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MESSAGE #189. Thu Feb 3 19:51:40 2000 . Eric Webster wrote:
Katrina if you are out there, email me webster@wam... re phil170: I really would like your take on the class, and whether you think the winterterm was a goo time to take it, etc.
MESSAGE #188. Wed Dec 22 21:54:30. Eric Webster wrote:
So what kind of Moon do the Shuttle crew fixing the Hubble see tonight? What kind of Earth? Don't forget, they're orbiting us once every ninety minutes!
A final word of THANKS to..
Katrina and Monique, lecture and homework buds. You guys made the pre-lecture time well-spent, productive, and entertaining. I'd love to share another class with you, but Philosophy? Chemistry? Uh-uh...
Dr. H -- Thanks for making some really challenging information accessible! Hey, now that I'm not in your lectures anymore, you can wear that pyjama-esque paisely shirt again!
If anyone is interested in joining me in commending Dr. H. to the dept & college, email me at _webster@wam.edu_ (just leave the underlines off the email address--prevents junk mail from arriving).
See you all around!
MESSAGE #187. Thu Dec 16 13:45:11. Prof. Doug Hamilton wrote:
MESSAGE #186. Thu Dec 16 13:44:37. Prof. Doug Hamilton wrote:
This is it! My last chance to teach before the Millenium tolls! Most of you probably remember me jabbering about lunar and solar eclipses; well we will actually have a lunar eclipse in about a month! This is definitely an event that is worth watching from wherever you will be over the holidays.
For those of you that will be here, the Astronomy Department will be hosting an event for the lunar eclipse on Thursday, January 20th. We will be running our normal Open House event at the Observatory according to the usual schedule. From 10:00 pm to 1:30 am, portable telescopes will be set up in Hornbake Plaza. Totality for the eclipse is 11:04pm to 12:23am, Eastern Standard Time.
MESSAGE #185. Wed Dec 15 14:52:01. Saadia-Yael Eisenberg wrote:
MESSAGE #184. Tue Dec 14 23:41:25. Eric Webster wrote:
the definition of a second: the duration of time it takes a cesium atom to resonate 9,192,631,770 times.
MESSAGE #183. Tue Dec 14 23:38:03. Eric Webster wrote:
Superfluous: the comments Eric makes on the message board -- like this one!
>> Wasn't the article from the URL you posted written about a new >> clock adapting to the Earth's rotation? I mean there's nothing much >> >> astronomers can do about Earth's rotation other than adapt to it...
Well, I really ought to have mentioned that I WAS KIDDING about astronomers 'sitting idly by'. We KNOW that astronomers are working hard to solve the imminent slowdown of the planet's rotation. [sic]
Actually the super-accurate clock (there was a guest lecture on time courtesy of Physics Dept today, but I missed it) needs to be ADJUSTED since the days are getting longer and longer. I think Earth slows by a second every 600,000 years or so. You need a timepiece a significantly more accurate than a Swatch to make that kind of observation.
>> Personally, I wouldn't welcome extra time in a day because it would just >> give professors an excuse to assign more homework. For every minute added to a >> day, I can picture professors adding an extra hour or so of work.
Aren't we here to learn? We should endeavor to understand all that the profs are trying to impart to us. I'm not satisfied with the dark matter 'answers', though.
MESSAGE #182. Tue Dec 14 20:12:52. Katrina Martinez wrote:
Eric--in response to your message in #179, I don't think astronomers are "sitting idly by," allowing the Earth's rotation to slow. Wasn't the article from the URL you posted written about a new clock adapting to the Earth's rotation? I mean there's nothing much astronomers can do about Earth's rotation other than adapt to it...unless you can think of something feasible. Also, the article says the Earth is slowing down "at a very slow rate," something we should be worried about, but not as much as the upcoming Astronomy final.
Personally, I wouldn't welcome extra time in a day because it would just give professors an excuse to assign more homework. For every minute added to a day, I can picture professors adding an extra hour or so of work.
MESSAGE #181. Tue Dec 14 14:03:47. Prof. Doug Hamilton wrote:
This year will be the first full moon to occur on the winter solstice, December 22, commonly called the First Day of Winter, in 133 years. Since the full moon on the winter solstice will occur in conjunction with a lunar perigee, (the point in the moon's orbit that is closest to Earth) the moon will appear about 14 per cent larger than it does at apogee, (the point in its elliptical orbit that is farthest from the Earth). The Earth is also several million miles closer to the sun than in the summer, and sunlight striking the moon will be about 7 per cent stronger making it brighter. Also, this will be the closest perigee of the Moon of the year, since the moon's orbit is constantly deforming.
In layman's terms, it will be a super bright full moon, much more than the usual AND it hasn't happened this way for 133 years. If the weather is clear and there isn't a snow cover where you live, it is believed that even car headlights will be superfluous. (...get your dictionaries out.....) Our ancestors 133 years ago saw this. Our descendants 100 or so years from now will see this again.
Happy Holidays!
MESSAGE #180. Tue Dec 14 10:36:13. Prof. Doug Hamilton wrote:
I haven't forgotten your question! Enormous explosions in space (supernovas) do create black holes. But the material that falls into the black hole gets scrunched up and stored inside the black hole and the black hole becomes more massive. The black hole hoards its mass - it doesn't release material into another galaxy or universe as far as we know!
Eric - what's so bad about the day getting longer? Most people I know have too much to do in our current 24 hour day and would welcome a little extra time!
MESSAGE #179. Tue Dec 14 7:12:14. Eric Webster wrote:
How can astronomers sit idly by and ALLOW this to happen?
MESSAGE #178. Mon Dec 13 22:08:41. Eric Webster wrote:
Didja see Mars just to the right of the Moon?
MESSAGE #177. Mon Dec 13 20:49:54. Ian Ullman wrote:
MESSAGE #176. Mon Dec 13 18:19:22. Christina Roney wrote:
MESSAGE #175. Mon Dec 13 17:38:33. Katrina Martinez wrote:
One of the astronomers quoted in the article goes to the Max Planck Institute; isn't that where Dr. Hamilton did his postdoctorate?
MESSAGE #174. Mon Dec 13 17:22:49. Eric Webster wrote:
May Jupiter have possibly ejected a previous planet or two?
Of course, I bet noone checks this board, anymore..
MESSAGE #173. Sun Dec 12 17:39:16. Eric Webster wrote:
Does this mean we'll be seeing the 'pink planet'* in approximately the same position for the next few days?
Sniff.. one more lecture.. one more exam... no more homework.. boohoo, I can't stand it..
*it looks more pink than red to me!
