Ankaa
Star Ankaa (α Phoenicis) |
|||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
AladinLite | |||||||||||||||||||||
Observation dates equinox : J2000.0 , epoch : J2000.0 |
|||||||||||||||||||||
Constellation | Phoenix | ||||||||||||||||||||
Right ascension | 00 h 26 m 17.05 s | ||||||||||||||||||||
declination | -42 ° 18 ′ 21.5 ″ | ||||||||||||||||||||
Apparent brightness | 2.4 mag | ||||||||||||||||||||
Typing | |||||||||||||||||||||
B − V color index | +1.09 | ||||||||||||||||||||
U − B color index | +0.88 | ||||||||||||||||||||
R − I index | +0.60 | ||||||||||||||||||||
Spectral class | K0 III ... | ||||||||||||||||||||
Astrometry | |||||||||||||||||||||
Radial velocity | (75.2 ± 3.9) km / s | ||||||||||||||||||||
parallax | (38.50 ± 0.73) mas | ||||||||||||||||||||
distance | (84.7 ± 1.6) ly (25.97 ± 0.49) pc |
||||||||||||||||||||
Visual absolute brightness M vis | +0.33 mag | ||||||||||||||||||||
Proper movement | |||||||||||||||||||||
Rec. Share: | (233.05 ± 0.65) mas / a | ||||||||||||||||||||
Dec. portion: | (−356.30 ± 0.74) mas / a | ||||||||||||||||||||
Physical Properties | |||||||||||||||||||||
Dimensions | (2.5) M ☉ | ||||||||||||||||||||
radius | (13) R ☉ | ||||||||||||||||||||
Luminosity |
(86) L ☉ |
||||||||||||||||||||
Effective temperature | (4800) K | ||||||||||||||||||||
Other names and catalog entries |
|||||||||||||||||||||
|
|||||||||||||||||||||
annotation | |||||||||||||||||||||
|
Ankaa (from Arabic عنقاء, DMG ʿanqāʾ ' phoenix') is the proper name of the star α Phoenicis (Alpha Phoenicis , α Phe for short ). Instead of a phoenix, medieval Arab astronomers saw a small boat in the star constellation and therefore gave Ankaa the proper name -Nair az-Zauraq /النائر الزورق / an-nāʾir az-zawraq / 'the shining end of the boat'.
Ankaa is the brightest star in Phoenix with an apparent magnitude of +2.4 mag and belongs to the spectral class K0 III. The star's distance from Earth is 85 light years . It is a spectroscopic binary star with an orbital period of 3849 days. In a relatively "short" time in astronomical terms, it will repel its outer shell as a planetary nebula and become a white dwarf .
See also
Individual evidence
- ↑ a b c Hipparcos catalog (ESA 1997)
- ↑ a b c Bright Star Catalog
- ↑ Pulkovo radial velocities for 35493 HIP stars
- ↑ a b c Hipparcos, the New Reduction (van Leeuwen, 2007)
- ↑ a b c d Ankaa. Jim Kaler, accessed October 13, 2018 .