A low-density gas giant exoplanet discovered orbiting a high-metallicity red dwarf star TOI-5688 A

2. 9. 2024 (accepted)

TOI-5688 is a binary star almost 750 light years away from the Sun. The newly discovered planet orbits the primary star every 2.9 days and has radius 10 times bigger than Earth which is similar to Saturn.

Scientific study

Searching for GEMS: TOI-5688 A b, a low-density giant orbiting a high-metallicity early M-dwarf external link

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Relevant stars in the catalog

TOI 5688

0.6 M☉

741 ly

A low-density gas giant exoplanet discovered orbiting a high-metallicity red dwarf star TOI-5688 A

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