MESSAGE #172. Fri Dec 10 0:23:09. Brandon Wise wrote:
MESSAGE #171. Thu Dec 9 17:16:36. George Morgan wrote:
MESSAGE #170. Thu Dec 9 16:19:44. Eric Webster wrote:
MESSAGE #169. Thu Dec 9 15:49:45. Ihuarulam Ukeje-Eloagu wrote:
MESSAGE #168. Thu Dec 9 15:40:07. Ihuarulam Ukeje-Eloagu wrote:
MESSAGE #167. Thu Dec 9 14:36:12. Prof. Doug Hamilton wrote:
It turns out that it has faded significantly and is now much harder to find. What I was looking at turns out to be a star ...
MESSAGE #166. Thu Dec 9 12:25:07. Olumuyiwa Lawal wrote:
MESSAGE #165. Thu Dec 9 12:23:32. Olumuyiwa Lawal wrote:
MESSAGE #164. Thu Dec 9 9:25:11. Prof. Doug Hamilton wrote:
Using a pair of binoculars, I was able to spot the new nova from the Astronomy observatory last night! We couldn't see it without binoculars, but it is easy to pick out with them. The hardest part is figuring out which point of light is the nova. I'll bring my sky maps again on Friday if anyone is interested - they are very helpful!
Here's a quick sketch of what to do to find the nova. In the evening an hour or two after sunset, find a fairly dark place where lots of stars are visible. Spot Jupiter high in the sky and Saturn nearby and pat yourself on the back. Now comes the hard part. Look toward the direction of sunset and identify the summer triangle - a very large triangle formed from three of the brightest stars Vega, Altair, and Deneb. The star furthest from the other two is Altair. Now break out the binoculars and look at Altair. There is a pretty bright star next to Altair, visible in the same field of view of the binoculars. Draw an imaginary line between these two, and mark an imaginary spot midway between them. Now start from the imaginary spot and move the binoculars downward toward the horizon, in a direction perpendicular to the imaginary line between the two stars. Move the binoculars about three times the distance between the two stars. There are two more bright stars there (fainter than Altair and its friend though) - the brightest one ought to be centered in your binoculars. That's the nova! The nova looked distinctly red to me.
Let the class know if you are successful at finding it! Of course, you'll want to go back to that same part of the sky in a few weeks and see if the star is gone!
I also saw three of Jupiter's four Galilean satellites (Io and Europa were together and appeared as one object). Focus and steady the binoculars and you should be able to spot them as well. They are very close to Jupiter (Io, Europa, Ganymede, and Callisto are up to 3, 5, 8, and 13 Jupiter diameters out, respectively) and will all lie in a straight line.
MESSAGE #163. Thu Dec 9 7:13:47. Eric Webster wrote:
MESSAGE #162. Thu Dec 9 6:56:34. Eric Webster wrote:
TIA
MESSAGE #161. Tue Dec 7 17:48:52. Katrina Martinez wrote:
Park's article does provide an interesting refutation to criticism of the "apparent" failure of the Mars mission. However, Park does exaggerate when he portrays criticism as people saying "the agency is mismanaged...the agency is incompetent...the agency should be killed." It may be effective for his audience, but it does little to strengthen his argument.
I personally have no problem with astronomy. I admire astronomers' curiosity in uncovering mysteries of the universe, uncovering truth no one else dares to seek. But you have to understand why people are angry. They pay taxes, money going to the government to fund programs like NASA. Of course they'd be angry if a mission failed: that's $165 million that could have gone to improving life here on Earth. Not that the money would have made much of a difference anyway; I suspect that one reason astronomy is so popular is that people are looking for new planets to colonize because we already screwed up life here on Earth.
Also, the last part of Park's article seems to be an argument against the space program. According to him, as we explore further the scale of the universe, we realize more how insignificant we are, how we are "fragile, self-replicating specks of matter, trapped on a tiny planet...in one of billions of galaxies." Why should we explore space further if the result will "diminish the specialness of Earth and its inhabitants?"
But that's no reason to stop exploring space. The goal of life, according to philosophers, is to uncover truth, one of the most painful aspects of life's journey. Of course it hurts to know we're not the center of the universe. But I think it's a little extreme to denigrate the human character as much as Park does, especially when it ends up hurting his argument.
In short: people aren't so quick to judge. They're angry, and justifiably so in some respects. But that doesn't mean we should stop the space program; it just means the more failures NASA has, the more it has to answer for.
MESSAGE #160. Tue Dec 7 9:43:06. Ian Ullman wrote:
Lets hope that those who are quick to judge read it.
MESSAGE #159. Mon Dec 6 22:23:10. Katrina Martinez wrote:
MESSAGE #158. Mon Dec 6 21:48:09. Shan Hsiung wrote:
MESSAGE #157. Mon Dec 6 21:32:13. Eric Webster wrote:
Woo-hoo!
MESSAGE #156. Mon Dec 6 18:58:26. Prof. Doug Hamilton wrote:
Our panel of judges are proud to present eight awards this year:
Most ranting message: Charles Greenwell (Msg. #153).
Angriest: April Jackson (Msg. #83)
Most apologetic: Eric Webster (Msgs. #85, #154).
Most chatty: Eric Webster (46 Msgs out of 154).
Chatty wanna be: Prof. Hamilton (22 Msgs).
Best vocabulary: Saadia-Yael Eisenberg (Msg #23).
Happiest: Imran Shaikh (Msgs. #35, #72)
Worst Paid TA: Eric Webster ($0 for answering lots and lots
of Bulletin Board questions)
MESSAGE #155. Thu Dec 2 16:24:49. TA Charles Greenwell wrote:
I have a bit more faith behind the theories than most, but I definitely agree that they defy common sense. All I'm saying is that quite a bit about the universe actually does defy common sense. Something really weird should happen when you pile that much mass together, and a black hole is the weird thing that the theories currently predict. I never expect too much from my intuition; it's led me astray far too many times.
By the way, no self-respecting quantum mechanic would leave their oven on. The turkey might get burnt! I'd be more likely to skip dinner, in case a cooked turkey managed to appear in my stomach. Always consider the probability of a free meal.
MESSAGE #154. Wed Dec 1 21:33:57. Eric Webster wrote:
I DO have a problem with relativity. If it's got mass, it's gotta have volume, right? At the beginning of the semsester it's like Newton's the greatest; by the end, Newton is hung out to dry on THEORIES.
My brother says that quantum physicists will turn the oven on with nothing in it, because there is a greater than zero probability that a turkey will appear fully cooked if he waits long enough!
Seriously, no offense Charles. You're a great TA, except for the Trekkie digressions..
