astro.wikisort.org - Star

Search / Calendar

θ1 Microscopii, Latinized as Theta1 Microscopii, is a suspected binary star[10] system in the southern constellation of Microscopium. It is visible to the naked eye was a faint, white-hued point of light with an apparent visual magnitude of 4.82.[2] The distance to this system is approximately 179 light years based on parallax.[1]

For other stars with the name θ Microscopii, see Theta Microscopii.
Theta1 Microscopii
Location of θ1 Microscopii (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Microscopium
Right ascension 21h 20m 45.62633s[1]
Declination −40° 48′ 34.3607″[1]
Apparent magnitude (V) 4.82[2]
Characteristics
Spectral type A7VpSrCrEu[3]
U−B color index -0.07[2]
B−V color index +0.02[2]
Variable type α2 CVn[4]
Astrometry
Radial velocity (Rv)+2.30[5] km/s
Proper motion (μ) RA: +75.480[1] mas/yr
Dec.: +8.657[1] mas/yr
Parallax (π)18.2678 ± 0.5314 mas[1]
Distance179 ± 5 ly
(55 ± 2 pc)
Absolute magnitude (MV)1.03[6]
Details[7]
Mass2.32+0.18
−0.26 M☉
Radius2.35±0.34 R☉
Luminosity36.3+8.4
−6.8 L☉
Surface gravity (log g)4.06±0.12 cgs
Temperature9,240±480 K
Metallicity [Fe/H]0.00[8] dex
Rotational velocity (v sin i)43.7±1.7 km/s
Age437±209 Myr
Other designations
θ1 Mic, CD−41°14475, FK5 802, GC 29854, HD 203006, HIP 105382, HR 8151, SAO 230644, WDS J21208-4049[9]
Database references
SIMBADdata

The primary is an α2 CVn variable with a period of 2.125 days and a magnitude ranging from 4.77 to 4.87,[4] as well as an Ap star, a chemically peculiar star with strong metallic lines in its spectrum.[3][6] It is an A-type main-sequence star with a stellar classification of A7VpSrCrEu,[3] where the suffix notation indicates abundance anomalies of strontium, chromium, and europium. The star is 437 million years old with 2.3 times the mass of the Sun and 2.4 times the Sun's radius. It is radiating 36 times the luminosity of the Sun from its photosphere at an effective temperature of 9,240 K.[7]

Its companion is a magnitude 7.42 star at an angular separation of 0.10″ from the primary along a position angle of 46°, as of 2018.[11]


References


  1. Brown, 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 at VizieR.
  2. Ducati, 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. Abt, Helmut A.; Morrell, Nidia I. (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. Watson, C. L. (2006). The International Variable Star Index (VSX). The Society for Astronomical Sciences 25th Annual Symposium on Telescope Science. Held May 23–25. Vol. 25. p. 47. Bibcode:2006SASS...25...47W.
  5. Wilson, R. E. (1953). "General Catalogue of Stellar Radial Velocities". Carnegie Institute Washington D.C. Publication. Carnegie Institution of Washington. Bibcode:1953GCRV..C......0W. ISBN 9780598216885. LCCN 54001336.
  6. Anderson, 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. Vizier catalog entry
  7. Sikora, J.; et al. (February 2019). "A Volume-Limited Survey of mCP Stars Within 100pc I: Fundamental Parameters and Chemical Abundances". Monthly Notices of the Royal Astronomical Society. 483 (2): 2300–2324. arXiv:1811.05633. Bibcode:2019MNRAS.483.2300S. doi:10.1093/mnras/sty3105. S2CID 119089236.
  8. Gontcharov, G. A. (2012). "Dependence of kinematics on the age of stars in the solar neighborhood". Astronomy Letters. 38 (12): 771–782. arXiv:1606.08814. Bibcode:2012AstL...38..771G. doi:10.1134/S1063773712120031. S2CID 118345778. Vizier catalog entry
  9. "tet01 Mic". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-09-03.{{cite web}}: CS1 maint: postscript (link)
  10. Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv:0806.2878. Bibcode:2008MNRAS.389..869E. doi:10.1111/j.1365-2966.2008.13596.x. S2CID 14878976.
  11. Mason, B. D.; et al. (2014). "The Washington Visual Double Star Catalog". The Astronomical Journal. 122 (6): 3466. Bibcode:2001AJ....122.3466M. doi:10.1086/323920.

На других языках

- [en] Theta1 Microscopii

[es] Theta1 Microscopii

Theta1 Microscopii (θ1 Mic / HD 203006 / HR 8151)[1] es una estrella de la constelación de Microscopium. De magnitud aparente +4,78, es la tercera más brillante de la constelación detrás de γ Microscopii y ε Microscopii, siendo su brillo ligeramente mayor que el de α Microscopii. Comparte la denominación de Bayer Theta con Theta2 Microscopii, esta última unas tres veces más alejada que Theta1 Microscopii, que se encuentra a 187 años luz del Sistema Solar.


Текст в блоке "Читать" взят с сайта "Википедия" и доступен по лицензии Creative Commons Attribution-ShareAlike; в отдельных случаях могут действовать дополнительные условия.

Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.

2019-2025
WikiSort.org - проект по пересортировке и дополнению контента Википедии