Arid
报告编号N20010094058
Asteroid Size-Frequency Distribution (The ISO Deep Asteroid Survey).
Tedesco, E. F.
英文摘要A total of six deep exposures (using AOT CAM01 with a 6 (inch) PFOV) through the ISOCAM LW10 filter (IRAS Band 1, i.e., 12 micro-m) were obtained on an approximately 15 arcminute square field centered on the ecliptic plane. Point sources were extracted using the technique described by Desert, et al. Two known asteroids appear in these frames and 20 sources moving with velocities appropriate for main belt asteroids are present. Most of the asteroids detected have flux densities less than 1 mJy, i.e., between 150 and 350 times fainter than any of the asteroids observed by Infrared Astronomy Satellite (IRAS). These data provide the first direct measurement of the 12 micro-m sky-plane density for asteroids on the ecliptic equator. The median zodiacal foreground, as measured by ISOCAM during this survey, is found to be 22.1 +/- 1.5 mJy per pixel, i.e., 26.2 +/- 1.7 MJy/sr. The results presented here imply that the actual number of kilometer-sized asteroids is significantly greater than previously believed and in reasonable agreement with the Statistical Asteroid Model.
英文关键词Asteroids Infrared astronomy Sky surveys(Astronomy) Infrared space observatory(Iso) Spaceborne astronomy Asteroid detection Mathematical models Asteroid belts Infrared astronomy satellite Astronomical catalogs Size distribution Eclip
出版年2001
语种英语
国家United States
URLhttp://r.cnki.net/KCMS/detail/detail.aspx?DbCode=KJBG&dbname=KJBGW&filename=59fac19331c97d1d549b0d7a
来源机构National Aeronautics and Space Administration
资源类型科技报告
条目标识符http://119.78.100.177/qdio/handle/2XILL650/272978
推荐引用方式
GB/T 7714
Tedesco, E. F.. Asteroid Size-Frequency Distribution (The ISO Deep Asteroid Survey).,2001.
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