The Discovery and Physical Characteristics of 1996 JA1
Authors: Spahr T.B.1; Hergenrother C.W.2; Larson S.M.2; Hicks M.2; Marsden B.G.3; Williams G.V.3; Tholen D.J.4; Whiteley R.J.4; Osip D.J.1
Source: Icarus, Volume 129, Number 2, October 1997 , pp. 415-420(6)
Publisher: Academic Press
Abstract:
1996 JA1, which approached to 0.003 AU of the Earth on 1996 May 19.7 UT, was discovered on films exposed 5 days earlier during the course of the high-ecliptic-latitude Bigelow Sky Survey. The utility of high-latitude surveying for near-Earth objects is demonstrated by the fact that 1996 JA1 traveled through the usual ecliptic survey region at a rate of 5? hr-1, and would likely have escaped detection even at V = 11. Rapid astrometry and communication through the Minor Planet Center and the World Wide Web facilitated follow-up observations that indicate 1996 JA1 has a mean diameter of 170 m, a rotational period of 5.23 hr, and an albedo of 0.30. With a spectrum consistent with the V class, it is possible that 1996 JA1 shares the same source as the HED meteorites. Copyright 1997 Academic Press.
Language: English
Document Type: Research article
Affiliations: 1: Astronomy Department, University of Florida, Gainesville, Florida, 32611 2: Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona, 85721 3: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts, 02138 4: Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, Hawaii, 96822
Publication date: 1997-10-01
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- In this Subject: Astronomy
- By this author: Spahr T.B. ; Hergenrother C.W. ; Larson S.M. ; Hicks M. ; Marsden B.G. ; Williams G.V. ; Tholen D.J. ; Whiteley R.J. ; Osip D.J.

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