Location of V518 Carinae in IC 2602 (circled) | |
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Carina |
| Right ascension | 10h 42m 14.12927s [1] |
| Declination | −64° 27′ 59.1340″ [1] |
| Apparent magnitude (V) | 4.63 - 4.82 [2] |
| Characteristics | |
| Evolutionary stage | main sequence [1] |
| Spectral type | B3/5V [3] |
| U−B color index | −0.58 [4] |
| B−V color index | −0.14 [4] |
| Variable type | γ Cas? [5] |
| Astrometry | |
| Proper motion (μ) | RA: −17.821 [1] mas/yr Dec.: +11.580 [1] mas/yr |
| Parallax (π) | 6.7516±0.0843 mas [1] |
| Distance | 483 ± 6 ly (148 ± 2 pc) |
| Absolute magnitude (MV) | −1.169 [6] |
| Details | |
| Mass | 6.2 [7] M☉ |
| Radius | 3.30±0.07 [8] R☉ |
| Luminosity | 753 [6] L☉ |
| Surface gravity (log g) | 4.015 [9] cgs |
| Temperature | 15,397 [6] K |
| Rotational velocity (v sin i) | 120 [9] km/s |
| Age | 17.2 [10] Myr |
| Other designations | |
| V518 Carinae, HD 92938, HIP 52370, HR 4196 | |
| Database references | |
| SIMBAD | data |
V518 Carinae (HR 4196) is a naked eye variable star in the constellation Carina. It is a member of the bright open cluster IC 2602 near the Carina Nebula.
V518 Carinae lies in the open cluster IC 2602, 5 arc minutes from its brightest member θ Carinae.
V518 Carinae was discovered to change in brightness after analysis of Hipparcos photometry. [12] The amplitude of the variations seen is 0.2 magnitudes, with possible periods of 100 and 971 days. [13] It is classified as a γ Cassiopeiae variable. [14] [5]
V518 Carinae is classified as a B-type main sequence star between B3 and B5. [15] It is also catalogued as a helium star, a chemically peculiar star with abnormally strong helium absorption lines in its spectrum and relatively weak hydrogen lines. It is possibly a blue straggler. [16]
V518 Carinae is also a Be star, a hot star with emission lines in its spectrum due to a disk of material around the star. Be stars that show irregular brightness changes due to the disk are grouped as γ Cassiopeiae variables. V518 Carinae is known to produce disk outbursts lasting several hundred days. [17]