MESSAGE #153. Wed Dec 1 18:25:14. TA Charles Greenwell wrote:
I am trying to stem a horrible tide, Mr. Webster. You are bringing about the downfall of our education system. What would America be like if students arrogantly demanded proofs and reasons for what their instructors dictated? If they foolishly followed their own ideas rather than the ideas of others? I suppose that next you're going to claim that Newton was wrong about gravity, or that Einstein was wrong about quantum mechanics? You, sir, are leading others down the path to anti-intellectualism, and I for one will not stand by and watch you ruin others' faith in the infallibility of science!!!
MESSAGE #152. Wed Dec 1 13:53:41. Katrina Martinez wrote:
MESSAGE #151. Mon Nov 29 20:17:48. Eric Webster wrote:
Congratulations Dr Hamilton -- the Diamondback on Monday got some good sound bites from your Astronomy Open House!
MESSAGE #150. Mon Nov 29 20:09:43. Eric Webster wrote:
Do they REALLY shrink down to a 'mathematical point', or are they just so dense that their escape velocity exceeds the speed of light? The book hems and haws, saying that black holes 'could be made of gerbils or corn flakes' and that we really don't know what exists in them and furthermore we can't know, by their definition.
While I reject the notion that gerbils or corn flakes are at the center of black holes (I may be going out on a limb here), I have difficulty conceiving of mass without ANY VOLUME whatsoever. The TA tried to foist some hypothetical wormhole proof on us, but I say whatever gets close enough to 'look' inside a black hole becomes "one with the void"!
Is it really the limit of our knowledge that we simply don't know what happens when gravity overcomes the neutrons' ability to pack together?
ps the book had a good density-of-a-neutron-star example: a teaspoon of one would weigh sixteen tons!
MESSAGE #149. Mon Nov 29 15:10:40. Prof. Doug Hamilton wrote:
I have been noticing these 3 stars which sort of lie in almost a straight line. They seem to be pretty bright and the line that they form seems to be pretty prominent and obvious. I started noticing them around the time the meteor shower occured. It would be very interesting to know what they are, and if they are sort of part of the same system. If you understand which stars I am referring to then please do reply.
Thanks a whole lot!! -Ambreen.
Hey Ambreen,
I bet that you are seeing Orion's belt. Take a look at the inside cover of your ASTR100 book at the picture "The Night Sky in Spring". Look near the Western Horizon. Orion's belt is composed of the three stars near the "N" in the word "ORION". The stars are not members of the same star system, but are just a chance alignment in the sky. Orion is a particularly interesting constellation - the bright star Betelgeuse is a red giant (and appears noticeably red) and the bright blue star Rigel is a high mass main sequence star. See if you can spot Orion in the sky!
Doug Hamilton
MESSAGE #148. Wed Nov 24 7:55:55. Prof. Doug Hamilton wrote:
A quick reminder ... the LAST day for attending the open house is Sunday December 5! Don't forget to do this important part of ASTR100.
MESSAGE #147. Tue Nov 23 15:01:05. Eric Webster wrote:
It really depends on how you define "messed with". Trees and buildings make decent FM barriers, but lousy AM barriers. And AM waves will 'bounce' off buildings, cliffsides, and even the atmosphere while FM waves get scattered by them. The AM bounce-off-the-atmosphere is recognizable to anyone who has driven across the country; near Mt. Shasta, my International TravelAll's AM radio got its best nighttime signal from KFI in LA some 700 miles away!
Now I know TV uses VHF and UHF, but the ad $$ are much smaller for UHF channels. Does the higher frequency of the UHF signal allow it to get more easily disturbed than the VHF signal?
What bandwith are the radio waves we 'see' from stellar nebulae? It must be a whole range, right? Those radio telescopes probably get good AM radio reception!
MESSAGE #146. Tue Nov 23 14:46:29. Prof. Doug Hamilton wrote:
Driving through a tunnel you can get an FM station but not an AM one (I just tried this again the other day on 395 North under the mall in downtown DC). This is because the (shorter) FM waves can follow you into the tunnel while the AM waves (longer) cannot. To fit through an aperture, the wavelength of EM radiation must be much smaller than the size of the aperture. AM radio waves have wavelengths of a few hundred meters while FM radio waves have wavelengths of a few meters (see below). The tunnel might be 10 meters wide. So FM can get in and AM can't.
The dish for a radio telescopes can be built from wire mesh for the same reason - radio waves won't get through the holes. The same happens for visible light. Light can get through a normal-sized hole in a sheet of paper, but not through a very tiny hole. How tiny? About the size of the wavelength of visible light. Any hole smaller that about a micron or 1/50 the width of a human hair will not let visible light through.
You can also work out the wavelength that a radio station transmits at yourself from the station's frequency. It turns out that
(frequency)*(wavelength) = (speed of light)
for all EM radiation. So
(wavelength)=(speed of light)/(frequency)
Maybe your favorite FM station has a frequency of 101.1 MHz (Megahertz or million Hertz where Hertz has units of 1/s). The station transmits at a wavelength of
(wavelength) = (3*10^8 m/s)/(101.1*10^6 Hz) = 2.97 m
While an AM station that you never listen to transmits at 1000 kHz transmits at a wavelength of
(wavelength) = (3*10^8 m/s)/(1000*10^3 Hz) = 300 m
So, why do you never listen to that AM station? It because no one else does either! A station with relatively few listeners gets little advertising money and can't buy into the "expensive" FM part of the EM spectrum! Why is FM expensive? Because it transmits with less interference (see above) so everyone wants their station to transmit there. If an AM station got popular, it would make more money, and eventually buy its way into the FM frequency. I know of one case where that actually happened! Notice also that the "coolest" FM stations are usually in the 100 MHz range rather than the 90MHz range as well.
So, if advertising $$ are all important, at what frequency do you suppose TV station transmit?
MESSAGE #145. Tue Nov 23 7:16:47. Eric Webster wrote:
So in the VISIBLE part of the spectrum, blue (shorter) gets scattered all over the 'dome' of the sky more easily than the red, which makes more of a direct path from Sun to eye.
Does this help?
MESSAGE #144. Mon Nov 22 23:00:13. Katrina Martinez wrote:
MESSAGE #143. Mon Nov 22 20:35:35. Christina Roney wrote:
The correct answer is (shortest to longest): gamma rays, x-rays, ultraviolet, blue, yellow, red, infrared, and radio.
This however, does not make sense to me because I thought the sky was blue because of the longer wavelength getting "stuck" in our atmosphere so that's the color we see bending towards our eyes. So how can blue light have a shorter wavelength and red have a longer one if we see blue as the color of the sky and not red?
MESSAGE #142. Mon Nov 22 15:05:22. Eric Webster wrote:
It's kind of off-topic, I suppose, but it IS the grading for ASTR100 so there's a justification. And two points out of 750 still isn't likely to make or break anyone's grade..
