61 Cygni A

61 Cygni A

Star

61 Cygni A — the brighter of a wide pair of orange dwarfs (K5V) 11.4 light-years away in Cygnus. About 70% of the Sun's mass, it is a chromospherically active star. The pair is historic: in 1838 it became the first star to have its distance measured by parallax.

Open in 3D viewSee 61 Cygni A in the live, interactive 3D map

Key facts

Mutual orbit
678 Earth years
247,640 Earth days
Mass
1.39 × 10³⁰ kg
0.7 M☉
Radius
462,640 km
66% of the Sun's radius
Surface temperature
4,374 K (4,101 °C)
Luminosity
5.86 × 10²⁵ W
Spectral type
K5V (orange dwarf)

Science

Physical

Mass
1.39 × 10³⁰ kg · 0.7 M☉
Radius
462,640 km · 66% of the Sun's radius
Density
3,357 kg/m³ · 3.4× water
Computed from mass and radius
Spectral type
K5V (orange dwarf)

Motion through space

Note
The motion of the pair's common centre of mass, computed as the mass-weighted mean of its stars' catalogued motions.
Proper motion
5.23 arcseconds per year · its drift across our sky
SIMBAD — 2020yCat.1350....0G
Radial velocity
-65.1 km/s · approaching the Sun
SIMBAD — 2020yCat.1350....0G
Speed across our line of sight
86.7 km/s
Computed from proper motion and parallax
Speed through space, relative to the Sun
108 km/s
Computed from proper motion, parallax and radial velocity

Orbit (around the system barycenter)

Semi-major axis
40.3 AU
From the visual-binary orbit (P ≈ 678 yr, a ≈ 85 AU, e ≈ 0.48)
Eccentricity
0.48
From the visual-binary orbit (P ≈ 678 yr, a ≈ 85 AU, e ≈ 0.48)
Orbital period
678.00 years
From the visual-binary orbit (P ≈ 678 yr, a ≈ 85 AU, e ≈ 0.48)

Rotation

Note
Rotates about once every 35 days.

Composition

By mass
An orange main-sequence star about 70% of the Sun's mass and a sixth of its luminosity. It is chromospherically active, with starspots and a magnetic cycle (a BY Draconis-type variable).

Temperature

Surface
4,374 K (4,101 °C)

Radiation & temperature

Luminosity
5.86 × 10²⁵ W · 0.153 L☉
Surface temperature
4,374 K (4,101 °C)
Peak wavelength
662 nm · red light
Computed (Wien's law) from the surface temperature

Discovery & history

Method
Naked-eye star
Name
'61 Cygni' is a Flamsteed number in Cygnus, the Swan. The pair is nicknamed 'Bessel's Star' and the 'Flying Star' for its role in history and its motion.

Noted by Giuseppe Piazzi in 1804 for its large proper motion — the 'Flying Star'. In 1838 Friedrich Bessel used that motion to select 61 Cygni for a parallax measurement, and succeeded: the FIRST reliable distance to any star beyond the Sun, opening the true scale of the cosmos.

Images

Images from open archives · credit shown per image