Red circle marks arc distance separating other bright stars viewed from our place in the galaxy.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS)
Constellation
Hydra
Right ascension
08h 48m 25.97057s[1]
Declination
+05° 50′ 16.1283″[1]
Apparent magnitude (V)
4.34[2]
Characteristics
Spectral type
A0 Vn[3]
U−B color index
−0.04[2]
B−V color index
−0.04[2]
Astrometry
Radial velocity (Rv)
+32.8[4] km/s
Proper motion (μ)
RA: −17.33[1] mas/yr Dec.: −29.41[1] mas/yr
Parallax (π)
9.21 ± 0.21 mas[1]
Distance
354 ± 8 ly (109 ± 2 pc)
Absolute magnitude (MV)
−0.83[5]
Details[3]
Mass
3.24±0.05M☉
Radius
2.0[6]R☉
Luminosity
242 L☉
Temperature
9,795 K
Rotational velocity (v sin i)
128 km/s
Age
350[7] Myr
Other designations
ρ Hya, 13 Hya, BD+06°2040, HD 75137, HIP 43234, HR 3492, SAO 117146[8]
Database references
SIMBAD
data
Rho Hydrae, equally written ρ Hydrae, is a binary star[9] in the equatorial constellation of Hydra. It is visible to the naked eye with an apparent visual magnitude of 4.34.[2] The distance to this system, based upon an annual parallax shift of 9.21 mas,[1] is about 354 light years. At that distance, the visual magnitude is diminished by an interstellar extinction of 0.06 magnitudes, due to intervening dust.[7]
The primary component is an A-type main sequence star with a stellar classification of A0 Vn.[3] It has around double[6] the radius of the Sun and 3.2 times the Sun's mass. Rho Hydrae is around 350 million years old[7] and has a high rate of spin, with a projected rotational velocity of 128 km/s. It radiates 242 times the solar luminosity from its outer atmosphere at an effective temperature of 9,795 K.[3] The companion is a magnitude 11.9 star at an angular separation of 12.1 arc seconds along a position angle of 146°, as of 2000.[10]
^ abcdefCite error: The named reference vanLeeuwen2007 was invoked but never defined (see the help page).
^ abcdCite error: The named reference Mermilliod1986 was invoked but never defined (see the help page).
^ abcdCite error: The named reference Zorec2012 was invoked but never defined (see the help page).
^Cite error: The named reference Wilson1953 was invoked but never defined (see the help page).
^Cite error: The named reference Anderson2012 was invoked but never defined (see the help page).
^ abCite error: The named reference PasinettiFracassini2001 was invoked but never defined (see the help page).
^ abcCite error: The named reference Gontcharov2012 was invoked but never defined (see the help page).
^Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
^Cite error: The named reference Eggleton2008 was invoked but never defined (see the help page).
^Cite error: The named reference WDSC2014 was invoked but never defined (see the help page).
RhoHydrae, equally written ρ Hydrae, is a binary star in the equatorial constellation of Hydra. It is visible to the naked eye with an apparent visual...
heliosphere. In 2006, a far infrared bow shock was detected near the AGB star R Hydrae. Bow shocks are also a common feature in Herbig Haro objects, in which a...
Kellogg, Kendra (11 April 2016). "The Nearest Isolated Member of the TW Hydrae Association is a Giant Planet Analog". Astrophysical Journal Letters. 821...
Epsilon Hydrae Quintuple star system 3.38 Zeta Virginis Binary star system Slightly variable 3.386 3.38 Nu Centauri Binary star system 3.39 3.30 Rho Persei...
Formerly part of the GAYA (Great Austral Young Association) TW Hydrae association TW Hydrae Hydra 160 10 Carina Association Carina 200 45 Formerly part of...
signature, this object was determined to belong to the ~8-million-year-old TW Hydrae association, and the mass of the secondary was determined to be 8 ± 2 MJ...
النِّطَاق Zeta Orionis Alphard al-Fard the Solitary one الفرد الفَرْد Alpha Hydrae Alphecca (Nayyir) al-Fakkah (the Bright one of) the Broken (Ring) نير الفكة...
variability in 1784. Chi Cygni was identified in 1686 by G. Kirch, then R Hydrae in 1704 by G. D. Maraldi. By 1786, ten variable stars were known. John Goodricke...
formation and wind acceleration around the aluminum oxide-rich AGB star W Hydrae". Science Advances. 3 (11): id.eaao2149. Bibcode:2017SciA....3O2149T. doi:10...