Number of the records: 1
Formation of asteroid pairs by rotational fission
- 1.
SYSNO ASEP 0355351 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Formation of asteroid pairs by rotational fission Author(s) Pravec, Petr (ASU-R) RID, ORCID
Vokrouhlický, D. (CZ)
Polishook, D. (IL)
Scheeres, D.J. (US)
Harris, A. W. (US)
Galád, Adrián (ASU-R) RID
Vaduvescu, O. (ES)
Pozo, F. (CL)
Barr, A. (CL)
Longa, P. (CL)
Vachier, F. (FR)
Colas, F. (FR)
Pray, D. P. (US)
Pollock, J. (US)
Reichart, D. E. (US)
Ivarsen, K.M. (US)
Haislip, J.B. (US)
LaCluyze, A. (US)
Kušnirák, Peter (ASU-R)
Henych, Tomáš (ASU-R) ORCID, RID
Marchis, F. (US)
Macomber, B. (US)
Jacobson, S.A. (US)
Krugly, Yu. N. (UA)
Sergeev, A.V. (UA)
Leroy, A. (FR)Source Title Nature. - : Palgrave Macmillan - ISSN 0028-0836
Roč. 466, č. 7310 (2010), s. 1085-1088Number of pages 4 s. Language eng - English Country GB - United Kingdom Keywords full 2-body problem ; binary asteroids ; stability Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects GA205/09/1107 GA ČR - Czech Science Foundation (CSF) GD205/08/H005 GA ČR - Czech Science Foundation (CSF) CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000281203600035 DOI 10.1038/nature09315 Annotation We report photometric observations of a sample of asteroid pairs, revealing that the primaries of pairs with mass ratios much less than 0.2 rotate rapidly, near their critical fission frequency. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2011
Number of the records: 1