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

被引：48

作者：

Kaasalainen, M

Kwiatkowski, T

Abe, M

Piironen, J

Nakamura, T

Ohba, Y

Dermawan, B

Farnham, T

Colas, F

Lowry, S

Weissman, P

Whiteley, RJ

Tholen, DJ

Larson, SM

Yoshikawa, M

Toth, I

Velichko, FP

机构：

[1] Univ Helsinki, Observ, FIN-00014 Helsinki, Finland

[2] Adam Mickiewicz Univ Poznan, Astron Observ, PL-60286 Poznan, Poland

[3] Inst Space & Astronaut Sci, Kanagawa 2298510, Japan

[4] Natl Astron Observ, Tokyo 1818588, Japan

[5] Univ Tokyo, Sch Sci, Tokyo 1130033, Japan

[6] Univ Texas, Dept Astron, Austin, TX 78712 USA

[7] Observ Paris, IMCCE, F-75014 Paris, France

[8] CALTECH, Jet Prop Lab, Div Earth & Space Sci, Pasadena, CA 91109 USA

[9] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA

[10] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA

[11] Konkoly Observ Budapest, H-1525 Budapest, Hungary

[12] Kharkiv Natl Univ, Astron Observ, UA-61022 Kharkov, Ukraine

来源：

ASTRONOMY & ASTROPHYSICS | 2003年 / 405卷 / 03期

关键词：

solar system : minor planets; asteroids; techniques : photometric; methods : numerical;

D O I：

10.1051/0004-6361:20030819

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 = 355degrees; beta = - 84degrees +/- 5 degrees, and its sidereal rotation period is P = 12.132 +/- 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.

引用

页码：L29 / L32

页数：4

共 11 条

[1] CCD photometry of the MUSES-C mission target: Asteroid (25143) 1998 SF36 [J].