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Beta Canum Venaticorum information


β Canum Venaticorum
Location of β Canum Venaticorum (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Canes Venatici
Right ascension 12h 33m 44.54425s[1]
Declination +41° 21′ 26.9214″[1]
Apparent magnitude (V) 4.25[2]
Characteristics
Spectral type G0 V[3]
U−B color index 0.04[4]
B−V color index 0.58[4]
Astrometry
Radial velocity (Rv)+6.9[5] km/s
Proper motion (μ) RA: −704.702[1] mas/yr
Dec.: +292.155[1] mas/yr
Parallax (π)118.0266 ± 0.1530 mas[1]
Distance27.63 ± 0.04 ly
(8.47 ± 0.01 pc)
Absolute magnitude (MV)4.64[6]
Details
Mass0.97±0.04[7] M
Radius1.123±0.028[8] R
Luminosity1.151±0.018[8] L
Surface gravity (log g)4.60[9] cgs
Temperature6043±183[7] K
Metallicity [Fe/H]−0.18[7] dex
Rotational velocity (v sin i)2.9±0.4[10] km/s
Age3.4[7] to 7.1[6] Gyr
Other designations
Chara, Asterion, Beta CVn, 8 CVn, BD +42 2321, FK5 470, HD 109358, HIP 61317, HR 4785, SAO 44230[11]
Database references
SIMBADdata
ARICNSdata

Beta Canum Venaticorum (β Canum Venaticorum, abbreviated Beta CVn, β CVn), also named Chara /ˈkɛərə/,[12][13] is a G-type main-sequence star in the northern constellation of Canes Venatici. At an apparent visual magnitude of 4.25, it is the second-brightest star in the constellation. Based upon an annual parallax shift of 118 mas,[1] this star is 27.6 light-years (8.5 parsecs) distant from the Sun.

Along with the brighter star Cor Caroli, the pair form the "southern dog" in this constellation that represents hunting dogs.

  1. ^ a b c d e f Cite error: The named reference edr3 was invoked but never defined (see the help page).
  2. ^ Cite error: The named reference apj694_2_1085 was invoked but never defined (see the help page).
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  4. ^ a b Cite error: The named reference mnras133 was invoked but never defined (see the help page).
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  6. ^ a b Cite error: The named reference cgssn09 was invoked but never defined (see the help page).
  7. ^ a b c d Cite error: The named reference lda2021 was invoked but never defined (see the help page).
  8. ^ a b Cite error: The named reference apj746_1_101 was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference apj131 was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference aaa537_A147 was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  12. ^ Kunitzsch, Paul; Smart, Tim (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, Massachusetts: Sky Pub. ISBN 978-1-931559-44-7.
  13. ^ "IAU Catalog of Star Names". Retrieved 28 July 2016.

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Beta Canum Venaticorum

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Beta Canum VenaticorumCanum Venaticorum, abbreviated Beta CVn, β CVn), also named Chara /ˈkɛərə/, is a G-type main-sequence star in the northern constellation...

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Cor Caroli

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Caroli /ˌkɔːr ˈkærəlaɪ/ is a binary star designated Alpha Canum Venaticorum or α Canum Venaticorum. The International Astronomical Union uses the name "Cor...

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Canes Venatici

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contains no very bright stars. The Bayer designation stars, Alpha and Beta Canum Venaticorum are only of third and fourth magnitude respectively. Flamsteed catalogued...

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Solar analog

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stars are sometimes mentioned as solar-twin candidates such as: Beta Canum Venaticorum; however it has too low metallicities (−0.21) for solar twin. 16...

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NGC 4244

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Way. In the sky, it is located near the yellow naked-eye star, Beta Canum Venaticorum, but also near the barred spiral galaxy NGC 4151 and irregular galaxy...

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Chara

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array, a telescope Beta Canum Venaticorum or Chara, a star Chara or Southern dogs, a constellation including Beta Canum Venaticorum and Cor Caroli Chara...

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Stellar classification

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yellow supergiant class. Spectral standards: G0V – Beta Canum Venaticorum G0IV – Eta Boötis G0Ib – Beta Aquarii G2V – Sun G5V – Kappa1 Ceti G5IV – Mu Herculis...

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NGC 4490

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4490 has a double nucleus. NGC 4490 is located 3/4° northwest of beta Canum Venaticorum and with apparent visual magnitude 9.8, can be observed with 15x100...

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Beta Lyrae variable

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least one giant or supergiant component KE = contact binary RS = RS Canum Venaticorum variable SD = semi-detached binary "MAST: Barbara A. Mikulski Archive...

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Margaret Turnbull

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the basis of SETI radio searches with the Allen Telescope Array (Beta Canum Venaticorum, HD 10307, HD 211415, 18 Scorpii, and 51 Pegasi). The second are...

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List of brightest natural objects in the sky

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magnitude derived from adding the magnitudes of Alpha2 Canum Venaticorum (2.88) and Alpha1 Canum Venaticorum (5.60) as per the formula: 2.79 ≈ − 2.5 log 10 ⁡...

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Beta Hydrae

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along a position angle of 28.5°. The brighter component is an α2 Canum Venaticorum variable that changes in brightness with a period of 2.344 days and...

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Beta Sculptoris

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Beta Sculptoris, Latinized from β Sculptoris, is a single, blue-white hued star in the southern constellation of Sculptor. It has an apparent visual magnitude...

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AF Leporis

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resulting from the presence of starspots. AF Leporis is a member of the Beta Pictoris moving group, with an astronomically young age of about 24 million...

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Variable star

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vary by less than 0.5 magnitudes (70% change in luminosity). Alpha2 Canum Venaticorum (α2 CVn) variables are main-sequence stars of spectral class B8–A7...

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Rapidly oscillating Ap star

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The roAp stars are sometimes referred to as rapidly oscillating α2 Canum Venaticorum variables. Both the roAp stars and some α2 CVn variables lie on the...

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Ursa Minor

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4.22. A yellow giant of spectral type G5III, the primary is a RS Canum Venaticorum variable star. It is a spectroscopic binary, with a companion 0.36 AU...

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Outline of astronomy

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Draconis variable Magnetic fields Alpha² Canum Venaticorum variable SX Arietis Pulsar Eclipsing binary Algol variable Beta Lyrae variable W Ursae Majoris variable...

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XX Trianguli

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about 1.5° to the WNW of Beta Trianguli along the constellation border with Andromeda. It is classified as a RS Canum Venaticorum variable and ranges in...

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Lyra

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Flamsteed, 19 Lyrae, is also a small-amplitude variable, an Alpha2 Canum Venaticorum variable with a period of just over one day. Another evolved star...

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Leo Minor

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with average magnitudes 4.54 and 5.34 respectively. Both are RS Canum Venaticorum variables, with 10 Leonis Minoris varying by 0.012 magnitude over...

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Capella

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which are also variable. The system has been classified as an RS Canum Venaticorum variable, a class of binary stars with active chromospheres that cause...

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Orbital period

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Binary star Orbital period. AM Canum Venaticorum 17.146 minutes Beta Lyrae AB 12.9075 days Alpha Centauri AB 79.91 years Proxima Centauri – Alpha Centauri...

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