61 Cygni

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61 Cygni A/B
Observation data
Epoch J2000
Constellation Cygnus
Right ascension 21h 06m 54.0/55.3s
Declination +38° 44' 57"/31"
Apparent magnitude (V) 5.20/6.05
Characteristics
Spectral type K5 V/K7 V
B-V color index 1.17/1.36
U-B color index 1.11/1.23
Variable type Suspected
Astrometry
Radial velocity (Rv) -65.0/-64.1 km/s
Proper motion (μ) RA: 4.155/4.107"/yr
Dec.: 3.259/3.144"/yr
Parallax (π) 0.28604" ± 0.00056"
Distance 11.40 ly (3.496 pc)
Absolute magnitude (MV) 7.48/8.33
Details
Mass 0.70/0.63 M
Radius 0.72/0.67 R
Luminosity 0.085/0.039 L
Temperature 4,450/4,120 K
Metallicity 79/79% Sun
Rotation period
Age >4.6 × 109 years
Visual binary orbit
Companion 61 Cygni B
Period (P) 653.2 years
Semimajor axis (a) 24.4"
Eccentricity (e) 0.40
Inclination (i) 51.85°
Node (Ω) 172.3°
Periastron epoch (T) 1689.7
Other designations
61 Cyg A/B, HD 201091/201092 HR 8085/8086 BD +38°4343/4344 GCTP 5077.00 A/B, GJ 820 A/B, LHS 62/63, Struve 2758 A/B, ADS 14636 A/B, and HIP 104214/104217.

61 Cygni is a star in the constellation Cygnus. Though it is among the least conspicuous of stars visible in the night sky to an observer without an optical instrument, 61 Cygni attracted the attention of astronomers due to its large proper motion. The star is in fact a double star system.

This system should not be confused with 16 Cygni, which includes a Sun-like star with a very eccentric planet.

Contents

General information

61 Cygni's proper motion is so great, relatively speaking, that its apparent position shifts by an amount equal to the width of the full moon in a mere 150 years.

This large proper motion, the largest known for any star at the time, made 61 Cygni a candidate for the determination of its distance by the method of parallax when the quality of astronomical observations first made this possible. The star therefore has the distinction of being the first star (excluding the Sun) to have its distance determined. This was accomplished by Friedrich Wilhelm Bessel in 1838 who arrived at a figure close to the currently accepted value of 11.4 light years.

Only a few years later, however, Groombridge 1830 was discovered to have a larger proper motion. 61 Cygni retains the distinction of having the largest proper motion of any star visible with the naked eye (although Groombridge 1830 at magnitude 6.4 can be seen with the naked eye under exceptionally dark skies).

Subsequent observations showed that, in addition to the closeness of the star, the high proper motion was attributable to its actual velocity relative to the Sun being large and almost transverse to our line of sight to the star.

From the point of the view of the casual astronomical observer, 61 Cygni is not particularly spectacular.

The binary system

Although it appears to be a single star to the naked eye, 61 Cygni is in fact a widely separated binary system, composed of two K class (orange) main sequence stars, 61 Cygni A and 61 Cygni B. The brighter star 61 Cygni A is of apparent magnitude 5.2, the fainter 61 Cygni B is 6.1. The two orbit their common barycenter in a period of 653.2 years.

An observer using 7×50 binoculars can find 61 Cygni two binocular fields south-east of the bright star Deneb. An observer using larger binoculars, or a telescope, will be able to resolve the two components of the binary.

61 Cygni B's planet

61 Cygni B has been claimed to have a planet or brown dwarf companion, but the claim has not been confirmed.

61 Cygni in Fiction

See also

External links



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