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Planet formation

The scientific study of how planets form from protoplanetary disks via accretion, collisions, and migration, shaping their final orbits and compositions.

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scienceOne report1 publisher

Gemini South spectra put WASP-189b's magnesium-to-silicon ratio close to its star's

WASP-189b, nearly 320 light-years away, has a magnesium-to-silicon ratio that closely matches its host star's, astronomers report. Teams that predict rocky-planet makeup from stellar chemistry now have a check, made on a giant planet.

Publishers:sciencedaily.com

Reality

Evidence35
Adoption
Not scored
Hype gap+40
Incentives55
Confidence40
scienceOne report1 publisher

Webb and Spitzer spectra split 21 extreme debris disks into silica-rich and silica-poor groups

Kate Su's team combined Webb and Spitzer spectra to sort 21 extreme debris disks around young stars into silica-rich and silica-poor groups. NASA says the minerals encode how violent each dust-making collision was, a possible check on Moon-formation ideas.

Publishers:sciencedaily.com

Reality

Evidence60
Adoption
Not scored
Hype gap+20
Incentives55
Confidence55
scienceConfirmed4 publishers

Archival NASA-funded data confirm youngest known planet at under a million years old

Elias 2-24 b sits in a disk gap 55 times Earth's distance from its star, where formation models ask for at least five million years to build a Jupiter. Keck coronagraph images from 2018 and 2020 put it under a million years old.

Perspective Coverage

5 publishers
Builder
Builder 55%
Operator
Operator 31%
Investor
Investor 14%

Reality

Evidence68
Adoption
Not scored
Hype gap+20
Incentives40
Confidence66
scienceOne report1 publisher

Webb sorts 21 extreme debris disks by the violence of the crashes that made them

Kate Su's team used Webb and Spitzer spectra of 21 extreme debris disks to infer that about a third come from vaporizing impacts between Mars-sized bodies. Silica marks those violent cases, and it turns up only around stars younger than 300 million years.

Publishers:nasa.gov phys.org

Reality

Evidence60
Adoption
Not scored
Hype gap+10
Incentives40
Confidence55
scienceOne report1 publisher

Astronomers propose a second, tilted disk to explain GJ 3090 b's backward orbit around a red dwarf

University of Geneva astronomers and colleagues report that GJ 3090 b circles its red dwarf backward, 136 degrees out of line with the star's spin. Finding no companion able to flip it, the team suggests the planet formed in a second, tilted disk.

Publishers:livescience.com

Reality

Evidence58
Adoption
Not scored
Hype gap+8
Incentives
Not scored
Confidence50
scienceOne report1 publisher

Mantle chemistry suggests Earth grew mostly by pebble accretion and Mars mostly from planetesimals

University of Copenhagen researchers estimate at least 75% of Earth's mass came via pebble accretion and about three-quarters of Mars' from planetesimals. On this evidence, rocky neighbours can grow by different routes, though the models have to assume what the building blocks were made of.

Publishers:phys.org

Reality

Evidence45
Adoption
Not scored
Hype gap+10
Incentives
Not scored
Confidence45
scienceOne report1 publisher

Magnetic winds give way to stellar radiation as planet-forming disks age in a 72-star JWST survey

Astronomers led by the University of Arizona's Naman Bajaj used archival JWST data on 72 young Sun-like stars to show disk-stripping winds change with age. The survey identifies which force removes planet-building gas at each stage, but it does not yet put the giant-planet deadline in years.

Publishers:sciencedaily.com

Reality

Evidence55
Adoption
Not scored
Hype gap+20
Incentives30
Confidence55
scienceOne report1 publisher

Early Webb analyses put giant planet HATS-6 b about 300 degrees Celsius below its standard estimate

University of Maryland astronomers using Webb found ammonia on HATS-6 b and early temperatures near 120 C, against the 425 C usually cited. Their leading suspect is reflective cloud, and the planet's chemistry readings depend on that temperature.

Publishers:phys.org

Reality

Evidence55
Adoption
Not scored
Hype gap+15
Incentives
Not scored
Confidence50
scienceOne report1 publisher

ALMA images a planet five times Jupiter's mass interacting with the gas it formed in

MPIA astronomers used ALMA to image WISPIT 2b, a gas giant five times Jupiter's mass, interacting with the gas it formed in. Formation models have rested on simulations and indirect evidence, so a planet still feeding on its birth gas gives them a direct check.

Publishers:phys.org

Reality

Evidence55
Adoption
Not scored
Hype gap+15
Incentives30
Confidence55
scienceOne report1 publisher

GJ 3090 b runs backward around its M dwarf at 136 degrees to the star's equator

Planets inherit their direction of travel from the disk that formed them. A planet running backward around a small cool star is therefore a formation problem, and one team's answer is a second disk, tilted from the first.

Reality

Evidence66
Adoption
Not scored
Hype gap+12
Incentives38
Confidence62
scienceOne report1 publisher

ETH Zurich reanalysis caps Earth's outer Solar System material below 2 percent of its mass

Paolo Sossi and Dan Bower ran published meteorite data through ten isotope systems instead of the usual two, and found Earth's composition matches inner Solar System material alone, with under 2 percent from beyond Jupiter.

Publishers:sciencedaily.com

Reality

Evidence58
Adoption
Not scored
Hype gap+22
Incentives62
Confidence55
scienceOne report1 publisher

Feeding the young Sun a super-Earth squares its helioseismology with its missing lithium

In MNRAS, Ege University's Mutlu Yildiz reports solar models that swallow a planet of five to 10 Earth masses matching interior structure and low surface lithium in the same run, a fit that needs an independent detection before it means much.

Publishers:phys.org

Reality

Evidence56
Adoption
Not scored
Hype gap+18
Incentives62
Confidence54