MESSAGE #141. Mon Nov 22 11:37:33. Katrina Martinez wrote:
Anyway, Kristina asked about posting something on the bulletin board: I think the very first message posted was by Dr. Hamilton, who said that you'll earn 4 bonus (extra credit) points for posting something. But I don't think it's incorporated yet into the grades that are posted on the web. Makes sense, because you'd want to wait until the end of the semester to record all the points.
MESSAGE #140. Mon Nov 22 10:48:18. Kristina Mechelis wrote:
MESSAGE #139. Mon Nov 22 8:18:11. Prof. Doug Hamilton wrote:
Well, we messed up again ... that multiple choice question was graded incorrectly on almost everyone's test. I graded most of the makeup exams by hand (correctly!) later, which is when I first noticed the problem. So Linking telescopes together is the correct answer!
If you marked the correct answer and got it wrong, show your exam to your TA in section and we'll add two points to your score. If you marked the wrong answer and got it right, you win - you get to keep the points!
Sorry about the confusion.
MESSAGE #138. Sun Nov 21 21:10:01. Eric Webster wrote:
MESSAGE #137. Sun Nov 21 14:23:20. Katrina Martinez wrote:
I also put as my answer to the telescope question, "linking a series of telescopes together." From the way they're presented in the book, resolution and resolving power appear to be the same. Since resolving power depends on diameter, linking telescopes together would increase resolution by making a bigger diameter. Didn't Dr. Hamilton put up a transparency in class that showed many telescopes linked together?
Anyway, I don't think the two points on that multiple choice question really matters. If we got that question right, most of the grades in the entire class would be shifted 2 up, and so the curve would actually stay the same.
MESSAGE #136. Sat Nov 20 21:02:14. Monique Koppel wrote:
MESSAGE #135. Sat Nov 20 14:17:04. Eric Webster wrote:
Now: There was a question on the test about increasing the resolution of a radio telescope. By resolution, I interpreted resolving power. Therefore, I put as an answer that they would link a series of telescopes together. However, the correct answer was something like measuring one side of the object and then the other. I REALLY don't understand this approach. Perhaps a TA or the test-writer can clarify this for us..
MESSAGE #134. Fri Nov 19 18:58:31. Katrina Martinez wrote:
MESSAGE #133. Wed Nov 17 23:55:02. Katrina Martinez wrote:
The next best way of viewing the Leonids is by looking at today's Astronomy Picture of the Day. This one is good because it's a moving image of the 1998 meteor shower that was seen in New Mexico. However, a better picture is an archived stationary image of the 1998 Leonids because the frame freezes right when the meteor takes on a form. Some people said that it looks like an angel; I thought it looked more like the mythological Phoenix bird that destroys itself every 500 years, but always rises from its ashes. I like my interpretation better because it's much more creative.
MESSAGE #132. Wed Nov 17 10:40:44. Prof. Doug Hamilton wrote:
Remember the corona is about 1,000,000 degrees while the Sun's visible surface is only 6000 degrees. This is unusual - since the corona is further from the center of the Sun we might expect it to be cooler than the visible surface.
The first step toward answering this question is to figure out what energy sources are available for heating the corona. The main possibilities with enough energy include 1) the photons streaming off the Sun's visible surface and 2) magnetic fields which are known to determine some of the corona's structure. The first energy source has problems. The corona is so hot that atoms do not exist there - just atomic nuclei and electrons. These are not very efficient at absorbing light, so not enough sunlight is absorbed to heat the corona up much.
So we are left with magnetic fields. Most everyone agrees that magnetic fields are responsible, but the details of exactly how this works are not understood. There are two or three rather technical theories, one of which might be right, but there is not enough evidence yet to say which is right (if any are right!).
The book talks about magnetic waves being responsible, but there are a whole zoo of different types of magnetic waves - we don't know which ones are the important ones. People have also argued that magnetic reconnection (which is a different magnetic effect) might be more important than waves. The question is of exactly how the corona is heated is not really settled yet and thus it is an area of active research in solar physics!
MESSAGE #131. Tue Nov 16 11:26:39. Katrina Martinez wrote:
MESSAGE #130. Mon Nov 15 20:20:49. Eric Webster wrote:
MESSAGE #129. Mon Nov 15 20:19:26. Eric Webster wrote:
It was raining last Thursday, so they are scheduling the sunspot viewing for tomorrow. It's supposed to be pretty cloudy tomorrow, so we'll see if they show..
Dr. H or George -- Can you shed any light [sic] on the second part of post 119 on the hot corona conundrum? TIA..
MESSAGE #128. Mon Nov 15 17:46:54. Ambreen Ilyas wrote:
MESSAGE #127. Mon Nov 15 16:45:15. Prof. Doug Hamilton wrote:
The Leonids come from Comet Tempel-Tuttle which has a 33 year orbit around the Sun. Since the comet has just passed Earth, and the region just behind the comet has lots of debris, this should be a particularly good year for a meteor storm. In a typical year the Leonids cause something like 10 meteors per hour - a "storm" this year could result in 1000 meteors per hour! Pretty impressive if it happens, but these things are hard to predict.
Last year was also pretty good - even though it was cloudy then, I saw 10-20 very bright shooting stars from College Park. If you can get to a darker site, you will be likely to see lots more this year.
MESSAGE #126. Sun Nov 14 23:44:57. Benjamin Rodeffer wrote:
MESSAGE #125. Sun Nov 14 17:05:11. Eric Webster wrote:
I believe you are referring to a Dobsonian telescope. Pretty easy and inexpensive to build, but you still need to purchase the focusing mirror, reflecting mirror and the eyepiece. All told, it sounds like a coupla hundred for the optics and about fifty for the rest.
A list of Dobson DIY (do it yourself) sites are at:
http://dir.yahoo.com/science/astronomy/telescopes/amateur/telescope_making/dobsonian_telescope/
From the links there you can get to the optics suppliers for pricing info.
If you make one, let the board know and you'll be a hero!
MESSAGE #124. Sun Nov 14 16:42:49. Benjamin Rodeffer wrote:
MESSAGE #123. Thu Nov 11 11:32:22. Christina Roney wrote:
MESSAGE #122. Wed Nov 10 19:01:44. Prof. Doug Hamilton wrote:
Focus George, Focus! Those are interesting questions, but not exam II material! We'll get to black holes soon, though! They do absorb all light that falls upon them (which is why they are black), but there are not enough of them to cause space to be cold. Space is cold simply because there is so much of it between the hot things (stars). If we didn't have the Sun, for example, starlight wouldn't be able to heat things up too much. Trying to heat up space with starlight is a little like trying to warm up a dank old castle with a single candle.
