KIC 9832227

KIC 9832227

KIC 9832227 (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 19h 29m 15.950s[1]
Declination +46° 37′ 19.86″[1]
Apparent magnitude (V) 12.27 – 12.46[2]
Characteristics
Spectral type K2III/IV[3]
Variable type Eclipsing[4]
Astrometry
Proper motion (μ) RA: −9.505[1] mas/yr
Dec.: −5.718[1] mas/yr
Parallax (π)1.5798 ± 0.0134 mas[1]
Distance2,060 ± 20 ly
(633 ± 5 pc)
Orbit[5]
Period (P)0.4282579 days
Semi-major axis (a)2.992 R
Inclination (i)53.2°
Periastron epoch (T)2455688.49913
Details[5]
A
Mass1.395 M
Radius1.581 R
Luminosity2.609 L
Surface gravity (log g)4.19 cgs
Temperature5800 K
Rotational velocity (v sin i)149.7 km/s
B
Mass0.318 M
Radius0.830 R
Luminosity0.789 L
Surface gravity (log g)4.10 cgs
Temperature5920 K
Rotational velocity (v sin i)84.7 km/s
Other designations
2MASS J19291594+4637198, KIC 9832227, ASAS J192916+4637.3, GSC 03543-01211
Database references
SIMBADdata
KICdata

KIC 9832227 is a contact binary star system in the constellation Cygnus, located about 2,060 light-years away. It is also identified as an eclipsing binary with an orbital period of almost 11 hours.[4]

  1. ^ a b c d e Cite error: The named reference dr3 was invoked but never defined (see the help page).
  2. ^ Cite error: The named reference AAVSO was invoked but never defined (see the help page).
  3. ^ Cite error: The named reference frasca2016 was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference Kinemuchi, Karen was invoked but never defined (see the help page).
  5. ^ a b Molnar, Lawrence A.; Van Noord, Daniel M.; Steenwyk, Steven D.; Spedden, Chris J.; Kinemuchi, Karen (2015). "A prediction of a luminous red nova eruption" (PDF). American Astronomical Society. 225 (225): 415.05. Bibcode:2015AAS...22541505M. Archived from the original (PDF) on 7 January 2017.