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The small satellites of Pluto as observed by New Horizons.

Authors :
Weaver HA
Buie MW
Buratti BJ
Grundy WM
Lauer TR
Olkin CB
Parker AH
Porter SB
Showalter MR
Spencer JR
Stern SA
Verbiscer AJ
McKinnon WB
Moore JM
Robbins SJ
Schenk P
Singer KN
Barnouin OS
Cheng AF
Ernst CM
Lisse CM
Jennings DE
Lunsford AW
Reuter DC
Hamilton DP
Kaufmann DE
Ennico K
Young LA
Beyer RA
Binzel RP
Bray VJ
Chaikin AL
Cook JC
Cruikshank DP
Dalle Ore CM
Earle AM
Gladstone GR
Howett CJ
Linscott IR
Nimmo F
Parker JW
Philippe S
Protopapa S
Reitsema HJ
Schmitt B
Stryk T
Summers ME
Tsang CC
Throop HH
White OL
Zangari AM
Source :
Science (New York, N.Y.) [Science] 2016 Mar 18; Vol. 351 (6279), pp. aae0030.
Publication Year :
2016

Abstract

The New Horizons mission has provided resolved measurements of Pluto's moons Styx, Nix, Kerberos, and Hydra. All four are small, with equivalent spherical diameters of ~40 kilometers for Nix and Hydra and ~10 kilometers for Styx and Kerberos. They are also highly elongated, with maximum to minimum axis ratios of ~2. All four moons have high albedos (~50 to 90%) suggestive of a water-ice surface composition. Crater densities on Nix and Hydra imply surface ages of at least 4 billion years. The small moons rotate much faster than synchronous, with rotational poles clustered nearly orthogonal to the common pole directions of Pluto and Charon. These results reinforce the hypothesis that the small moons formed in the aftermath of a collision that produced the Pluto-Charon binary.<br /> (Copyright © 2016, American Association for the Advancement of Science.)

Details

Language :
English
ISSN :
1095-9203
Volume :
351
Issue :
6279
Database :
MEDLINE
Journal :
Science (New York, N.Y.)
Publication Type :
Academic Journal
Accession number :
26989256
Full Text :
https://doi.org/10.1126/science.aae0030