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solar system formation and gal
solar system formation and gal

... • Over time it flattens into a disc-like shape while spinning in one direction • Astronomers theorize that any planets forming during this phase would form in the same flat plane and would rotate and revolve around the star in the same way • Using technology, astronomers have discovered flattening n ...
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... The next major obstacle is that the charts that astrologers use are hopelessly out of date. When they were originally drawn, the sun may have risen in a given constellation. However, due to a change over time of the earth’s axis of rotation, the sun does not rise in those constellations that your bi ...
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... Charles Messier – charts nebulous objects in sky mistaken for comets Kepler’s laws of planetary motion – allow relative distances between planets and sun to be determined (but not absolute / actual distances) Astronomical Unit – Earth Sun distance Parallax method for determining distance – how does ...
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Correspondence Course Form - The Indian Planetary Society

... Make crossed Cheque / Draft / Postal Order payable to The Indian Planetary Society. Please do not send Money Order or give the amount in cash. All the course material will be sent to you. You should complete all the assignments and send them to us. ...
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... • White dwarfs are only about the size of Earth, but they have about as much mass as the sun. • Since a white dwarf has the same mass as the sun but only one millionth the volume, it is one million times as dense as the sun. A spoonful of material from a white dwarf has as much mass as a large truc ...
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... mass-radius relationship. This is that The higher the mass, the smaller the radius, thus no stable white dwarf can exist. White dwarfs evolve from other stars with three, four, sometimes higher solar masses. It then swells to a red giant, and expels its outer layer in an incredibly catastrophic even ...
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... burning in the core has stopped? How? (20pt) (Hint: What particles that are generated by the fusion of hydrogen can escape from the interior of the Sun immediately?) 2. Chapter 11, Review Question 7. What is the defining characteristic of a main-sequence star? How is surface temperature related to l ...
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