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MESSAGE #69. Wed May 19 11:21:24. Prof. Doug Hamilton wrote:
How much of the book will be obsolete in 25 years?
Well, astronomy is changing so fast that ASTR100 books come out with new editions every 2 years! But very little of the material in our book will be proved outright wrong. Partially, this is because astronomers try to be pretty sure of what is going on before putting it in a textbook! But we we will definitely get a more complete view of various topics as further advances are made. For example, ten years ago, we hadn't detected any objects in the Kuiper belt or any planets around other stars. Astronomy books for back then say that the Kuiper Belt is "a theoretically-predicted belt of icy objects out beyond Pluto" and that other sunlike stars "probably have planets circling them like our own solar system." Today's books can make more definitive statements now that we have actual observations of both types of objects.
How close is science to bridging Einstein's relativity and quantum mechanics?
Relativity applies for objects that move very fast while quantum mechanics applies to objects that are really small. When really small objects move fast, our theories can't handle it! The physics right near a black hole is an example of a place where our theories break down. We have only vague ideas of what should happen. Physicists have worked for years trying to come up with a theory that combines relativity and quantum mechanics - so far, without success. Some theories show promise, but my feeling is that we still have a long way to go! It could even turn that we will never find a unifying theory.
MESSAGE #68. Wed May 19 11:00:38. Prof. Doug Hamilton wrote:
Jason - I put an extra question on the second midterm by accident which made the exam worth 105 points instead of 100. With the extra credit, a perfect exam would have gotten 108 points.
MESSAGE #67. Wed May 19 6:44:38. Patrick Flores wrote:
MESSAGE #66. Wed May 19 3:21:21. Jason Ross wrote:
MESSAGE #65. Tue May 18 17:49:38. Prof. Doug Hamilton wrote:
So some hints! First up: the exam is weighted pretty heavily on stars and galaxies (stuff since the second midterm). More than 1/2 of the exam is on this material. The other 40% or so is scattered over the first few months of the course.
The test is significantly shorter than two midterms. So you should be able to finish with plenty of time. There are 50 multiple choice answers and seven short answer questions, some with multiple parts. There is one question that focuses on equations; this question has two parts. Use the extra time to check over your answers carefully!!
A Hint: Answers that include the word "alien" are probably wrong!
A Better Hint: Make sure that you have a good sense of how big things are, and how far apart things are. These are some of the most fundamental properties of objects in astronomy! Having this "framework" will help you make sense of what otherwise must seem like an overwhelming number of isolated facts.
MESSAGE #64. Tue May 18 16:24:16. Jesse Ray wrote:
MESSAGE #63. Tue May 18 13:28:31. Prof. Doug Hamilton wrote:
Over the next several days we'll have a lot to do - homework #8, final section grades, and the last open house papers all need to be graded in addition to the final exam. Try to be patient! We should have most things graded and posted by the weekend.
Garett, I'm going to defer your question until after the final - but check back afterwards!
MESSAGE #62. Tue May 18 2:03:32. Garrett Cooper wrote:
MESSAGE #61. Mon May 17 19:48:10. Michelle Sutton wrote:
MESSAGE #60. Sat May 15 16:42:15. Prof. Doug Hamilton wrote:
Hints on short answer questions? I'll post some early next week after I've made the exam up!
Homework Solution Sets for #7 and #8 are posted under "Assignments"!
MESSAGE #59. Sat May 15 16:29:14. Prof. Doug Hamilton wrote:
The Alpha Centauri system is composed of three stars, two like our Sun and a third, Proxima Centauri, that is much less massive than the Sun. Proxima Centauri is the one nearest to us currently. We get some light (and some heat) from each of these stars, but it is an incredibly tiny amount. Take one of the sunlike stars as an example. I remember that the nearest stars are 7,000 times further away than Pluto is, and Pluto is 40 times further away than the Sun is. So Alpha Centauri is 280,000 times further away than the Sun. Remember this equation: F= L/4(pi)d2 ? If we assume that the Sun and one of the Alpha Centauri stars have the same Luminosity, L, we can use the different distances, d, to solve for the different Fluxes of light and/or heat, F. (280,000)^2 is 78,400,000,000. We get 78,400,000,000 times less light and heat from Alpha Centauri as from the Sun!!
The Sun experiences variations in its brightness that are millions of times larger than the amount of light and heat the we receive from Alpha Centauri. In fact, if a 3km asteroid moved between the Sun and the Earth, it would cause a larger variation!
MESSAGE #58. Fri May 14 10:53:06. Jennifer Plopa wrote:
MESSAGE #57. Fri May 14 10:44:28. Katrice Leach wrote:
MESSAGE #56. Fri May 14 10:32:34. Jason Ross wrote:
On our final, I know that you are giving us any equations that we need. But will we need to know the Units of the answer to the equations. Also could you give us a few hints on what the short answer questions will be.
