2 Ceti

Star in the constellation Cetus From Wikipedia, the free encyclopedia

2 Ceti, also named Hydor,[13] is a single[14] star in the equatorial constellation of Cetus, near the border with Aquarius. It is visible to the naked eye with an apparent visual magnitude of 4.483.[2] The distance to 2 Ceti can be estimated from its annual parallax shift of 12.0 mas,[1] which yields a value of around 272 light years. It appears to be moving further from the Earth with a heliocentric radial velocity of about +8 km/s.[8]

Right ascension00h 03m 44.38784s[1]
Declination−17° 20 09.5719[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
2 Ceti
Location of 2 Ceti (circled in red)
Observation data
Epoch J2000      Equinox J2000
Constellation Cetus
Right ascension 00h 03m 44.38784s[1]
Declination −17° 20 09.5719[1]
Apparent magnitude (V) 4.483[2]
Characteristics
Evolutionary stage main sequence[3][4]
Spectral type B9 IVn[5]
U−B color index −0.12[6]
B−V color index −0.047±0.003[7]
Astrometry
Radial velocity (Rv)+8.0±4.6[8] km/s
Proper motion (μ) RA: +25.17[1] mas/yr
Dec.: −9.16[1] mas/yr
Parallax (π)11.98±0.26 mas[1]
Distance272 ± 6 ly
(83 ± 2 pc)
Absolute magnitude (MV)−0.06[7]
Details
Mass2.58[9] M
Radius3.92[9] R
Luminosity119+6
−5
[4] L
Surface gravity (log g)3.66[9] cgs
Temperature11,419±388[10] K
Metallicity [Fe/H]+0.00±0.24[5] dex
Rotational velocity (v sin i)116[4] or 237[11] km/s
Age217[10] Myr
Other designations
Hydor, 2 Cet, BD−18°6417, FK5 905, HD 225132, HIP 301, HR 9098, SAO 147059[12]
Database references
SIMBADdata
Close

The stellar classification for this star is B9 IVn,[5] matching a B-type subgiant star with "nebulous" absorption lines due to rapid rotation.[15] Estimates of the rotation rate range from 116[4] to 237[11] km/s, and this high rate of spin is giving the star an equatorial bulge that is 12% larger than the polar radius.[15] 2 Ceti is about 217 million years old[10] with 2.6 times the mass of the Sun and 3.9 times the Sun's radius.[9] It is radiating 119 times the Sun's luminosity[4] from its photosphere at an effective temperature of 11,419 K.[10] An infrared excess has been detected around this star by the Akari satellite at a wavelength of 18μm, suggesting there is an orbiting debris disk.[16]

Naming

The ancient Greek term Hydor (ὕδωρ), meaning water, originally referred to a constellation of faint stars in the region of Aquarius and Cetus.[17] The IAU Working Group on Star Names approved the name Hydor for 2 Ceti, on 25 August 2025 and it is now so entered in the IAU Catalog of Star Names;[13] it had previously been used for λ Aquarii, for which the IAU adopted the Indian name Shatabhisha.[17]

References

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