M67

E584561

M67 is an ancient, metal-rich open star cluster in the constellation Cancer, notable for its well-studied stellar population and importance in understanding stellar evolution.

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Observed surface forms (1)

Surface form Occurrences
M 67 1

Statements (46)

Predicate Object
instanceOf open star cluster
addedToMessierCatalogue 1780
age about 4 billion years
comparable to the Sun
angularSize about 30 arcminutes
apparentMagnitudeV about 6.1
bestSeenIn spring in the Northern Hemisphere
catalogNumber M67
Messier 67 NERFINISHED
NGC 2682 NERFINISHED
constellation Cancer NERFINISHED
contains blue straggler stars
red giant stars
solar analogs
white dwarfs
coreRadius about 1 parsec
declination +11° 49′
discoveredBy Johann Gottfried Koehler NERFINISHED
discoveryYear 1779
distanceFromEarth about 2700–3000 light-years
about 800–900 parsecs
estimatedMass about 1000 solar masses
estimatedNumberOfStars about 500
several hundred
galacticLatitude +32°
galacticLongitude about 215°
galacticPopulation Galactic disk
has near-solar metallicity
hasHigh binary star fraction
locatedIn Milky Way
metallicity metal-rich
metallicityRelativeToSun approximately solar or slightly above
notableFor importance in understanding stellar evolution
rich population of solar-type stars
well-studied stellar population
observedBy Charles Messier NERFINISHED
rightAscension 08h 51m
tidalRadius about 10 parsecs
usedAs benchmark open cluster for stellar evolution models
reference for gyrochronology studies
reference for stellar isochrone calibration
usedToStudy mass loss in stars
stellar activity
stellar rotation
white dwarf cooling sequences
visibility visible with binoculars under dark skies

Referenced by (2)

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

Messier 67 catalogCode M67
Messier 67 hasAlternativeName M67
this entity surface form: M 67