MESSAGE #121. Wed Nov 10 18:53:22. Prof. Doug Hamilton wrote:
I dont quite understand why the sunsets and sunrises are red. I dont
particularly understand how come the light has to go through more
atmosphere when the sun is at the horizon I would appreciate it if you could explain this to me.
Thanks in advance.
-Ambreen
Hi Ambreen,
Those are good questions! Sorry for the delayed response ...
Try drawing a picture! Too bad I can't do this in HTML. Draw a
circular Earth so that it takes up most of a sheet of paper. Then draw
a thin atmosphere around the Earth (a slightly bigger circle). Now
draw a tiny little portrait of yourself at the 12 o'clock position on
the Earth's surface. Finally, draw a vertical line from your portrait
straight up (that's the light ray to the noontime Sun) and another one
out horizonally out to the 9 o'clock position (that's sunset). If you
drew the picture well, it should be clear that the horizontal line
cuts through more atmosphere than the vertical line does. For the
actual size of the Earth and the thickness of the atmosphere, the
sunset ray travels through something like 20 times more atmosphere
than the noontime ray.
All wavelengths of light are scattered in the Earth's
atmosphere. Yellow, for example is scattered more than red but less
than blue. When we look toward the Sun, we see the light that is not
scattered (it comes straight to us). So sunsets are a mixture of lots
of red, a little yellow, and even less blue since the yellow and blue
are mostly scattered to other directions. This combination looks red
to our eyes. Conversely, when we look away from the Sun, we see the
scattered light which is mostly blue, a little yellow, and even less
red. This combination looks blue to our eyes.
Whew! Does that all make any sense??
MESSAGE #120. Wed Nov 10 18:16:38. George Morgan wrote:
George
MESSAGE #119. Wed Nov 10 14:36:57. Katrina Martinez wrote:
Essay 2 seems irrelevant to what we're studying right now because it's on keeping time.
In short, out of Essay Two, Overview 4, and Overview 5, my guess is the only things that may appear on Exam II is Overview 4 pp. 214-215, and Overview 5 pp. 319 to 321.
MESSAGE #118. Wed Nov 10 13:56:00. Eric Webster wrote:
I feel pretty sure this WON'T be asked on the exam, but I need a better explanation on why the corona gets so hot.
The book mentions that the density further away from the surface of the Sun is much less, and the gravitational fields of the Sun (which are not decreasing) excite the farther atoms to a much greater extent than the closer-in atoms, heating them intensely in the process.
eg force of e/m energy constant, but fewer number of atoms to excite = very excited remaining atoms
In fact, the book goes so far as to state that it excites the atoms so much as to cause the 'solar wind'. Is this a fair assessment of the phenomenon?
MESSAGE #117. Tue Nov 9 19:26:56. Prof. Doug Hamilton wrote:
We'll get to this stuff next week (after the exam!).
MESSAGE #116. Tue Nov 9 19:13:00. Monique Koppel wrote:
MESSAGE #115. Mon Nov 8 17:42:26. Eric Webster wrote:
We also know stars come in much hotter varieties than Sol.
How much hotter are the interiors of the really hot stars? Charles took a guess at it in section, but the speed of his backpedaling (and his subsequent confession) indicated he wasn't too sure. Is there a formula for deducing the interior temperature of a star from its exterior temperature?
MESSAGE #114. Sun Nov 7 17:09:07. Courtney Perkins wrote:
MESSAGE #113. Sun Nov 7 17:08:02. Courtney Perkins wrote:
MESSAGE #112. Sat Nov 6 9:16:05. Eric Webster wrote:
I wasn't there for Ji-Hoon's comet-tail lecture, so I can offer my own understanding of the phenomenona. Two discrete tails form from comets, one a gas plume; one composed of dust and teeny tiny pieces of rock. The gas is lighter, so the solar wind can "blow" it more effectively and consistently in the direction AWAY from the Sun. The dust tail has heavier "pieces", so it kind of drags behind the gas tail. If you remember that the dust plume is heavier than the gas plume and you can draw a picture of a comet's motion around the Sun, it's easier to understand. Fig. 10.15 on page 309 in the book is just that sort of diagram!
Exam alert! The inside scoop is that there are going to be lots of questions about asteroids, comets, and the physics of light (aka electromagnetic radiation) on the exam. The good news is that there are only 10 lectures worth of material to review!
MESSAGE #111. Fri Nov 5 16:53:56. Courtney Perkins wrote:
MESSAGE #110. Fri Nov 5 16:44:49. Eric Webster wrote:
Sorry I can't help on the sunspot question -- you didn't miss anything! We know the sunspots are cooler, but we haven't yet heard from Prof Hamilton why they are cooler. If not knowing about the 'spots keeps you awake tonight, the book offers its own reasons: it never fails to put me to sleep!
MESSAGE #109. Fri Nov 5 11:43:15. Ambreen Ilyas wrote:
MESSAGE #108. Thu Oct 28 16:08:32. Ambreen Ilyas wrote:
MESSAGE #107. Thu Oct 28 7:00:18. Eric Webster wrote:
BTW, I discovered numerous websites for plans for homemade telescopes. The optical stuff (mirror, eyepiece) cost real money (150 or so), but the other material (tube, base, etc) is inexpensive. It's probably cheaper and more fun to go to the OPen Houses at Campus...
MESSAGE #106. Wed Oct 27 21:03:25. Monique Koppel wrote:
MESSAGE #105. Wed Oct 27 19:32:36. Eric Webster wrote:
If I may, let me try giving your question a shot. And please, if I'm totally wrong, correct me!
All the planets (Sun, Moon, Saturn, Mars, etc) rise and set ech day, rising in the East and setting in the West.
All this rising and setting activity is due to Earth's rotation. We spin and our view changes like your view on a carousel changes while it's moving.
From day to day, Earth's position changes due to our orbit of the Sun. The other planets' positions change too due to THEIR orbits of the Sun. So from day to day, the planets' positions in the sky change because 1) they are moving around the Sun (Merc and Venus more quickly than Earth, outer planets progressively less quickly than Earth) and 2) our position relative to theirs is changing as well.
Imagine being on a carousel, looking out at the crowd. Then you notice a couple of kids running around the carousel at different speeds. Sometimes you see one kid, sometimes you see both, sometimes you don't see either (when the carousel is in the way). Does that metaphor hold water? (just practicing a little metaphor-mixing Does this help at all?
