JWST spots newly forming, and cloudy exoplanets

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Caption: Artist rendition of the YSES-1 System consisting of the ~16 Myr Sun-like star in the center, YSES-1 b and its dusty circumplanetary disk (right), and YSES-1 c with silicate clouds in its atmosphere (left). Credit: Ellis Bogat.
Caption: Artist rendition of the YSES-1 System consisting of the ~16 Myr Sun-like star in the center, YSES-1 b and its dusty circumplanetary disk (right), and YSES-1 c with silicate clouds in its atmosphere (left). Credit: Ellis Bogat.

The James Webb Space Telescope (JWST) has spied out two small planets - known as exoplanets - orbiting a young Sun-like star, a mere 310 light years away, say international researchers. The star, named YSES-1 has previously been seen to have two celestial bodies orbiting it, creatively named YSES-1 b and YSES-1 c. But now, with the help of the JWST, the researchers say one of the two exoplanets has an atmosphere filled with dusty clouds, and the other is surrounded by a disk, which is indicative of a newly forming planet.

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From: Springer Nature

JWST detects cloudy and newly forming exoplanets

Direct imaging of two exoplanets around the young Sun-like star YSES-1 reveals that one has an atmosphere filled with dusty clouds and the other is surrounded by a disk (indicative of a newly forming planet). These detailed observations, reported in Nature this week, were made by the JWST.

The YSES-1 system is made up of a young Sun-like star and two gas giants: YSES-1 b is closest to the star and YSES-1 c is the smaller outer planet. YSES-1 b and c are redder than other exoplanets (or brown dwarfs), suggesting that they may have distinct atmospheric properties. The system was observed with several telescopes before JWST; however, detailed observations of this system were not possible prior to the JWST programme.

New JWST images of the YSES-1 system are presented by Kielan Hoch and colleagues. These include the first direct observations of silicate clouds in the atmosphere of the exoplanet YSES-1 c, confirming previous theories about the composition of its atmosphere. The authors constrain the cloud composition, particle size and location in the atmosphere, reporting that the silicate clouds are likely to also contain iron, which may rain back down onto the planet. They estimate that the cloud particles are 0.1 μm or smaller. The authors also report the first observation of a silicate disk around YSES-1 b, a rare observation for substellar companion exoplanets. This observation indicates that YSES-1 b may be a relatively newly formed planet.

The findings offer new insights into early phases of exoplanet formation and atmosphere evolution

Journal/
conference:
Nature
Research:Paper
Organisation/s: Space Telescope Science Institute, Baltimore, MD, USA
Funder: S.P. is supported by the ANID FONDECYT Postdoctoral program No. 3240145 and an appointment to the NASA Postdoctoral Program at the NASA–Goddard Space Flight Center, administered by Oak Ridge Associated Universities under contract with NASA. Support for program JWST-GO-02044 was provided by NASA through a grant from the Space Telescope Science
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