An early extrasolar planetary system revealed by planetesimal belts in beta Pictoris.
beta Pictoris (beta Pic) is a main-sequence star with an edge-on dust disk 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 comets. 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 beta 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'.
Okamoto
Yoshiko Kataza
YK
Center for Natural Sciences, College of Liberal Arts and Sciences, Kitasato University, 1-15-1 Kitazato, Sagamihara, Kanagawa 228-8555, Japan. okamtoys@cc.nao.ac.jp
Kataza
Hirokazu
H
Honda
Mitsuhiko
M
Yamashita
Takuya
T
Onaka
Takashi
T
Watanabe
Jun-Ichi
J
Miyata
Takashi
T
Sako
Shigeyuki
S
Fujiyoshi
Takuya
T
Sakon
Itsuki
I