1 / 19

LECTURE 3, AUGUST 31, 2010

LECTURE 3, AUGUST 31, 2010. ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu. Question 10. a) distances to stars increase. b) the baseline gets larger. c) the baseline gets smaller. d) the Earth moves faster in its orbit. The angle of parallax increases as. Question 10.

novia
Download Presentation

LECTURE 3, AUGUST 31, 2010

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. LECTURE 3, AUGUST 31, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu ASTR 101-3, FALL 2010

  2. ASTR 101-3, FALL 2010

  3. ASTR 101-3, FALL 2010

  4. ASTR 101-3, FALL 2010

  5. ASTR 101-3, FALL 2010

  6. Question 10 a) distances to stars increase. b) the baseline gets larger. c) the baseline gets smaller. d) the Earth moves faster in its orbit. The angle of parallax increases as

  7. Question 10 a) distances to stars increase. b) the baseline gets larger. c) the baseline gets smaller. d) the Earth moves faster in its orbit. The angle of parallax increases as The greater the distance between two observation points (the baseline), the larger the angle of parallax.

  8. ASTR 101-3, FALL 2010

  9. Question 12 a) the same phase in 24 hours. b) different phases in 24 hours. c) a lunar eclipse once a month. d) different sides of the Moon. Considering the Moon’s phases, everyone on Earth sees

  10. Question 12 a) the same phase in 24 hours. b) different phases in 24 hours. c) a lunar eclipse once a month. d) different sides of the Moon. Considering the Moon’s phases, everyone on Earth sees The Moon goes through its cycle of phases in about 30 days; the Earth rotates once in only 24 hours. So everyone has a chance to see the same phase!

  11. ASTR 101-3, FALL 2010

  12. Question 7 a) during the new moon phase. b) when the Sun blocks the Moon. c) during the full moon phase. d) always around the summer solstice. A total lunar eclipse occurs

  13. Question 7 a) during the new moon phase. b) when the Sun blocks the Moon. c) during the full moon phase. d) always around the summer solstice. A total lunar eclipse occurs

  14. ASTR 101-3, FALL 2010

  15. ASTR 101-3, FALL 2010

  16. ASTR 101-3, FALL 2010

  17. Question 9 a) every month at new moon. b) every week at the quarter phases. c) every month at full moon. d) about every six months at new moon. e) every year at new moon. A solar eclipse happens

  18. Question 9 a) every month at new moon. b) every week at the quarter phases. c) every month at full moon. d) about every six months at new moon. e) every year at new moon. A solar eclipse happens

  19. ASTR 101-3, FALL 2010

More Related