Astronomy:Eta Piscis Austrini

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Short description: Star in the constellation Piscis Austrinus
η Piscis Austrini
Piscis Austrinus constellation map.svg
Red circle.svg
Location of η Piscis Austrini (circled)
Observation data
{{#ifeq:J2000.0|J2000.0 (ICRS)|Epoch J2000.0      Equinox J2000.0 (ICRS)| [[History:Epoch|Epoch J2000.0]]      [[Astronomy:Equinox (celestial coordinates)|Equinox J2000.0}}
Constellation Piscis Austrinus
A
Right ascension  22h 00m 50.22454s[1]
Declination −28° 27′ 13.4587″[1]
Apparent magnitude (V) 5.742[2]
B
Right ascension  22h 00m 50.34936s[3]
Declination −28° 27′ 14.1460″[3]
Apparent magnitude (V) 6.825[2]
Characteristics
Spectral type B6 III shell + B8.5 V[4]
U−B color index −0.30[5]
B−V color index −0.10[5]
Variable type suspected[6]
Astrometry
Absolute magnitude (MV)−1.53[7]
A
Proper motion (μ) RA: +15.289[1] mas/yr
Dec.: −0.096[1] mas/yr
Parallax (π)3.8087 ± 0.0932[1] mas
Distance860 ± 20 ly
(263 ± 6 pc)
B
Proper motion (μ) RA: +17.554[3] mas/yr
Dec.: −1.229[3] mas/yr
Parallax (π)4.5342 ± 0.3306[3] mas
Distance720 ± 50 ly
(220 ± 20 pc)
Details
η PsA A
Mass4.01±0.18[8] M☉
Luminosity881[9] L☉
Surface gravity (log g)3.48[9] cgs
Temperature12,310[9] K
Rotational velocity (v sin i)320[9] km/s
Age115[10] Myr
η PsA B
Mass3.6[11] M☉
Surface gravity (log g)4.17[11] cgs
Temperature14,144[11] K
Other designations
η PsA, 12 Piscis Austrini, CPD−29° 6659, HD 209014, HIP 108661, HR 8386, SAO 190822, WDS J22008-2827AB[12]
Database references
SIMBADdata

Eta Piscis Austrini (η Piscis Austrini) is binary star[2] system in the southern constellation of Piscis Austrinus. As of 2000, the two components had an angular separation of 1.818 arc seconds along a position angle of 113.4°. The pair have a combined apparent visual magnitude of +5.43,[5] which is bright enough to be seen with the naked eye. Based upon an annual parallax shift of 3.99 mas as seen from the Earth,[13] the system is located roughly 820 light years from the Sun.

Although not catalogued formally as a variable star, brightness changes between magnitude 5,33 and 5.44 have been widely reported.[6][14] The type of variability is thought to be related to its rapid rotation and a surrounding shell, and is tentatively given as a combination of a Be star and Maia variable.[15]

The magnitude 5.7 primary, component A,[2] is a blue-white hued Be star[10] with a stellar classification B6 III.[4] At 115 million years old,[10] the star is spinning rapidly with a projected rotational velocity of 265.[8] It has an estimated four times the mass of the Sun and is radiating 604 times the solar luminosity at an effective temperature of 11,272 K.[8] The secondary, component B, has a visual magnitude of 6.8[2] and a spectral class of B8.5 V.[4]

Eta Piscis Austrini is moving through the Galaxy at a speed of 11.3 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,600 and 30,800 light years from the center of the Galaxy.[16][unreliable source?]

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 Fabricius, C.; Makarov, V. V. (April 2000), "Two-colour photometry for 9473 components of close Hipparcos double and multiple stars", Astronomy and Astrophysics 356: 141–145, Bibcode: 2000A&A...356..141F. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  4. ↑ 4.0 4.1 4.2 Corbally, C. J. (August 1984), "Close visual binaries. I - MK classifications", The Astrophysical Journal Supplement Series 55: 657, doi:10.1086/190973, ISSN 0067-0049, Bibcode: 1984ApJS...55..657C. 
  5. ↑ 5.0 5.1 5.2 Feinstein, A.; Marraco, H. G. (November 1979), "The photometric behavior of Be Stars", Astronomical Journal 84: 1713–1725, doi:10.1086/112600, Bibcode: 1979AJ.....84.1713F. 
  6. ↑ 6.0 6.1 Samus, N. N. 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. 
  7. ↑ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A. 
  8. ↑ 8.0 8.1 8.2 Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics 537: A120, doi:10.1051/0004-6361/201117691, Bibcode: 2012A&A...537A.120Z. 
  9. ↑ 9.0 9.1 9.2 9.3 Zorec, J.; Frémat, Y.; Domiciano De Souza, A.; Royer, F.; Cidale, L.; Hubert, A.-M.; Semaan, T.; Martayan, C. et al. (2017), "Critical study of the distribution of rotational velocities of Be stars", Astronomy & Astrophysics 595: A132, doi:10.1051/0004-6361/201628760, Bibcode: 2016A&A...595A.132Z. 
  10. ↑ 10.0 10.1 10.2 Zorec, J. et al. (October 2005), "On the evolutionary status of Be stars. I. Field Be stars near the Sun", Astronomy and Astrophysics 441 (1): 235–248, doi:10.1051/0004-6361:20053051, Bibcode: 2005A&A...441..235Z. 
  11. ↑ 11.0 11.1 11.2 Anders, F.; Khalatyan, A.; Queiroz, A. B. A.; Chiappini, C.; Ardevol, J.; Casamiquela, L.; Figueras, F.; Jimenez-Arranz, O. et al. (2022), "VizieR Online Data Catalog: StarHorse2, Gaia EDR3 photo-astrometric distances (Anders+, 2022)", Vizier Online Data Catalog, Bibcode: 2022yCat.1354....0A. 
  12. ↑ "eta PsA -- Be Star", SIMBAD Astronomical Database (Centre de Données astronomiques de Strasbourg), http://simbad.u-strasbg.fr/simbad/sim-id?Ident=eta+PsA, retrieved 2017-05-18. 
  13. ↑ van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V. 
  14. ↑ NSV 13993, AAVSO, https://www.aavso.org/vsx/index.php?view=detail.top&oid=52617, retrieved 2023-04-02 
  15. ↑ Balona, L. A.; Handler, G.; Chowdhury, S.; Ozuyar, D.; Engelbrecht, C. A.; Mirouh, G. M.; Wade, G. A.; David-Uraz, A. et al. (2019), "Rotational modulation in TESS B stars", Monthly Notices of the Royal Astronomical Society 485 (3): 3457, doi:10.1093/mnras/stz586, Bibcode: 2019MNRAS.485.3457B. 
  16. ↑ Eta Piscis Austrini (HIP 108661)[yes|permanent dead link|dead link}}]



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