E-Type Asteroid (2867) Steins as Imaged by OSIRIS on Board Rosetta

Author:

Keller H. U.1,Barbieri C.2,Koschny D.3,Lamy P.4,Rickman H.56,Rodrigo R.7,Sierks H.1,A’Hearn M. F.8,Angrilli F.2,Barucci M. A.9,Bertaux J.-L.10,Cremonese G.2,Da Deppo V.11,Davidsson B.12,De Cecco M.2,Debei S.2,Fornasier S.9,Fulle M.13,Groussin O.4,Gutierrez P. J.7,Hviid S. F.1,Ip W.-H.14,Jorda L.4,Knollenberg J.15,Kramm J. R.1,Kührt E.15,Küppers M.16,Lara L.-M.7,Lazzarin M.2,Moreno J. Lopez7,Marzari F.2,Michalik H.17,Naletto G.2,Sabau L.18,Thomas N.19,Wenzel K.-P.3,Bertini I.7,Besse S.4,Ferri F.2,Kaasalainen M.20,Lowry S.21,Marchi S.2,Mottola S.15,Sabolo W.7,Schröder S. E.1,Spjuth S.1,Vernazza P.3

Affiliation:

1. Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany.

2. University of Padova, Padova, Italy.

3. European Space and Technology Centre, Noordwijk, Netherlands.

4. Laboratoire d'Astrophysique de Marseille, Université de Provence, Marseille, France.

5. Institute för Astronomi och Rymdfysik, Uppsala, Sweden.

6. Polish Academy of Sciences Space Research Center, Warsaw, Poland.

7. Instituto de Astrofísica de Andalucía–Consejo Superior de Investigaciones Científicas, Granada, Spain.

8. University of Maryland, College Park, MD 20742, USA.

9. Observatoire de Paris, Meudon, France.

10. Services d’Aéronomie de CNRS, Verrières le Buisson, France.

11. Consiglio Nazionale delle Ricerche-Istituto Nazionale per la Fisica della Materia, Luxor, Padova, Italy.

12. Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden.

13. International School for Advanced Studies, Trieste, Italy.

14. National Central University, Jhongli City, Taiwan.

15. German Aerospace Center, Berlin, Germany.

16. European Space Astronomy Centre (ESAC), Madrid, Spain.

17. Institute of Computer and Network Engineering, Braunschweig, Germany.

18. Instituto Nacional de Técnica Aérospacial, Torrejon de Ardoz, Spain.

19. Physikalisches Institut der Universität Bern, Switzerland.

20. Tampere University of Technology, Tampere, Finland.

21. University of Kent, Canterbury, UK.

Abstract

Smooth Space Pebble In September 2008, on its way to meet comet 67P/Churyumov-Gerasimenko, the Rosetta spacecraft flew by asteroid Steins, a member of a very rare class of asteroids that had never been observed closely by spacecraft. Keller et al. (p. 190 ) analyzed the images to generate a reconstruction of the asteroid's shape. Steins is oblate with an effective spherical diameter of 5.3 kilometers, and it lacks small craters, which may have been erased by surface reshaping. Indeed, Steins's shape resembles that of a body that was spun-up by the YORP effect—a torque produced by incident sunlight, which can alter the rotation rate of a small body—that causes material to slide toward the equator. This effect may have produced Steins's distinctive diamond-like shape.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference34 articles.

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4. C. R Chapman in Asteroids III W. F. Bottke P. Paolicchi R. P. Binzel A. Cellino Eds. (Univ. of Arizona Press Tucson AZ 2002) pp. 315–329.

5. D. C. Richardson et al . in Asteroids III W. F. Bottke P. Paolicchi R. P. Binzel A. Cellino Eds. (Univ. of Arizona Press Tucson AZ 2002) pp. 501–515.

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