Arid
报告编号NASA-CR-177089, NAS 1.26:177089
来源IDNTRS_Document_ID: 19860021993
The size, shape, density, and albedo of Ceres from its occultation of BD+8 deg 471
Millis, R. L.; Wasserman, L. H.; Franz, O. G.; Nye, R. A.; Oliver, R. C.; Kreidl, T. J.; Jones, S. E.; Hubbard, W.; Lebofsky, L.; Goff, R.
英文摘要The occultation of BD+8 degrees 471 by Ceres on 13 November 1984 was observed photoelectrically at 13 sites in Mexico, Florida, and the Caribbean. These observations indicate that Ceres is an oblate spheroid having an equatorial radius of 479.6 + or - 2.4 km and a polar radius of 453.4 + or - 4.5 km. The mean density of this minor planet is 2.7 gm/cubic cm + or - 5%, and its visual geometric albedo is 0.070. While the surface appears globally to be in hydrostatic equilibrium, firm evidence of real limb irregularities is seen in the data.
英文关键词ALBEDO ASTRONOMICAL PHOTOGRAPHY CERES ASTEROID DIAMETERS OCCULTATION LIGHT CURVE SIGNAL TO NOISE RATIOS STELLAR RADIATION TOPOGRAPHY
出版年1986
报告类型Technical Report
语种英语
国家美国
URLhttp://hdl.handle.net/2060/19860021993
资源类型科技报告
条目标识符http://119.78.100.177/qdio/handle/2XILL650/259045
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Millis, R. L.,Wasserman, L. H.,Franz, O. G.,et al. The size, shape, density, and albedo of Ceres from its occultation of BD+8 deg 471,1986.
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