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Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Columba |
Right ascension | 05h 30m 51.45227s[1] |
Declination | −36° 37′ 50.8957″[1] |
Apparent magnitude (V) | 15.57±0.03[2] |
Characteristics | |
Evolutionary stage | main sequence star[3] |
Spectral type | M0.5[3] |
B−V color index | +1.37[2] |
R−I color index | +1.39[4] |
Astrometry | |
Radial velocity (Rv) | 97.18±0.01[3] km/s |
Proper motion (μ) | RA: −31.887 mas/yr[1] Dec.: −41.077 mas/yr[1] |
Parallax (π) | 4.5935 ± 0.017 mas[1] |
Distance | 710 ± 3 ly (217.7 ± 0.8 pc) |
Details[3] | |
Mass | 0.617+0.023 −0.062 M☉ |
Radius | 0.573±0.077 R☉ |
Luminosity | (7.03±0.09)×10−2[5] L☉ |
Surface gravity (log g) | 4.71±0.23 cgs |
Temperature | 3,916+71 −63 K |
Rotational velocity (v sin i) | <1.0 km/s |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
NGTS-1, also designated as TOI-551 is a solitary star located in the southern constellation Columba, the dove. With an apparent magnitude of 15.52,[2] NGTS-1 can only be seen through a powerful telescope. Gaia DR3 parallax measurements imply a distance of 710 light-years[1] and it is drifting away rapidly with a heliocentric radial velocity of 97.2 km/s.[3]
GaiaDR3
was invoked but never defined (see the help page).Zacharias2013
was invoked but never defined (see the help page).Bayliss2017
was invoked but never defined (see the help page).Denis2005
was invoked but never defined (see the help page).GaiaDR2
was invoked but never defined (see the help page).