The shape and surface variation of 2 pallas from the hubble space telescope

Science

Volumn 326, Issue 5950, 2009, Pages 275-278

  Schmidt, B E ^a   Thomas, P C ^b   Bauer, J M ^c   Li, J Y ^d   McFadden, L A ^d   Mutchler, M J ^e   Radcliffe, S C ^f   Rivkin, A S ^g   Russell, C T ^a   Wm Parker, J ^h   Stern, S A ^h  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b Department of Obstetrics Gynecology   (United States)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d Bldg 142   (United States)

^e STScI   (United States)

^f Hydraulx Santa Monica   (United States)

^g APPLIED PHYSICS LABORATORY   (United States)

^h SOUTHWEST RESEARCH INSTITUTE   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ASTEROID; OBSERVATIONAL METHOD; SATELLITE IMAGERY; SHAPE ANALYSIS; SPACE TECHNOLOGY; ULTRAVIOLET RADIATION; WATER AVAILABILITY;

ARTICLE; ASTRONOMY; COLOR; DEVICE; PRIORITY JOURNAL; TELESCOPE;

EID: 70349887758     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1177734     Document Type: Article

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30. Based on observations made with the NASA/ESA Hubble Space Telescope, obtained al. the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy Inc. under NASA contract NAS 5-26555. The observations are associated with program 11115. Supported by STScl grant HST-GO-11115.01 (C.T.R.).