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The slow rotation of 253 Mathilde
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory.
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1995 (English)In: PLANETARY AND SPACE SCIENCE, ISSN 0032-0633, Vol. 43, no 12, 1609-1613 p.Article in journal (Refereed) Published
Abstract [en]

CCD photometry of the NEAR mission fly-by target 253 Mathilde is presented. Measurements taken during 52 nights of observations, from February to June 1995, allow a rotation period of 17.406 +/- 0.010 days and a lightcurve amplitude of 0.45 +/- 0.02 mag t

Place, publisher, year, edition, pages
PERGAMON-ELSEVIER SCIENCE LTD , 1995. Vol. 43, no 12, 1609-1613 p.
Keyword [en]
National Category
Astronomy, Astrophysics and Cosmology
URN: urn:nbn:se:uu:diva-85386OAI: oai:DiVA.org:uu-85386DiVA: diva2:113294
Addresses: Mottola S, DLR, INST PLANETARY EXPLORAT, RUDOWER CHAUSSEE 5, D-12489 BERLIN, GERMANY. CALTECH, JET PROP LAB, PASADENA, CA 91109. ASTRON OBSERV, S-75120 UPPSALA, SWEDEN. NATL OPT ASTRON OBSERV, TUCSON, AZ 85719. OBSERV PARIS, F-92195 MEUDON, FRAAvailable from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-15

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