Author
Listed:
- Yoshiko Kataza Okamoto
(Kitasato University
Japan Aerospace Exploration Agency
Ibaraki University)
- Hirokazu Kataza
(Japan Aerospace Exploration Agency)
- Mitsuhiko Honda
(University of Tokyo)
- Takuya Yamashita
(National Astronomical Observatory of Japan)
- Takashi Onaka
(University of Tokyo)
- Jun-ichi Watanabe
(National Astronomical Observatory of Japan)
- Takashi Miyata
(University of Tokyo)
- Shigeyuki Sako
(University of Tokyo)
- Takuya Fujiyoshi
(National Astronomical Observatory of Japan)
- Itsuki Sakon
(University of Tokyo)
Abstract
β Pictoris (β Pic) is a main-sequence star with an edge-on dust disk1,2,3 that might represent a state of the early Solar System. The dust does not seem to be a remnant from the original protoplanetary disk, but rather is thought to have been generated from large bodies like planetesimals and/or comets4,5. The history and composition of the parent bodies can therefore be revealed by determining the spatial distribution, grain size, composition and crystallinity of the dust through high-resolution mid-infrared observations. Here we report that the sub-micrometre amorphous silicate grains around β Pic have peaks in their distribution around 6, 16 and 30 au (1 au is the Sun–Earth distance), whereas the crystalline and micrometre-sized amorphous silicate grains are concentrated in the disk centre. As sub-micrometre grains are blown quickly out from the system by radiation pressure from the central star, the peaks indicate the locations of ongoing dust replenishment, which originates from ring-like distributions of planetesimals or ‘planetesimal belts’.
Suggested Citation
Yoshiko Kataza Okamoto & Hirokazu Kataza & Mitsuhiko Honda & Takuya Yamashita & Takashi Onaka & Jun-ichi Watanabe & Takashi Miyata & Shigeyuki Sako & Takuya Fujiyoshi & Itsuki Sakon, 2004.
"An early extrasolar planetary system revealed by planetesimal belts in β Pictoris,"
Nature, Nature, vol. 431(7009), pages 660-663, October.
Handle:
RePEc:nat:nature:v:431:y:2004:i:7009:d:10.1038_nature02948
DOI: 10.1038/nature02948
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