SN 1604

E481643

SN 1604, also known as Kepler's Supernova, was a historically significant stellar explosion observed in 1604 that became one of the brightest recorded supernovae in the Milky Way.

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Statements (46)

Predicate Object
instanceOf astronomical object
historical supernova
supernova
alsoKnownAs Kepler supernova NERFINISHED
Kepler's Star NERFINISHED
Kepler's Supernova NERFINISHED
approximateAge over 400 years
discoveredBy Johannes Kepler NERFINISHED
distanceFromEarth approximately 20000 light-years
approximately 6 kiloparsecs
documentedIn De Stella Nova in Pede Serpentarii NERFINISHED
epochOfObservation early 17th century
explosionMechanism thermonuclear disruption of white dwarf
firstObservedOn 1604-10-09
galacticLatitude high galactic latitude
historicalSignificance challenged Aristotelian idea of immutable heavens
last supernova in Milky Way observed with naked eye
hostGalaxy Milky Way NERFINISHED
influencedWorkOf Johannes Kepler NERFINISHED
locatedIn Milky Way
constellation Ophiuchus
observedAs new star
observedBy Arabic astronomers
Chinese astronomers
European astronomers
Galileo Galilei NERFINISHED
Johannes Kepler NERFINISHED
Korean astronomers
observedByTelescope Chandra X-ray Observatory NERFINISHED
Hubble Space Telescope NERFINISHED
peakBrightnessApparentMagnitude approximately −2.5
peakBrightnessComparison almost as bright as Venus
brighter than Jupiter
remnantAngularSize about 3 arcminutes
remnantCatalogName G4.5+6.8
remnantDesignation Kepler's Supernova Remnant NERFINISHED
remnantObservedIn X-ray
optical
radio
supernovaType Type Ia supernova
usedFor calibration of supernova models
studies of Type Ia supernova remnants
studies of shock physics in interstellar medium
visibleDuration several months
visibleToNakedEye true
yearOfPeakBrightness 1604

Referenced by (1)

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