TOI-5624 c

TOI-5624 c
Discovery
Discovered byAndrea Bonfant et al.
Discovery siteTransiting Exoplanet Survey Satellite
Discovery dateApril 22, 2026
Transit
Orbital characteristics
0.07374+0.00072
−0.00075
 AU
Eccentricity0 (fixed)
7.885385±0.000018 d
Inclination89.58+0.28
−0.27
90 (fixed)
Semi-amplitude1.70+0.69
−0.68
 m/s
StarTOI-5624
Physical characteristics
2.474±0.042 R🜨
Mass4.8±1.9 M🜨
Mean density
1.72+0.70
−0.69
 g/cm3
Temperature857 ± 11 K (583.9 ± 11.0 °C; 1,082.9 ± 19.8 °F)

TOI-5624 c is the second closest of the discovered exoplanets orbiting the star TOI-5624, located approximately 331 light-years from Earth in the constellation Ursa Major. The planet was confirmed in April 2026 using the transit method.[1][2]

Characteristics

Physical characteristics

Size comparison
Neptune TOI-5624 с

The planet is classified as a sub-Neptune, with a mass of 4.8±1.9 M🜨 determined by the radial velocity method, and a radius of 2.474±0.042 R🜨 determined by the CHEOPS telescope, with an uncertainty of less than 1.7%.[1][2] The object's average density is 1.72+0.70
−0.69
 g/cm3
.[1][2] Such a low value indicates a higher proportion of volatiles or a hydrogen-helium mixture in its composition.[1][2]

Orbit

The orbital period around its host star is approximately 7.885385±0.000018 Earth days. The semi-major axis of the orbit is estimated to be 0.07374+0.00072
−0.00075
 AU
.[1][2] The equilibrium temperature is approximately 858 K, or 584 °C.[1][2]

See also

References

  1. ^ a b c d e f Bonfanti, A.; et al. (2026-04-21). "The multi-planet system TOI-5624: Four transiting sub-Neptunes with an outer companion revealed by transit-timing variations". arXiv:2604.15035 [astro-ph.EP].
  2. ^ a b c d e f Cowing, Keith (2026-04-19). "The Multi-planet System TOI-5624: Four Transiting Sub-Neptunes With An Outer Companion Revealed By Transit-timing Variations". Astrobiology.com. Retrieved 2026-04-19.