Thanks Jason Ross.
MESSAGE #54. Mon May 10 15:39:08. Prof. Doug Hamilton wrote:
Nearby galaxies do not obey Hubble's law. Why? Well, first that is simply what observations of galaxies tell us: Hubble's law is observed to work only for distant galaxies. We can understand that observation by realizing that nearby galaxies are strongly tied together by their mutual gravity which keeps them from flying apart.
QUESTION 2: The Sun's magnetic field gives rise to the solar wind which can influence the upper atmosphere of the Earth (especially by creating auroras). Some people have argued that it can affect Earth's weather, but this is still controversial! It probably has a very small effect, but certainly is NOT responsible for noticeable large-scale weather patterns like el Nino and la Nina. The most important forces shaping Earth's weather are: 1) the Earth's rotation (this leads to spinning storm systems like hurricanes and tornados, and also the jet stream) and 2) solar heating (differences in temperatures drive strong winds).
MESSAGE #53. Mon May 10 10:53:25. Nisha Amin wrote:
Hi Dr. Hamilton I have a question about the Hubble law. First one is what has gravitation force got to do with the nearby galaxies and the units of Hubble constant (when using the formula to find the velocity), because it said in one of the chapters that hubble law just holds for far away and not for nearby galaxies. My second question is that I know Sun's magnetic field has something to do with the changes in the climate on the earth , but then how would that explain el nino and el nina. Is it the sun's gravity that causes this changes. I confused on this two things. thanks nisha
MESSAGE #51. Thu May 6 13:53:05. Prof. Doug Hamilton wrote:
Two bonus points for anyone who posts a message to the webpage! (You can only earn this once though!). Maybe we'll have some lively discussion here as the semestere winds down ....
MESSAGE #50. Wed May 5 11:03:21. Prof. Doug Hamilton wrote:
The sky is blue because of the way that air molecules scatter light. The Earth's atmosphere does a great job of scattering light - if light didn't scatter, all sunlight would come straight from the Sun and the sky would look black in all other directions. This happens on the Moon which has no atmosphere. On Earth, when you look up in the sky away from the Sun (don't look at the Sun - you'll fry your eyes out and die in agony!), you are seeing light that has come from the Sun and then been scattered off an atmospheric molecule, changing its direction of motion to come to your eyes.
Now, if the scattering objects (the air molecules) are smaller than the wavelength of light, then short wavelength blue light is scattered more efficiently than long wavelength red light. This type of scattering is called Rayleigh scattering. Since we are seeing scattered light when we look at the sky, the sky looks a lot bluer than sunlight.
So where is the red light? It is scattered too, but not as much. You see it when you look close to the Sun. This is especially noticeable when we look at the Sun near sunrise and sunset where the sunlight has to travel at a shallow angle through lots of Earth's atmosphere. The sky near sunrises and sunsets look distinctly red.
Small dust grains or water droplets can also scatter light like this. Sunsets are often even redder after volcanic eruptions blast lots of dust into our upper atmosphere. Also, note that the dust in the Milky Way galaxy causes stars to appear fainter and redder than they actually are for exactly the same reason given here.
MESSAGE #49. Wed May 5 10:39:43. Prof. Doug Hamilton wrote:
Sara - I don't have email for you. We haven't been able to locate your open house paper. Please come see me and bring an extra copy of your paper.
MESSAGE #48. Tue May 4 14:54:48. Sara Stoner wrote:
MESSAGE #47. Wed Apr 28 13:42:56. Keisha Stewart wrote:
MESSAGE #46. Wed Apr 28 13:41:21. Keisha Stewart wrote:
But enough venting, I'm a little behind. I'm still on Chapter 12 because it's more difficult for me (being that I'm a senior journalism major and by this time, math and science deficient). Can someone give me any tips for remembering and applying these formulas in Chapter 12?? Or maybe some kind of word game I can play with myself to remember the whole point of the equations??
MESSAGE #45. Tue Apr 27 14:01:46. Prof. Doug Hamilton wrote:
In the meantime, is anyone else finding any new Solar Systems out there?
You might be interested in a new tool "The Satellite Viewer" which allows you to watch a planet's moons as they orbit. Take a look at http://janus.astro.umd.edu/solarsystem.html and let me know what you think!
