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SPACE MATHEMATICS WORKSHEET 1
SPACE MATHEMATICS WORKSHEET 1

... of sunspots can be used to determine the rotation speed of the Sun. As it turns out, the Sun's rotation is quite different from that of most of the planets. A rigid body such as the Earth will clearly have a single rotation rate. But since the Sun is made of gas, different parts of it rotate at diff ...
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... If you can spot Polaris in the sky, you can always tell which way is north. Because of this, Polaris was the most important star for navigating at sea. ...
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What are 2 motions of the Earth?

... earth revolves Observing the Sky: Motion of the Sun and Stars - The Night Sky around the 2) The Sun appears to be larger sun? during the winter months and smaller as summer approaches. • Perihelion – earth closest to the sun •Aphelion – earth furthest away from the sun ...
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Class 1 and 2 lecture slides (Solar System Formation)

... CH4 above 60K, and then condenses to CH4.6H2O. From Lissauer and DePater, Planetary Sciences ...
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... The tilt of the Earth also has on effect on the length of daylight. When you are tilted toward the Sun in the summer, the Sun rises higher overhead at noon. Days are longer with shorter nights . Longer days mean more hours the sunlight can heat the ground. In the w inter, the Sun is not as high in t ...
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29:52 Characteristics and Origins of the Solar System January 25

... The second of these lines is the ecliptic. The ecliptic is the projection of the Earth’s orbital plane on the celestial sphere. If we plotted up all the positions of the Sun against the background stars, it would trace out the ecliptic. Because of the 23.5 degree tilt of the Earth’s axis, the celest ...
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Grade 9 Unit 4: Space

... remains of the formation of the solar system pieces of rock floating through space pieces of rock that have entered Earth’s atmosphere ...
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PHS 111 Test 3 Review Chapters 26-28

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PHS 111 Test 3 Review Chapters 26-28

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... a radius of 6.4 cm. If you were to construct a scale model of the solar system using the rubber ball to represent the earth, what is the radius of a ball needed to represent the sun in your model? a. 7.0105 cm b. 7.0 cm c. 700 cm ...
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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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