Iota1 Cygni

Binary star system in the constellation Cygnus From Wikipedia, the free encyclopedia

Iota1 Cygni is a probable binary star[7] system in the northern constellation Cygnus. Its name is a Bayer designation that is Latinized from ι1 Cygni, and abbreviated Iota1 Cyg or ι1 Cyg. It is separated by less than a degree from its brighter visual neighbor, Iota2 Cygni.[10] It is near the lower limit of visibility to the naked eye with an apparent visual magnitude of 5.75.[9] The system is located approximately 387 light years away based on parallax,[2] and it is drifting further away with a radial velocity of +2 km/s.[5]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
Iota1 Cygni
Location of ι1 Cygni (circled in red)
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus[1]
Right ascension 19h 27m 25.96022s[2]
Declination +52° 19 13.5871[2]
Apparent magnitude (V) 5.73[1]
Characteristics
Evolutionary stage main sequence[3]
Spectral type A1V[4]
B−V color index −0.002±0.002[1]
Astrometry
Radial velocity (Rv)+1.90[5] km/s
Proper motion (μ) RA: −12.639[2] mas/yr
Dec.: −27.567[2] mas/yr
Parallax (π)8.4332±0.0867 mas[2]
Distance387 ± 4 ly
(119 ± 1 pc)
Absolute magnitude (MV)+0.57[1]
Details
Mass2.59±0.03[3] M
Radius3.0[6] R
Luminosity74.1+11.0
−20.5
[7] L
Surface gravity (log g)4.18[7] cgs
Temperature9,683+89
−178
[3] K
Metallicity [Fe/H]0.00[8] dex
Rotational velocity (v sin i)51.6±2.2[7] km/s
Age386[8] Myr
Other designations
ι1 Cyg, 7 Cygni, BD+52°2434, HD 183534, HIP 95656, HR 7408, SAO 31673[9]
Database references
SIMBADdata
Close

This is a candidate double-lined spectroscopic binary system.[7] It has a stellar classification of A1V,[4] suggesting the primary component is an A-type main-sequence star. The star is about 400 million years old[8] with a moderate rotation rate, showing a projected rotational velocity of 52 km/s.[7] It has 2.6 times the mass of the Sun[3] and is radiating 74 times the Sun's luminosity[7] from its photosphere at an effective temperature of 9,683 K.[3]

References

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