HK Aquarii
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]
|
Absolute magnitude (MV) | +9.13[6] |
Details Myr | |
HIP 114252 | |
Database references | |
SIMBAD | data |
HK Aquarii is a singlelight 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
- doi:10.1086/168347. Retrieved 17 October 2021.
- ^ .
- ^ .
- ^ S2CID 125853869.
- ^ S2CID 16080025.
- ^ .
- ^ S2CID 119231169
- ^ .
- ^ doi:10.1046/j.1365-8711.2001.04649.x.)
{{cite journal}}
: CS1 maint: multiple names: authors list (link - ^ S2CID 53138126. A13.
- ^ a b Crosswell, Ken (1992). A Star that Breaks all the Rules. Kalmbach Books. pp. 54–59.
{{cite book}}
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ignored (help) - .
- .