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Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Octans[1] |
Right ascension | 21h37m 32.864s[2] |
Declination | −77° 58′ 43.51″[2] |
Characteristics | |
Evolutionary stage | main sequence star |
Spectral type | M0V |
Variable type | planetary transit |
Astrometry | |
Radial velocity (Rv) | −4.43±0.36[2] km/s |
Proper motion (μ) | RA: 120.333(19) mas/yr[2] Dec.: −91.503(18) mas/yr[2] |
Parallax (π) | 16.2487 ± 0.0184 mas[2] |
Distance | 200.7 ± 0.2 ly (61.54 ± 0.07 pc) |
Details | |
Mass | 0.6296 ±0.0086 M☉ |
Radius | 0.599 ±0.013 R☉ |
Luminosity | −1.13+0.03 −0.03 L☉ |
Temperature | 3901 ±69 K |
Other designations | |
Database references | |
SIMBAD | data |
TOI-4342 is a red dwarf star in the constellation Octans located 201 light-years from Earth.
It hosts two planets discovered in 2023.[4][5] They are locked in a near 2:1 orbital resonance.
TOI-4342 b is a Neptune-like body located 0.05251 AU from its star. Its orbital period around the star is 5.5 days. TOI-4342 b has a radius that is 0.202 that of Jupiter and a mass of 5.76 that of Earth. Its discovery in early 2023 was made through the use of a transit detection method of TOI-4342. The transit method was performed by the Transiting Exoplanet Survey Satellite (TESS). TOI-4342 b was the first of two exoplanets found orbiting TOI-4342. The other planet is TOI-4342 c.[4]
TOI-4342 c is a Neptune-like body located 0.0814 AU from its star. Its orbital period around the star is 10.7 days. TOI-4342 c has a radius that is 0.215 that of Jupiter and a mass of 6.41 that of Earth. Its discovery in early 2023 was made through the use of a transit detection method of TOI-4342. The transit method was performed by the Transiting Exoplanet Survey Satellite (TESS). TOI-4342 b was the first of two exoplanets found orbiting TOI-4342. The other planet is TOI-4342 b.[5]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 5.76 M🜨 | 0.05251 | 5.5 | 0 | — | — |
c | 6.41 M🜨 | 0.0814 | 10.7 | 0 | — | — |