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EAPS 105 Exam 3 Units 7–9 Questions & Answers 2026 | 180+ Practice Questions | Planetary Atmospheres, Mars, Asteroids, Comets, Moons & Planetary Rings | Purdue University

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This comprehensive EAPS 105 Exam 3 Units 7–9 study guide contains more than 180 carefully structured exam-style questions and verified answers covering planetary atmospheres, climate systems, planetary habitability, Mars exploration, asteroids, comets, Kuiper Belt objects, dwarf planets, moon formation, tidal interactions, planetary rings, and comparative planetology. Designed specifically for Purdue University's EAPS 105: Introduction to Planet Earth course, this resource serves as an essential preparation tool for Exam 3, unit assessments, cumulative finals, quizzes, and astronomy-focused coursework. The document begins with an in-depth examination of planetary atmospheres and atmospheric evolution throughout the Solar System. Students review the composition of primary atmospheres, atmospheric escape processes, escape velocity calculations, atmospheric retention mechanisms, greenhouse warming, atmospheric pressure variations, and the major differences between Earth, Venus, and Mars. Particular emphasis is placed on understanding why terrestrial planets evolved dramatically different climates despite originating from similar primordial materials. The guide explores atmospheric chemistry, planetary temperature regulation, greenhouse gas behavior, atmospheric layers, cloud formation, and planetary weather systems that influence planetary habitability. A substantial portion of the material focuses on climate science and planetary habitability. Students gain a strong understanding of Earth's greenhouse effect, albedo feedback mechanisms, Milankovitch cycles, climate change drivers, atmospheric circulation patterns, and the scientific factors that make Earth uniquely capable of supporting complex life. Topics include the role of liquid water, magnetic fields, plate tectonics, atmospheric composition, ozone protection, and orbital stability in sustaining long-term biological evolution. Comparative analyses of Venus' runaway greenhouse effect and Mars' atmospheric loss provide critical insights into planetary climate evolution and environmental change. The guide also provides extensive coverage of Mars and the search for extraterrestrial life. Students examine evidence for ancient rivers, lakes, oceans, deltas, permafrost deposits, and past climate conditions that may have supported habitable environments. The material reviews rover missions, Jezero Crater exploration, Martian geology, water preservation mechanisms, and the scientific methods used to search for biosignatures and evidence of ancient microbial life. These concepts align closely with current NASA exploration objectives and modern astrobiology research initiatives. Advanced sections focus on asteroids, comets, dwarf planets, and the outer Solar System. Learners explore asteroid classifications, regolith formation, asteroid belt dynamics, Kirkwood gaps, asteroid composition, cryovolcanism on Ceres, Vesta's protoplanetary characteristics, comet nuclei, comet tails, dust jets, Kuiper Belt objects, Oort Cloud formation, meteor showers, and the discoveries of NASA's New Horizons mission. The resource also examines Pluto's reclassification debate, the International Astronomical Union's planetary definition, and emerging evidence for a potential ninth planet in the outer Solar System. The final portion of the guide covers natural satellites, moon formation theories, giant impacts, tidal evolution, orbital dynamics, planetary rings, Roche limits, and the major moons of Jupiter, Saturn, Neptune, and Pluto. Students learn how moons form through accretion, capture, and impact processes while exploring unique worlds such as Io, Europa, Ganymede, Callisto, Titan, Enceladus, Triton, Charon, Phobos, and Deimos. The material further explains ring formation processes, tidal migration, orbital resonances, and the long-term evolution of planetary satellite systems throughout the Solar System. Key Topics Covered: • Primary and Secondary Atmospheres • Atmospheric Escape and Escape Velocity • Atmospheric Retention Mechanisms • Earth, Venus, and Mars Atmospheric Evolution • Greenhouse Effect and Climate Science • Greenhouse Gases and Global Warming • Albedo and Climate Feedbacks • Milankovitch Cycles • Atmospheric Layers and Weather Systems • Planetary Habitability Requirements • Habitable Zone Theory • Mars Climate History • Ancient Water on Mars • Jezero Crater and Astrobiology • Mars Rover Missions • Giant Planet Atmospheres • Jupiter's Great Red Spot • Uranus and Neptune Atmospheric Dynamics • Asteroids and Asteroid Belt Structure • Kirkwood Gaps and Orbital Resonances • C-Type Asteroids • Vesta and Ceres • Comets and Comet Tails • Kuiper Belt Objects • Oort Cloud Formation • Meteor Showers • Pluto and Dwarf Planet Classification • New Horizons Mission Discoveries • Planet Nine Hypothesis • Moon Formation Theories • Giant Impact Hypothesis • Galilean Moons • Titan, Triton, Enceladus and Charon • Tidal Forces and Orbital Evolution • Roche Limit and Ring Formation • Saturn's Rings and Ring Dynamics • Comparative Planetology According to Planetary Sciences by Imke de Pater and Jack J. Lissauer, The New Solar System (Beatty, Petersen & Chaikin), and peer-reviewed research published in Icarus, Nature Astronomy, The Astrophysical Journal, Science, and Annual Review of Earth and Planetary Sciences, planetary atmospheres, climate systems, small Solar System bodies, moons, and ring systems provide critical evidence for understanding planetary formation and evolution. Modern planetary science integrates astronomy, geology, atmospheric physics, astrobiology, and orbital dynamics to investigate how planets and satellites develop, maintain habitable environments, and evolve over billions of years. The concepts covered throughout Units 7–9 represent foundational learning outcomes in university-level planetary science and Earth-space science curricula. Relevant for: EAPS 105 Students Introduction to Planet Earth Students Planetary Science Students Earth and Atmospheric Sciences Students Astronomy Students Astrobiology Students Climate Science Students Planetary Geology Students Space Science Students Environmental Science Students STEM Undergraduates Physical Science Students General Education Science Students Mars Exploration Students Planetary Atmospheres Students Solar System Science Students Exam 3 Preparation Students Final Exam Review Students Undergraduate Science Majors Comparative Planetology Students Keywords EAPS 105 Exam 3, EAPS 105 Units 7 9, EAPS 105 answers, planetary atmospheres, atmospheric evolution, greenhouse effect, greenhouse gases, climate change, global warming, albedo, Milankovitch cycles, planetary habitability, habitable zone, Mars atmosphere, ancient water on Mars, Jezero Crater, Mars rover missions, astrobiology, asteroid belt, Kirkwood gaps, C type asteroids, Vesta, Ceres, cryovolcanism, comets, comet tails, Kuiper Belt, Oort Cloud, meteor showers, Pluto, dwarf planets, New Horizons mission, Planet Nine, moon formation, giant impact hypothesis, Galilean moons, Titan, Enceladus, Triton, Charon, Roche limit, planetary rings, comparative planetology, Purdue University EAPS 105

