V Hydrae

V Hydrae (V Hya) is a carbon star in the constellation Hydra. To date perhaps uniquely in our galaxy it has plasma ejections/eruptions on a grand scale every 8.5 years caused by its near, unseen companion in an 8.5 year orbit, inferred by its ultraviolet excess and periastron passage likely through the outer parts of the star itself.

V Hydrae
Location of V Hydrae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Hydra
Right ascension 10h 51m 37.25661s
Declination 21° 15 00.3245
Apparent magnitude (V) 6.0 - 12.3
Characteristics
Spectral type C6,3e-C7,5e(N6e)
B−V color index +5.43
Variable type SRa
Astrometry
Radial velocity (Rv)14.80 km/s
Proper motion (μ) RA: 11.02 ± 1.14 mas/yr
Dec.: 2.29 ± 1.16 mas/yr
Parallax (π)1.44 ± 1.41 mas
Distanceapprox. 2,000 ly
(approx. 700 pc)
Absolute magnitude (MV)3.5 to +1.8
Orbit
Period (P)8.5 yr
Eccentricity (e)≥0.6
Details
A
Mass1.0 M
Radius420–430 R
Luminosity7,850 L
Surface gravity (log g)0.5 cgs
Temperature2,650 K
Rotational velocity (v sin i)11 - 14 km/s
B
Mass<1 M
Other designations
V Hya, BD20°3283, HIP 53085, 2MASS J10513724-2115002, IRAS 10491-2059, WDS J10516-2115
Database references
SIMBADdata
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