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Published byJemima Shaw Modified over 9 years ago
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Terrestrial Planets Mercury Venus Earth Mars Source of images Planetary photojournal: http://photojournal.jpl.nasa.govhttp://photojournal.jpl.nasa.gov
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Mercury ☿ Mean radius 2439 km = 0.38R E Mass 3.3 ˣ 10 23 kg = 0.055M E Mean density 5427 kg/m 3 Rotation period 58.646 d (length of day) Orbital period 88 d (length of year) → 3:2 spin – orbit resonance Sun distance ~0.387 AU http://messenger.jhuapl.edu/ Mercury Volcano
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Inner structure 1 Crust 100 – 200 km 2 Mantle -600 km Nucleus – 1800 km Core ~42% of volume Higher iron content than any other planet
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Mercury surface map All images: NASA & JHUAPL Messenger Mission
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Mercury Kepler Debussy Pantheon Fossae Impact ejecta spokes
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Venus Mean radius 6051 km = 0.949 R E Mass 4868 ˣ 10 24 kg = 0.815 M E Mean density 5204 kg/m 3 Rotation period -243 d Orbital period 224.7 d Sun distance ~0.7 AU Surface pressure 93 bar http://nssdc.gsfc.nasa.gov/planetary/factsheet/venusfact.html
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Venus Magellan Radar Images Ridges formed by crustal shortening Eistla region with Gula Mons in the Background
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Image resolution Venera vs. Magellan
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Earth Mean radius 6371 km Mass 5.973 ˣ 10 24 kg Mean density 5515 kg/m 3 Rotation period -1 d Orbital period 365.256 d Sun distance 1 AU Surface pressure 1 bar Earth Moon system to scale
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Mars Mean radius 3396 km = 0.533 R E Mass 6418 ˣ 10 23 kg = 0.107 M E Mean density 3933 kg/m 3 Rotation period 1.026 d = 24.623h Orbital period 686.98 d Sun distance ~1.5 AU Surface pressure 0.7 mbar http://nssdc.gsfc.nasa.gov/planetary/factsheet/marsfact.html Opportunity: Greeley Haven winter stopover
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Mars “Homestake” mineral, possibly Gypsum vein from Oportunity MRO North polar erg with sand dunes Snake River Rocks, Curiosity
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Mars MEX: Buried glaciers around Phlegra Montes
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Mars MRO Chemical alteration by water, Jezero Crater Delta
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