Exam 6: The Solar System: Comparative Planetology and Formation Models
Exam 1: Charting the Heavens: The Foundations of Astronomy94 Questions
Exam 2: The Copernican Revolution: The Birth of Modern Science100 Questions
Exam 3: Radiation: Information from the Cosmos102 Questions
Exam 4: Spectroscopy: The Inner Workings of Atoms94 Questions
Exam 5: Telescopes: The Tools of Astronomy102 Questions
Exam 6: The Solar System: Comparative Planetology and Formation Models151 Questions
Exam 7: Earth: Our Home in Space102 Questions
Exam 8: The Moon and Mercury: Scorched and Battered Worlds112 Questions
Exam 9: Venus: Earth's Sister Planet98 Questions
Exam 10: Mars: A Near Miss for Life?102 Questions
Exam 11: Jupiter: Giant of the Solar System101 Questions
Exam 12: Saturn: Spectacular Rings and Mysterious Moons104 Questions
Exam 13: Uranus and Neptune: The Outer Worlds of the Solar System108 Questions
Exam 14: Solar System Debris: Keys to Our Origin114 Questions
Exam 15: Exoplanets: Planetary Systems Beyond Our Own74 Questions
Exam 16: The Sun: Our Parent Star113 Questions
Exam 17: The Stars: Giants,Dwarfs,and the Main Sequence107 Questions
Exam 18: The Interstellar Medium: Gas and Dust among the Stars100 Questions
Exam 19: Star Formation: A Traumatic Birth108 Questions
Exam 20: Stellar Evolution: The Life and Death of a Star107 Questions
Exam 21: Stellar Explosions: Novae,Supernovae,and the Formation of the Elements104 Questions
Exam 22: Neutron Stars and Black Holes: Strange States of Matter113 Questions
Exam 23: The Milky Way Galaxy: A Spiral in Space105 Questions
Exam 24: Galaxies: Building Blocks of the Universe106 Questions
Exam 25: Galaxies and Dark Matter: The Large-Scale Structure of the Cosmos104 Questions
Exam 26: Cosmology: The Big Bang and the Fate of the Universe101 Questions
Exam 27: The Early Universe: Toward the Beginning of Time110 Questions
Exam 28: Life in the Universe: Are We Alone?105 Questions
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Describe how the observable properties of the solar system are related to its process of formation.
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All the orbital and rotational motions can be explained as preserving the original rotation of the nebula from which the solar system formed.Accretion explains planetary isolation.Temperature differences explain differentiation.Asteroids and comets are left over debris.And irregularities can be explained by collisions during the planetesimal era.
What support for the solar nebula theory has come from observations of nearby young stars?
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Many show dusty disks,with large infrared excesses,forming around the stars' equators as the stars condense.In some cases,these disks are seen as dark profiles in front of the star,such as in the Orion Nebula.
At what point does the accretion process turn a clump of debris into a planetesimal?
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The average density of each planet in the solar system is determined by taking its mass and dividing that by its:
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Jupiter and the other jovian planets may have formed significantly closer to the Sun than their current orbits.
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What are the properties of the Sun that any theory of the origin of the solar system must explain?
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All of the jovian planets rotate more rapidly than any of the terrestrial planets.
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The ________ theory describes the origin of the planets as having been formed by accretion of small particles into progressively larger and larger bodies.
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________ is the only planet with a mean density less than water.
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By itself,________ makes up 70% of the masses of all the planets combined.
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One possible way that future scientists may determine whether the core-accretion model or the gravitational instability theory better explains the formation of the jovian planet is:
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What aspects of the planets orbits are nearly the same for most planets?
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