Physical modeling of triple near-Earth asteroid (153591) 2001 SN 263 from radar and optical light curve observations

Tracy Becker, (1) , Ellen S. Howell (2) , Michael, C. Nolan, (2) , Christopher Magri (3) , Petr Pravec (4) , Patrick A. Taylor, (2) , Julian Oey (5) , David Higgins (6) , Jozef Világi (7) , Leonard Kornoš (7) , Adrián Galád (7) , Stefan Gajdoš (7) , Ninel M. Gaftonyuk (8) , Yurij N. Krugly, (9) , Igor E. Molotov (10) , Michael D. Hicks, (11) , Albino Carbognani (12) , Brian D. Warner (13) , Frédéric Vachier (14) , Franck Marchis (15) , Joseph T. Pollock (16)

1 UCF - University of Central Florida [Orlando]
2 NAIC - Arecibo Observatory, National Astronomy and Ionosphere Center
3 University of Maine
4 Ondřejov Observatory of the Prague Astronomical Institute
5 Leura Observatory
6 Hunters Hill Observatory
7 Modra Observatory
8 CrAO - Crimean Astrophysical Observatory
9 Institute of Astronomy [Kharkiv]
10 Keldysh Institute of Applied Mathematics
11 JPL - Jet Propulsion Laboratory
12 OAVDA - Astronomical Observatory of the Autonomous Region of the Aosta Valley
13 CS3 - Center for Solar System Studies
14 IMCCE - Institut de Mécanique Céleste et de Calcul des Ephémérides
15 Carl Sagan Center
16 Department of Physics and Astronomy [Boone]

We report radar observations (2380-MHz, 13-cm) by the Arecibo Observatory and optical light curves observed from eight different observatories and collected at the Ondrejov Observatory of the triple near-Earth asteroid system (153591) 2001 SN263. The radar observations were obtained over the course of ten nights spanning February 12-26, 2008 and the light curve observations were made throughout January 12 - March 31, 2008. Both data sets include observations during the object's close approach of 0.06558 AU on February 20th, 2008. The delay-Doppler images revealed the asteroid to be comprised of three components, making it the first known triple near-Earth asteroid. Only one other object, (136617) 1994 CC is a confirmed triple near-Earth asteroid. We present physical models of the three components of the asteroid system. We constrain the primary's pole direction to an ecliptic longitude and latitude of (309 °, - 80 °) ± 15 ° . We find that the primary rotates with a period 3.4256 ± 0.0002 h and that the larger satellite has a rotation period of 13.43 ± 0.01 h , considerably shorter than its orbital period of approximately 6 days. We find that the rotation period of the smaller satellite is consistent with a tidally locked state and therefore rotates with a period of 0.686 ± 0.002 days (Fang et al. [2011]. Astron. J. 141, 154-168). The primary, the larger satellite, and the smaller satellite have equivalent diameters of 2.5 ± 0.3 km , 0.77 ± 0.12 km , 0.43 ± 0.14 km and densities of 1.1 ± 0.2 g /cm3, 1.0 ± 0.4 g /cm3, 2.3 ± 1.3 g /cm3 , respectively.

Mots clés: Asteroid; Asteroids; Near-Earth objects; rotation; Photometry; Radar observations; Satellites of asteroids

Domaines: Planète et Univers [physics]

Tracy Becker,, Ellen S. Howell, Michael, C. Nolan,, Christopher Magri, Petr Pravec, et al.. Physical modeling of triple near-Earth asteroid (153591) 2001 SN 263 from radar and optical light curve observations. 2014. ⟨hal-01101387⟩