Remote sensing analysis of solar-system objects

被引:5
|
作者
Encrenaz, Therese [1 ]
机构
[1] Observ Paris, LESIA, F-92195 Meudon, France
关键词
D O I
10.1088/0031-8949/2008/T130/014037
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Most of our knowledge of solar-system objects has been achieved by remote sensing observations, and, in particular, by spectroscopy at all wavelengths. Solar-system spectra mainly show two components: a reflected solar component that peaks in the visible range, and a thermal component that extends in the infrared and millimetre range. Remote sensing observations of planets, satellites and comets have demonstrated the amazing variety of their atmospheric and surface properties; this variety is to be kept in mind when observations of extrasolar planets become available.
引用
收藏
页数:7
相关论文
共 50 条
  • [21] ISOTOPIC ANALYSIS OF EARLY SOLAR-SYSTEM OBJECTS BY AN ION MICROPROBE - PARAMETRIC STUDIES AND INITIAL RESULTS
    GOSWAMI, JN
    SRINIVASAN, G
    PROCEEDINGS OF THE INDIAN ACADEMY OF SCIENCES-EARTH AND PLANETARY SCIENCES, 1994, 103 (01): : 57 - 82
  • [22] THE GENERATION AND USE OF NUMERICAL SHAPE MODELS FOR IRREGULAR SOLAR-SYSTEM OBJECTS
    SIMONELLI, DP
    THOMAS, PC
    CARCICH, BT
    VEVERKA, J
    ICARUS, 1993, 103 (01) : 49 - 61
  • [23] ANOTHER SOLAR-SYSTEM
    不详
    DISCOVER, 1983, 4 (10): : 12 - 12
  • [24] DEUTERIUM IN THE SOLAR-SYSTEM
    OWEN, T
    IAU SYMPOSIA, 1992, (150): : 97 - 101
  • [25] CHAOS IN THE SOLAR-SYSTEM
    TYSON, ND
    NATURAL HISTORY, 1995, 104 (07) : 14 - +
  • [26] SOLAR-SYSTEM CHAOS
    NOBILI, AM
    BURNS, JA
    SCIENCE, 1989, 244 (4911) : 1425 - 1425
  • [27] THE BOUNDARY OF THE SOLAR-SYSTEM
    SMOLUCHOWSKI, R
    TORBETT, M
    NATURE, 1984, 311 (5981) : 38 - 39
  • [28] DUST IN THE SOLAR-SYSTEM
    FECHTIG, H
    ZEITSCHRIFT FUR NATURFORSCHUNG SECTION A-A JOURNAL OF PHYSICAL SCIENCES, 1989, 44 (10): : 877 - 882
  • [29] COSMOGONY OF THE SOLAR-SYSTEM
    HOREDT, GP
    MOON AND THE PLANETS, 1979, 21 (01): : 63 - 121
  • [30] IS THE SOLAR-SYSTEM UNIQUE
    WHITEHOUSE, D
    NEW SCIENTIST, 1980, 88 (1221) : 14 - 17