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W.-H. Ip Zhongyi Lin, Ian Lai, Vickie Lee. Yuan Li NCU/MUST
Rosetta/OSIRIS W.-H. Ip Zhongyi Lin, Ian Lai, Vickie Lee. Yuan Li NCU/MUST
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Outline 4. Pits
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W2 D=3.3x4.0x3.5 km T1 D=7.6x4.9 km2 T1 D=7.6x4.9 km2 T1 D=7.6x4.9 km2 T1 D=7.6x4.9 km H2 D= km
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81P Wild 2 Depressions with quasi-circular p;anforms at size up to 2 km across/depth ~ 140 m. Nearly vertical wall/rubbles found at base. Size frequency distribution lies well above equilibrium cratering on Phobos and Deimos. Vapor flow driven-erosion and collapse and subsidence.
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Cumulative Size Frequency Distribution/Wild 2
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Comparison with Impact Craters
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Sublimation-driven erosion?
Impact crater ? Steep-walled flat-floored circular depression
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8P Tempel 1 Layering/repeated fluidization flow episodes
because of release of supervolatile (CO/CO2) vapor trapped in amorphorous water ice ~ 100 m deep (Belton and Melosh 2009)?
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103P Hartley 2 No Wild 2 crater-like depressions/no Tempel 1 layering.
High outgassing activity. Water vapor emerging mostly from the waist region and CO2 from the small end.
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Surface evolutionary track
Belton (2010, 2012) Wild 2 (new) -> Tempel 1 -> Hartley 2 (old) Cheng, Lisse and A’Hearn (2013) Hartley 2 (new) -> Wild 2 -> Tempel 1 (old) 67P has characteristics of all three types.
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Hatmehit and other landforms
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67P circular depressions
NAC_ T Z_ID30_ _F22 NAC_ T Z_ID30_ _F22 WAC_ T Z_ID30_ _F18_2
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NAC_ T Z_ID30_ _F22 NAC_ T Z_ID30_ _F15 WAC_ T Z_ID30_ _F18 WAC_ T Z_ID30_ _F18 WAC_ T Z_ID30_ _F18 WAC_ T Z_ID30_ _F18
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Wild2 circle depression
n2075we02r n2069we02r
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Size-frequency distribution
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Size-frequency distribution
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Possible Erosion Effect
Cheng, Lisse and A’Hearn (2013)
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The q – variation of 67P (100 clones)
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The q – variation of 81P Wild 2 (100 clones)
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The q – variation of 9P Tempel 1 (100 clones)
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Orbital History 81P Wild 2 103P Hartley 2 67P and 103P Hartley 2
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Orbital statistics Comet Wild 2 youngest
To be followed by comet Hartley 2 Comet Tempel 1 and comet 67P oldest
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Pits & Jetlets Vincent et al. (2015) Vincent et al. (2015)
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Lunar pits
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Evolution of a cometary pit
Lunar pits Lunar pits Lunar pits Evolution of a cometary pit Vincent et al. (2015) (2013)
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Active pits Vincent et al. (2015)
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Sublimation-driven erosion?
Impact crater ? Steep-walled flat-floored circular depression
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