MESSAGE #44. Mon Apr 26 1:35:48. Tomeka Reid wrote:
MESSAGE #43. Thu Apr 22 11:28:16. Darryl Butler wrote:
Sincerely your friend DJ Butler
MESSAGE #42. Thu Apr 22 11:20:08. Darryl Butler wrote:
Oh yeah and my question: What is the deal with this new solar system Hamilton? How come nobody discovered this before me? I mean these planets are huge like 3 times the size of Jupiter
MESSAGE #41. Sat Apr 17 11:40:21. Gregg Aronson wrote:
MESSAGE #40. Sat Apr 17 0:05:25. Gregg Aronson wrote:
MESSAGE #39. Thu Apr 15 22:07:30. Yue Cao wrote:
and there is going to be a lot of multiple choice questions on what's the biggest, smallest, longerest day, longerest year, hottest, most massive, ...
the above are just my guess, hopefully intelligent ones and close to what Dr. Hamilton's view. ^_^. good luck to us all..
Jason
MESSAGE #38. Thu Apr 15 19:34:54. Prof. Doug Hamilton wrote:
The test has 25 multiple choice questions and seven short answer questions. Two of the seven question have a part a) and part b).
There is one question which involves an equation.
I think that the exam is a little easier than the last one! Some of the multiple choice questions have only 4 choices, so it is a little easier to find the correct answer.
Good Luck Tomorrow!!
MESSAGE #37. Thu Apr 15 11:34:08. Prof. Doug Hamilton wrote:
Kenneth, I'll be happy to give you an explanation for why the sky is blue, but I'd rather another student try to explain it first! Can anyone help?
EXAM HINTS!!! (as promised)
I will not emphasize the chapter on the Sun as much as the other chapters (no short answer questions on the Sun, and only 2 or 3 multiple choice questions). I'll ask only about the simple but important points, and I won't ask about the details of the solar cycle which is pretty complicated!
I'm making up the exam right now, so stay tuned for more hints!!
MESSAGE #36. Wed Apr 14 20:26:23. Kenneth Wood wrote:
MESSAGE #35. Wed Apr 14 20:25:31. Kenneth Wood wrote:
MESSAGE #34. Mon Apr 12 17:32:00. Angela Bettick wrote:
MESSAGE #32. Fri Apr 9 13:20:02. Prof. Doug Hamilton wrote:
It turns out that the book is wrong on the number of moons for both Saturn and Uranus. Saturn and Uranus have 18 and 17 known moons, respectively, (as I said in class) -- not 22 and 15 as stated on Arny page 221. For Uranus, the discrepancy is clear: two new moons of Uranus were discovered in 1997! Actually, two of the discoverers of those moons were my thesis advisors at Cornell! Arny noted the discovery in a footnote on page 221, but forgot to increase his number of Uranian moons by two. I don't know where his 22 moons of Saturn came from though - it's just wrong!
On the exams, I won't ask you exactly how many moons the giant planets have, since these numbers will probably increase in the future as new moons are discovered. How moons formed, and some of the details about the more famous ones are fair game, though!
MESSAGE #31. Fri Apr 9 11:47:59. Karla Cabrera wrote:
I have a small doubt about the number of moons that some of the Jovian planets have. In the book on page 221, it says that Saturn has 22, and that Uranus has 15. However, in the notes I took in class on March 19th, you said that Saturn has 18 moons and that Uranus has 15 (chart). Which inofrmation is correct and which information should I know and memorize for the exam? Thanx.
Karla Cabrera Sect 204
MESSAGE #30. Fri Apr 9 11:47:12. Karla Cabrera wrote:
I have a small doubt about the number of moons that some of the Jovian planets have. In the book on page 221, it says that Saturn has 22, and that Uranus has 15. However, in the notes I took in class on March 19th, you said that Saturn has 18 moons and that Uranus has 15 (chart). Which inofrmation is correct and which information should I know and memorize for the exam? Thanx.
Karla Cabrera Sect 204
MESSAGE #29. Fri Apr 2 17:20:08. Gregg Aronson wrote:
MESSAGE #28. Thu Apr 1 12:54:08. Prof. Doug Hamilton wrote:
MESSAGE #27. Sat Mar 20 18:37:56. Prof. Doug Hamilton wrote:
MESSAGE #26. Fri Mar 19 10:55:09. Prof. Doug Hamilton wrote:
MESSAGE #25. Thu Mar 18 23:14:07. Timothy Wendland wrote:
MESSAGE #24. Wed Mar 10 20:33:44. Courtney Britt wrote:
MESSAGE #23. Wed Mar 10 14:31:06. Prof. Doug Hamilton wrote:
MESSAGE #22. Mon Mar 8 11:04:37. Nidhi Sarin wrote:
MESSAGE #21. Sun Mar 7 18:55:02. Jason Robshaw wrote:
MESSAGE #20. Fri Mar 5 10:13:45. Prof. Doug Hamilton wrote:
Response to MSG #19: The problem is that I've set up the web site so that many different classes - not just ASTR100 - can use the scientific notation page (and the other tools as well). Some other classes at other colleges even use my site. It is not easy to have links that send you back to where you came from! There are some things that I can do to make this easier though - I'll look into it.
