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Extremely strong polarization of an active asteroid (3200) Phaethon
Takashi Ito1, Masateru Ishiguro2, Tomoko Arai3
1Center for Computational Astrophysics, National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka, Tokyo, 181-8588, Japan. tito.geoph.s@95.alumni.u-tokyo.ac.jp.
Polarimetric observations of near-Earth asteroid (3200) Phaethon reveal extremely high linear polarization. This suggests Phaethon may have a lower albedo or a surface dominated by large grains and high porosity.
Area of Science:
- Planetary Science
- Asteroid Research
- Observational Astronomy
Background:
- Near-Earth asteroid (3200) Phaethon is the parent body of the Geminid meteor stream.
- Phaethon is characterized as an active asteroid with a distinct blue spectral signature.
Purpose of the Study:
- To conduct polarimetric observations of asteroid (3200) Phaethon during its close approach to Earth.
- To analyze the relationship between solar phase angle and Phaethon's polarization properties.
- To investigate the implications of observed polarization on Phaethon's surface characteristics and albedo.
Main Methods:
- Utilized polarimetric observations over a broad range of solar phase angles (α).
- Conducted observations during the asteroid's close approach to Earth in autumn 2016.
- Analyzed the degree of linear polarization (P) as a function of solar phase angle.
Main Results:
- Observed exceptionally high linear polarization for Phaethon, reaching P = 50.0 ± 1.1% at α = 106.5°.
- The maximum polarization values observed were even greater.
- The results indicate a significant deviation from expected polarization patterns for typical asteroids.
Conclusions:
- The extreme polarization suggests Phaethon's geometric albedo may be lower than previously estimated from radiometric data.
- Alternatively, Phaethon's surface might be dominated by large grains (approx. 300 μm) possibly formed by perihelion heating.
- High surface porosity is also proposed as a significant factor contributing to the observed strong polarization.
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