The distribution of bright and dark material on Ganymede in relationship to surface elevation and slopes

被引:18
|
作者
Oberst, J [1 ]
Schreiner, B
Giese, B
Neukum, C
机构
[1] DLR, Inst Planetary Explorat, D-12489 Berlin, Germany
[2] Brown Univ, Dept Geol Sci, Providence, RI 02912 USA
[3] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA
关键词
satellites of Jupiter; surfaces; Ganymede;
D O I
10.1006/icar.1999.6143
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The unique high-resolution digital terrain data set available for Ganymede's Uruk Sulcus area and Galileo Regio is analyzed by quantitative image analysis techniques to identify relationships between surface brightness, elevation, and slopes. Broad and narrow ridges and grooves of the Uruk Sulcus terrain model are found to be aligned with bright and dark lineament patterns visible in images. These prominent lineaments represent areas covered by bright and dark albedo material, not effects of photometric shading. There is a strong correlation between material locations and elevation: bright material is found on topographic highs, whereas dark material is located in depressions; the relative abundance of the dark material increases with lower elevation. In Galileo Regio, we find that bright material is also located on slopes facing north. We suggest that the bright material in Uruk Sulcus and Galileo Regio was emplaced or exposed during or after formation of the terrain in its present location, whereas the dark material was eroded and redistributed down-slope. Effects of net solar illumination may play a role in the peculiar azimuthal distribution of bright and dark material on slopes. (C) 1999 Academic Press.
引用
收藏
页码:283 / 293
页数:11
相关论文
共 50 条
  • [1] The relationship between the bright and dark matter
    Silk, J
    THIRD STROMLO SYMPOSIUM: THE GALACTIC HALO, 1999, 165 : 27 - 33
  • [2] ON THE JOINT DISTRIBUTION OF SURFACE ELEVATION AND SLOPES FOR A NONLINEAR RANDOM SEA, WITH AN APPLICATION TO RADAR ALTIMETRY
    SROKOSZ, MA
    JOURNAL OF GEOPHYSICAL RESEARCH-OCEANS, 1986, 91 (C1): : 995 - 1006
  • [3] STABILITY OF BRIGHT AND DARK SURFACE-WAVES
    CHEN, YJ
    JOURNAL OF THE OPTICAL SOCIETY OF AMERICA B-OPTICAL PHYSICS, 1993, 10 (06) : 1077 - 1080
  • [4] Dark and bright localized surface plasmons in nanocrosses
    Verellen, Niels
    Van Dorpe, Pol
    Vercruysse, Dries
    Vandenbosch, Guy A. E.
    Moshchalkov, Victor V.
    OPTICS EXPRESS, 2011, 19 (12): : 11034 - 11051
  • [5] DISTRIBUTION OF SLOPES ON A CRATERED PLANETARY SURFACE
    MARCUS, AH
    TRANSACTIONS-AMERICAN GEOPHYSICAL UNION, 1969, 50 (04): : 218 - &
  • [6] BRIGHT AND DARK SURFACE-WAVES AT A NONLINEAR INTERFACE
    CHEN, YJ
    PHYSICAL REVIEW A, 1992, 45 (07): : 4974 - 4978
  • [7] Iapetus dark and bright material: giving compositional interpretation some latitude
    Vilas, F
    Jarvis, KS
    Barker, ES
    Lederer, SM
    Kelley, MS
    Owen, TC
    ICARUS, 2004, 170 (01) : 125 - 130
  • [8] Spectral properties and geology of bright and dark material on dwarf planet Ceres
    Thangjam, G.
    Nathues, A.
    Platz, T.
    Hoffmann, M.
    Cloutis, E. A.
    Mengel, K.
    Izawa, M. R. M.
    Applin, D. M.
    METEORITICS & PLANETARY SCIENCE, 2018, 53 (09) : 1961 - 1982
  • [9] Bright and Dark Polar Deposits on Mercury: Evidence for Surface Volatiles
    Neumann, Gregory A.
    Cavanaugh, John F.
    Sun, Xiaoli
    Mazarico, Erwan M.
    Smith, David E.
    Zuber, Maria T.
    Mao, Dandan
    Paige, David A.
    Solomon, Sean C.
    Ernst, Carolyn M.
    Barnouin, Olivier S.
    SCIENCE, 2013, 339 (6117) : 296 - 300
  • [10] Titan's surface reviewed: the nature of bright and dark terrain
    Lorenz, RD
    Lunine, JI
    PLANETARY AND SPACE SCIENCE, 1997, 45 (08) : 981 - 992