Barycentric Celestial Reference System

E855203

The Barycentric Celestial Reference System is a relativistic, solar-system–centered coordinate framework used in astronomy and astrometry to precisely describe the positions and motions of celestial bodies with respect to the solar system’s center of mass.

Try in SPARQL Jump to: Statements Referenced by

Statements (49)

Predicate Object
instanceOf astronomical coordinate system
celestial reference system
relativistic reference system
abbreviation BCRS NERFINISHED
application analysis of VLBI observations
construction of planetary and lunar ephemerides
appliesToRegion solar system vicinity
basedOnTheory general relativity
coordinateCenter solar system barycenter NERFINISHED
coordinateOrigin center of mass of all solar system bodies
coordinateSymbol (t, x, y, z)
definedBy International Astronomical Union NERFINISHED
definedIn IAU 1991 resolutions NERFINISHED
distinguishedFrom heliocentric reference system
topocentric reference system
documentedIn IAU 2000 Resolution B1.3 NERFINISHED
IAU 2000 Resolution B1.5 NERFINISHED
IAU 2006 Resolution B2 NERFINISHED
epochDefinition kinematically non-rotating with respect to distant extragalactic objects
governingBody IAU Division A NERFINISHED
includesEffects Shapiro time delay GENERATED
aberration of light GENERATED
gravitational time dilation GENERATED
relativistic light deflection GENERATED
mathematicalFramework post-Newtonian approximation of general relativity
neglects external gravitational fields beyond the solar system at leading order
orientation aligned with ICRS axes
precisionGoal microarcsecond astrometry
primaryUse modeling light propagation in the solar system
modeling motion of solar system bodies
referenceFrameType barycentric
referenceToRealization International Celestial Reference System NERFINISHED
referenceToRealizationAbbreviation ICRS NERFINISHED
refinedIn IAU 2000 resolutions NERFINISHED
IAU 2006 resolutions NERFINISHED
relatedSystem Geocentric Celestial Reference System NERFINISHED
relatedSystemAbbreviation GCRS GENERATED
spatialCoordinatesType quasi-Cartesian coordinates
spatialMetric post-Newtonian metric
timeCoordinate Barycentric Coordinate Time NERFINISHED
timeCoordinateAbbreviation TCB NERFINISHED
timeSymbol t = TCB
transformationDefinedWith GCRS NERFINISHED
usedIn astrometry
celestial mechanics
ephemeris computation
high-precision timing
pulsar timing
spacecraft navigation

Referenced by (1)

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

International Celestial Reference System relatedTo Barycentric Celestial Reference System