The sun could come from a large, loose-knit clan or a small family thats always fighting.
New computer simulations of young stars suggest two pathways to forming the solar system. The sun could have formed in a calm, large association of 10,000 stars or more, like NGC 2244 in the present-day Rosette Nebula, an idea thats consistent with previous research. Or the sun could be from a violent, compact cluster with about 1,000 stars, like the Pleiades, researchers report July 2 in the Astrophysical Journal.
Whether a star forms in a tight, rowdy cluster or a loose association can influence its future prospects. If a star is born surrounded by lots of massive siblings that explode as supernovas before a cluster spreads out, for example, that star will have more heavy elements to build planets with (SN: 8/9/19).
To nail down a stellar birthplace, astronomers have considered the solar systems chemistry, its shape and many other factors. Most astronomers who study the suns birthplace think the gentle, large association scenario is most likely, says astrophysicist Fred Adams of the University of Michigan in Ann Arbor, who was not involved in the new work.
But most previous studies didnt include stars motions over time. So astrophysicists Susanne Pfalzner and Kirsten Vincke, both of the Max Planck Institute for Radio Astronomy in Bonn, Germany, ran thousands of computer simulations to see how often different kinds of young stellar families produce solar systems like ours.
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The main solar system feature that the pair looked for was the distance to the farthest planet from the star. Planet-forming disks can extend to hundreds of astronomical units, or AU, the distance between the Earth and the sun (SN: 7/16/19). Theoretically, planets should be able to form all the way to the edge. But the suns planetary material is mostly packed within the orbit of Neptune.
You have a steep drop at 30 AU, where Neptune is, Pfalzner says. And this is not what you expect from a disk.
In 2018, Pfalzner and her colleagues showed that a passing star could have truncated and warped the solar systems outer edge long ago. If thats what happened, it could help point to the suns birth environment, Pfalzner reasoned. The key was to simulate groupings dense enough that stellar flybys happen regularly, but not so dense that the encounters happen too often and destroy disks before planets can grow up.
We were hoping wed get one answer, Pfalzner says. It turned out there are two possibilities. And they are wildly different from each other.
Large associations have more stars, but the stars are more spread out and generally leave each other alone. Those associations can stay together for up to 100 million years. Compact clusters, on the other hand, see more violent encounters between young stars and dont last as long. The stars shove each other away within a few million years.
This paper opens up another channel for what the suns birth environment looked like, Adams says, referring to the violent cluster notion.
The new study doesnt cover every aspect of how a tight cluster could have affected the nascent solar system. The findings dont account for how radiation from other stars in the cluster could erode planet-forming disks, for example, which could have shrunk the suns disk or even prevented the solar system from forming. The study also doesnt explain certain heavy elements found in meteorites, which are thought to come from a nearby supernova and so could require the sun come from a long-lived stellar family.
I think [the research] is an interesting addition to the debate, Adams says. It remains to be seen how the pieces of the puzzle fit together.
Pfalzner thinks that the star cluster would break apart before radiation made a big difference, and there are other explanations for the heavy elements apart from a single supernova. She hopes future studies will be able to use that sort of cosmic chemistry to narrow the suns birthplace down even further.
For us humans, this is an important question, Pfalzner says. Its part of our history.
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