| Literature DB >> 29950658 |
Takashi Ito1, Masateru Ishiguro2, Tomoko Arai3, Masataka Imai4, Tomohiko Sekiguchi5, Yoonsoo P Bach2, Yuna G Kwon2, Masanori Kobayashi3, Ryo Ishimaru3, Hiroyuki Naito6, Makoto Watanabe7, Kiyoshi Kuramoto4.
Abstract
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.Entities:
Year: 2018 PMID: 29950658 PMCID: PMC6021421 DOI: 10.1038/s41467-018-04727-2
Source DB: PubMed Journal: Nat Commun ISSN: 2041-1723 Impact factor: 14.919