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47 Capricorni

From Wikipedia, the free encyclopedia
Star in the constellation Capricornus
This article is about c2 Capricorni. For other stars with thisBayer designation, seec Capricorni.
47 Capricorni

Alight curve for AG Capricorni, plotted fromHipparcos data[1]
Observation data
Epoch J2000      Equinox J2000
ConstellationCapricornus
Right ascension21h 46m 16.26887s[2]
Declination−09° 16′ 33.3799″[2]
Apparent magnitude (V)6.00[3](5.90 - 6.14)[4]
Characteristics
Evolutionary stagegiant
Spectral typeM2III[5]
B−Vcolor index1.629±0.010[3]
Variable typeSRb[4]
Astrometry
Radial velocity (Rv)+19.80±0.89[6] km/s
Proper motion (μ)RA: +18.731[2]mas/yr
Dec.: +8.387[2]mas/yr
Parallax (π)2.7933±0.2052 mas[2]
Distance1,170 ± 90 ly
(360 ± 30 pc)
Absolute magnitude (MV)−1.76[3]
Details
Radius102+11
−10
[2] R
Luminosity1,940±162[2] L
Temperature3,784+188
−186
[2] K
Other designations
c2 Cap,47 Cap,AG Cap,BD−09°5833,HD 207005,HIP 107487,HR 8318,SAO 145648[7]
Database references
SIMBADdata

47 Capricorni is avariable star located around 1,170[2] light years from the Sun in the southernconstellationCapricornus,[7] near the northern border withAquarius. It has thevariable star designation ofAG Capricorni and aBayer designation ofc2 Capricorni;[8]47 Capricorni is theFlamsteed designation. This object is visible to thenaked eye as a dim, red-hued point of light with anapparent visual magnitude that varies between 5.90 and 6.14. The star is receding from the Earth with a heliocentricradial velocity of +20 km/s.[6]

In 1963,Alan William James Cousins announced that 47 Capricorni is a variable star.[9] It was given its variable star designation in 1973.[10]

This is an agingred giant star with astellar classification of M2III.[5] It is asemiregular variable star of subtype SRb with a period of 30.592 days and a maximum brightness of 5.9 magnitude.[4] With the supply of hydrogen at itscore exhausted, the star has expanded to around 102[2] times theSun's radius. It is radiating 1,940[2] times theluminosity of the Sun from its swollenphotosphere at aneffective temperature of 3,784 K.[2]

References

[edit]
  1. ^"Hipparcos Tools Interactive Data Access".Hipparcos. ESA. Retrieved8 December 2021.
  2. ^abcdefghijklBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  3. ^abcAnderson, 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.
  4. ^abcSamus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)".VizieR On-line Data Catalog: B/gcvs.1.Bibcode:2009yCat....102025S.
  5. ^abHouk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars".Michigan Spectral Survey.5.Bibcode:1999MSS...C05....0H.
  6. ^abFamaey, B.; et al. (2009). "Spectroscopic binaries among Hipparcos M giants,. I. Data, orbits, and intrinsic variations".Astronomy and Astrophysics.498 (2): 627.arXiv:0901.0934.Bibcode:2009A&A...498..627F.doi:10.1051/0004-6361/200810698.S2CID 18739721.
  7. ^ab"47 Cap".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2014-05-12.
  8. ^Kostjuk, N. D. (2002)."HD 207005".HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index. Institute of Astronomy of Russian Academy of Sciences;CDS.IV/27A
  9. ^Cousins, A. W. J. (1963)."Photometric Data for Stars in the Equatorial Zone (Third List)".Monthly Notes of the Astron. Soc. Southern Africa.22: 12.Bibcode:1963MNSSA..22...12C. Retrieved8 December 2024.
  10. ^Kukarkin, B. V.; Kholopov, P. N.; Kukarkina, N. P.; Perova, N. B. (October 1973)."59th Name-List of Variable Stars"(PDF).Information Bulletin on Variable Stars.834.Bibcode:1973IBVS..834....1K. Retrieved8 December 2024.
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