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  • Thumbnail for Lobate debris apron
    Lobate debris aprons (LDAs) are geological features on Mars, first seen by the Viking Orbiters, consisting of piles of rock debris below cliffs. These...
    22 KB (2,495 words) - 11:03, 15 January 2024
  • Thumbnail for Bathocyroe fosteri
    of lobate ctenophore found at intermediate depths in all the world's oceans. The species is very common and abundant near the Mid-Atlantic Ridge. It...
    3 KB (224 words) - 11:18, 4 January 2023
  • Thumbnail for Geology of solar terrestrial planets
    ejecta from the Caloris basin. In addition, distinct color units, some of lobate shape, are observed in newly processed color data. Such relations strongly...
    44 KB (5,592 words) - 02:25, 9 September 2024
  • Thumbnail for Mapping of Venus
    plains embay the wrinkle ridges containing regional plains, which suggested that lobate plains are younger. However, as the lobate plains, smooth plains...
    48 KB (5,433 words) - 17:23, 22 August 2024
  • Thumbnail for Brain terrain
    complex ridges found on lobate debris aprons, lineated valley fill and concentric crater fill. It is so named because it suggests the ridges on the surface...
    8 KB (1,113 words) - 10:23, 23 December 2020
  • Thumbnail for Glaciers on Mars
    distributed at times in the past. Lobate convex features on the surface known as viscous flow features and lobate debris aprons, which show the characteristics...
    49 KB (5,966 words) - 18:02, 3 August 2024
  • Thumbnail for Terra Sabaea
    where ground water has frozen. Wide CTX view showing mesa and buttes with lobate debris aprons and lineated valley fill around them. Location is Ismenius...
    19 KB (2,497 words) - 21:58, 19 June 2022
  • Thumbnail for Lorica segmentata
    The fitments that closed the various plate sections together (buckles, lobate hinges, hinged straps, tie-hooks, tie-rings, etc.) were made of brass. In...
    11 KB (1,442 words) - 21:52, 13 September 2024
  • complex ridges found on lobate debris aprons, lineated valley fill and concentric crater fill. It is so named because it suggests the ridges on the surface...
    116 KB (14,179 words) - 15:56, 23 June 2024
  • Thumbnail for Guinevere Planitia
    southern flank of Var Mons lies narrow, lobate flows which extend for ~500 km where they overlie dark, ridged plains. North of the summit extends a prominent...
    12 KB (1,435 words) - 09:07, 25 April 2024
  • a substantial challenge to that hypothesis. Galileo imagery reveals no lobate features or vents indicative of cryovolcanic flow. Furthermore, in regions...
    20 KB (2,366 words) - 06:45, 4 September 2024
  • Thumbnail for Michelangelo quadrangle
    the lobate ridges described by Strom follow arcuate patterns along rings of the Barma-Vincente Basin; Hero Rupes is an example. These lobate ridges appear...
    22 KB (3,350 words) - 11:56, 30 May 2024
  • Thumbnail for Volcano
    observations of morphology and surface roughness of volcanic cones and lobate lava flows in the Marius Hills". Journal of Geophysical Research: Planets...
    89 KB (9,963 words) - 06:45, 5 September 2024
  • Thumbnail for Amazonis Planitia
    polygonal ridges, as seen by HiRISE under HiWish program Wide view of large ridge network, as seen by HiRISE under HiWish program Close view of ridge network...
    16 KB (1,982 words) - 02:52, 6 February 2024
  • Thumbnail for Alyogyne huegelii
    leaves are divided in three to five in outline; margins are irregular, lobate to toothed; pubescent and strongly veined lobes are coarse in shape. The...
    6 KB (790 words) - 01:33, 4 May 2022
  • Thumbnail for Arcadia quadrangle
    terrain Glaciers on Mars HiRISE HiWish program Impact crater Linear ridge networks Lobate debris apron Martian Gullies Perepelkin (Martian crater) Davies...
    47 KB (5,963 words) - 00:28, 3 September 2024
  • Thumbnail for Evidence of water on Mars found by Mars Reconnaissance Orbiter
    at times in the past.[page needed] Lobate convex features on the surface known as viscous flow features and lobate debris aprons, which show the characteristics...
    81 KB (9,712 words) - 07:17, 11 June 2024
  • Thumbnail for Occator (crater)
    attempts were made to discern the age of Occator. The age dating models of the lobate flows and crater ejecta range from 200 million years to 78 million years...
    17 KB (1,850 words) - 20:40, 20 May 2024
  • Thumbnail for Pillow lava
    point nearer the vent. This process produces a series of interconnecting lobate shapes that are pillow-like in cross-section. The skin cools much faster...
    7 KB (830 words) - 18:37, 18 April 2024
  • Thumbnail for Arabia Terra
    HiWish program Wide view of mesa with CTX showing cliff face and location of lobate debris apron (LDA). Location is Ismenius Lacus quadrangle. Enlargement of...
    30 KB (3,689 words) - 14:51, 16 August 2024
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