MESSAGE #104. Wed Oct 27 14:07:29. Saadia-Yael Eisenberg wrote:
MESSAGE #103. Wed Oct 27 14:04:21. Peter Miller wrote:
MESSAGE #102. Wed Oct 27 13:51:26. Ambreen Ilyas wrote:
MESSAGE #101. Wed Oct 27 11:04:40. Prof. Doug Hamilton wrote:
The Open House Papers are mostly graded, and will be posted by Monday at the very latest. Those of you who have not done the Open House Paper yet will have artificially low grades on the grade page since you'll have a zero for the assignment until you turn it in! Don't be too alarmed by this!
Finally HOMEWORK #5 is due on Friday! These will be graded and posted by Monday or Tuesday.
MESSAGE #100. Tue Oct 26 23:24:21. James Blassingame wrote:
MESSAGE #99. Tue Oct 26 22:07:33. Jillian Martin wrote:
MESSAGE #98. Mon Oct 25 18:43:15. Prof. Doug Hamilton wrote:
MESSAGE #97. Mon Oct 25 18:34:20. Christina Roney wrote:
MESSAGE #96. Mon Oct 25 14:22:31. Saadia-Yael Eisenberg wrote:
MESSAGE #95. Mon Oct 25 14:20:29. Saadia-Yael Eisenberg wrote:
MESSAGE #94. Mon Oct 25 1:10:34. Shelley Dezelon wrote:
MESSAGE #93. Sun Oct 24 9:31:19. Eric Webster wrote:
To the left of the full moon was Jupiter, super-bright with two visible moons on its right.
Further to the left of the Moon and Jupiter, there was a brightish-star-like body that I guessed was Saturn. I tried to hold the binocs as steady as possible, contorting my viewing position so I could hold them close to the side of the house. (So I'm too cheap to spring for a tripod!) Anwyay, I THINK I saw the rings of Saturn. The jiggling around made it pretty tough. Maybe I'll start pricing tripods. Or telescopes..
Does anyone know where one can find plans online for make-em-yourself telescopes? I heard there was a fellow in SF who is sort of a Johnny Appleseed of DIY large scale scopes.
MESSAGE #92. Sat Oct 23 20:25:21. Quan Luu wrote:
Quan
MESSAGE #91. Wed Oct 20 16:55:32. George Morgan wrote:
As far as it goes, they will use this new-found information to determine more information about the longevity of our Sun.
MESSAGE #90. Wed Oct 20 13:38:26. Saadia-Yael Eisenberg wrote:
MESSAGE #89. Sun Oct 17 22:31:28. April Jackson wrote:
MESSAGE #88. Sun Oct 17 19:23:24. Benjamin Rohan wrote:
MESSAGE #87. Fri Oct 15 21:09:02. Eric Webster wrote:
MESSAGE #86. Fri Oct 15 19:19:53. April Jackson wrote:
MESSAGE #85. Fri Oct 15 7:33:28. Eric Webster wrote:
I am NOT trying to sound like a know-it-all but I AM trying to figure this astronomy stuff out. If someone posts an observation that doesn't jibe with what I've read, I want to understand where the difference lies.
I do remember from the book that Venus and Mercury are always observed in the general direction of the Sun from Earth's direction--their orbits are closer to the Sun, so from Earth, they can be a maximum of maybe 27? degrees from the Sun (Mercury) and 40? degrees from the Sun (Venus). So my theory (and you are right April, it is just a theory--I wasn't there observing with you) is that at 10pm the sun is long set, and Venus would either be very low in the western sky or not visible.
Anyway, will you accept my apology April
MESSAGE #84. Fri Oct 15 4:16:17. Prof. Doug Hamilton wrote:
Actually, the person who finds the fainter planet should get the cookie! Fainter planets are much harder to find. Can anyone find Saturn from my description and the fact that it must lie along the ecliptic (the path taken by the Sun, Moon and planets across the sky)? The secret is "connect the dots". Connect up the Moon to Jupiter and extend the line to the two horizons. Then look for other bright objects along the line (which is just the ecliptic).
Saw the Moon from Italy - it's a thin waxing crescent. Waxing means getting more full! It is visible in the evening and will be rising higher and higher in the sky in the coming days.
MESSAGE #83. Fri Oct 15 0:11:03. April Jackson wrote:
MESSAGE #82. Thu Oct 14 15:59:11. Akisha Jones wrote:
MESSAGE #81. Thu Oct 14 6:54:33. Eric Webster wrote:
MESSAGE #80. Wed Oct 13 13:08:03. Saadia-Yael Eisenberg wrote:
MESSAGE #79. Wed Oct 13 7:14:55. Eric Webster wrote:
Not a very dense asteroid either. Using the effect of gravity on the captured moon, they have inferred that Eugenia has a density of only 2.5 gm/cm3
I guess this gravity biz isn't limited to giant spheroids!
MESSAGE #78. Mon Oct 11 4:30:10. Prof. Doug Hamilton wrote:
4 New Moons of Uranus have been discovered! The first one was found in images from Voyager from 1986 - it was overlooked all of these years. It is located close to Uranus, and probably formed when the planet did.
The other three were discovered with ground-based telescopes. They move on distant orbits and are probably captured objects.
MESSAGE #77. Sun Oct 10 21:14:34. Eric Webster wrote:
MESSAGE #76. Sun Oct 10 18:43:32. April Jackson wrote:
MESSAGE #75. Sun Oct 10 16:02:17. James Blassingame wrote:
MESSAGE #74. Sat Oct 9 13:29:59. Prof. Doug Hamilton wrote:
Don't forget to watch the Moon while I'm gone!
MESSAGE #73. Fri Oct 8 10:20:49. Prof. Doug Hamilton wrote:
Juhi found a pair of glasses after one of her Wednesday sections in CSS2400. They are in a hard case which is black on the front and silver on the back. The front side has a picture of an eagle and the words "Harley-Davidson Motorcycles".
If these are yours, you can pick them up in the Astronomy Mailroom, CSS1204.
MESSAGE #72. Thu Oct 7 20:50:37. Imran Shaikh wrote:
i have finished my hw #4!!!!! and right now i'm listing to Indian song on line so anywayyyyy if anyone need helpe e-mail me at ishaikh@wam.umd.edu * * * * )* * /\ * * /\ * || || || || || WELCOME || |||||||||||||||||||| || |||||||||||| || |||||||||||||||||||| ||||||||||||||||||||
MESSAGE #71. Thu Oct 7 19:37:48. George Morgan wrote:
GEMII
MESSAGE #70. Wed Oct 6 10:32:58. Prof. Doug Hamilton wrote:
When an object is low near the horizon (as compared to high in the sky), its light has to go through more of Earth's atmosphere before it gets to us. This effect is why the Moon usually appears reddish on the horizon (and sunrises and sunsets look reddish too). Red light is better able to get through the atmosphere than other colors. And, more relevant to your question, if there are thin clouds or haze, the Moon will look a lot fainter when it is on the horizon.
