in the direction of their cooler side (the warmer side has more push). If they rotate in a prograde manner (in the direction that they are moving around the Sun), then the back of the asteroid is warmer, so the asteroid speeds up and moves into an orbit farther from the Sun. But, if an asteroid rotates in a retrograde manner (the other way), then the front side is warmer, so the asteroid slows down and falls closer to the Sun. Solar sails on a spacecraft could work this way, too. Set one way, they could speed up the spacecraft and it would spiral outwards from the Sun. Set the other way, then the spacecraft would slow down and spiral inwards closer to the Sun. And best of all, there is no need for propellant. The problem, though, is that you need a huge mirror, and it has to be lightweight. This becomes an engineering problem: to build a mirror of several square miles area, but only a few tons of mass. Right now, we can't do that, but it is theoretically possible.

If someone finally manages to make a working solar sail, then we could ride sunbeams anywhere we wanted in the Solar System, using just light pressure.

-Astroprof

July 29

The Moon at Apogee

The Moon is at apogee today. For those of you not familiar with astrolingo, that means that the Moon is as far as it is going to get from Earth today, and will start moving closer. The Moon's orbit is elliptical. The actual astronomical term is eccentric. It takes the Moon about 27.3 days to orbit Earth. However, the phases of the Moon depend upon the relative orientation of the Moon, Earth, and the Sun. So, while the Moon has gone all the way around the Earth in 27.3 days, the Earth has moved, so the Moon must go two more days to line up with the Sun again. The phases, thus repeat every 29.5 days. In ancient times, people would mark time by how many times the Moon went through a cycle of phases. So, if something happened "many moons ago" that meant many lunar cycles ago. If you were conducting business and were about to leave on a long journey, and you told your business partner that you would be back in 7 moons, then that meant that you expected to return in a bit over 200 days. The term month came from this cycle. A month is a moonth. Some calendars, such as the Jewish calendar or the Islamic calendar still reckon time in lunar cycles. The months start with the first sighting of the Moon after New Moon. The modern Jewish calendar calculates when this should be. The Islamic calendar still requires someone to actually see the Moon.

But, as the Moon orbits Earth, its orbit is slightly eccentric. Sometimes it is closer, and sometimes farther form us. The difference between closest and farthest from Earth is almost 10%, hardly enough to notice unless you were really carefully measuring how big the Moon appears in the sky. In fact, this difference in size would be pretty close to the naked eye limit for measuring, so you'd need some decent equipment to measure the change in size. The "huge" moon that some people sometimes report seeing is merely an optical illusion due to the Moon being low in the sky near the horizon. I might blog more on this later. Today, the Moon reaches a distance of 405,406km from Earth. It was last at apogee on July 1, when it was 404,448km from Earth, and it will next be at apogee o, August 26, when it will be at a distance of 406,269km (all distances measured from the center of the Earth). But, wait, these distances are all different by a little bit! What gives? Does this happen at the Moon's closest approach, too? Let's see. The Moon was last closest to Earth, what astronomers call perigee, on July 13, when it was 364,288km away. Its next perigee will be August 10, when it will be a distance of 359,749km. So, it seems that the perigee distance must do the same thing. But, why?

Well, if the Earth and the Moon were the only things in the universe, then the Moon's orbit would be nice and perfectly repeating. However, there are other factors involved. The Sun tugs on the Moon and the Earth as they orbit, and that can distort the orbit slightly. This effect will be most pronounced when you look at perigee and apogee near Full Moon or New Moon, when the Earth, Moon, and Sun are all lined up (something called syzygy), and then you compare that to what happens then perigee or apogee occur near First Quarter or Last Quarter Moon, when the line between the Sun and the Earth is perpendicular to the line between the Moon and the Earth. Since the Moon's orbital period (called the sidereal month) is not the same as the lenght of the cycle of phases (called the synodic month), then apogee and perigee slowly shift through the phases. This causes the apogee and perigee distances to slowly change. However, perigee is always the closest that the orbit comes to Earth in that particular orbital cycle, and apogee is always the farthest that the Moon gets from Earth in that particular orbital cycle. Besides solar effects, the Moon's orbit is also affected by the gravitational interactions of the other planets, irregularities caused by massive impacts, and a host of other things. But, the solar effects are by far the biggest effects.

The Moon is just a few days after New Moon, so it will be a crescent Moon in the western sky just after sunset, setting a few hours after sunset. It will be perigee just the day after Full Moon. The tides are highest at Full Moon and New Moon, because tides come from both the Sun and the Moon and they are working together then. The Moon will be particularly close to Earth this next Full Moon, increasing its effects. So, that means that there will be rather higher high tides and lower low tides than normal during the week of the Full Moon in August. Those planning a trip to the beach might want to observe the bigger than normal range of tides then.

Happy Moon watching!

-Astroprof