The lightcurve and colors of unusual Minor Planet 1996 PW

被引:21
作者
Davies, JK
McBride, N
Green, SF
Mottola, S
Carsenty, U
Basran, D
Hudson, KA
Foster, MJ
机构
[1] Joint Astron Ctr, Hilo, HI 96720 USA
[2] Univ Kent, Sch Phys Sci, Unit Space Sci & Astorphys, Canterbury CT2 7NR, Kent, England
[3] DLR, Inst Planetary Explorat, D-12489 Berlin, Germany
关键词
asteroids; rotation; photometry; infrared; comets;
D O I
10.1006/icar.1998.5888
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Minor Planet 1996 PW is unusual in having the orbital characteristics of a long period comet but showing no sign of cometary activity around the time of its discovery. We present optical data which reveals a double peaked lightcurve (period 35.44 +/- 0.02 hrs and amplitude 0.44 +/- 0.03 magnitudes) and VRIJHK photometry which shows colors (V - R = 0.56 +/- 0.04, V - I = 1.03 +/- 0.06, V - J = 1.80 +/- 0.05, V - H = 2.19 +/- 0.05, and V - K = 2.32 +/- 0.05) typical of D type asteroids and suspected bare comet nuclei. A low signal to noise reflectance spectrum in the K band shows a flat continuum with no evidence for spectral features. Image profiles from coadded frames in the R band indicate no apparent cometary activity with an implied upper limit to the dust production rate of 0.03 kg s(-1). (C) 1998 Academic Press.
引用
收藏
页码:418 / 430
页数:13
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