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Exomoons
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Exomoons

Exomoons are natural satellites orbiting planets outside our solar system. Just as our Moon accompanies Earth, exomoons circle distant exoplanets. Finding them is extremely difficult—it’s like trying to spot a gnat flying around a firefly next to a distant lighthouse. While we know hundreds of moons in our system, we only have promising candidates like Kepler-1625b-i and Kepler-1708b-i around foreign stars. In young systems, scientists observe dust disks where these moons are still forming. They could be key to finding life, as they might maintain stable conditions similar to planets.
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Latest news from Exomoons

Radial velocity reveals for the first time planetary mass object around brown dwarf CD-35 2722 B
icon7. 7. 2026
iconStars | Exoplanets | Brown dwarfs | Exomoo
Image: Radial velocity reveals for the first time planetary mass object around brown dwarf CD-35 2722 B
Evidence for satellites orbiting the brown dwarf CD-35 2722 B has been identified using precise light measurements. While thousands of planets have been found orbiting stars, satellites around objects outside our solar system—known as exosatellites—have remained elusive and controversial. This study presents a strong detection of at least one, and possibly two, massive objects circling this brown dwarf, providing new data on how such systems form and evolve. The research utilized radial v...
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Radial velocity study puts upper limits on massive moons around Beta Pictoris b
icon4. 6. 2026
iconStars | Exoplanets | Exomoo
Image: Radial velocity study puts upper limits on massive moons around Beta Pictoris b
Radial velocity monitoring of Beta Pictoris b sets new upper limits on potential massive exomoons. While no moon was detected, the data constrains moon masses to 80 Earth masses at short periods and 1 Jupiter mass at longer periods, with future improvements planned....
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Exomoon signal in the Kepler 1513 system might be caused by a second exoplanet
icon5. 10. 2023 (accepted)
iconStars | Exoplanets | Kepler | Exomoo
Image: Exomoon signal in the Kepler 1513 system might be caused by a second exoplanet
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