HK Aquarii

Source: Wikipedia, the free encyclopedia.
HK Aquarii

A visual band light curve for HK Aquarii, adapted from Young et al. (1990)[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension 23h 08m 19.55110s[2]
Declination 15° 24′ 35.7682″[2]
Apparent magnitude (V) 10.99±0.02[3]
10.72 - 10.94[4]
Characteristics
Evolutionary stage Main sequence
Spectral type M0Ve[5]
U−B color index +1.118[6]
B−V color index +1.31[3]
Variable type
UV Cet[4]
Distance
81.25 ± 0.09 ly
(24.91 ± 0.03 pc)
Absolute magnitude (MV)+9.13[6]
Details
Myr
HIP
 114252
Database references
SIMBADdata

HK Aquarii is a single

light years from the Sun based on parallax.[2] The radial velocity is poorly constrained but it appears to be drifting further away at a rate of ~2 km/s.[7]

This is a small

HK Aquarii is classified as a

flares.[11] Star spots have been reported at a variety of latitudes, but not at the poles.[12] Flaring activity was reported in 1987, and a steady X-ray emission has been detected.[9] These are characteristic of very young stars; although it is not close to any youthful open cluster, it is a possible ejected member of the Pleiades.[11] (A 2016 study instead suggests it is a member of the Octans association.[10]
)

The signature of prominences has been detected in the star's atmosphere. These display evidence of periodic oscillations and can reach altitudes greater than two-third's of the star's radius. The prominences can obtain a higher mass and volume compared to similar features on the Sun.[13]

References