Nova Persei 1901

E554035

Nova Persei 1901 is a bright classical nova that erupted in 1901 in the constellation Perseus and became one of the most intensely studied novae in astronomical history.

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Statements (48)

Predicate Object
instanceOf astronomical object
cataclysmic variable star
classical nova
alsoKnownAs GK Per NERFINISHED
GK Persei NERFINISHED
apparentMagnitudeAtMaximum 0.0
0.2
binarySystem true
catalogue General Catalogue of Variable Stars NERFINISHED
declination_J2000 +43° 54′ 16″
discoveredBy Thomas David Anderson NERFINISHED
discoveryDate 1901-02-21
distanceFromEarth_approx 1500 light-years
470 parsecs
eruptionYear 1901
eventType nova eruption
galacticLatitude_approx -10 degrees
galacticLongitude_approx 150 degrees
galacticPopulation Milky Way NERFINISHED
GCVSName GK Per NERFINISHED
hasCompanionType K-type subgiant
white dwarf
hasNovaRemnant true
hostGalaxy Milky Way NERFINISHED
lightCurveFeature rapid rise to maximum
subsequent irregular variations
lightEchoDiscoveryYear 1901
lightEchoSignificance first light echo observed from a nova
locatedInConstellation Perseus NERFINISHED
magneticWhiteDwarf true
notableFor early observation of expanding light echo from circumstellar dust
novaRemnantExpansion measurable proper motion of knots
novaRemnantMorphology asymmetric shell
novaShellDetected true
orbitalPeriod 1.9968 days
outburstType fast nova
peakBrightnessRank one of the brightest novae of the 20th century
radioSource true
remnantObservedIn X-ray wavelengths
optical wavelengths
radio wavelengths
rightAscension_J2000 03h 31m 12s
scientificImportance one of the most intensely studied novae in history
prototype for studies of nova remnants
showsLightEcho true
spectralType K1IV
variableStarDesignation GK Per NERFINISHED
xRaySource true

Referenced by (1)

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

Perseus constellation contains Nova Persei 1901