A binary main-belt comet
Jessica Agarwal (),
David Jewitt,
Max Mutchler,
Harold Weaver and
Stephen Larson
Additional contact information
Jessica Agarwal: Max Planck Institute for Solar System Research
David Jewitt: Planetary and Space Sciences, University of California at Los Angeles
Max Mutchler: Space Telescope Science Institute
Harold Weaver: The Johns Hopkins University Applied Physics Laboratory
Stephen Larson: Lunar and Planetary Laboratory, University of Arizona
Nature, 2017, vol. 549, issue 7672, 357-359
Abstract:
Analysis based on high-resolution observations from the Hubble Space Telescope shows that the asteroid 288P is a binary main-belt comet, with properties unlike any known binary asteroid.
Date: 2017
References: Add references at CitEc
Citations:
Downloads: (external link)
https://www.nature.com/articles/nature23892 Abstract (text/html)
Access to the full text of the articles in this series is restricted.
Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.
Export reference: BibTeX
RIS (EndNote, ProCite, RefMan)
HTML/Text
Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:549:y:2017:i:7672:d:10.1038_nature23892
Ordering information: This journal article can be ordered from
https://www.nature.com/
DOI: 10.1038/nature23892
Access Statistics for this article
Nature is currently edited by Magdalena Skipper
More articles in Nature from Nature
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().