HR 8832

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HR 8832
Observation data
Epoch J2000      Equinox J2000
Constellation Cassiopeia
Right ascension 23h 13m 16.97632s[1]
Declination +57° 10′ 06.0823″[1]
Apparent magnitude (V) 5.574[2]
Characteristics
Spectral type K3 V[3]
U−B color index +0.902[2]
B−V color index +0.983[2]
Variable type Suspected[4]
Astrometry
Radial velocity (Rv) –18.5[5] km/s
Proper motion (μ) RA: +2,075.07 ± 0.33[1] mas/yr
Dec.: +295.45 ± 0.25[1] mas/yr
Parallax (π) 152.76 ± 0.29[1] mas
Distance 21.35 ± 0.04 ly
(6.55 ± 0.01 pc)
Absolute magnitude (MV) 6.50
Details
Mass 0.794+0.037
−0.022
[6] M
Radius 0.80 ± 0.04[7] R
Luminosity 0.28[note 1] L
Surface gravity (log g) 4.50[3] cgs
Temperature 4,710[3] K
Metallicity [Fe/H] +0.20[3] dex
Rotational velocity (v sin i) 6.94[8] km/s
Age ~12.46[6] Gyr
Other designations
BD+56 2966, FK5 875, GCTP 5616.00, Gl 892, HD 219134, HIP 114622, LFT 1767, LHS 71, LTT 16826, SAO 35236.[9]

HR 8832 is a main sequence star in the constellation of Cassiopeia. It is smaller and less luminous than our Sun, with a spectral class of K3V, which makes it an orange-red hued star. HR 8832 is relatively close to our system, with an estimated distance of 21.25 light years. This star is close to the limit of apparent magnitude that can still be seen by the unaided eye. The limit is considered to be magnitude 6 for most observers.

This star has a magnitude 9.4 companion at an angular separation of 106.6 arcseconds.[10]

Distance[edit]

HR 8832 distance estimates

Source Parallax, mas Distance, pc Distance, ly Distance, Pm Ref.
Woolley et al. (1970) 147 ± 4 6.8+0.19
−0.18
22.2 ± 0.6 209.9+5.9
−5.6
[11]
Gliese & Jahreiß (1991) 146.4 ± 4.7 6.83+0.23
−0.21
22.3 ± 0.7 210.8+7
−6.6
[12]
van Altena et al. (1995) 153.8 ± 1.0 6.5 ± 0.04 21.21 ± 0.14 200.6 ± 1.3 [13]
Perryman et al. (1997) (Hipparcos) 153.24 ± 0.65 6.526 ± 0.028 21.28 ± 0.09 201.4 ± 0.9 [14]
Perryman et al. (1997) (Tycho) (absents) [15]
van Leeuwen (2007) 152.76 ± 0.29 6.546 ± 0.012 21.35 ± 0.04 202 ± 0.4 [16]
RECONS TOP100 (2012) 152.84 ± 0.28[note 2] 6.543 ± 0.012 21.34 ± 0.04 201.9 ± 0.4 [17]

Non-trigonometric distance estimates are marked in italic.

References[edit]

  1. ^ a b c d e van Leeuwen, F. (November 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. 
  2. ^ a b c Oja, T. (August 1986), "UBV photometry of stars whose positions are accurately known. III", Astronomy and Astrophysics Supplement Series 65 (2): 405–409, Bibcode:1986A&AS...65..405O. 
  3. ^ a b c d Frasca, A. et al. (December 2009), "REM near-IR and optical photometric monitoring of pre-main sequence stars in Orion. Rotation periods and starspot parameters", Astronomy and Astrophysics 508 (3): 1313–1330, Bibcode:2009A&A...508.1313F, doi:10.1051/0004-6361/200913327. 
  4. ^ Kukarkin, B. V. et al. (1981), "Nachrichtenblatt der Vereinigung der Sternfreunde e.V. (Catalogue of suspected variable stars)", Nachrichtenblatt der Vereinigung der Sternfreunde e.V. (1981) (Moscow: Academy of Sciences USSR Shternberg): 0, Bibcode:1981NVS...C......0K. 
  5. ^ Wielen, R. et al. (1999), "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions", Veröff. Astron. Rechen-Inst. Heidelb (Astronomisches Rechen-Institut Heidelberg) 35 (35): 1, Bibcode:1999VeARI..35....1W. 
  6. ^ a b Takeda, Genya et al. (February 2007), "Structure and Evolution of Nearby Stars with Planets. II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog", The Astrophysical Journal Supplement Series 168 (2): 297–318, arXiv:astro-ph/0607235, Bibcode:2007ApJS..168..297T, doi:10.1086/509763. 
  7. ^ Perrin, M.-N.; Karoji, H. (1987), "Stellar radius determination from IRAS 12-micron fluxes", Astronomy and Astrophysics 172: 235–240, Bibcode:1987A&A...172..235P. 
  8. ^ Martínez-Arnáiz, R. et al. (September 2010), "Chromospheric activity and rotation of FGK stars in the solar vicinity. An estimation of the radial velocity jitter", Astronomy and Astrophysics 520: A79, arXiv:1002.4391, Bibcode:2010A&A...520A..79M, doi:10.1051/0004-6361/200913725. 
  9. ^ "HR 8832 -- Flare Star", SIMBAD Astronomical Object Database (Centre de Données astronomiques de Strasbourg), retrieved 2012-04-08. 
  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. 
  11. ^ Woolley R.; Epps E. A.; Penston M. J.; Pocock S. B. (1970). "Woolley 892". Catalogue of stars within 25 parsecs of the Sun. 
  12. ^ Gliese, W. and Jahreiß, H. (1991). "Gl 892". Preliminary Version of the Third Catalogue of Nearby Stars. 
  13. ^ Van Altena W. F., Lee J. T., Hoffleit E. D. (1995). "GCTP 5616". The General Catalogue of Trigonometric Stellar Parallaxes (Fourth ed.). 
  14. ^ Perryman et al. (1997). "HIP 114622". The Hipparcos and Tycho Catalogues. 
  15. ^ Perryman et al. (1997). "HIP 114622". The Hipparcos and Tycho Catalogues. 
  16. ^ van Leeuwen F. (2007). "HIP 114622". Validation of the new Hipparcos reduction. 
  17. ^ "RECONS TOP100". THE ONE HUNDRED NEAREST STAR SYSTEMS brought to you by RECONS (Research Consortium On Nearby Stars). 2012. 

Notes[edit]

  1. ^ From \begin{smallmatrix}L=4 \pi R^2 \sigma T_{\rm eff}^4 \end{smallmatrix}, where \begin{smallmatrix}L \end{smallmatrix} is the luminosity, \begin{smallmatrix}R \end{smallmatrix} is the radius, \begin{smallmatrix}T_{\rm eff}\end{smallmatrix} is the effective surface temperature and \begin{smallmatrix}\sigma \end{smallmatrix} is the Stefan–Boltzmann constant
  2. ^ Weighted parallax based on parallaxes from van Altena et al. (1995) and van Leeuwen (2007).

External links[edit]

Coordinates: Sky map 23h 13m 16.98s, +57° 10′ 06.1″