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AR Cassiopeiae information


AR Cassiopeiae

A light curve for AR Cassiopeiae, plotted from TESS data[1]
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cassiopeia[2]
AB
Right ascension 23h 30m 01.93946s[3]
Declination +58° 32′ 56.1120″[3]
Apparent magnitude (V) 4.883 (4.912 / 8.814)[4]
CD
Right ascension 23h 29m 52.2802s[5]
Declination +58° 32′ 54.458″[5]
Apparent magnitude (V) 7.09[6]
Characteristics
AB
Spectral type B4 V + A6 V[4]
U−B color index −0.62[7]
B−V color index −0.12[7]
Variable type Algol[8]
CD
Spectral type B9 V[6]
U−B color index −0.14[7]
B−V color index +0.01[7]
FG
Spectral type F7 IV + F9 V[9]
Astrometry
Radial velocity (Rv)−15.9±0.9[10] km/s
Proper motion (μ) RA: 17.90[3] mas/yr
Dec.: 4.15[3] mas/yr
Parallax (π)5.25 ± 0.52 mas[3]
Distance620 ± 60 ly
(190 ± 20 pc)
Aa
Absolute magnitude (MV)−1.87±0.13[4]
Absolute bolometric
magnitude (Mbol)
−3.56±0.13[4]
Ab
Absolute magnitude (MV)2.20±0.11[4]
Absolute bolometric
magnitude (Mbol)
2.18±0.11[4]
Orbit[4]
PrimaryAa
CompanionAb
Period (P)6.0663170 d
Eccentricity (e)0.240
Inclination (i)85.34±0.50°
Periastron epoch (T)JD 2436847.9404±0.0055
Argument of periastron (ω)
(secondary)
41.82±0.47°
Details[4]
Aa
Mass5.90±0.20 M
Radius5.05±0.06 R
Surface gravity (log g)3.80±0.02 cgs
Temperature17,200±500 K
Ab
Mass1.86±0.06 M
Radius1.60±0.03 R
Surface gravity (log g)4.30±0.02 cgs
Temperature8,150±200 K
Other designations
ADS 16795, CCDM J23300+5833, WDS J23300+5833
AR Cassiopeiae (AB): 1H. Cas[11], AR Cas, BD+57°2748, HD 221253, HIP 115990, HR 8926, SAO 35478[8]
HD 221237 (CD): BD+57°2747, HD 221237, SAO 35476
FG: UCAC4 743-089692
Database references
SIMBADAR Cas (AB)
CD
D
F
G

AR Cassiopeiae (AR Cas) is a variable star in the constellation of Cassiopeia. It is thought to be a member of a septuple star system, one of only two known star systems with a multiplicity of 7, the other being Nu Scorpii.[12][9]

  1. ^ Cite error: The named reference MAST was invoked but never defined (see the help page).
  2. ^ WikiSky, "HD 221253" (accessed 2010-10-27)
  3. ^ a b c d e van Leeuwen, F.; et al. (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.
  4. ^ a b c d e f g h Holmgren, D. E.; Hadrava, P.; Harmanec, P.; Eenens, P.; Corral, L. J.; Yang, S.; Ak, H.; Bozić, H. (1999). "Search for forced oscillations in binaries. III. Improved elements and the detection of line-profile variability of the B4V + A6V: system AR Cassiopeiae". Astronomy and Astrophysics. 345: 855. Bibcode:1999A&A...345..855H.
  5. ^ a b Gaia Collaboration (2016). "Gaia Data Release 1". Astronomy & Astrophysics. 595: A2. arXiv:1609.04172. Bibcode:2016A&A...595A...2G. doi:10.1051/0004-6361/201629512. S2CID 1828208.
  6. ^ a b "HD 221237". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 23 August 2017.
  7. ^ a b c d Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.
  8. ^ a b "V* AR Cas". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 23 August 2017.
  9. ^ a b Cite error: The named reference MSC was invoked but never defined (see the help page).
  10. ^ Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Washington. Bibcode:1953GCRV..C......0W.
  11. ^ Cite error: The named reference Somerville was invoked but never defined (see the help page).
  12. ^ Cite error: The named reference Eggleton was invoked but never defined (see the help page).

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AR Cassiopeiae

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1H

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system, the system can be considered a sextuple. Jabbah AR Cassiopeiae V871 Centauri Gamma Cassiopeiae QZ Carinae Exoplanet Solar System The term optical multiple...

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Eta Cassiopeiae

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common error in sextant readings was made. Alternatively, the star AR Cassiopeiae may have been observed, again with the position recorded incorrectly...

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Alpha Lacertae

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π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae...

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9 Cassiopeiae

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Tau Cassiopeiae

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consisting of τ Cassiopeiae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, AR Cassiopeiae, 9 Lacertae...

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Nu Scorpii

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star system. It is one of only two such known systems, the other being AR Cassiopeiae. Higher-multiplicity star systems are uncommon because they are less...

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Beta Lacertae

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SN 1572

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SN 1572 (Tycho's Supernova, Tycho's Nova), or B Cassiopeiae (B Cas), was a supernova of Type Ia in the constellation Cassiopeia, one of eight supernovae...

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Gamma Cassiopeiae variable

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A Gamma Cassiopeiae variable (γ Cassiopeiae variable) is a type of variable star, named for its prototype γ Cassiopeiae. γ Cassiopeiae variables show irregular...

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Omicron Cassiopeiae

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S Cassiopeiae

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Kappa Andromedae

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Sigma Cassiopeiae

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consisting of σ Cassiopeiae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae...

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Epsilon Cassiopeiae

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Nu Cassiopeiae

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Mu Cassiopeiae

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Kappa Cassiopeiae

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Phi Cassiopeiae

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AO Cassiopeiae

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