Age data show planetesimals provided building materials for water-rich planets in the early solar system

Age data for certain classes of meteorite have made it possible to gain new findings on the origin of small water-rich astronomical bodies in the early solar system. These so-called planetesimals continually supplied building materials for planets—also for the Earth, whose original material contained little water.

The Earth received its actual water through planetesimals, which emerged at low temperatures in the outer solar system. Ice was available there as solid-state water—unlike with small bodies which had evolved earlier and were too hot for that, being closer to the sun.

Computational models carried out by an international research team, with participation by Earth scientists from Heidelberg University, have shown this on the basis of the age data, from which they were also able to read the parent bodies’ thermal evolution. The research is published in the journal Scientific Reports.

The planets of our solar system formed together with their mother star, and the Earth did likewise, emerging about 4.5 billion years ago around the sun. This happened in the habitable zone, which meant that water was able to exist in liquid form on its surface. The Earth, like other planets, also grew out of planetesimals. They emerge when large quantities of dust particles accrete in high pressure zones several thousand kilometers in diameter, and collapse under their own gravity.

“These small bodies did not just supply the building materials for the planets,” explains Prof. Dr. Mario Trieloff, who directs the Klaus Tschira Laboratory for Cosmochemistry at Heidelberg University’s Institute of Earth Sciences. They are also the source of the Earth’s water, the scientist adds.

The circumstances under which the planetesimals actually originated in the early solar system, and whether this was also possible for considerable periods of time, have so far not been finally clarified. Important information in this regard is supplied by the age data of certain classes of meteorites, which at some stage separated from small planets.

In cooperation with colleagues from Berlin, Bayreuth and Zurich (Switzerland), the Heidelberg scientists have derived the thermal evolution and point of origin of the mother bodies from this data. They show that some of the planetesimals formed very quickly, meaning within less than 2 million years. In that case, they heated up so strongly that they melted and lost all volatile elements, including their water.

Other planetesimals, according to the findings of the current study, arose later at lower temperatures in the outer solar system; they were partly able to conserve their water bound up in crystals.

The fact that these small bodies were also able to continually form at later stages of the solar system is, according to the scientists, due to various delaying effects counteracting the mechanisms of rapid origin, for example, collisions between dust agglomerates—the building materials of planetesimals—which prevented the rapid growth of small planets.

“The Earth accreted such small water-rich planets or their fragments in the form of asteroids or meteorites during its growth process and that is the only reason why it did not become a bone-dry planet, hostile to life,” says Dr. Wladimir Neumann, first author of the study, which is based on research carried out at Heidelberg University, the Institute of Planetary Research at the German Aerospace Center and the Institute of Geodesy at TU Berlin.

Since the origin of planetesimals in extrasolar planetary systems is based on the same physical laws as in our solar system, the scientists assume that there could also be planets similar to the Earth in other regions of space. If they have received water from small bodies in the course of their evolutionary history, they could meet the preconditions for the origin of life, according to Prof. Trieloff.