1 / 29

Survey of the Universe Tom Burbine tburbine@mtholyoke

Discover the wonders of celestial objects like the Moon, planets, and stars through their cycles, phases, eclipses, and historical astronomical models. Learn about lunar and solar eclipses, the phases of the Moon, and the ancient geocentric model of the universe. Explore the motion of planets, retrograde motion, and Ptolemy's model of the universe. Gain insights into how observations have shaped our understanding of the cosmos.

mcglone
Download Presentation

Survey of the Universe Tom Burbine tburbine@mtholyoke

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. Survey of the UniverseTom Burbinetburbine@mtholyoke.edu

  2. Moon, Planets, and Stars • All celestial objects appear to rise in the east and set in the west

  3. Moon • Besides the Sun, the Moon is the brightest object in the sky • The Moon reflects light from the Sun • Light areas are called highlands • Dark areas are called maria (huge impact basins filled with lava) http://sos.noaa.gov/datasets/solar_system/moon.html

  4. Cycle • The Moon’s changes in the sky follow a 29.5 day cycle • This is why each month has approximately 30 days

  5. Phases of the Moon-29.5 day cycle

  6. http://en.wikipedia.org/wiki/File:Lunar-Phase-Diagram.png

  7. Color of lunar eclipse • The Moon does not completely disappear because of the refraction of sunlight by the Earth’s atmosphere • If the Earth had no atmosphere, the Moon would be completely dark during an eclipse. • The red color arises because sunlight reaching the Moon must pass through the Earth’s atmosphere, where it is scattered. • Shorter wavelengths are more likely to be scattered by the small particles. By the time the light has passed through the atmosphere, the longer wavelengths dominate. This resulting light reflected from the Moon we perceive as red.

  8. Solar eclipse

  9. http://en.wikipedia.org/wiki/Image:Solar_eclips_1999_4_NR.jpghttp://en.wikipedia.org/wiki/Image:Solar_eclips_1999_4_NR.jpg • Solar eclipses occur approximately every 18 months • However, they recur (on average) at any given place only once every 370 years • Moon's umbra moves eastward at over 1,700 km/hr • Every year, there are at least two lunar eclipses. • Can be viewed anywhere on the night side of the Earth http://home.cogeco.ca/~astrosarnia/Photos/Lunar%20eclipse%20binocular.jpg

  10. http://www.explorelearning.com/index.cfm?method=cresource.dspexpguide&resourceid=556http://www.explorelearning.com/index.cfm?method=cresource.dspexpguide&resourceid=556

  11. Eclipses Moon is tilted at an angle of 5 degrees to Earth’s orbit

  12. Solar eclipse of July 22, 2009 • Lasted a maximum of 6 minutes and 39 seconds off the coast of Southeast Asia http://upload.wikimedia.org/wikipedia/commons/f/f2/Solar_eclipse_animate_%282009-Jul-22%29.gif http://en.wikipedia.org/wiki/File:Solar_eclipse_22_July_2009_taken_by_Lutfar_Rahman_Nirjhar_from_Bangladesh.jpg

  13. Solar eclipse of July 11, 2010 • Occurred over the Southern Pacific Ocean • Very remote • Seen over French Polynesia, the Cook Islands, and Easter Island

  14. Models • When you have a model of how something works, you should be able to predict what will happen • If observations do not fit the model, either the observations or the model is wrong • The ancient astronomers wanted to predict the positions of planets in the sky

  15. What did the ancients think • That the Earth was the center of the universe (geocentric model) • That the celestial sphere was rotating around the Earth • However, there was two observations that caused problems with this idea • Apparent retrograde motion • Inability to detect stellar parallax

  16. Greek model

  17. Motion of planets • Planets always appear to rise in the east and set in the west • But planets usually move from west to east past the stars • The exception is retrograde motion

  18. Figure 2.6

  19. Figure 2.7

  20. Apparent Retrograde Motion = “backward” motion

  21. Ptolemy’s (100-170 AD) Model of the Universe epicycle

  22. Occam’s Razor • The principle that generally recommends selecting the hypothesis that makes the fewest new assumptions

  23. Retrograde Motion

  24. Any Questions?

More Related