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JWST is currently being used to study exoplanets, particularly sub-Neptunes, providing valuable data on their atmospheric composition. A recent study utilized JWST spectroscopy to analyze the atmosphere of the sub-Neptune GJ 3090b. This planet orbits a late-type, low-mass star and its radius places it at the outer edge of the radius valley. Sub-Neptunes are the most common type of planet in the Milky Way, however their formation and composition are not well understood, making these studies especially important.
The JWST's observations of GJ 3090b revealed a low-amplitude helium signature, suggesting a metal-enriched atmosphere. The presence of heavy molecules like water, carbon dioxide, and sulfur further contributes to the understanding of the planet's atmospheric properties. These atmospheric observations help clarify how hydrogen and helium may be escaping the planet’s atmosphere, with the presence of metals slowing down mass loss and weakening the helium signature.
While JWST is making significant contributions to exoplanet research, it won't find the very first stars. Other telescopes will be needed to make those observations. JWST however contains some of the latest discoveries, including the new cosmic record-holder for the most distant galaxy, MoM-z14.
ImgSrc: aasnova.org
References :
- StartsWithABang: Earlier this week, I gave a talk about JWST to the RASC Toronto audience through York University, and it has the latest and greatest of its discoveries inside, including the new cosmic record-holder for most distant galaxy: MoM-z14. Check it out!
- aasnova.org: Abundant but Ambiguous: Understanding the Atmospheres of Sub-Neptunes with JWST
Classification:
- HashTags: #JWST #Exoplanets #Astrochemistry
- Company: AASNova
- Target: Exoplanets
- Product: Astronomy
- Feature: Atmosphere
- Type: Research
- Severity: Informative