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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...

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Autores principales: 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
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2018
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.
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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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