Knowledge Resource Center for Ecological Environment in Arid Area
报告编号 | NASA-CR-177089, NAS 1.26:177089 |
来源ID | NTRS_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 |
URL | http://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 |
推荐引用方式 GB/T 7714 | 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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