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Extremely strong polarization of an active asteroid (3200) Phaethon
The near-Earth asteroid (3200) Phaethon is the parent body of the Geminid meteor stream. Phaethon is also an active asteroid with a very blue spectrum. We conducted polarimetric observations of this asteroid over a wide range of solar phase angles α during its close approach to the Earth in autumn 2...
Autores principales: | , , , , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
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Nature Publishing Group UK
2018
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6021421/ https://www.ncbi.nlm.nih.gov/pubmed/29950658 http://dx.doi.org/10.1038/s41467-018-04727-2 |
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author | Ito, Takashi Ishiguro, Masateru Arai, Tomoko Imai, Masataka Sekiguchi, Tomohiko Bach, Yoonsoo P. Kwon, Yuna G. Kobayashi, Masanori Ishimaru, Ryo Naito, Hiroyuki Watanabe, Makoto Kuramoto, Kiyoshi |
author_facet | Ito, Takashi Ishiguro, Masateru Arai, Tomoko Imai, Masataka Sekiguchi, Tomohiko Bach, Yoonsoo P. Kwon, Yuna G. Kobayashi, Masanori Ishimaru, Ryo Naito, Hiroyuki Watanabe, Makoto Kuramoto, Kiyoshi |
author_sort | Ito, Takashi |
collection | PubMed |
description | The near-Earth asteroid (3200) Phaethon is the parent body of the Geminid meteor stream. Phaethon is also an active asteroid with a very blue spectrum. We conducted polarimetric observations of this asteroid over a wide range of solar phase angles α during its close approach to the Earth in autumn 2016. Our observation revealed that Phaethon exhibits extremely large linear polarization: P = 50.0 ± 1.1% at α = 106.5°, and its maximum is even larger. The strong polarization implies that Phaethon’s geometric albedo is lower than the current estimate obtained through radiometric observation. This possibility stems from the potential uncertainty in Phaethon’s absolute magnitude. An alternative possibility is that relatively large grains (~300 μm in diameter, presumably due to extensive heating near its perihelion) dominate this asteroid’s surface. In addition, the asteroid’s surface porosity, if it is substantially large, can also be an effective cause of this polarization. |
format | Online Article Text |
id | pubmed-6021421 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2018 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-60214212018-06-29 Extremely strong polarization of an active asteroid (3200) Phaethon Ito, Takashi Ishiguro, Masateru Arai, Tomoko Imai, Masataka Sekiguchi, Tomohiko Bach, Yoonsoo P. Kwon, Yuna G. Kobayashi, Masanori Ishimaru, Ryo Naito, Hiroyuki Watanabe, Makoto Kuramoto, Kiyoshi Nat Commun Article The near-Earth asteroid (3200) Phaethon is the parent body of the Geminid meteor stream. Phaethon is also an active asteroid with a very blue spectrum. We conducted polarimetric observations of this asteroid over a wide range of solar phase angles α during its close approach to the Earth in autumn 2016. Our observation revealed that Phaethon exhibits extremely large linear polarization: P = 50.0 ± 1.1% at α = 106.5°, and its maximum is even larger. The strong polarization implies that Phaethon’s geometric albedo is lower than the current estimate obtained through radiometric observation. This possibility stems from the potential uncertainty in Phaethon’s absolute magnitude. An alternative possibility is that relatively large grains (~300 μm in diameter, presumably due to extensive heating near its perihelion) dominate this asteroid’s surface. In addition, the asteroid’s surface porosity, if it is substantially large, can also be an effective cause of this polarization. Nature Publishing Group UK 2018-06-27 /pmc/articles/PMC6021421/ /pubmed/29950658 http://dx.doi.org/10.1038/s41467-018-04727-2 Text en © The Author(s) 2018 Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/. |
spellingShingle | Article Ito, Takashi Ishiguro, Masateru Arai, Tomoko Imai, Masataka Sekiguchi, Tomohiko Bach, Yoonsoo P. Kwon, Yuna G. Kobayashi, Masanori Ishimaru, Ryo Naito, Hiroyuki Watanabe, Makoto Kuramoto, Kiyoshi Extremely strong polarization of an active asteroid (3200) Phaethon |
title | Extremely strong polarization of an active asteroid (3200) Phaethon |
title_full | Extremely strong polarization of an active asteroid (3200) Phaethon |
title_fullStr | Extremely strong polarization of an active asteroid (3200) Phaethon |
title_full_unstemmed | Extremely strong polarization of an active asteroid (3200) Phaethon |
title_short | Extremely strong polarization of an active asteroid (3200) Phaethon |
title_sort | extremely strong polarization of an active asteroid (3200) phaethon |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6021421/ https://www.ncbi.nlm.nih.gov/pubmed/29950658 http://dx.doi.org/10.1038/s41467-018-04727-2 |
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