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63 Andromedae

From Wikipedia, the free encyclopedia
Star in the constellation Andromeda
63 Andromedae
Location of 63 Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAndromeda
Right ascension02h 20m 58.202s[1]
Declination+50° 09′ 05.39″[1]
Apparent magnitude (V)5.59[2]
Characteristics
Spectral typeB9VpSi[3]
B−Vcolor index−0.089[4]
Variable typeα2 CVn[2]
Astrometry
Radial velocity (Rv)−0.30[5] km/s
Proper motion (μ)RA: 39.818[1]mas/yr
Dec.: −31.607[1]mas/yr
Parallax (π)8.5275±0.1684 mas[1]
Distance382 ± 8 ly
(117 ± 2 pc)
Absolute magnitude (MV)+0.26[6]
Details[6]
Mass3.07±0.14 M
Radius2.4±0.3 R
Luminosity110 L
Surface gravity (log g)4.29±0.11 cgs
Temperature11,967 K
Rotation4.189 days
Other designations
PZ And,BD+49 640,HD 14392,HIP 10944,HR 682,NSV 790,SAO 37960,PPM 27476
Database references
SIMBADdata

63 Andromedae (abbreviated63 And) is anAlpha2 Canum Venaticorum (α2 CVn) variablestar in theconstellationAndromeda. Itsvariable star designation isPZ Andromedae. With anapparent magnitude of about 5.6, it is bright enough to be seen by naked eye. Based upon an annualparallax shift of8.53 mas, it is located 382 light years away.

The spectral type of this star is B9VpSi, indicating that it is a chemically peculiarmain sequence star with abnormally strongsilicon lines. Although it has a B-type spectral class, this type of star is known as anAp star, a class of stars with very strong spectral lines of certain heavy elements and strong magnetic fields. The chemical peculiarities are caused by stratification in the atmosphere due to slow rotation.[7]

The star has 3 times themass of the Sun and 2.4 times theSun's radius. It is radiating 110 times theSun's luminosity from itsphotosphere at aneffective temperature of 11,967 K.[6]

Alight curve for PZ Andromedae, plotted fromTESS data[8]

63 Andromedae varies in brightness by about 0.05 magnitudes with a period of 4.189 days. This is believed to occur as it rotates. This type ofvariable star is known as an α2 Canum Venaticorum variable after the first example to be studied.[2]

To the naked eye the star figures as a faint, denseasterism with 64 and 65 Andromedae (southwest and west), which together justify a rectangular projection (extreme) of the constellation (official boundaries).[9] North, west and east are an arm/hand, fictitiously and geometrically, of Perseus, whose character is related in traditional mythology as Andromeda's saviour, saving her from the sea monster, who forever retreats to beyondPisces,Cetus. The closest star in the asterisms commonly drawn up to represent the princess herself is51 Andromedae, to the east. At anapparent magnitude of 3.57, this star shines two magnitudes or 6.3 times brighter.[9]

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. ^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. Originally Published in: 2009yCat....102025S.1: B/GCVS.Bibcode:2009yCat....102025S.
  3. ^Abt, H. A.; Morrell, N. I. (July 1995), "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars",Astrophysical Journal Supplement,99: 135,Bibcode:1995ApJS...99..135A,doi:10.1086/192182.
  4. ^van Leeuwen, F. (2007)."Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.Vizier catalog entry
  5. ^de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics,546: 14,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  6. ^abcNorth, P. (June 1998), "Do SI stars undergo any rotational braking?",Astronomy and Astrophysics,334:181–187,arXiv:astro-ph/9802286,Bibcode:1998A&A...334..181N
  7. ^Renson, P.; Manfroid, J. (2009)."Catalogue of Ap, HgMn and Am stars".Astronomy and Astrophysics.498 (3): 961.Bibcode:2009A&A...498..961R.doi:10.1051/0004-6361/200810788.
  8. ^"MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved8 December 2021.
  9. ^ab"Constellations.gif". RetrievedJuly 7, 2022.

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