CCD photometry and model of MUSES-C target (25143) 1998 SF36

Details CCD photometry and model of MUSES-C target (25143) 1998 SF36 CCD photometry and model of MUSES-C target (25143) 1998 SF36

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26a...405l..29k&link_type=abstract

Astronomy and Astrophysics, v.405, p.L29-L32 (2003)

Astronomy and Astrophysics

Astrophysics

19

Solar System: Minor Planets, Asteroids, Techniques: Photometric, Methods: Numerical

Scientific paper

We present photometric observations of the near-Earth asteroid (25143) 1998 SF36 from the 2001 apparition campaign, and we discuss the corresponding physical model. The asteroid's photometric behaviour is consistent with an S-type object, it has a retrograde pole at lambda =355o, begin {equation}ta=-84opartialm 5o, and its sidereal rotation period is P=12.132partialm 0.0005 hours. 1998 SF36 is elongated, with rough global dimension ratios a/b=2.0, b/c=1.3, but the elongation is not due to a bifurcated shape. The surface is not likely to contain major concavities. No significant albedo variegation was detected.

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