Transcript
  • 2009--1

  • View Mars by Hubble Space TelescopeFlight into Mariner Valley

  • 603817 1960~1975 1964~19711975-121976~199217198811992~19921996 21/

  • NASA

  • 2009-2020

    200920112013201620182020MSLScoutGround Breaking (GBMSR)ScoutScoutMSLScoutScoutScoutMSLScoutMSR with RoverScoutMSLScoutGround Breaking (GBMSR)Scout

  • ESA Aurora Aurora2033

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  • 10-6CO2N240ArO2COH2O95.32.70.60.130.070.0339ArNeKrXeO352.530.080.040.2

  • 61035Km -33o100o17o-22o-123o- -133o

  • 65851600

  • Olympus55025

  • 5S, 297E, 2004-03-26, by G. Neukum

  • Mssbauer spectra show jarositeOpportunity/MRO, 2004-03-02small-scale cross bedding

  • Concentrations of Mg, Al, Cl and Br versus S in rocks and soils indicates water alteration L. A. Haskin et al., 2005, Nature Letters, Vol. 436

  • 10W2E5N6STES hematite abundance, is overlain on a daytime THEMISChristensen et al., 2001, JGR

  • Mars Hematite

  • The change of CO2 and H2O ice in North Polar

  • MARS ICE

  • Martian north polar layered deposits

    Fishbaugh, 2006, JGR

  • Colour view of crater with water ice(70.5 N,103 E, 35 Km wide, 2 km depth, 15 m/pixel)2 Feb. 2005, from G. Neukum

  • Nanedi VallisParana Valles

  • Olympica Fossae, 25.98N, 113.18W , http://www.msss.com/moc_gallery/ 2001-02-152000-03-19

  • Gullies in Newton Basin (MOC2-320 )39.0S, 166.1WNASA/JPL, 2002-10-07

  • Gullies Formation mechanismMGS_88923, 65S,15 W, NASA/JPL, 1997-12-29

  • Groundwater sapping Nirgal vallisJaumann, Reiss, 2002Recent (few Myr) outflow from Cerberus fossaeBurr et al., GRL, 2002

  • Colour nadir view of Nicholson Crater (100Km wide, 0.0 S, 195.5E, 15.3 m/pixel)

  • Hock, 2004

  • 2.23, 356.75, MOC Release No. MOC2-316, 2002-06-27 Partially-Exhumed Crater in Northern Terra Meridiani

  • West Arabia Terra, 8N, 7W MOC Release No. MOC2-261, 2000-10-4 Terra Meridiani mesas, 16.87, 331.23MOC Release No. M20-01357, 2000-10-23

  • Eberswalde Delta, MGS MOC Release No. MOC2-1225, 2005-09-20In northeast of Holden Crater near 24.0S, 33.7W

  • Water Alteration at Gusev Crater Rocks in the Gusev Crater show evidence for interaction with waterhighly elevated levels of S, Cl, K, P, Br basaltic chemistry, but highly oxidized and lacking in primary basaltic minerals, IR spectrum fit well by basaltic glassgoethite ( FeO(OH), Hydrated Iron Oxide )fine to coarse layered sedimentsSpirit landing site

  • MGS

  • MGS TES Basalt MapBasalt (Type 1 spectra) concentrated in Southern HighlandsBandfield et al. (2000), Hamilton et al. (2001)

  • MGS TES Andesite MapAndesite (type 2 spectra) appears concentrated in Northern Lowlands, but also intermixed with basalt in Southern Highlands.Bandfield et al. (2000), Hamilton et al. (2001)

  • Distribution of the HCPs and LCPs on Mars (Bibring et al. Science, vol. 307, 2005)OMEGA confirms the TES mapping of HCPs, obtained at moderate (>3 km) resolution, identifies LCPs at higher resolution (
  • 1997X

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  • Apollo(3300)10-9 T 32

  • 3219

  • 14%25%37%

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  • [McKay, 1996 #82] (PAHs)[McKay, 1996 #82] (biofilm)

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  • 20122017

  • 1 (2) (3) (4) (5) (6)

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  • 1234C, H, O, N, P , S56

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