Theia and Earth Were Neighbors

Table of Contents

New research, published in Max Planck Institute for Solar System Research, suggests that Theia, the body that collided with Earth 4.5 billion years ago, creating the Moon, originated in the inner Solar System.

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. Image credit: © MPS / Mark A. Garlick

About 4.5 billion years ago, the most momentous event in the history of our planet occurred: a huge celestial body called Theia collided with the young Earth. How the collision unfolded and what exactly happened afterwards has not been conclusively clarified. What is certain, however, is that the size, composition, and orbit of the Earth changed as a result – and that the impact marked the birth of our constant companion in space, the Moon.

What kind of body was it that so dramatically altered the course of our planet’s development? How big was Theia? What was it made of? And from which part of the Solar System did it hurtle toward Earth? Finding answers to these questions is difficult. After all, Theia was completely destroyed in the collision. Nevertheless, traces of it can still be found today, for example in the composition of present-day Earth and Moon. In the study published on November 20, 2025, in the journal Science, researchers led by the Max Planck Institute for Solar System Research (MPS) and the University of Chicago used this information to deduce the possible “list of ingredients” of Theia – and thus its place of origin.

“The composition of a body archives its entire history of formation, including its place of origin.” Thorsten Kleine, Director at MPS and co-author of the new study

The ratios in which certain metal isotopes are present in a body are particularly revealing. Isotopes are variants of the same element that differ only in the number of neutrons in their atomic nucleus – and thus in their weight. In the early Solar System, the isotopes of a given element were probably not evenly distributed: At the outer edge of the Solar System, for example, the isotopes occurred in a slightly different ratio than near the Sun. Information about the origin of its original building blocks is thus stored in the isotopic composition of a body, the MPS’ article about the study explains.

Searching for traces of Theia in Earth and Moon
#

In the cited study, the research team determined the ratio of different iron isotopes in Earth and Moon rocks with unprecedented precision. To this end, they examined 15 terrestrial rocks and six lunar samples that astronauts from the Apollo missions brought back to Earth. The result is hardly surprising: as earlier measurements of the isotope ratios of chromium, calcium, titanium, and zirconium had already shown, Earth and Moon are indistinguishable in this respect.

However, the great similarity does not allow any direct conclusions about Theia. There are simply too many possible collision scenarios. Although most models assume that the Moon was formed almost exclusively from material from Theia, it is also possible that it consists primarily of material from the early Earth’s mantle or that the rocks from Earth and Theia mixed inseparably.

Reverse engineering of a planet
#

In order to learn more about Theia, the researchers applied a kind of reverse engineering for planets. Based on the matching isotope ratios in today’s terrestrial and lunar rocks, the team played through which compositions and sizes of Theia and which composition of the early Earth could have led to this final state.

In their investigations, the researchers looked not only at iron isotopes, but also at those of chromium, molybdenum, and zirconium. “These elements have different affinities for metal and therefore partition into planetary mantles in different proportions; this is why gold is so rare and precious!” explained Nicolas Dauphas of the University of Chicago and the University of Hong Kong. “They give us access to different phases of planetary formation,” he added.

Long before the devastating encounter with Theia, a kind of sorting process had taken place inside the early Earth. With the formation of the iron core, some elements such as iron and molybdenum accumulated there; they were afterwards largely absent from the rocky mantle. The iron found in the Earth’s mantle today can therefore only have arrived after the core was formed, for example on board of Theia. Other elements such as zirconium, which did not sink into the core, document the entire history of our planet’s formation.

Meteorites as a reference
#

Of the mathematically possible compositions of Theia and the early Earth that result from the calculations, some can be ruled out as implausible.

The most convincing scenario is that most of the building blocks of Earth and Theia originated in the inner Solar System. Earth and Theia are likely to have been neighbors. Timo Hopp, MPS scientist and lead author of the new study

While the composition of the early Earth can be represented predominantly as a mixture of known meteorite classes, this is not the case with Theia. Different meteorite classes originated in different areas of the outer Solar System. They therefore serve as reference material for the building material that was available during the formation of the early Earth and Theia. In the case of Theia, however, previously unknown material may also have been involved. Researchers believe this material’s origin to be closer to the Sun than Earth. The calculations therefore suggest that Theia originated closer to the Sun than our planet.

Citation
#

The article The Moon-forming impactor Theia originated from the inner Solar System was published in the Science journal. Authors: Timo Hopp, Nicolas Dauphas, Maud Boyet, Seth A. Jacobson, and Thorsten Kleine.

Acknowledgments
#

We thank CAPTEM and R. A. Ziegler -the researchers said- for providing the Apollo lunar samples; H. Becker (FU Berlin), N. T. Arndt (CNRS, Grenoble), and B. Marty (CNRS, Nancy) for providing the terrestrial samples; and the Robert A. Pritzker Center for Meteoritics at the Field Museum of Natural History (Chicago), the Smithsonian National Museum for Natural History (Washington, DC), the Institut für Planetologie Münster, and the National Aeronautics and Space Administration (NASA) for providing the meteorite samples. US Antarctic meteorite samples were recovered by the Antarctic Search for Meteorites (ANSMET) program, which has been funded by the National Science Foundation (NSF) and NASA, and characterized and curated by the Department of Mineral Sciences of the Smithsonian Institution and the Astromaterials Curation Office at the NASA Johnson Space Center.

Funding:
#

N.D. was supported by NASA grants 80NSSC20K1409, 80NSSC23K1022, 80NSSC21K0380, 80NSSC20K0821, and 80NSSC23K1163; NSF grant EAR-2001098; and Department of Energy grant DE-SC0022451. T.K. was supported by the Deutsche Forschungsgemeinschaft (DFG) project ID 263649064 and the European Research Council advanced grant no. 101019380.

Contact [Notaspampeanas](mailto: notaspampeanas@gmail.com)