Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Hydra |
Right ascension | 09h 41m 17.00785s[1] |
Declination | −23° 35′ 29.4325″[1] |
Apparent magnitude (V) | 4.76[2] |
Characteristics | |
Spectral type | B5 V[3] |
B−V color index | −0.117±0.015[2] |
Astrometry | |
Radial velocity (Rv) | +16.05±1.5[4] km/s |
Proper motion (μ) | RA: −29.969[1] mas/yr Dec.: +1.914[1] mas/yr |
Parallax (π) | 6.5733 ± 0.2851 mas[1] |
Distance | 500 ± 20 ly (152 ± 7 pc) |
Absolute magnitude (MV) | −1.19[2] |
Details | |
Mass | 4.57±0.08[5] M☉ |
Radius | 4.00±0.08[6] R☉ |
Luminosity | 708+60 −55[5] L☉ |
Surface gravity (log g) | 2.54±0.03[6] cgs |
Temperature | 15,000±150[6] K |
Rotational velocity (v sin i) | 315[5][7] km/s |
Other designations | |
Database references | |
SIMBAD | data |
HD 83953 (I Hydrae) is a single,[9] blue-white hued star in the equatorial constellation of Hydra. It is visible to the naked eye, having an apparent visual magnitude of 4.76.[2] Based upon an annual parallax shift of 6.6 mas,[1] the distance to this star is estimated as 500 light years. It is moving further from Earth with a heliocentric radial velocity of +16 km/s.[4]
This is a B-type main-sequence star with a stellar classification of B5 V.[3] It has been known to be a Be star since 1926, when an Hβ emission line was discovered in the stellar spectrum by Mount Wilson Observatory.[10] This energy is coming from a circumstellar envelope of heated gas that has been expelled from the central star and formed a thin orbiting disk.[11] HD 83953 is spinning rapidly with a projected rotational velocity of 315 km/s, giving the star an oblate shape with an equatorial bulge that is 18% larger than the polar radius.[7]
HD 83953 has 4.6[5] times the mass of the Sun and 4.0[6] times the Sun's radius. It is radiating 708[5] times the Sun's luminosity from its photosphere at an effective temperature of 15,000 K.[6]
GaiaDR2
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