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Beta Circini

From Wikipedia, the free encyclopedia
Star in the constellation Circinus
β Circini
Location of β Circini (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationCircinus
Right ascension15h 17m 30.84945s[1]
Declination−58° 48′ 04.3453″[1]
Apparent magnitude (V)4.069[2]
Characteristics
Spectral typeA3 Va[2]
U−Bcolor index+0.09[3]
B−Vcolor index+0.09[3]
Astrometry
Radial velocity (Rv)9.6±2[2] km/s
Proper motion (μ)RA: −97.182[1]mas/yr
Dec.: −136.055[1]mas/yr
Parallax (π)35.8205±0.2515 mas[1]
Distance91.1 ± 0.6 ly
(27.9 ± 0.2 pc)
Absolute magnitude (MV)+1.64[4]
Details
Mass1.96+0.03
−0.01
[5] M
Radius1.92[6] R
Luminosity19[4] L
Surface gravity (log g)4.281[7] cgs
Temperature8676±33[5] K
Metallicity[Fe/H]0.16[4] dex
Rotational velocity (v sin i)59[3] km/s
Age370–500[5] Myr
Other designations
β Cir, Beta Circini, Beta Cir,CPD−58 5875,FK5 561,GC 20526,GJ 580.1,GJ 9516,HD 135379,HIP 74824,HR 5670,PPM 343590,SAO 242384.[2]
Database references
SIMBADdata

Beta Circini,Latinized fromβ Circini, is anA-typemain sequencestar and is the second-brightest star in theconstellation ofCircinus.[2] It has anapparent visual magnitude of approximately 4.069,[2] which is bright enough to be viewed with the naked eye. Based upon an annualparallax shift of35.8 mas as seen from the Earth, it is located 91 light years from theSun.

With astellar classification of A3 Va,[2] this is anmain-sequence star fusing atoms ofhydrogen intohelium at its core. It is between 370 and 500 million years old[5] with around 1.9[6] times theSun's radius. The star is radiating 19[4] times theSun's luminosity from itsphotosphere at aneffective temperature of 8,676 K.[5] It has one known sub-stellar companion.

Substellar companion

[edit]

Beta Circini b is a distantbrown dwarf companion orbiting the host star at a distance of 6,656 AU. It was detected as aproper motion companion to Beta Circini in 2015 by L.C. Smith and collaborators. Using BHAC15 isochrones, its mass is estimated at 0.056 M, or59 MJ. It has astellar classification of L1 and a temperature of 2,084 K (1,811 °C).[5]

The β Circini planetary system[5]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b58.7±7.3 MJ6,656

References

[edit]
  1. ^abcdeVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^abcdefg"* bet Cir".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedSeptember 5, 2008.
  3. ^abcHR 5670, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr.,CDS IDV/50. Accessed on line September 5, 2008.
  4. ^abcdAnderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",Astronomy Letters,38 (5): 331,arXiv:1108.4971,Bibcode:2012AstL...38..331A,doi:10.1134/S1063773712050015,S2CID 119257644.
  5. ^abcdefgSmith, L. C.; et al. (2015)."Discovery of a brown dwarf companion to the A3V star β Circini".Monthly Notices of the Royal Astronomical Society.454 (4):4476–4483.arXiv:1509.09226.Bibcode:2015MNRAS.454.4476S.doi:10.1093/mnras/stv2290.hdl:2299/16835.S2CID 18570256.
  6. ^abCotten, Tara H.; Song, Inseok (2016-07-01)."A Comprehensive Census of Nearby Infrared Excess Stars".The Astrophysical Journal Supplement Series.225 (1): 15.arXiv:1606.01134.Bibcode:2016ApJS..225...15C.doi:10.3847/0067-0049/225/1/15.ISSN 0067-0049.Beta Circini's database entry atVizieR.
  7. ^Song, Inseok; et al. (February 2001), "Ages of A-Type Vega-like Stars from uvbyβ Photometry",The Astrophysical Journal,546 (1):352–357,arXiv:astro-ph/0010102,Bibcode:2001ApJ...546..352S,doi:10.1086/318269,S2CID 18154947
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