| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Taurus |
| Right ascension | 03h45m 54.47676s[1] |
| Declination | +24° 33′ 16.2418″[1] |
| Apparent magnitude (V) | 5.76[2] |
| Characteristics | |
| Evolutionary stage | main sequence[2] |
| Spectral type | B8 V[3] |
| B−V color index | +0.04[2] |
| Astrometry | |
| Radial velocity (Rv) | +6.0±0.6[4] km/s |
| Proper motion (μ) | RA: +20.025[5] mas/yr Dec.: −45.949[5] mas/yr |
| Parallax (π) | 7.5658 ± 0.1321 mas[1] |
| Distance | 431 ± 8 ly (132 ± 2 pc) |
| Absolute magnitude (MV) | +0.34[6] |
| Details | |
| Mass | 2.93±0.07[2] M☉ |
| Luminosity | 100+15 −13[2] L☉ |
| Surface gravity (log g) | 4.250±0.113[7] cgs |
| Temperature | 11,041±76[2] K |
| Rotational velocity (v sin i) | 159[8] km/s |
| Age | 100[9] Myr |
| Other designations | |
Asterope, Sterope I[10], 21 Tau, BD+24° 553, GC 4502, HD 23432, HIP 17579, HR 1151, SAO 76159[11] | |
| Database references | |
| SIMBAD | data |
21 Tauri, formally known as Asterope /əˈstrɛrəpiː/,[12][13] is a component of the Asterope double star in the Pleiades open cluster. 21 Tauri is the stars' Flamsteed designation. This star is potentially faintly visible to the naked eye with an apparent visual magnitude of 5.76 in ideal conditions,[2] although anybody viewing the object is likely to instead see the pair as a single elongated form of magnitude 5.6.[14] The distance to 21 Tauri can be estimated from its annual parallax shiftof7.6 mas,[1] yielding a range of around 431 light years. It is moving further from the Earth with a heliocentric radial velocity of +6 km/s.[4]
Asterope was one of the Pleiades sistersinGreek mythology. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[15] to catalogue and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems.[16] It approved the name Asterope for 21 Tauri on 21 August 2016 and it is now so included in the List of IAU-approved Star Names.[13]
21 Tauri is a blue-white hued B-type main sequence star with a stellar classification of B8 V.[3] It is a single[17] star with around three[2] times the mass of the Sun and is 100[9] million years old. The star is radiating 100[2] times the Sun's luminosity from its photosphere at an effective temperature of 11,041 K.[2] It displays an infrared excess, but this is due to reflection nebula rather than a circumstellar disk.[9]