MESSAGE #19. Fri Feb 26 2:00:07. Samuel Smith wrote:
MESSAGE #18. Wed Feb 24 21:59:42. Angela Ricciuti wrote:
MESSAGE #17. Tue Feb 23 19:27:21. Michelle Sutton wrote:
MESSAGE #16. Mon Feb 22 14:29:34. Nidhi Sarin wrote:
MESSAGE #15. Mon Feb 22 14:28:10. Nidhi Sarin wrote:
MESSAGE #14. Thu Feb 18 20:05:20. Prof. Doug Hamilton wrote:
MESSAGE #13. Thu Feb 18 19:57:22. Prof. Doug Hamilton wrote:
For the Moon to be a thin crescent, it must be almost between the Earth and the Sun like this (distances are inaccurate!): S M E. Why? At all times, exactly half of the Moon is in sunlight. So if we see only a thin lit crescent from Earth, most of the sunlit part of the Moon must face away from Earth. This occurs only when the Moon is nearly between the Sun and the Earth.
So answer A is correct: the Moon is closer to the Sun than the Earth is. Since the Sun and Moon are nearly in the same direction as seen from Earth, they will set just a few hours apart. Since the crescent Moon is visible at sunset, it must set soon: answer B is correct.
Finally, the Moon is full when the Earth is roughly between the Sun and the Moon, i.e. the object are in this configuration: S E M. The Moon takes about 4 weeks to go around the Earth, so it takes about two weeks to go from new Moon to full Moon. It takes just a little less time because it is just after new Moon (You need to draw a better picture than I can here to show this - Try it!). So answer F is also correct. All other answers are incorrect.
Correct answers are: A B F
MESSAGE #12. Mon Feb 15 15:25:32. Joseph Simons wrote:
MESSAGE #11. Sun Feb 14 14:27:23. Yue Cao wrote:
MESSAGE #10. Sun Feb 14 12:51:47. Kevin Marchbanks wrote:
MESSAGE #9. Sun Feb 14 11:14:01. Yue Cao wrote:
Jason
MESSAGE #8. Sat Feb 13 15:40:55. Prof. Doug Hamilton wrote:
Today the Moon is just before new Moon. It won't be easily visible for another week or so because, as seen from Earth, the Moon is roughly in the direction of the Sun. The Moon will become visible at the end of next week just after sunset. It will first appear as a very thin crescent near where the Sun dips below the horizon. With each passing day, the lit part of the Moon will become larger, and the Moon will set later and later. Watch for the Moon in the evenings just after it gets dark! You can see its phase and position against the stars change from one night to the next.
MESSAGE #7. Sat Feb 13 13:46:20. Jesse Ray wrote:
MESSAGE #6. Fri Feb 12 18:13:17. Andrea Jordan wrote:
MESSAGE #5. Thu Feb 11 10:07:32. Angela Ricciuti wrote:
MESSAGE #4. Thu Feb 11 0:44:58. Angela Bettick wrote:
MESSAGE #3. Wed Feb 10 12:25:40. Terry Gray wrote:
MESSAGE #2. Mon Feb 8 15:51:24. Prof. Doug Hamilton wrote:
In order to encourage class participation on this site, I'll credit you 2 extra credit points at the end of the semester if you post a well-reasoned message (question, answer, etc.) on this bulletin board at least once during the course of the semester! What I want to encourage most is that you use this page as a way to communicate with other students in the class. You can learn a lot from each other!
Here's an Earth-Moon-Sun question to get you started. It requires visualizing the relationship between the three bodies. Try drawing a picture!
You see a very thin crescent moon in the evening just after sunset,
which of the following statements is true right then? Why?
A. The Moon-Sun distance is smaller than the Earth-Sun distance
B. The Moon will set in just a few hours
C. The Moon is at its highest point in the sky
D. The Moon will be visible all night
E. The Moon will be full in about 5 days
F. The Moon will be full just under two weeks
G. The Moon will be full in just over two weeks
H. The Moon will be full in just over three weeks
I. There will be a solar eclipse soon
J. There will be a lunar eclipse soon
K. The Moon will slam into the Earth and blast it to pieces
This is much harder than the typical questions that I will ask on exams, because there are lots of possible answers and more than one of them is correct! It is a good question for discussion, though. Can you argue that one of the answers has to be right (or wrong?)?
MESSAGE #1. Sun Feb 7 0:34:02. Prof. Doug Hamilton wrote:
HINT for Intro, problem 7: The speed of light in meters per second can be found in the Intro. Convert this to km per second (km/s) using the fact that there are 1000 meters in a kilometer. Now you'll need the distance from the Sun to Pluto in kilometers. Use Table 1 and the definition of the AU from problem 2.
Remember to turn the homework in at the BEGINNING of class Monday Feb. 15! No credit is given for late homework!!