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Star in the constellation Circinus From Wikipedia, the free encyclopedia
Alpha Circini (α Cir, α Circini) is a variable star in the faint, southern, circumpolar constellation of Circinus. At an apparent visual magnitude of 3.19,[4] it is the brightest star in the constellation and can be readily seen with the naked eye from the southern hemisphere to as far north as 25° north latitude. Parallax measurements of this star yield an estimated distance of 54.0 light-years (16.6 parsecs) from the Earth.[1]
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Circinus |
Right ascension | 14h 42m 30.41958s[1] |
Declination | −64° 58′ 30.4934″[1] |
Apparent magnitude (V) | 3.18 - 3.21[2] |
Characteristics | |
Spectral type | A7 Vp SrCrEu[3] |
U−B color index | +0.12[4] |
B−V color index | +0.24[4] |
Variable type | roAp[2] |
Astrometry | |
Radial velocity (Rv) | +7.2[5] km/s |
Proper motion (μ) | RA: −192.53[1] mas/yr Dec.: −233.51[1] mas/yr |
Parallax (π) | 60.35 ± 0.14 mas[1] |
Distance | 54.0 ± 0.1 ly (16.57 ± 0.04 pc) |
Absolute magnitude (MV) | +2.18[6] |
Details | |
Mass | 1.5–1.7[7] M☉ |
Radius | 1.967 ± 0.066[8] R☉ |
Luminosity | 10.51 ± 0.60[7] L☉ |
Surface gravity (log g) | 4.1[7] cgs |
Temperature | 7,500[7] K |
Metallicity [Fe/H] | 0.13[9] dex |
Rotation | 4.4790 ± 0.0001 days[10] |
Rotational velocity (v sin i) | 13.0 ± 1.5[10] km/s |
Age | ~12 million[11] years |
Other designations | |
Database references | |
SIMBAD | data |
This star belongs to a class of variables known as rapidly oscillating Ap stars. It oscillates with multiple, non-radial pulsation cycles and a dominant cycle of 6.8 minutes.[10] The spectrum shows peculiar features caused by chemical stratification of the outer atmosphere. It displays a moderate deficiency of carbon, nitrogen and oxygen, while there is an overabundance of chromium (Cr).[7] The stellar classification of A7 Vp SrCrEu[3] indicates that this is a main sequence star with enhanced levels of strontium (Sr), chromium, and europium (Eu) in its atmosphere (compared to a typical star like the Sun).[14]
The mass of Alpha Circini is about 150% to 170% the mass of the Sun[7] and it has double the Sun's radius,[8] while the luminosity is more than 10 times that of the Sun. The effective temperature of the outer envelope is about 7,500 K, giving it the white hue typical of A-type stars.[7][15] It is rotating with a period of 4.5 days and the pole is inclined by about 37 ± 4° to the line of sight from the Earth.[10]
Based upon its location and motion through space, Alpha Circini is a candidate member of a stellar kinematic group known as the Beta Pictoris moving group. This group shares a common origin and has an estimated age of about 12 million years. At the birth of this group, Alpha Circini was estimated to be located at a distance of about 91 ly (28 pc) from the center of the assemblage.[11]
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