Ursa Major Ro ( ρ Ursae Majoris , ρ UMa ) is a single [9] star in the northern constellation Ursa Major . It is poorly visible to the naked eye, has a visible magnitude of 4.74. [2] The distance to this star obtained by measuring parallax equal to 10.37 msd [1] is about 315 light years .
| Ro Big Dipper | |||
|---|---|---|---|
| Star | |||
| Observational data ( Age J2000) | |||
| Right ascension | 09 h 02 m 32.69092 s [1] | ||
| Declination | + 67 ° 37 ′ 46.6280 ″ [1] | ||
| Visible magnitude ( V ) | 4.74 [2] | ||
| Constellation | |||
| Astrometry | |||
| Radial velocity ( R v ) | 4.75 ± 0.19 [3] km / s | ||
| Own movement (μ) | RA: −22.83 [1] Dec: +18,13 [1] | ||
| Parallax (π) | 10.37 ± 0.25 [1] mas | ||
| Absolute magnitude (V) | +0.06 [4] | ||
| Specifications | |||
| Spectral class | M3 III [5] | ||
| Color Index ( B - V ) | +1.56 [2] | ||
| Color Index ( U - B ) | +1.84 [2] | ||
| physical characteristics | |||
| Radius | 58 [6] R ☉ | ||
| Temperature | 3725 [7] K | ||
| Luminosity | 464 [7] L ☉ | ||
| |||
| Database Information | |||
| SIMBAD | data | ||
Belongs to the spectral class M3 III, [5] that is, it is a red giant on the asymptotic branch of giants . [10] Probably a variable star with a small amplitude. [11] The measured angular diameter of the star after correction for darkening to the edge is 5.64 ± 0.15 mas , [12] which corresponds to a linear size of about 58 solar radii. [6] The luminosity ρ of Ursa Major is 464 of the luminosity of the Sun, the effective temperature is estimated at 3715 K. [7] Based on the data on the spatial motion of the star, the probability of belonging to its Sirius flux is estimated at 60.6%. [four]
Notes
- ↑ 1 2 3 4 5 6 van Leeuwen, F. (2007), " Validation of the new Hipparcos reduction ", Astronomy and Astrophysics T. 474 (2): 653–664 , DOI 10.1051 / 0004-6361: 20078357
- ↑ 1 2 3 4 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalog of Eggen's UBV data (SIMBAD)
- ↑ de Bruijne, JHJ & Eilers, A.-C. (October 2012), " Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project ", Astronomy & Astrophysics T. 546: 14, A61 , DOI 10.1051 / 0004-6361 / 201219219
- ↑ 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 (1): 165 –186 , DOI 10.1051 / 0004-6361: 20041272
- ↑ 1 2 Marrese, PM; Boschi, F. & Munari, U. (August 2003), " High resolution spectroscopy over lambda lambda 8500-8750 Å for GAIA. IV. Extending the cool MK stars sample ", Astronomy and Astrophysics T. 406: 995–999 , DOI 10.1051 / 0004-6361: 20030647
- ↑ 1 2 Lang, Kenneth R. (2006), Astrophysical formulae , vol. 1 (3rd ed.), Astronomy and astrophysics library, Birkhäuser, ISBN 3-540-29692-1 , < https://books.google.com/books?id=OvTjLcQ4MCQC&pg=PA41 > The radius (R * ) is determined by the relation
- ↑ 1 2 3 McDonald, I .; Zijlstra, AA & Boyer, ML (2012), " Fundamental Parameters and Infrared Excesses of Hipparcos Stars ", Monthly Notices of the Royal Astronomical Society T. 427 (1): 343–57 , DOI 10.1111 / j.1365-2966.2012.21873 .x
- ↑ rho UMa - Variable Star , Center de Données astronomiques de Strasbourg , < http://simbad.u-strasbg.fr/simbad/sim-id?Ident=rho+Uma > . Retrieved February 25, 2017.
- ↑ Eggleton, PP & Tokovinin, AA (September 2008), " A catalog of multiplicity among bright stellar systems ", Monthly Notices of the Royal Astronomical Society T. 389 (2): 869–879 , DOI 10.1111 / j.1365-2966.2008 .13596.x
- ↑ Eggen, OJ (1992), " Asymptotic giant branch stars near the sun ", The Astronomical Journal T. 104: 275 , DOI 10.1086 / 116239
- ↑ Percy, JR; Wong, N .; Bohme, D. & Curott, DR (1994), " Photometric surveys of suspected small-amplitude red variables. III: An AAVSO photometric photometry survey ", Astronomical Society of the Pacific T. 106 (700): 611-615 , DOI 10.1086 / 133420
- ↑ Richichi, A .; Percheron, I. & Khristoforova, M. (February 2005), " CHARM2: An updated Catalog of High Angular Resolution Measurements ", Astronomy and Astrophysics T. 431: 773–777 , DOI 10.1051 / 0004-6361: 20042039