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Formation of Kuiper-belt binaries by dynamical friction and three-body encounters

Formation of Kuiper-belt binaries by dynamical friction and three-body encounters

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_72754618

Formation of Kuiper-belt binaries by dynamical friction and three-body encounters

About this item

Full title

Formation of Kuiper-belt binaries by dynamical friction and three-body encounters

Publisher

London: Nature Publishing Group UK

Journal title

Nature (London), 2002-12, Vol.420 (6916), p.643-646

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

The Kuiper belt is a disk of icy bodies that orbit the Sun beyond Neptune
1
; the largest known members are Pluto and its companion Charon. A few per cent of Kuiper-belt bodies have recently been found to be binaries with wide separations and mass ratios of the order of unity
2
,
3
,
4
,
5
,
6
,
7
,
8

Alternative Titles

Full title

Formation of Kuiper-belt binaries by dynamical friction and three-body encounters

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_72754618

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_72754618

Other Identifiers

ISSN

0028-0836

E-ISSN

1476-4687

DOI

10.1038/nature01227

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