Atlas (star)

Atlas
Image of the Pleiades star cluster
Atlas in the Pleiades cluster (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
Right ascension 03h 49m 09.74258s
Declination +24° 03′ 12.3003″
Apparent magnitude (V) 3.63 (3.84 / 5.46)
Characteristics
Spectral type B8III
U−B color index −0.36
B−V color index −0.08
Variable type SPB
Astrometry
Radial velocity (Rv) 8.5±2 km/s
Proper motion (μ) RA: +17.70 mas/yr
Dec.: −44.18 mas/yr
Parallax (π) 8.53 ± 0.39 mas
Distance 431 ± 13 ly
(132±4 pc)
Absolute magnitude (MV) −1.82
Orbit
Primary Aa1
Companion Aa2
Period (P) 290.984±0.079 d
Semi-major axis (a) 13.08±0.12 mas
Eccentricity (e) 0.2385±0.0063
Inclination (i) 107.87±0.49°
Longitude of the node (Ω) 154.0±0.7°
Periastron epoch (T) JD 2450583.0±1.9
Argument of periastron (ω)
(secondary)
151.9±2.2°
Semi-amplitude (K1)
(primary)
26.55±1.41 km/s
Semi-amplitude (K2)
(secondary)
36.89±0.22 km/s
Details
Aa1
Mass 4.74±0.25 M
Radius 7.9 R
Surface gravity (log g) 3.32±0.09 cgs
Temperature 13,446±218 K
Rotational velocity (v sin i) 280 km/s
Aa2
Mass 3.42±0.25 M
Radius 3.2 R
Surface gravity (log g) 3.96±0.09 cgs
Temperature 13,660 K
Ab
Mass 2.09 M
Other designations
27 Tau, BD+23°557, FK5 142, HD 23850, HIP 17847, HR 1178, SAO 76228
Database references
SIMBAD data

Atlas , designation 27 Tauri, is a triple star system in the constellation of Taurus. It is a member of the Pleiades, an open star cluster (M45). It is 431 light-years (132 parsecs) away, and is 3.92 degrees north of the ecliptic.

Nomenclature

27 Tauri is the star's Flamsteed designation.

In 2016 the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalogue and standardize proper names for stars. The WGSN approved the name Atlas for this star on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names.

Mythology

Atlas was a Titan and the father of the Pleiades sisters in Greek mythology.

Properties

Atlas is a triple star system, with the inner pair orbiting in under a year and the outer star orbiting in 260 years. The outer star, component Ab (sometimes component B, such as in CCDM and SIMBAD), has been resolved at a distance of 0.784 from the unresolved spectroscopic binary. It is too close to have been assigned a spectral class, but has an apparent magnitude of 6.8, three magnitudes fainter than the combined magnitude of the closer pair. Its mass is estimate to be twice that of the Sun. In the WDS catalog, there are 8 other stars, ranging from B-I, which have been classed as companions of Atlas.

A light curve for Atlas, adapted from White et al. (2017)

The inner pair have a well-defined orbit with a period of 291 days, a semi-major axis of 13 mas, and an eccentricity of 0.24. At an inclination of 108°, it is not thought to show eclipses. Although the two stars cannot be resolved, the primary, component Aa1, is calculated to be 1.6 magnitudes brighter than the secondary, component Aa2.

Low amplitude variability of the brightness of Atlas was tentatively detected in observations by STEREO and clearly detected by Kepler/K2. The light curve varies with several periods, the most prominent being 2.427, 0.7457 and 1.214 days.