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The slow rotation of 253 Mathilde

Mottola, S (author)
Uppsala universitet,Astronomiska observatoriet
Sears, WD (author)
Erikson, A (author)
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Harris, AW (author)
Young, JW (author)
Hahn, G (author)
Dahlgren, M (author)
Mueller, BEA (author)
Owen, B (author)
GilHutton, R (author)
Licandro, J (author)
Barucci, MA (author)
Angeli, C (author)
Neukum, G (author)
Lagerkvist, CI (author)
Lahulla, JF (author)
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 (creator_code:org_t)
PERGAMON-ELSEVIER SCIENCE LTD, 1995
1995
English.
In: PLANETARY AND SPACE SCIENCE. - : PERGAMON-ELSEVIER SCIENCE LTD. - 0032-0633. ; 43:12, s. 1609-1613
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • 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

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

GALILEO PHYSICAL MODEL
Astronomy and astrophysics
Astronomi och astrofysik

Publication and Content Type

ref (subject category)
art (subject category)

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