TOI-1117

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TOI-1117

The location of TOI-1117 in the sky, the star is located in the white circle.
Observation data
Epoch J2000      Equinox J2000
Constellation Pavo[1]
Right ascension 18h 14m 24.534s[2]
Declination −66° 25 11.31[2]
Apparent magnitude (V) 11.016[citation needed]
Characteristics
Evolutionary stage main sequence[2]
Astrometry
Radial velocity (Rv)−24.73±0.24[2] km/s
Proper motion (μ) RA: −15.491 mas/yr[2]
Dec.: −38.741 mas/yr[2]
Parallax (π)5.9951±0.0154 mas[2]
Distance544 ± 1 ly
(166.8 ± 0.4 pc)
Details[3]
Mass0.97±0.02 M
Radius1.05±0.03 R
Luminosity0.363 L
Surface gravity (log g)4.41±0.03 cgs
Temperature5635±62 K
Metallicity [Fe/H]+0.136±0.044 dex
Rotation40 days
Rotational velocity (v sin i)1.32±0.04 km/s
Age4.42±1.50[4] Gyr
Other designations
TOI-1117, TIC 295541511, 2MASS J18142452-6625113[5]
Database references
SIMBADdata
Exoplanet Archivedata

TOI-1117 is a single G-type star in the constellation of Pavo.[6] It has approximately 0.97 times the mass and 1.05 times the radius of the Sun, with a surface temperature of 5,635±62 K and a spectral type of G7.[3] TOI-1117 is too faint to be visible to the naked eye. Based upon parallax measurements, it is located 544 light-years (166.8 parsecs) from the Sun.[7] The object is drifting towards the Sun with a radial velocity of −24.73 km/s.[8]

See also

References

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