L 98-59

L 98-59
Observation data
Epoch J2000      Equinox J2000
Constellation Volans
Right ascension 08h 18m 07.62144s
Declination −68° 18 46.8054
Apparent magnitude (V) 11.69±0.05
Characteristics
Evolutionary stage Red dwarf (main sequence)
Spectral type M3V
B−V colour index +1.53
R−I colour index +1.28
Variable type None
Astrometry
Radial velocity (Rv)−6.10±0.19 km/s
Proper motion (μ) RA: 94.794(18) mas/yr
Dec.: −340.084(20) mas/yr
Parallax (π)94.2664±0.0155 mas
Distance34.599 ± 0.006 ly
(10.608 ± 0.002 pc)
Details
Mass0.273±0.030 M
Radius0.303+0.026
−0.023
 R
Luminosity (bolometric)0.01128±0.00042 L
Surface gravity (log g)4.86±0.13 cgs
Temperature3415±135 K
Metallicity [Fe/H]−0.46±0.26 dex
Rotation80.9+5.0
−5.3
 d
Age>800 Myr
Other designations
L 98-59, NLTT 19357, TOI-175, TIC 307210830, TYC 9193-2365-1, 2MASS J08180763-6818468
Database references
SIMBADdata
Exoplanet Archivedata

L 98-59 (TOI-175, TIC 307210830) is a bright M dwarf star, located in the constellation of Volans, at a distance of 10.608 parsecs (34.60 light-years), as measured by the Gaia spacecraft.

Broadband photometry shows that it is an M3 dwarf star with three confirmed terrestrial-sized planets in transit, which were announced in March 2019 by TESS, as well as a fourth non-transiting planet and fifth candidate.

In August 2021, new evidence was announced for a fifth, potentially habitable planet, labeled L 98-59 f. Though still unconfirmed, this planet is believed to have 2.46 times Earth's mass, and an orbital period of 23.15 days.