Once the Moon rises high in the sky, though, its light has to travel through less atmosphere and it will appear brighter - bright enough to be seen in the daytime!
So everyone keep an eye out for the Moon during the day too!
MESSAGE #70. Thu Sep 30 21:57:02. Crystal Koch wrote:
(This was posted to the wrong place! - D. Hamilton)
MESSAGE #69. Tue Oct 5 23:33:49. Christina Roney wrote:
MESSAGE #68. Tue Oct 5 13:38:53. Prof. Doug Hamilton wrote:
Peter - just because it's simple doesn't necessarily mean its wrong! Try drawing a picture.
MESSAGE #67. Tue Oct 5 13:07:14. Peter Miller wrote:
MESSAGE #66. Tue Oct 5 12:56:00. Peter Miller wrote:
MESSAGE #65. Mon Oct 4 14:56:54. Eric Webster wrote:
MESSAGE #64. Mon Oct 4 10:17:45. Peter Miller wrote:
MESSAGE #63. Fri Oct 1 7:06:07. Eric Webster wrote:
The teams, located at the National Aeronautics and Space Administration's Jet Propulsion Laboratory in Pasadena and at Lockheed Martin Astronautics in Colorado, complicated matters further by failing to realize the error, the agency said in a statement.
I guess this is what happens when you don't convert units properly!
MESSAGE #62. Thu Sep 30 20:52:28. Saadia-Yael Eisenberg wrote:
MESSAGE #61. Thu Sep 30 20:51:01. Saadia-Yael Eisenberg wrote:
MESSAGE #60. Thu Sep 30 19:30:49. Eric Webster wrote:
Hope that helps!
MESSAGE #59. Thu Sep 30 19:25:07. Heather Grimes wrote:
MESSAGE #58. Thu Sep 30 11:06:08. Eric Webster wrote:
That's where the constant comes in handy. It puts into the equation just the right units that you need, if the equation lacks it.
Otherwise, a meter divided by a meter disappears off the equation.
A meter cubed divided by a meter squared is a meter
and so on
Note that meters of radius or distance when cubed become m3 or cubic meters: a measurement of volume.
Keeping track of the units helps you check for errors in the math. If you get a rate of speed that is in kilograms (for instance), something didn't cancel out correctly!
Does this help?
MESSAGE #57. Thu Sep 30 9:43:53. Kristina Mechelis wrote:
MESSAGE #56. Wed Sep 29 14:10:54. Eric Webster wrote:
1012 x 1014
add exponents 1026
Like wise to divide, subtract exponents..
to make an exponent of an exponent ie (1022 ) 3
multiply the exponents: 10 66
Likewise, to take a root power of an exponent, divide the exponent by the root
Beyond this, mathematicians will have to step forward...
MESSAGE #55. Tue Sep 28 21:52:58. Prof. Doug Hamilton wrote:
MESSAGE #54. Tue Sep 28 20:57:28. Michael Trezza wrote:
MESSAGE #53. Tue Sep 28 16:11:45. Eric Webster wrote:
Volume of a sphere etc etc.
BTW, you can put that cd in any of the WAM workstations and it will work. The CSS building has great new G3s and there is never a wait!
MESSAGE #52. Tue Sep 28 15:41:01. Saadia-Yael Eisenberg wrote:
MESSAGE #51. Tue Sep 28 11:50:18. Eric Webster wrote:
I just tried running the solar system viewer on the Macs here at Hornbake and I got the same security code violation error.
I guess I'll have to try one of the Wintel machines next..
MESSAGE #50. Mon Sep 27 19:25:45. Eric Webster wrote:
Did you run into Francis Everitt in Houston?
The class misses you!
MESSAGE #49. Mon Sep 27 19:21:36. Eric Webster wrote:
MESSAGE #48. Mon Sep 27 13:38:45. Prof. Doug Hamilton wrote:
MESSAGE #47. Mon Sep 27 10:40:19. Kristina Mechelis wrote:
MESSAGE #46. Fri Sep 24 23:02:18. Eric Webster wrote:
I was bummed that my Sears 10x binoculars didn't pick up the rings of Saturn, but I did get to see the Gallilean satellites. Pretty darn cool. If you're not sure about what you're looking at, the cd that came with the book has a decent planetarium software package.
MESSAGE #45. Fri Sep 24 19:39:28. George Morgan wrote:
->George
MESSAGE #44. Fri Sep 24 19:19:58. Eric Webster wrote:
If you see Francis Everitt of Stanford (he's been working on Gravity Probe B) at the NASA funding panel. say hello to him for me. He's good friends with my family in Palo Alto.
I had to get the 'noculars out last night to prove to the wife that the Moon wasn't QUITE full last night. Should be pretty round tonight!
See you in a week!
MESSAGE #43. Fri Sep 24 7:47:33. Prof. Doug Hamilton wrote:
Watch the sky over the next week to see how close the Moon gets to Jupiter and how close it gets to Saturn. You can measure the distance in Moon diameters.
Mars is also visible high in the sky at sunset. Unfortunately, George's rumor is true - it looks like the latest US Mars mission, Mars Climate Orbiter, burned up in the martian atmosphere early yesterday.
MESSAGE #42. Thu Sep 23 23:47:00. George Morgan wrote:
-GEMII
MESSAGE #41. Thu Sep 23 16:53:18. Saadia-Yael Eisenberg wrote:
MESSAGE #40. Thu Sep 23 16:42:36. Saadia-Yael Eisenberg wrote:
MESSAGE #39. Thu Sep 23 14:16:14. Eric Webster wrote:
Travis --
Draw a little picture of Tycho's model of the solar system and see if the perspective from the Earth MIGHT give you phases or not. I think the answer allows you to say that it wouldn't work, as long as you can explain why..
Good luck!
Eric
MESSAGE #38. Wed Sep 22 13:09:10. Saadia-Yael Eisenberg wrote:
MESSAGE #37. Wed Sep 22 1:09:30. Travis Winn wrote:
MESSAGE #36. Sun Sep 19 21:22:51. George Morgan wrote:
http://www.bc.cc.ca.us/programs/sea/astronomy/nakedeye/nakedeya.htm
This is an excellent Astronomy source. I want to forewarn you, this page is very big and takes a while to load. If you want more notes from this online book, go all the way at the bottom and click the URL to start at the beginning. Good luck to all on your work, and if you have Internet access problems/PC problems feel free to ask..
