Peter 393
Star gliese 393 |
|||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
AladinLite | |||||||||||
Observation dates equinox : J2000.0 , epoch : J2000.0 |
|||||||||||
Constellation | sextant | ||||||||||
Right ascension | 10 h 28 m 55.55 s | ||||||||||
declination | + 00 ° 50 ′ 27.6 ″ | ||||||||||
Apparent brightness | 9.65 likes | ||||||||||
Typing | |||||||||||
Spectral class | M2.0 Ve | ||||||||||
Astrometry | |||||||||||
parallax | (142.19 ± 0.05) mas | ||||||||||
distance | 23.0 ± 0.4 ly 7.1 ± 0.1 pc |
||||||||||
Physical Properties | |||||||||||
Dimensions | 0.41 M ☉ | ||||||||||
radius | 0.41 R ☉ | ||||||||||
Luminosity |
0.0235 L ☉ |
||||||||||
Metallicity [Fe / H] | −0.11 ± 0.04 | ||||||||||
Other names and catalog entries |
|||||||||||
|
Gliese 393 is a red dwarf star in the constellation Sextant . With an apparent magnitude of 9.65 mag, the star shines far too weakly to be seen with the naked eye. As a small star, it has about 41% the mass and radius of the Sun, but only 2.35% of its luminosity .
Individual evidence
- ↑ a b c d BD +01 2447. In: SIMBAD . Center de Données astronomiques de Strasbourg , accessed August 26, 2018 .
- ↑ a b c d Maldonado, J. et al .: Stellar parameters of early-M dwarfs from ratios of spectral features at optical wavelengths . In: Astronomy & Astrophysics . 577, 2015, p. 13. arxiv : 1503.03010 . A132. bibcode : 2015A & A ... 577A.132M . doi : 10.1051 / 0004-6361 / 201525797 .