Ptolemaic magnitude scale

E1022097

The Ptolemaic magnitude scale is an ancient astronomical system, originating with Claudius Ptolemy, that ranks stars by their apparent brightness in six broad classes from first (brightest) to sixth (faintest) magnitude.

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Statements (47)

Predicate Object
instanceOf astronomical brightness scale
historical astronomical system
stellar magnitude scale
appliesTo fixed stars
approximateDate circa 150 CE
assumes stars grouped into discrete brightness classes
assumesObserver average human eye under dark skies
brightestClass first magnitude
catalogueAssociated Ptolemy star catalogue NERFINISHED
classificationBasis naked-eye visual impression
classificationType visual brightness class
classRangeLowerBound 1
classRangeUpperBound 6
comparedToModernScale qualitative rather than quantitative
dataType ordinal scale
developedBy Claudius Ptolemy NERFINISHED
documentationLanguage Ancient Greek
era 2nd century
faintestClass sixth magnitude
field astrometry
astronomy
hasMagnitudeClass fifth magnitude GENERATED
first magnitude GENERATED
fourth magnitude GENERATED
second magnitude GENERATED
sixth magnitude GENERATED
third magnitude GENERATED
historicalStatus superseded
influenced Pogson magnitude scale NERFINISHED
modern logarithmic magnitude scale
limitingMagnitude approximately sixth magnitude
measures apparent brightness of stars
apparent magnitude
namedAfter Claudius Ptolemy NERFINISHED
numberOfClasses 6
observationMethod unaided eye
orderingPrinciple smaller magnitude number indicates brighter star
originatedIn ancient Greece
precision coarse
relatedConcept apparent magnitude
naked-eye limiting magnitude
visual magnitude
replacedBy Pogson magnitude scale
logarithmic stellar magnitude system
usedFor cataloguing stars
ranking stellar brightness
usedInWork Almagest NERFINISHED

Referenced by (1)

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

Al-Sufi's Book of Fixed Stars uses Ptolemaic magnitude scale