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Psi Big Dipper

Psi Big Dipper ( lat. Psi Ursae Majoris , Ursae Majoris , UMa ) is a star in the northern constellation Ursa Major . It has an apparent magnitude of +3.01, [2] while the star is visible with the naked eye and is one of the brightest stars in the constellation. Parallax measurements provide an estimate of the distance of 144.5 light years (44.3 parsec ) from the Sun. [1] This is a fairly close distance, so the star's brightness is attenuated only by approximately 0.05 stellar magnitude due to interstellar extinction [3] . In Chinese astronomy, the star is called Tien Tsan or Ta Tsun , "Very Honorable." [11] The name may have come from the word 太 尊, pinyin : Tàizūn, which means royal , since the star is very prominent.

ψ Ursa Major
Star
Ursa Major IAU.svg
Locator Dot2.gif
Observational data
( Epoch J2000.0 )
Right ascension
Declination
Distance144.5 sv. of the year
Visible magnitude ( V )+3.01 [2]
Constellation
Astrometry
Radial velocity ( R v )–3.39 [3] km / s
Proper motion (μ)RA: –62.02 [1] mas per year
Dec: –27,41 [1] mas per year
Parallax (π)22.57 ± 0.14 [1] mas
Absolute magnitude (V)−0.27 [4]
Specifications
Spectral classK1III [5]
Color Indicator ( B - V )+1.14 [2]
Color Index ( U - B )+1.12 [2]
physical characteristics
Radius19.7 ± 0.6 [6] R ☉
Age1.11 ± 0.39 [7] billion years
Temperature4520 [5] K
Luminosity148 ± 12 [6] L ☉
Metallicityfrom –0.13 [6] to 0.16 [5]
Rotation5.5 [8] km / s
Other designations
ψ Ursae Majoris, ψ UMa, Psi UMa, 52 Ursae Majoris, BD +45 1897, FK5 420, GC 15340, HD 96833, HIP 54539, HR 4335, PPM 52277, SAO 43629. [9]
Information in databases
SIMBADdata

The spectrum of the star corresponds to the spectral class K1 III, [5] the luminosity class 'III' means that the star is a giant that has exhausted the supply of hydrogen in the core. Consequently, the star has expanded to 20 [6] the radii of the Sun. The luminosity in 148 [6] exceeds the solar, the external atmosphere has an effective temperature of 4520 K [5]. At this temperature, the star has an orange color of the surface. [12] .

Psi Big Dipper is a representative of the population of the Milky Way thin disk . It is in orbit with a small eccentricity of 0.02, as a result of which the distance from the star to the center of the Galaxy varies from 26.5 to 27.8 thousand light years. A small orbital inclination means that the star is only 130 light years away from the galactic plane . [7]

Notes

  1. ↑ 1 2 3 4 5 6 van Leeuwen, F. (November 2007), " Validation of the New Hipparcos reduction ", Astronomy and Astrophysics T. 474 (2): 653–664 , DOI 10.1051 / 0004-6361: 20078357  
  2. ↑ 1 2 3 4 Jennens, PA & Helfer, HL (September 1975), " A & C Giants . ", Monthly Notices of the Royal Astronomical Society T. 172: 667–679 , DOI 10.1093 / mnras / 172.3.667  
  3. ↑ 1 2 Famaey, B .; Jorissen, A .; Luri, X. & Mayor, M. (January 2005), “ Local kinematics of K and M giants from CORAVEL / Hipparcos / Tycho-2 data. Revisiting the concept of superclusters ”, Astronomy and Astrophysics T. 430: 165–186 , DOI 10.1051 / 0004-6361: 20041272  
  4. ↑ Cardini, D. (January 2005), " Mg II chromospheric radiative and quiet stars ", Astronomy and Astrophysics T. 430: 303–311 , DOI 10.1051 / 0004-6361: 20041440  
  5. ↑ 1 2 3 4 5 Frasca, A .; Covino, E .; Spezzi, L. & Alcalá, JM (December 2009), " Orion. Rotational periods and stars parameters ", Astronomy and Astrophysics T. 508 (3): 1313– 1330 , DOI 10.1051 / 0004-6361 / 200913327  
  6. ↑ 1 2 3 4 5 Piau, L .; Kervella, P .; Dib, S. & Hauschildt, P. (February 2011), " Surface convection and red-giant radius measurements ", Astronomy and Astrophysics T. 526: A100 , DOI 10.1051 / 0004-6361 / 201014442  
  7. ↑ 1 2 Soubiran, C .; Bienaymé, O .; Mishenina, TV & Kovtyukh, VV (2008), " Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants ", Astronomy and Astrophysics T. 480 (1): 91–101 , DOI 10.1051 / 0004-6361: 20078788  
  8. ↑ Massarotti, Alessandro; Latham, David W .; Stefanik, Robert P .; Fogel, Jeffrey. Rotational and Radial Velocities for a Sample of 761 Hipparcos Giants and the Role of Binarity (English) // The Astronomical Journal : journal. - IOP Publishing , 2008. - January ( vol. 135 , no. 1 ). - P. 209–231 . - DOI : 10.1088 / 0004-6256 / 135/1/209 . - .
  9. ↑ psi UMa - Star , Center de Données astronomiques de Strasbourg , < http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Psi+Ursae+Majoris > . Retrieved January 16, 2012.  
  10. ↑ VizieR
    <a href=" https://wikidata.org/wiki/Track:Q1662358 "> </a>
  11. ↑ Allen, Richard Hinckley (1963), Star Names - Their Lore and Meaning: Ursa Major (Dover ed.), University of Chicago , < http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/ _Texts / secondary / ALLSTA / Ursa_Major * .html >  
  12. ↑ The Color of Stars , Commonwealth Scientific and Industrial Research Organization, December 21, 2004 , < http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html > . Retrieved January 16, 2012.  
Source - https://ru.wikipedia.org/w/index.php?title=Psi_Big_Medveditsy&oldid=101020904


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