テイアと地球は隣り合う天体だった:月形成に関する新証拠(Theia and Earth were neighbors)

2025-11-20 マックス・プランク研究所(MPG)

若い地球に約45億年前に衝突し、月(Moon)を形成したとされる惑星衝突体“Theia”の起源に関する新しい研究では、Theiaが地球よりも太陽側、すなわち太陽系の「内側」から来た可能性が高いと結論づけられた。研究チームは、地球と月の岩石中に含まれる鉄同位体比を精密に測定し、さらにクロム、モリブデン、ジルコニウムなどの同位体比とも照合。これらの元素は惑星体がどこで、どのように形成されたかを示す手がかりになる。解析結果によると、地球と月は同位体組成がほぼ同じであったが、Theiaの構成物質は地球のものとは少し異なり、「ほぼ隣接する成分」で形成された惑星として位置づけられる。つまり、地球とTheiaは同じく内太陽系起源であり、互いに近い位置で誕生・進化した可能性がある。この発見は、月形成の「大衝突仮説」において衝突体の起源をめぐる謎解きの大きな前進となる。

テイアと地球は隣り合う天体だった:月形成に関する新証拠(Theia and Earth were neighbors)
Artist’s impression of the collision between the early Earth and Theia. Since Theia originated in the inner Solar System, in this perspective the Sun can be seen in the background.  © MPS / Mark A. Garlick

<関連情報>

月形成衝突体テイアは太陽系内部から発生した The Moon-forming impactor Theia originated from the inner Solar System

Timo Hopp, Nicolas Dauphas, Maud Boyet, Seth A. Jacobson, and Thorsten Kleine
Science  Published:20 Nov 2025
DOI:https://doi.org/10.1126/science.ado0623

Editor’s summary

In the early Solar System, a small planet known as Theia collided with proto-Earth. The debris from that giant impact formed the Moon, with material from Theia incorporated into both the Moon and Earth. Hopp et al. measured iron isotopes in lunar samples, Earth samples, and meteorites. They then combined these results with previous measurements of other elements with different geochemical behaviors. By simultaneously calculating the contributions of Theia material to each of those elements in both bodies, the authors concluded that Theia formed in the inner Solar System, nearby to Earth but possibly slightly closer to the Sun. —Keith T. Smith

Abstract

The Moon formed from a giant impact of a planetary body, called Theia, with proto-Earth. It is unknown whether Theia formed in the inner or outer Solar System. We measured iron isotopes in lunar samples, terrestrial rocks, and meteorites representing the isotopic reservoirs from which Theia and proto-Earth might have formed. Earth and the Moon have indistinguishable mass-independent iron isotopic compositions; both define one end of the range measured in meteorites. Combining our results with those for other elements, we performed mass balance calculations for Theia and proto-Earth. We found that all of Theia and most of Earth’s other constituent materials originated from the inner Solar System. Our calculations suggest that Theia might have formed closer to the Sun than Earth did.

1702地球物理及び地球化学
ad
ad
Follow
ad
タイトルとURLをコピーしました