In today's world,
Sigma1 Ursae Majoris has become a topic of increasing interest to a large number of people. Since its emergence,
Sigma1 Ursae Majoris has generated debates, discussions and reflections in various areas. Regardless of age, gender or educational background,
Sigma1 Ursae Majoris has managed to capture the attention of audiences around the world. Its impact is not limited to a single context, but extends to multiple fields, influencing the way people think, act, and relate to each other. In this article, we will explore in detail the
Sigma1 Ursae Majoris phenomenon and the effects it has had on our society.
Solitary star in the constellation Ursa Major
Sigma1 Ursae Majoris (σ1 UMa ) is the Bayer designation for a solitary[ 8] star in the northern circumpolar constellation of Ursa Major . With an apparent visual magnitude of 5.14[ 2] it is faintly visible to the naked eye on dark nights. Based upon an annual parallax shift of 6.26 mas ,[ 1] it is located roughly 520 light years from the Sun . At that distance, the visual magnitude of the star is diminished by an extinction factor of 0.06[ 3] due to interstellar dust .
This is an evolved K-type giant star with a stellar classification of K5 III.[ 3] It is a suspected variable with an amplitude of 0.03 magnitude.[ 3] The measured angular diameter of the star after correcting for limb darkening is 2.67± 0.04 mas ,[ 9] which, at the estimated distance of this star, yields a physical size of about 46 times the radius of the Sun .[ 5] The star is radiating around 560[ 3] times the solar luminosity from its outer atmosphere at an effective temperature of 3,940 K.[ 6]
Naming
With π1 , π2 , σ2 , ρ , A and d , it composed the Arabic asterism Al Ṭhibā᾽ , the Gazelle.[ 10] According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars , Al Ṭhibā were the title for seven stars : A as Althiba I , this star (π1 ) as Althiba II , π2 as Althiba III , ρ as Althiba IV , this star (σ1 ) as Althiba V , σ2 as Althiba VI , and d as Althiba VII .[ 11]
References
^ a b c d e f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics , 474 (2): 653– 664, arXiv :0708.1752 , Bibcode :2007A&A...474..653V , doi :10.1051/0004-6361:20078357 , S2CID 18759600 .
^ a b c d Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data , SIMBAD , Bibcode :1986EgUBV........0M .
^ a b c d e f g Groenewegen, M. A. T. (April 2012), "Infrared excess around nearby red giant branch stars and Reimers law", Astronomy & Astrophysics , 540 : 21, Bibcode :2012A&A...540A..32G , doi :10.1051/0004-6361/201118287 , A32.
^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics , 546 : 14, arXiv :1208.3048 , Bibcode :2012A&A...546A..61D , doi :10.1051/0004-6361/201219219 , S2CID 59451347 , A61.
^ a b Lang, Kenneth R. (2006), Astrophysical formulae , Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser , ISBN 3-540-29692-1 . The radius (R* ) is given by:
2
⋅
R
∗
=
(
159.7
⋅
2.67
⋅
10
−
3
)
AU
0.0046491
AU
/
R
⨀
≈
91.7
⋅
R
⨀
{\displaystyle {\begin{aligned}2\cdot R_{*}&={\frac {(159.7\cdot 2.67\cdot 10^{-3})\ {\text{AU}}}{0.0046491\ {\text{AU}}/R_{\bigodot }}}\\&\approx 91.7\cdot R_{\bigodot }\end{aligned}}}
^ a b c d Soubiran, C.; et al. (June 2010), "The PASTEL catalogue of stellar parameters", Astronomy and Astrophysics , 515 : A111, arXiv :1004.1069 , Bibcode :2010A&A...515A.111S , doi :10.1051/0004-6361/201014247 , S2CID 118362423 .
^ "sig01 UMa" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2017-02-25 .{{cite web }}
: CS1 maint: postscript (link )
^ 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 .
^ Richichi, A.; et al. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics , 431 (2): 773– 777, Bibcode :2005A&A...431..773R , doi :10.1051/0004-6361:20042039 .
^ Allen, Richard Hinckley (1899), Star-Names and Their Meanings , New York: G. E. Stechert, p. 444
^ Rhoads, Jack W. (November 15, 1971), Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars (PDF) , Jet Propulsion Laboratory, California Institute of Technology.