HD 186408

E919754

HD 186408 is a Sun-like star in the constellation Cygnus that has been studied as a solar analog and considered a potential host for habitable planets.

All labels observed (1)

Label Occurrences
HD 186408 canonical 1

How this entity was disambiguated

Statements (45)

Predicate Object
instanceOf G-type main-sequence star
solar analog
star
age similar to or slightly older than the Sun
apparentMagnitudeV 5.96
colorIndexBminusV about 0.64
constellation Cygnus
declination +50° 31′
distanceFromEarth about 69 light-years
effectiveTemperature about 5800 K
equatorialCoordinateSystem ICRS
galacticPopulation thin disk star
hasAlternativeName 16 Cygni A
BD+50 2790
HIP 96895
HR 7503
SAO 31898
hasBeenUsedFor comparative studies of solar composition
studies of stellar activity cycles
tests of stellar age-dating methods
hasCatalogEntry Bright Star Catalogue
Henry Draper Catalogue
Hipparcos Catalogue
hasCompanion 16 Cygni B
16 Cygni C
HD 186427
hasKnownPlanet false (as of current observations)
hasProperMotionDec about 385 mas/yr
hasProperMotionRA about 324 mas/yr
hasWideBinarySeparationWith HD 186427
isBrighterComponentOf 16 Cygni A–B pair
isCandidateHostFor habitable planets
isComponentOf 16 Cygni triple star system
isStudiedAs solar analog for stellar evolution
solar twin candidate
isSunLike true
luminosity about 1.2 times solar luminosity
mass about 1.05 solar masses
metallicity[Fe/H] slightly above solar
parallax 47.44 mas
radialVelocity about −28 km/s
radius about 1.1 solar radii
rightAscension about 19h 41m
spectralType G1V
variabilityType not known to be significantly variable

How these facts were elicited

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.

Cosmic Call 1999 targetedStarSystem HD 186408
subject linked to: Cosmic Call