Mu Aquarii

From Wikipedia, the free encyclopedia

Jump to: navigation, search


μ Aquarii
6 Aquarii.png
μ Aquarii
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
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 3.1 M
Radius 2.1 R
Luminosity 40 L
Temperature 7,500–10,000 K
Metallicity ?
Rotation 2.31441044 d
Age ? years
Orbit
Companion μ Aquarii B
Period (P) 4.8788501 yr
Semimajor axis (a) 0.1"
Inclination (i) 145°
Other designations
Albulaan, 6 Aquarii, HR 7990,
HD 198743, BD-09°5598,
FK5 1547, HIP 103045,
SAO 144895, GC 29109,
CCDM 20527-0859.
Database references
SIMBAD data
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)

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.

[edit] Location

Aquarius Constellation

[edit] References