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Eaps 105 Exam 3 Units 7-9
2026 Exam Questions and
Answers | Already Graded A+



main components of a primary atmosphere - ANSWER ✔✔hydrogen

& helium


factors that influence escape velocity of a planet - ANSWER ✔✔mass

of planet: greater the mass, higher the velocity needed to escape

,radius of planet: greater the radius, lower the velocity needed to escape

gravity (center of planet is farther away)


factors that influence gas molecule velocities - ANSWER

✔✔temperature: the higher the temp, faster it moves


atomic weight: lighter the molecule, faster it moves


the gases that should be retained by Mar's atmosphere - ANSWER

✔✔carbon dioxide


how the earth obtained most of the oxygen in its atmosphere -

ANSWER ✔✔life (microbes) converted most of the CO2 into O2


the major differences between the atmospheres of earth & venus -

ANSWER ✔✔venus: hot sun burned off all water vapor, causing CO2

to be released from rocks.

-its atmosphere is 90x greater than earths

earth: life converted CO2 into O2

the major differences between the atmosphere of venus and mars -

ANSWER ✔✔venus: atmosphere is 15,000x denser than that of Mars


-has sulfuric acid clouds

mars: 1.5% argo, venus is <1%

, the major reason why there is no liquid water on the surface of mars

today - ANSWER ✔✔atmosphere is too thin to enable water on its

surface regardless of temp


the history of water on the surface of mars - ANSWER ✔✔billions of

years ago there was a thicker atmosphere and a lot of water


the duration of water on mars in its past - ANSWER ✔✔we don't

know

where all the water that used to be on the surface of Mars disappear to -

ANSWER ✔✔mars has an ocean's worth of water trapped as ice

beneath the surface (permafrost)


the primary cause of Earth's seasons - ANSWER ✔✔tilt of the Earth's

axis

consequences of uranus spinning on its side regarding its seasons and

lengths of days - ANSWER ✔✔extreme seasons : 21-year-long

summers are one long day and 21-year-long winters are one long night

how the layers of terrestrial planetary atmospheres are defines -

ANSWER ✔✔by where they switch from cooling with altitude to

heating




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