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A Comparative Study of Infrared Asteroid Surveys: IRAS, AKARI, and WISE

机译:红外小行星调查的比较研究:IRas,aKaRI和WIsE

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摘要

We present a comparative study of three infrared asteroid surveys based onthe size and albedo data from the Infrared Astronomical Satellite (IRAS), theJapanese infrared satellite AKARI, and the Wide-field Infrared Survey Explorer(WISE). Our study showed that: (i) the total number of asteroids detected withdiameter and albedo information with these three surveyors is 138,285, which islargely contributed by WISE; (ii) the diameters and albedos measured by thethree surveyors for 1,993 commonly detected asteroids are in good agreement,and within +/-10% in diameter and +/-22% in albedo at 1sigma deviation level.It is true that WISE offers size and albedo of a large fraction (>20%) of knownasteroids down to a few km bodies, but we would suggest that the IRAS and AKARIcatalogs compensate for larger asteroids up to several hundred km, especiallyin the main belt region. We discuss the complementarity of these three catalogsin order to facilitate the use of these data sets for characterizing thephysical properties of minor planets.
机译:我们基于红外天文卫星(IRAS),日本红外卫星AKARI和宽视场红外勘测浏览器(WISE)的大小和反照率数据,对三种红外小行星勘测进行了比较研究。我们的研究表明:(i)这三名测量员利用直径和反照率信息检测到的小行星总数为138,285,这主要是由WISE贡献的; (ii)三位测量员测量的1,993个常见小行星的直径和反照率非常吻合,并且在1sigma偏差水平下直径在+/- 10%之内,反照率在22%之内。和大部分(> 20%)已知小行星的反照率,直至几公里的物体,但我们建议IRAS和AKARI目录对长达几百公里的较大小行星进行补偿,尤其是在主带地区。我们讨论这三个目录的互补性,以便于使用这些数据集来表征小行星的物理特性。

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