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Moon Formation / Processes ) Cea ag eae te 1115 ‏علا‎ Saeed ow are they different?

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Earth Moon 7930 miles (12,756.3 km) 2160 miles (3476 km) olan ‏كيتكت‎ ‎23 degree axis tilt 7 degree tilt (~no (seasons!) seasons) Surface temps -73 to 48 C Surface temps - 107 C to (-100 to 120F) -153 C (224 F to -243 ۲) Thick atmosphere, mild greenhouse effect No atmosphere Liquid water - lots! - at

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Moon No Magnetic Field Small Moon Quakes Small, Offset Core Earth

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Earth’s Moon * How did our Moon form? * What's been happening since?

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A few data to ponder .... Lower density - “lighter” - relative to planets Less iron than whole Earth, more aluminum and titanium Moon's chemical signature ~ Earth’s mantle

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A few more data to ponder Does not orbit in equatorial plane of Earth, or ecliptic Earth/Moon - high angular momentum How Did the Moon Form?

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Lunar Formation Models The moon is a sister world that formed in orbit around Earth as the Earth formed. The moon formed somewhere else in the solar system then was captured into orbit around Earth. Early Earth spun so fast that it spun off the moon.

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Impact by Mars- ۶ ۲ 93 sized proto-planet NA ۱8 RAI 7 5 ‏سس‎ HISTORY ۹ 5اةعلا موأااتط 5. ‎ago‏ ۱34 TH « ۲۷ ‏*ززه و(‎ ¢ High angular momentum

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lorie ce mea

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ی

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Copyrighted, LPI

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Copyrighted, LPI

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Fetes ater a]

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Lunar Geologic History

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Lunar Geologic History ( , ها 4.5 billion years ago, our Moon 10۳۳5 (lunar rocks and meteorites) ی

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ام ,600۲96۵

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Magma Ocean Rocks 16535 Troctolite 4.2-4.3 03 ‎TE‏ ا ‎ ‎60025 ‎Anorthosite ‎4.44-4.51 Ga ‎excise icy ‎Magma Ocean! No Water! ‎

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Lunar Geologic History Highlands - light, rough (Terrae) Mostly anorthosite NOE elae eS feldspars - lots of calcium and aluminum) “In place” rocks are 4.5 to 4.3 billion years old Pe fe ee

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Lunar Impact Basins os 20 2 Imbrium Rim Orientale Big, frequent impacts until 3.8 billion yearBagyo Impact events continue on all moons and planets

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Breccias and Impact Melts 15445 Impact melt + clasts 67016 52

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Lunar Geologic History Mare Volcanism Volcanism afterimpacts - most before 3 Ga ‏مس راوع‎

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Lunar Volcanism Arist ‏ات9‎ } 9 Marius

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Lava Tubes

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Lunar Basalts

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‎Geologic Lowlands - dark,‏ لیگ ‎smooth Maria (16%)‏ ۱۱۱۷ ‎ ‎Basalt - fine grained dark igneous rock rich in iron and magnesium (stuff that sank in magma ocean) ‎Few hundred meters thick ‎Rocks are 4.3 to 3.1 billion years old ... volcanic flows as recently as 1 billion

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And then .... All was quiet.

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۱ 23 for impacts... 7 November; ~30 Ib TNT 3 m-wide crater (estimate)

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٠ ‏وواللا هلا‎ * No Flowing Water * No Erosion

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۱ 23 for impacts...

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~ ov are they different in terms of geologic processes? ۸۵00 ۰۶

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Moon © NO Active wind/water erosion Impacts NO active volcanoes Small moonquakes NO active magnetic field Buckets of craters Geologically Inactive! Earth Active wind/water erosion Impacts Active volcanoes Earthquakes Active magnetic field Few craters Geologically Active!

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Moon هه نكل ‎NO plate tectonics‏ عغوام ‎tectonics!‏ ‎

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Earth Moon © HOT! Not so hot! 04 وا ۱۵۰

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What’s Our Plan for Space? Fly the shuttle as safely as possible until 2010 Complete the ISS - 6- person crew by 2009 Align science, exploration, and aeronautics to support human space flight ات هت عط وصتي8 Exploration Vehicle - CEV - on line 17 عقون ج لاؤتاطقاوع ‎that informs future‏ ‎missions to Mars and other‏ وك

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Why? Set up, for the first time, a full-fledged habitat on another world. Test advanced spacesuits and rovers. Try out methods for protecting explorers from deadly radiation. Learn to operate crucial life support and power needed on Mars. Gauge the effects of the absence of normal gravity on the body. New technology.

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Return to the Moon “9 Chandryaan - 2007! LRO - 2008 ! Identify Resources ‏عع13 ناك عط مدال‎ لعا لاسي 1 ©

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Return to the Moon! E * 2012 - Develop and test technologies for resource utilization, communications, power ¢ 2014 - CEV, Ares launch » vehicle

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‎eens ES od‏ ل ل لان او سس ‎Oext:‏ * ‎

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