Chinese Lunar Rover • 15Dec2013 First soft landing since 1976 • Chinese lunar rover still functioning but can’t move • • • • Moon 1 light second= 17days in a 747= 4days in Apollo 11 Moon is ¼ Earth’s diameter= 1/64 Earth’s volume BUT mass is 1/80 Earth’s mass so density 3.3gm/cc Rock=3 so no/small iron core=9gm/cc No Atmosphere • No Atmosphere => no erosion by wind/water • No air to moderate so Maximum temperature +123C & min -233C Surface Features: Mare (=sea) • Maria =Lowlands composed of dark basalt shown in blue • Far side of Moon has thicker crust so no mare • Lunar Highlands (Terrae): heavily cratered light colored rock in green Craters Copernicus and Tycho • Bowl shaped depressions caused by impacts • Rays, ejecta blankets, secondary craters • From ~100’s km across to microscopic Impact Crater Formation • • • • • Impactor has velocity 10 times rifle bullet Releases energy 10 times equal mass of dynamite Impactor vaporized when temperature reaches millions K Shock wave forms shocked quartz found only in impacts Rebound can launch rocks without destroying them Largest Impacts - Mare Orientale • Few large and far more small craters • Terminator separates day from night where shadows emphasize surface roughness Cratering History of the Moon • Radioactive dating of Lunar samples gives absolute age • Counting density of craters on surface gives relative age • Older surfaces have more craters • Can be extended throughout solar system Lunar Dust • • • • Regolith = crushed rock/dust; depth of a few meters Sharp edged black dust clings to suits -not like Earth dust Erosion: micrometeorites erase boot prints in millions years Breccias= rocks glued with glass from impacts Water on the Moon? • • • • • Regolith contains no H2O, but Few polar craters always in shadow Impacted by LCROSS 2009 Dust/gas plume shows water, OH… Important for future colonists? Volcanism - Hadley Rille • 150km long, 1.5km across, 300meters deep • Formed by flowing lava 3.3 billion years ago • Vesicular basalt from moon (gas bubbles) Formation of the Moon 1. Fission – Protoearth spun so fast that the moon budded off - but wrong angular momentum 2. Coformation (co-creation): formed near Earth from nebula - but small iron core & low volatiles 3. Capture: formed somewhere else- wrong oxygen isotopes + hard to capture + no iron or volatiles 4. Impact Theory=Collisional Ejection: Earth hit by Mars sized asteroid Impact Theory of Formation of Moon • Elapsed time is about 24 hours; moon forms in a year • Earth ends up spinning once in 5 hours, moon in low orbit • Earth was differentiated so moon is made from mantle material • Correct isotope ratio, no iron core, volatiles evaporate, • Robin Canup’s simulation “Eagle Has Landed” • Apollo 11 lands in Mare Tranquillitatis • Neil Armstrong & Buzz Aldrin • 20 July 1969 “One Small Step” • Neil Armstrong 20 July 1969 Hammer and Feather • 6 Moon missions &12 astronauts • A week to get there • Apollo 15 and Surveyor 3 Apollo 16 Moon Rover Last Man on the Moon? 1972 • Moon Rock at Cape Kennedy Which if any, of the following is incorrect? a. We know the Moon’s Maria are a younger terrain since they have fewer craters than the highlands. b. Neil Armstrong first set foot on the moon 1969. c. The moon is smaller than the Earth so we would expect it to have a cooler core. d. The density of the moon is less than the Earths’ so we expect it to have a smaller iron core e. All of these are correct When did the first man, Neil Armstrong, land on the moon? 20 July ___ a) 1609 b) 1959 c) 1969 d) 1979 e) 1989 Fox TV • No stars: Not enough exposure Moon Hoax • Illuminated astronaut: bright background • Parallel shadows: topography • Flag waving: no atmosphere so waved longer & liked it wrinkled Late Heavy Bombardment • Late Heavy Bombardment second surge in impacts • When Jupiter, Saturn, Uranus, Neptune change orbits scattering planetesimals? Rocky Surfaces Saturated with Craters • Planets formed from many meteorite impacts • Circular craters due to explosion caused by impact • Solar System “Full”? Erosion of Craters • Craters hidden by: 1. Volcanoes – lava flows 2. Continental drift 3. Erosion by atmosphere 4. Oceans Younger Terrain = Fewer Craters • The larger the terrestrial world; the more internal heat it will retain = higher temperature in core • The higher temperature; more geologically active so more craters are covered = fewer craters showing • Older terrains = more craters Rotation of the Moon • Revolves & rotates on axis in sidereal=27.3 d synodic=29.53d • Keeps one side facing the Earth = synchronous orbit/rotation • Moon & Earth orbit center of mass Internal Structure of the Moon • Seismic data from Apollo landers recording moonquakes from tides • Crust is thicker ~60km than Earth’s ~10km • Mantle 80% radius • Core <25% Impact Crater • All lunar craters seem to be impact craters not volcanic – no plate tectonics Giant Impactor • Painting by Kaufmann • Problem of the low density of the Moon • Solved by Moon being formed from low density mantle material • Is it Science? Testable Prediction = Disprovable No Atmosphere = No Erosion But Ice at Mercury’s & Moon’s Poles? • • • • VLA radar observations see echo from poles which resembles ice Surface temperature 100K to 700K, but inclination of rotation axes 0º South Pole of Moon with craters permanently in shadow in white Hydrogen detected from neutron spectrometer on Lunar Prospector Lunar Impact