MESSAGE #35. Sun Sep 19 19:06:59. Imran Shaikh wrote:
MESSAGE #34. Sun Sep 19 11:51:52. Elisabeth Seasonwein wrote:
MESSAGE #33. Fri Sep 17 20:09:50. Eric Webster wrote:
MESSAGE #32. Fri Sep 17 20:08:30. Eric Webster wrote:
sun's radius=100e 1 au = 8600*100e
40au (radius of solar system) = 40*100*8600e
2.5*108 (size of the Milky Way in solar system-size units) *40au=
2.5*108*40*100*8600*e=
2.5*4*1014*8.6 =
86*10&15* .1cm =
8.6*1015 cm =
8.6*1015 / 100 =
8.6*10 13 m =
8.6*1013 / 1000 =
8.6*1010 km
It's always the little things that trip me up!
MESSAGE #31. Fri Sep 17 19:57:26. Eric Webster wrote:
MESSAGE #30. Fri Sep 17 19:36:25. Eric Webster wrote:
Please modify the posting message boxes to allow html codes so we can use scientific notation on the message boards. I think you can easily exclude the html commands that you don't need or want here.
I just realized that my previous post looks like, well, an asteroid!
MESSAGE #29. Fri Sep 17 19:35:14. Monique Koppel wrote:
MESSAGE #28. Fri Sep 17 19:33:33. Eric Webster wrote:
let earth=e
sun's radius=100e 1 au = 8600*100e
40au (radius of solar system) = 40*100*8600e
2.5*10&sup8 (size of the Milky Way in solar system-size units) *40au=
2.5*10&sup8*40*100*8600*e=
2.5*4*10&sup14*8.6 =
86*10&sup15* .1cm =
8.6*10&sup15 cm =
8.6*10&sup15 / 100 =
8.6*10 &sup13 m =
8.6*1013 / 1000 =
8.6*10 &sup9 km
which is what I got. Can someone take me through a process that works differently, and better?
MESSAGE #27. Fri Sep 17 16:58:49. Ambreen Ilyas wrote:
MESSAGE #26. Fri Sep 17 13:59:34. Saadia-Yael Eisenberg wrote:
MESSAGE #25. Thu Sep 16 22:43:37. Agnes Lee wrote:
MESSAGE #24. Thu Sep 16 18:17:34. Eric Webster wrote:
>>MESSAGE #22. Thu Sep 16 17:00:36. Lauren Klein wrote:
>> Hey does anyone in ASTRO100 know how to do Essay 1 question 1? I'm a >> little confused.
Lauren see pg. 64 (in the new edition, anyway), Planetary Configurations. Does that help? Or you can pop the cd in the cd-rom and take a gander.
Floyd is preventing me from even basic observations of the moon etc...
MESSAGE #23. Thu Sep 16 17:36:29. Saadia-Yael Eisenberg wrote:
MESSAGE #22. Thu Sep 16 17:00:36. Lauren Klein wrote:
MESSAGE #21. Thu Sep 16 16:57:38. Leah Goldfine wrote:
MESSAGE #20. Thu Sep 16 14:36:39. Patrick Humphries wrote:
MESSAGE #19. Wed Sep 15 16:20:06. Ambreen Ilyas wrote:
MESSAGE #18. Wed Sep 15 8:28:53. Prof. Doug Hamilton wrote:
Last night the Moon came to me in a vision and said "I feel neglected. Go out and tell the masses to pay some attention to me!" There are almost 200 people in ASTR100 and you are the only masses that I know, so I need your help!
What I'd like you to do, if you are interested, is to occasionally report here on the ASTR100 Bulletin Board how the Moon looks. With so many people in this class, we can probably have a new observation of the Moon posted every few days - maybe even every day. Then, as a class, we can watch the Moon go through its motions across the sky and through its cycle of phases.
Here are some things you can note about the Moon. What is its phase (thin crescent, thicker crescent, half full, between half full and full, full Moon)? Where is it in the sky (close to the Sun, far from the Sun, near sunrise, near sunset)? What time was the Moon visible (daytime, early evening, midnight, early morning)?
MESSAGE #17. Tue Sep 14 14:09:50. Saadia-Yael Eisenberg wrote:
MESSAGE #16. Tue Sep 14 8:10:01. Jonathan Chin wrote:
MESSAGE #15. Tue Sep 14 7:45:15. Jonathan Chin wrote:
MESSAGE #14. Tue Sep 14 6:57:45. Jonathan Chin wrote:
MESSAGE #13. Mon Sep 13 18:20:18. Katrina Martinez wrote:
Response to Message #5: The number is big, but not as big as compared to most astronomical units. You can check your answer on the web page (see the extra credit problems).
MESSAGE #12. Mon Sep 13 16:54:52. Eric Webster wrote:
MESSAGE #11. Mon Sep 13 16:50:37. Eric Webster wrote:
mm = millimeter
m = meter
km = kilometer
1mm = 1/1000 m
1m = 1/1000 km
How many mm in a km? Sounds like a good application of scientific notation to me!
MESSAGE #10. Mon Sep 13 16:46:45. Eric Webster wrote:
MESSAGE #9. Mon Sep 13 16:26:26. Lavon Hooker wrote:
My Question is about HW#2 problem 3 about the size of a BB how can i convert this .1 centimeter radius to kilo..I need help...I am DUM..I cant get it!!!Please help....Thank You 8)
MESSAGE #8. Sun Sep 12 22:33:35. Shannon Maycher wrote:
MESSAGE #7. Sat Sep 11 18:47:31. Prof. Doug Hamilton wrote:
First, realize that the orbits of the satellites are actually inclined relative to the planet's equator - so the orbits are in 3D and need not actually intersect. But the orbits will evolve, and the will periodically intersect. Then it is possible for the satellites to collide! But the satellites are small and space is big. If we calculate how it should take, on average, until a collision, the answer is 5-15 billion years! This is older than the age of the Solar System, so they haven't had enough time to collide yet!
If anyone else has problems viewing the java applets - let me know here what configuration you are using (e.g. A PC with Windows 95, and netscape).
MESSAGE #6. Sat Sep 11 15:10:13. Courtney King wrote:
MESSAGE #5. Wed Sep 8 20:11:49. Tamara Smith wrote:
MESSAGE #4. Wed Sep 8 17:00:46. David Moyer wrote:
Also, Professor Hamilton, I noticed in the satellite Viewer that some of the outer planets had smaller moons with crossed orbits... what's the chance of a collision?
MESSAGE #3. Mon Sep 6 15:34:33. Eric Webster wrote:
http://janus.astro.umd.edu/astro/moons.html
to come up OK? I just got a security code violation from the applet..
MESSAGE #2. Mon Sep 6 15:27:10. Eric Webster wrote:
MESSAGE # 1 . Tue Aug 31 20:35:50. Prof. Doug Hamilton wrote: