24 Aquarii
| Observation data Epoch J2000 Equinox J2000 | ||
|---|---|---|
| Constellation | Aquarius | |
| Right ascension | 21h 39m 31.53468s[1] | |
| Declination | −00° 03′ 04.1095″[1] | |
| Apparent magnitude (V) | 6.66[2] | |
| Characteristics | ||
| Spectral type | F7 III[3] OR F7V + ? + F9V[4] | |
| B−V color index | +0.52[5] | |
| Absolute magnitude (MV) | 3.45[2] | |
Argument of periastron (ω)(secondary) | 293.0° | |
| Details Gyr | ||
LTT 8626 | ||
| Database references | ||
| SIMBAD | data | |
24 Aquarii is a
mas,[1] which is equivalent to a distance of 130 light-years (40 parsecs) from Earth. The system is moving closer to the Earth with a heliocentric radial velocity of −16 km/s.[2]
The calculated orbit of the visual binary has a
F-type main-sequence stars for components Aa and B.[4]
References
- ^ .
- ^ S2CID 119257644.
- ^ Bibcode:1966POHP....8...25F.
- ^ Bibcode:1996Obs...116..162G.
- Bibcode:1962RGOB...64..103C.
- ^ doi:10.1086/427870.
- S2CID 56118016.
External links
- Image 24 Aquarii
- Orbital elements of seven new spectroscopic binaries
- Calculating the Orbit of a Double Star with Visual, Speckle, and Radial Velocity Data
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