CORDIS Project
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The DISKS-ROCK project investigates the environments where rocky planets form around different types of stars. By analyzing data from the James Webb Space Telescope, it aims to understand the differences in gas composition around T Tauri and Very Low Mass stars, which could influence planet formation and evolution.
The James Webb Space Telescope (JWST) now peers for the first time into the rocky planet birth environments around Solar-type (T Tauri - TT) and Very Low Mass stars (VLMS) with ages of 1-4 Myr.
The data shows that disk gas around TT stars is oxygen-rich, while it is carbon-rich around VLMS; yet they formed inside the same molecular cloud. VLMS are the most abundant stars in the galaxy, hosting most rocky exoplanets known to date, making them key targets to search for life.
Yet today, it is param…
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