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as17-147-22462.JPGAS 17-147-22462 - America from Challanger57 visitenessun commentoMareKromium
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as17-147-22458.JPGAS 17-147-22458 - America from Challanger57 visitenessun commentoMareKromium
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as17-147-22605.JPGAS 17-147-22605 - Sun-struck (2)57 visiteALSEP pan. Central Station.MareKromium
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as17-147-22604.JPGAS 17-147-22604 - Sun-struck (1)57 visiteALSEP pan. LM, HFE, RTG.MareKromium
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as17-147-22473.JPGAS 17-147-22473 - Challanger's Shadow and small Crater Cluster57 visitePre-EVA-1 LM window pan. Looking below horizon at the LM shadow and the near surface.MareKromium
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as17-147-22503.JPGAS 17-147-22503 - Signs of Gravity Wasting?57 visiteEVA-1 at the LM. 4 o'clock pan. Near surface. Large boulder track.MareKromium
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as17-147-22502.JPGAS 17-147-22502 - North Massif57 visiteEVA-1 at the LM. 4 o'clock pan. North Massif, large boulder track.MareKromium
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as17-147-22505.JPGAS 17-147-22505 - Lunar Panorama57 visiteEVA-1 at the LM. 4 o'clock pan. Wessex Cleft and shadowed Sculptured Hills.MareKromium
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as15-91-12372.JPGAS 15-91-12372 - At the end of the trans-lunar coast (elab. Lunexit)57 visitenessun commentoMareKromium
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as17-147-22551.JPGAS 17-147-22551 - Geophone Panorama57 visiteGeophone 3 pan. This frame shows the rock that Jack examined after deploying Geophone #1, Geophone #2, Wessex Cleft.MareKromium
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OPP-SOL1220-1P236485480EFF85R9P2629L6M1.jpgMorning Mist over Victoria (2) - Sol 122057 visitenessun commentoMareKromium
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PSP_002620_1410_RED_browse-01.jpgGullies on the edge of Newton Basin (extra-detail mgnf)57 visiteThe gullies start near the top of the wall and can be traced across a break in slope partway down the wall (see here, 750 mt across). This break in slope occurs along the entire portion of the Crater wall in this image. The gullies appear shallower just above the break in slope, and deeper below the slope break.
This suggests that the fluid which eroded and carved out the wall materials forming the gullies, increased in velocity after the slope break, creating a deeper section of the gully.
MareKromium
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