惑星誕生の最初期を観測(Astronomers witness the dawn of a new solar system for the first time)

2025-07-16 ミシガン大学

惑星誕生の最初期を観測(Astronomers witness the dawn of a new solar system for the first time)This is HOPS-315, a baby star where astronomers have observed evidence for the earliest stages of planet formation. Image credit: ALMA(ESO/NAOJ/NRAO)/M. McClure et al.

ミシガン大学らの国際研究チームは、約1300光年先の若い恒星HOPS‑315周辺で、惑星の種「プラネテシマル」が誕生する瞬間を初めて観測。JWSTで検出されたシリコン一酸化物とALMAのデータから、小惑星帯相当の軌道上で塵とガスが結晶化し固体化し始めていることが確認された。これは地球型惑星形成の初期段階と一致し、太陽系以外でも類似過程が起こる可能性を示唆。成果はNature誌に発表された。

<関連情報>

原始惑星系円盤における難固体凝縮の検出 Refractory solid condensation detected in an embedded protoplanetary disk

M. K. McClure,Merel van’t Hoff,Logan Francis,Edwin Bergin,Will R. M. Rocha,J. A. Sturm,Daniel Harsono,Ewine F. van Dishoeck,John H. Black,J. A. Noble,D. Qasim & E. Dartois
Nature  Published:16 July 2025
DOI:https://doi.org/10.1038/s41586-025-09163-z

Abstract

Terrestrial planets and small bodies in our Solar System are theorized to have assembled from interstellar solids mixed with rocky solids that precipitated from a hot, cooling gas1,2. The first high-temperature minerals to recondense from this gaseous reservoir start the clock on planet formation3,4. However, the production mechanism of this initial hot gas and its importance to planet formation in other systems are unclear. Here we report the astronomical detection of this t = 0 moment, capturing the building blocks of a new planetary system beginning its assembly. The young protostar HOPS-315 is observed at infrared and millimetre wavelengths with the James Webb Space Telescope (JWST) and the Atacama Large Millimeter Array (ALMA), revealing a reservoir of warm silicon monoxide gas and crystalline silicate minerals low in the atmosphere of a disk within 2.2 au of the star, physically isolated from the millimetre SiO jet. Comparison with condensation models with rapid grain growth and disk structure models suggests the formation of refractory solids analogous to those in our Solar System. Our results indicate that the environment in the inner disk region is influenced by sublimation of interstellar solids and subsequent refractory solid recondensation from this gas reservoir on timescales comparable with refractory condensation in our own Solar System.

1701物理及び化学
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