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Eta Persei

From Wikipedia, the free encyclopedia
Star system in the constellation Perseus
η Persei
Location of η Per (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationPerseus
Right ascension02h 50m 41.810s[1]
Declination+55° 53′ 43.80″[1]
Apparent magnitude (V)3.79[2]
Characteristics
Evolutionary stageRed supergiant
Spectral typeK3 Ib[3]
U−Bcolor index+1.90[2]
B−Vcolor index+1.69[2]
Astrometry
Radial velocity (Rv)−1.07±0.27[4] km/s
Proper motion (μ)RA: +16.346mas/yr[1]
Dec.: −13.518mas/yr[1]
Parallax (π)3.2657±0.1873 mas[1]
Distance1,000 ± 60 ly
(310 ± 20 pc)
Absolute magnitude (MV)−4.29[5]
Details
Mass8±0.4[6] M
Radius173.1+9.69
−10.8
[7] R
Luminosity7,508±864[7] L
Surface gravity (log g)0.26[7] cgs
Temperature4082±30[7] K
Rotational velocity (v sin i)5.8[3] km/s
Age37.8±6.2[6] Myr
Other designations
Miram, η Persei, η Per,Eta Per,15 Persei,BD+55 714,CCDM J02506+5553A,FK5 99,GC 3390,HD 17506,HIP 13268,HR 834,IDS 02434+5529 A,PPM 28039,SAO 23655,WDS J02507+5554A
Database references
SIMBADdata

Eta Persei (η Persei, abbreviatedEta Per,η Per), is ared supergiant in theconstellation ofPerseus.Parallax measurements by theGaia spacecraft imply that it is 1,000 islight-years away fromEarth.[1] At such distance,interstellar dust diminishes its apparent brightness by 0.47 magnitudes.[7]

The two components of Eta Persei itself are designated Eta Persei A (officially namedMiram/ˈmræm/, a recent name for the system)[8] and B.

Nomenclature

[edit]
η Persei in optical light

η Persei (Latinised toEta Persei) is the binary star'sBayer designation. The designations of its two components asEta Persei A andB derive from the convention used by the Washington Multiplicity Catalog (WMC) formultiple star systems, and adopted by theInternational Astronomical Union (IAU).[9]

Eta Persei mysteriously gained the namedMiram in the 20th Century, though no source is known.[10][11] In 2016, the IAU organized aWorking Group on Star Names (WGSN)[12] to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entiremultiple systems.[13] It approved the nameMiram for the component Eta Persei A on 5 September 2017 and it is now so included in the List of IAU-approved Star Names.[8]

This star, together withDelta Persei,Psi Persei,Sigma Persei,Alpha Persei andGamma Persei has been calledthe Segment of Perseus.[11]

InChinese,天船 (Tiān Chuán), meaningCelestial Boat, refers to anasterism consisting of Eta Persei, Gamma Persei, Alpha Persei, Psi Persei, Delta Persei,48 Persei,Mu Persei andHD 27084. Consequently, theChinese name for Eta Persei itself is天船一 (Tiān Chuán yī, English:the First Star of Celestial Boat.)[14]

Properties

[edit]

The primary star (η Persei A) has aspectral classification of K3 Ib,[3] meaning that it is a lower luminosityred supergiant star. It has expanded to 170 times the Sun's size and currently is emitting 7,500 times itsluminosity. Its surface has aneffective temperature of4,082 K,[7] which is cooler than the Sun and gives it an orange hue, typical ofK-type stars.[15]

Multiple star catalogues list a number of companions to Eta Persei, but it is unclear if any are physically related.[16] The brightest close companion is 8th-magnitude HD 23700928 away, with 9th-magnitude HD 174564′ away. Of the six companions listed in theWashington Double Star Catalogue,[17] only HD 237009 has a similar parallax to Eta Persei.[18]

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. ^abcDucati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".CDS/ADC Collection of Electronic Catalogues.2237.Bibcode:2002yCat.2237....0D.
  3. ^abcDe Medeiros, J. R.; Udry, S.; Burki, G.; Mayor, M. (2002). "A catalog of rotational and radial velocities for evolved stars. II. Ib supergiant stars".Astronomy and Astrophysics.395:97–98.arXiv:1312.3474.Bibcode:2002A&A...395...97D.doi:10.1051/0004-6361:20021214.S2CID 263226802.
  4. ^Famaey, B.; Jorissen, A.; Luri, X.; Mayor, M.; Udry, S.; Dejonghe, H.; Turon, C. (2005). "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters".Astronomy and Astrophysics.430: 165.arXiv:astro-ph/0409579.Bibcode:2005A&A...430..165F.doi:10.1051/0004-6361:20041272.S2CID 17804304.
  5. ^Ryon, Jenna; Shetrone, Matthew D.; Smith, Graeme H. (2009). "Comparing the Ca ii H and K Emission Lines in Red Giant Stars".Publications of the Astronomical Society of the Pacific.121 (882): 842.arXiv:0907.3346.Bibcode:2009PASP..121..842R.doi:10.1086/605456.S2CID 17821279.
  6. ^abTetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (2011-01-01)."A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun".Monthly Notices of the Royal Astronomical Society.410 (1):190–200.arXiv:1007.4883.Bibcode:2011MNRAS.410..190T.doi:10.1111/j.1365-2966.2010.17434.x.ISSN 0035-8711.Eta Persei's database entry atVizieR.
  7. ^abcdefBaines, Ellyn K.; Clark, James H., III; Schmitt, Henrique R.; Stone, Jordan M.; von Braun, Kaspar (2023-12-01)."33 New Stellar Angular Diameters from the NPOI, and Nearly 180 NPOI Diameters as an Ensemble".The Astronomical Journal.166 (6): 268.arXiv:2505.23514.Bibcode:2023AJ....166..268B.doi:10.3847/1538-3881/ad08be.ISSN 0004-6256.
  8. ^ab"Naming Stars". IAU.org. Retrieved16 December 2017.
  9. ^Hessman, F. V.; Dhillon, V. S.; Winget, D. E.; Schreiber, M. R.; Horne, K.; Marsh, T. R.; Guenther, E.; Schwope, A.; Heber, U. (2010). "On the naming convention used for multiple star systems and extrasolar planets".arXiv:1012.0707 [astro-ph.SR].
  10. ^Kaler, Jim."Eta Persei". Retrieved2017-02-11.
  11. ^abAllen, R. H. (1963).Star Names: Their Lore and Meaning (Reprint ed.). New York: Dover Publications Inc. p. 331.ISBN 0-486-21079-0. Retrieved2012-09-04.{{cite book}}:ISBN / Date incompatibility (help)
  12. ^"IAU Working Group on Star Names (WGSN)". Retrieved22 May 2016.
  13. ^"WG Triennial Report (2015-2018) - Star Names"(PDF). p. 5. Retrieved2018-07-14.
  14. ^(in Chinese)AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 11 日Archived 2012-02-04 at theWayback Machine
  15. ^"The Colour of Stars".Australia National Telescope Facility. 6 March 2024. Retrieved2024-05-27.
  16. ^"Eta Persei".University of Illinois. Retrieved2025-02-27.
  17. ^Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog".The Astronomical Journal.122 (6): 3466.Bibcode:2001AJ....122.3466M.doi:10.1086/323920.
  18. ^Vallenari, 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.
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