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Solar System Formation

The processes by which the solar nebula collapsed into a protoplanetary disk, forming the sun and planets through gravity and magnetic fields.

Current stories

scienceOne report1 publisher

Meteorite grains from the solar system's first 200,000 years recorded a field stronger than Earth's

MIT researchers found magnetic traces in meteorite grains from the solar system's first 200,000 years that point to a field stronger than Earth's today. That places magnetism in the nebula while the sun was forming, though how much of the collapse it drove is still an estimate.

Publishers:sciencedaily.com

Reality

Evidence40
Adoption
Not scored
Hype gap+25
Incentives35
Confidence55
scienceOne report1 publisher

Half a gram of Bennu puts its birthplace at the solar system's water-ice line

An ETH Zurich lab measured iron, titanium and chromium in its share of the OSIRIS-REx return and found the same dust reservoir that produced Ryugu and the rare CI meteorites, a composition matching neither the inner nor the outer solar system.

Publishers:phys.org

Reality

Evidence66
Adoption30
Hype gap+12
Incentives55
Confidence62
scienceOne report1 publisher

Iron meteorite chemistry puts the earliest planetesimals at 8 to 17 percent icy dust

Yale researchers read the original makeup of planetesimals that melted so thoroughly their textures vanished, and place the Solar System's preference for heat-formed rock beads inside the first million years.

Publishers:sciencedaily.com

Reality

Evidence58
Adoption
Not scored
Hype gap+25
Incentives70
Confidence48
scienceOne report1 publisher

Melted meteorites date the sorting of rock over ice to the solar system's first million years

A Yale-led team could not sample planetesimals from the first million years, because every one of them melted, so it reconstructed their make-up from sulfur and iron oxidation in iron meteorites and got 8% to 17% icy dust.

Publishers:phys.org

Reality

Evidence62
Adoption
Not scored
Hype gap+18
Incentives55
Confidence58