Alpha Sextantis
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) |
|
|---|---|
| Constellation | Sextans |
| Right ascension | 10h 07m 56.29556s |
| Declination | −0° 22′ 17.8621″ |
| Apparent magnitude (V) | 4.49 |
| Characteristics | |
| Spectral type | A0 III |
| U−B color index | −0.07 |
| B−V color index | −0.04 |
| Astrometry | |
| Radial velocity (Rv) | 10.00 km/s |
| Proper motion (μ) |
RA: −25.83 mas/yr Dec.: −4.25 mas/yr |
| Parallax (π) | 11.51 ± 0.98mas |
| Distance | 280 ± 20 ly (87 ± 7 pc) |
| Details | |
| Mass | 2.96±0.12 M☉ |
| Radius | 4.5 R☉ |
| Luminosity | 120 L☉ |
| Surface gravity (log g) | 3.55 cgs |
| Temperature | 9,984 K |
| Metallicity [Fe/H] | −0.03±0.18 dex |
| Rotational velocity (v sin i) | 21 km/s |
| Age | 295 Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Alpha Sextantis (α Sex, α Sextantis) is the brightest star in the equatorial constellation of Sextans. It is visible to the naked eye on a dark night with an apparent visual magnitude of 4.49. The distance to this star, as determined from parallax measurements, is around 280 light years. This is considered an informal "equator star", as it lies less than a quarter of a degree south of the celestial equator. In 1900, it was 7 minutes of arc north of the equator. As a result of a shift in the Earth's axial tilt, it crossed over to the Southern Hemisphere in December 1923.
This is an evolved A-type giant star with a stellar classification of A0 III. It has around three times the mass of the Sun and 4.5 times the Sun's radius. The abundance of elements is similar to that in the Sun. It radiates 120 times the solar luminosity from its outer atmosphere at an effective temperature of 9,984 K. Alpha Sextantis is around 295 million years old with a projected rotational velocity of 21 km/s.
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