James Webb spots massive exoplanet challenging planet formation limits

08:40

By: Dakir Madiha

James Webb spots massive exoplanet challenging planet formation limits

The NASA James Webb Space Telescope has captured direct images of a massive exoplanet that appears to have formed like a planet rather than a star, reshaping assumptions about how large planets can grow. The findings, published in The Astrophysical Journal Letters, focus on 29 Cygni b, a gas giant with a mass about 15 times that of Jupiter. The planet orbits a Sun-like star at a distance comparable to Uranus from the Sun.

The object lies at the boundary between two competing formation models. Planets typically form through gradual accumulation of dust and ice in protoplanetary disks, while stars form from the gravitational collapse of large gas clouds. At roughly 15 Jupiter masses, 29 Cygni b sits at the upper limit of what core accretion models predict and near the lower bound of star-like formation processes. This overlap has made it a critical test case for understanding how such objects originate.

Using Webb’s NIRCam instrument in coronagraphic mode, researchers detected carbon dioxide and carbon monoxide in the planet’s atmosphere. The data showed that 29 Cygni b is enriched in heavy elements compared with its host star, containing the equivalent of about 150 Earth masses in metals. This composition supports a formation history driven by solid material accumulation rather than gas cloud fragmentation, pointing toward a planetary origin despite its extreme size.

The team reinforced this conclusion with observations from the CHARA Array. They confirmed that the planet’s orbit is aligned with the rotation axis of its host star, a feature commonly seen in planetary systems formed within disks. This alignment mirrors the structure observed in our own solar system and strengthens the case for disk-based formation.

The discovery builds on earlier Webb results in the HR 8799 system, where similarly massive planets also showed chemical signatures consistent with planetary formation. Together, these findings suggest that core accretion can produce far larger worlds than previously thought. Researchers plan to study additional targets across a range of masses to identify the precise threshold where planets transition into star-like objects, a boundary that now appears less defined than once assumed.