dc.contributor.author |
Newburn, R. L. Jr. |
en_US |
dc.contributor.author |
Duxbury, T. C. |
en_US |
dc.contributor.author |
Hanner, M. |
en_US |
dc.contributor.author |
Semenov, B. V. |
en_US |
dc.contributor.author |
Hirst, E. E. |
en_US |
dc.contributor.author |
Bhat, R. S. |
en_US |
dc.contributor.author |
Bhaskaran, S. |
en_US |
dc.contributor.author |
Wang, T. M. |
en_US |
dc.date.accessioned |
2004-09-16T21:28:10Z |
|
dc.date.available |
2004-09-16T21:28:10Z |
|
dc.date.issued |
2003-11-12 |
en_US |
dc.identifier.citation |
Journal of geophysical research, v. 108, no. e11, pp. 5117-5125 |
en_US |
dc.identifier.citation |
USA |
en_US |
dc.identifier.clearanceno |
03-0403 |
en_US |
dc.identifier.uri |
http://hdl.handle.net/2014/6585 |
|
dc.description.abstract |
Seventy-two images of the S-class asteroid 5535 Annefrank, acquired on 2 November 2002 at target ranges of 11,415??8.5 km, were transmitted to Earth as a part of an engineering readiness test of the Stardust mission. Forty-four of these were used to create a phase curve extending to 134, the largest angle yet achieved for any S-class asteroid. Flux fell by more than six magnitudes between the extrapolated 0 and 134. A maximum illuminated cross section of 16 km2 was seen at a phase angle of 47.2. Assuming a camera efficiency of 75%, a broadband (470?? nm) geometric albedo of 0.24 was derived for Annefrank. |
en_US |
dc.format.extent |
181768 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en_US |
|
dc.subject.other |
Solar system comets small bodies |
en_US |
dc.title |
Phase curve and albedo of asteroid 5534 Annefrank |
en_US |