Mu Aquarii
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| Observation data Epoch J2000 |
|
|---|---|
| Constellation (pronunciation) |
Andromeda |
| Right ascension | 20h 52m 39.2336s |
| Declination | -08° 58′ 59.944″ |
| Apparent magnitude (V) | 4.723 |
| Characteristics | |
| Spectral type | A3m |
| U-B color index | 0.11 |
| B-V color index | 0.32 |
| Astrometry | |
| Radial velocity (Rv) | -9.1 km/s |
| Proper motion (μ) | RA: 47.06 mas/yr Dec.: -32.91 mas/yr |
| Parallax (π) | 21.01 ± 1.04 mas |
| Distance | 155 ± 8 ly (48 ± 2 pc) |
| Absolute magnitude (MV) | 5.029 |
| Details | |
| Mass | ? M☉ |
| Radius | ? R☉ |
| Luminosity | ? L☉ |
| Temperature | ? K |
| Metallicity | ? |
| Rotation | ? |
| Age | ? years |
| Visual binary orbit | |
| Companion | μ Aquarii B |
| Period (P) | 4.8788501 yr |
| Semimajor axis (a) | 0.1" |
| Inclination (i) | 145° |
| Other designations | |
| Database references | |
| SIMBAD | data |
Mu Aquarii (μ Aqr / μ Aquarii) is a binary star in the constellation Aquarius. It is approximately 155 light years from Earth. It shares the traditional name Albulaan with ν Aquarii. The name derives from an Arabic term al-bulacān meaning "the two swallowers".
Mu Aquarii is a spectroscopic binary which has a stellar classification of A3m. Its two components have an orbital period of 1782 days and a separation of 0.1 arcseconds.

