Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Vulpecula |
Right ascension | 20h 01m 06.0486s[1] |
Declination | +27° 45′ 12.863″[1] |
Apparent magnitude (V) | 4.66[2] (4.62 - 4.67)[3] |
Characteristics | |
Spectral type | A4IIIm[3] or kA5hA7mA7 (IV–V)[4] |
U−B color index | +0.15[5] |
B−V color index | +0.18[5] |
Variable type | α2 CVn[3] |
Astrometry | |
Radial velocity (Rv) | −26.10[6] km/s |
Proper motion (μ) | RA: 57.817±0.081[1] mas/yr Dec.: 3.994±0.085[1] mas/yr |
Parallax (π) | 13.4427 ± 0.1050 mas[1] |
Distance | 243 ± 2 ly (74.4 ± 0.6 pc) |
Absolute magnitude (MV) | 0.36[2] |
Details | |
Luminosity | 59.76[2] L☉ |
Surface gravity (log g) | 3.45[4] cgs |
Temperature | 8,084[7] K |
Metallicity [Fe/H] | +0.02[2] dex |
Rotational velocity (v sin i) | 15.0[8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
15 Vulpeculae is a variable star in the northern constellation of Vulpecula, located approximately 243 light years away based on parallax.[1] It has the variable star designation NT Vulpeculae; 15 Vulpeculae is the Flamsteed designation. It is visible to the naked eye as a faint, white-hued star with a typical apparent visual magnitude of 4.66.[2] This object is moving closer to the Earth with a heliocentric radial velocity of −26 km/s.[6]
This is an Am star with a stellar classification of A4 IIIm,[3] matching an evolved A-type giant star. However, Gray & Garrison (1989) found a class of kA5hA7mA7 (IV–V),[4] which matches a blend of subgiant and main sequence luminosity classes with the K-line (kA5) of an A5 star and the hydrogen (hA7) and metal (mA7) absorption lines of an A7 star. It is an Alpha2 Canum Venaticorum-type variable with magnitude ranging from 4.62 down to 4.67 over a period of 14 days.[3] The star is radiating 60[2] times the Sun's luminosity from its photosphere at an effective temperature of 8,084 K.[7]
Gaia EDR3
was invoked but never defined (see the help page).Kuvshinov
was invoked but never defined (see the help page).