Astronomy:9 Andromedae

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Short description: Star in the constellation Andromeda
9 Andromedae
ANAndLightCurve.png
A light curve for AN Andromedae, plotted from TESS data[1]
Observation data
Equinox J2000.0]] (ICRS)
Constellation Andromeda
Right ascension  23h 18m 23.32202s[2]
Declination +41° 46′ 25.2031″[2]
Apparent magnitude (V) 5.98[3]
Characteristics
Spectral type A7 V[4] or A7m[3]
B−V color index 0.215±0.002[3]
Variable type β Lyr[5]
Astrometry
Radial velocity (Rv)−3.8±2.9[3] km/s
Proper motion (μ) RA: −10.266[2] mas/yr
Dec.: −9.791[2] mas/yr
Parallax (π)7.0976 ± 0.0544[2] mas
Distance460 ± 4 ly
(141 ± 1 pc)
Absolute magnitude (MV)0.43[3]
Orbit[6]
Period (P)3.2196 d
Eccentricity (e)0.03
Inclination (i)60.2[7]°
Periastron epoch (T)2,436,094.876 JD
Semi-amplitude (K1)
(primary)
71.6 km/s
Details[7]
9 And A
Mass2.48 M
Radius3.51 R
Luminosity49.2 L
Temperature8,200 K
Rotational velocity (v sin i)81[8] km/s
9 And B
Mass1.32 M
Luminosity17.5 L
Temperature6,330 K
Other designations
9 And, AN And, BD+40° 5043, HD 219815, HIP 115065, HR 8864, SAO 52881, PPM 64041[9]
Database references
SIMBADdata

9 Andromedae, abbreviated 9 And by convention, is a variable binary star system in the northern constellation Andromeda. 9 Andromedae is the Flamsteed designation, while it bears the variable star designation AN Andromedae, or AN And. The maximum apparent visual magnitude of the system is 5.98,[3] which places it near the lower limit of visibility to the human eye. Based upon an annual parallax shift of 7.1 mas,[2] it is located 460 light years from the Earth.

This system was determined to be a single-lined spectroscopic binary in 1916 by American astronomer W. S. Adams, and the initial orbital elements were computed by Canadian astronomer R. K. Young in 1920.[7] The pair orbit each other with a period of 3.2196 days and an eccentricity of 0.03.[6] It is an eclipsing binary, which means the orbital plane is inclined close to the line of sight and, from the perspective of the Earth, the stars pass in front of each other, causing two partial eclipses every orbit. During the transit of the secondary in front of the primary, the visual magnitude drops to 6.16, while the eclipse of the secondary by the primary lowers the net magnitude to 6.09.[10]

References

  1. "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html. 
  2. 2.0 2.1 2.2 2.3 2.4 2.5 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode2018A&A...616A...1G. 
  3. 3.0 3.1 3.2 3.3 3.4 3.5 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode2012AstL...38..331A. 
  4. Hill, G. et al. (1975), "MK Classifications of some Northern Hemisphere Binary Systems", Memoirs of the Royal Astronomical Society 79: 131, Bibcode1975MmRAS..79..131H. 
  5. Samus', N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (2017), "General catalogue of variable stars: Version GCVS 5.1", Astronomy Reports 61 (1): 80, doi:10.1134/S1063772917010085, Bibcode2017ARep...61...80S. 
  6. 6.0 6.1 Pourbaix, D. et al. (2004), "SB9: The Ninth Catalogue of Spectroscopic Binary Orbits", Astronomy & Astrophysics 424: 727–732, doi:10.1051/0004-6361:20041213, Bibcode2004A&A...424..727P. 
  7. 7.0 7.1 7.2 Tremko, Jozef; Bakos, Gustav A. (October 1978), "A Photometric Study of the Am Binary System AN Andromedae", Journal of the Royal Astronomical Society of Canada 72: 263, Bibcode1978JRASC..72..263T. 
  8. Royer, F. et al. (October 2002), "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i", Astronomy and Astrophysics 393: 897–911, doi:10.1051/0004-6361:20020943, Bibcode2002A&A...393..897R. 
  9. "9 And". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=9+And. 
  10. Avvakumova, E. A. et al. (October 2013), "Eclipsing variables: Catalogue and classification", Astronomische Nachrichten 334 (8): 860, doi:10.1002/asna.201311942, Bibcode2013AN....334..860A 

External links