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11.2b The Solar System Asteroids and Gas Giants
11.2b The Solar System Asteroids and Gas Giants

... water, ammonia and methane. Uranus has small icy/rocky core, a hot fluid mantle and gas atmosphere that is 83% hydrogen, 15% helium and 2 % methane. The methane gas is mostly in the upper atmosphere and gives the planet a blue look because it absorbs red from the sunlight falling on it. The hot liqu ...
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... Other variations relate to oxygen fugacity. Since H2 is the principal reductant and it dominates the gas, while O constitutes a significant fraction of condensed matter, variation in oxygen fugacity most likely reflects variation in the ratio of gas to dust. In addition, there must have been signifi ...
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... ● The solar system is made up of both inner and outer planets. The inner being closer to the Sun and the outer further away. ● The inner planets are referred to as the terrestrial planets because their composition is rocky like the Earth. ● They receive more of the Sun’s energy and have higher tempe ...
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SCI 103

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384 kb

... other essential materials for life. This discovery, when it comes, could have a fundamental and permanent impact on humanity: Where do we come from? What are we? People on this globe might even seriously consider a situation like that described in Carl Sagan’s novel Contact.” Other predictions for 5 ...
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... 46. The sidereal drive on a telescope mount38. If source A emits radio waves at a frequency ing turns the telescope westward about the polar 4 times that of source B, then the wavelength of axis to remain pointed toward a distant object. radio waves from A is (T) a. the same as that from B b. 16 tim ...
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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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