THERMAL MODEL CALIBRATION FOR MINOR PLANETS OBSERVED WITH WISE/NEOWISE: COMPARISON WITH INFRARED ASTRONOMICAL SATELLITE

被引:27
作者
Mainzer, A. [1 ]
Grav, T. [2 ]
Masiero, J. [1 ]
Bauer, J. [1 ,3 ]
Wright, E. [4 ]
Cutri, R. M. [3 ]
Walker, R. [5 ]
McMillan, R. S. [6 ]
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[3] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA
[4] UCLA Astron, Los Angeles, CA 90095 USA
[5] Monterey Inst Res Astron, Monterey, CA USA
[6] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
基金
美国国家航空航天局;
关键词
atlases; catalogs; infrared: general; minor planets; asteroids:; general; NEAR-EARTH ASTEROIDS; SURVEY-EXPLORER; PHOTOMETRY; IRAS;
D O I
10.1088/2041-8205/737/1/L9
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
With thermal infrared observations detected by the NEOWISE project, we have measured diameters for 1742 minor planets that were also observed by the Infrared Astronomical Satellite (IRAS). We have compared the diameters and albedo derived by applying a spherical thermal model to the objects detected by NEOWISE and find that they are generally in good agreement with the IRAS values. We have shown that diameters computed from NEOWISE data are often less systematically biased than those found with IRAS. This demonstrates that the NEOWISE data set can provide accurate physical parameters for the > 157,000 minor planets that were detected by NEOWISE.
引用
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页数:6
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