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AstroLesson4Slides
AstroLesson4Slides

... Can you understand why Ptolemy saw the Earth as the center of the Universe based on what you can see of the Sun, the Moon, and the stars? What major shift occurred with the Copernican view of the Universe? ...
Homework 2 (Due Sept 18, 2014)
Homework 2 (Due Sept 18, 2014)

... this chamber, a feather would fall at the same rate as a rock.! c. When an astronaut goes on a space walk outside the Space Station, she will quickly ! float away from the station unless she has a tether holding her to the station.! d. If the Sun were magically replaced with a giant rock that had pr ...
Our Solar System
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8.1 Touring the Night Sky Pg. 308 #1
8.1 Touring the Night Sky Pg. 308 #1

... 1. Astronomers study what is beyond Earth like stars, planets, and moons, solar systems, even other galaxy’s. 2. Being “luminous” means to have, produce or give off light. For example, the nuclear fusion on the light gives off light that shines on the earth. 3. The Moon reflects light from the sun w ...
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Unit 3 - Section 8.9 2011 Celestrial Objects from Earth
Unit 3 - Section 8.9 2011 Celestrial Objects from Earth

... The word retrograde applies to the apparent backward motion of a planet. An old encyclopedia of astrology describes this retrograde motion as "…the effect of a slow-moving train as viewed from another train traveling parallel to it but at a more rapid rate, wherein the slower train appears to be mov ...
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PowerPoint Presentation - Small Bodies in the Solar System

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Distribution of Elements in the Earth`s Crust

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... d. There is evidence that more than one planet or moon may have had liquid water. e. it is estimated to be slightly less than 5 million years old. 36. If two objects of the same density are formed at the same radius from the sun, which object is likely to remain geologically active longer? a. the sm ...
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Astronomy Notes
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... Giants and Supergiants 8. _____________________ - heats up enough to begin the next fusion step 9. _______________________ - for an unknown reason the core then continues to heat up 10. ______________________ - Energy wave from the core of the very massive star shoots outward overcoming gravity; the ...
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Early Observers (The Beginnings of Astronomy)
Early Observers (The Beginnings of Astronomy)

... Planets traveled in smaller circular paths as they traveled around the Earth (epicycles and deferents) Popular model of universe for 1,500 years. ...
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Foundations of Astronomy Presentation

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Geocentric vs. Heliocentric
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Neptune and Beyond, Asteroids, Comets
Neptune and Beyond, Asteroids, Comets

... But away from the Sun, beyond Neptune in coldest regions of the nebula, the density was low that planetesimals could not grow very large. They ended up like loosely packed dirty snow balls, most few kilometers in size. They became the family of Kuiper belt objects located in the region 30-50 AU from ...
Gravity in the Solar System Quiz
Gravity in the Solar System Quiz

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Email Template - Personal.psu.edu
Email Template - Personal.psu.edu

... Astro 001 Test #3 fall 2002 Name_____________________ Sect_____ 100 points = 100% Estimated to be this test: (1) (four points) If you were classifying the planets by size only, you might make three classes. What planets would be in each class? ...
Chapter 0
Chapter 0

... A planet has 4 times the mass of the earth, but the acceleration due to gravity on the planet’s surface is the same as on the earth’s surface. The planet’s radius is ...
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Comparative planetary science

Comparative planetary science or comparative planetology is a branch of space science and planetary science in which different natural processes and systems are studied by their effects and phenomena on and between multiple bodies. The planetary processes in question include geology, hydrology, atmospheric physics, and interactions such as impact cratering, space weathering, and magnetospheric physics in the solar wind, and possibly biology, via astrobiology.Comparison of multiple bodies assists the researcher, if for no other reason than the Earth is far more accessible than any other body. Those distant bodies may then be evaluated in the context of processes already characterized on Earth. Conversely, other bodies (including extrasolar ones) may provide additional examples, edge cases, and counterexamples to earthbound processes; without a greater context, studying these phenomena in relation to Earth alone may result in low sample sizes and observational biases.
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