stellar parallax of 61 Cygni

E579590

The stellar parallax of 61 Cygni is the first successfully measured trigonometric parallax of a star, providing direct evidence of stellar distances beyond the Solar System.

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Predicate Object
instanceOf astronomical measurement
trigonometric stellar parallax
angularUnit arcsecond
appliesTo 61 Cygni A NERFINISHED
61 Cygni B NERFINISHED
category stellar distance indicator
demonstrated applicability of geometric methods to stellar distances
finite distance to the stars
dependsOn Earth’s orbital motion around the Sun
distanceInLightYears about 11.4 light-years
distanceInParsecs about 3.5 parsecs
evidenceFor large scale of the Milky Way
historicalContext 19th-century astrometry
early empirical confirmation of stellar distances
influenced development of precise positional astronomy
subsequent stellar parallax programs
locatedInConstellation Cygnus NERFINISHED
measuredBy Friedrich Wilhelm Bessel NERFINISHED
measurementType annual parallax
measurementYear 1838
methodUsed trigonometric parallax method
objectOfStudy 61 Cygni NERFINISHED
observedFrom Earth NERFINISHED
observedWith Fraunhofer heliometer at Königsberg Observatory NERFINISHED
parallaxValue about 0.3136 arcseconds
about 0.314 arcseconds
partOf history of astrometry
history of astronomy
providesEvidenceFor existence of large distances between stars and the Solar System
heliocentric model of the Solar System
publicationYear 1838
publishedBy Friedrich Wilhelm Bessel NERFINISHED
relatedTo stellar parallax of Alpha Centauri
stellar parallax of Vega
significance first direct geometric distance determination to a star other than the Sun
first successfully measured trigonometric parallax of a star
usedAsExampleIn astronomy education
textbooks on stellar distances
usedIn calibration of the cosmic distance ladder
usedToDetermine distance to 61 Cygni

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Friedrich Bessel hasDiscovered stellar parallax of 61 Cygni