Minor Planet Center - Asteroid Orbital Datampc.mpcorbivo://org.gavo.dc/mpc/q/mpcorbThe GAVO DC teamWilliams, G.Keys, S.Rudenko, M.Galache, J.L.2024-03-25T15:44:04ZGAVO Data Center TeamMönchhofstrasse 12-14, D-69120 Heidelberggavo@ari.uni-heidelberg.de++49 6221 54 1837asteroidssurveys
Complete Asteroid Data from the Minor Planet Center (MPC),
updated once per month. The MPC operates at the Smithsonian Astrophysical
Observatory under the auspices of Division III of the International
Astronomical Union (IAU).
The MPC Orbit database contains orbital elements of minor
planets that have been published in the Minor Planet Circulars,
the Minor Planet Orbit Supplement and the Minor Planet
Electronic Circulars.http://dc.zah.uni-heidelberg.de/tableinfo/mpc.mpcorbCatalogMPC catalogue distributed by ARI/Zentrum für Astronomie Heidelberg.mpcMinor Planet Center - Asteroid Orbital Data
Complete Asteroid Data from the Minor Planet Center (MPC),
updated once per month. The MPC operates at the Smithsonian Astrophysical
Observatory under the auspices of Division III of the International
Astronomical Union (IAU).
The MPC Orbit database contains orbital elements of minor
planets that have been published in the Minor Planet Circulars,
the Minor Planet Orbit Supplement and the Minor Planet
Electronic Circulars.
mpc.mpcorb
Complete Asteroid Data from the Minor Planet Center (MPC),
updated once per month. The MPC operates at the Smithsonian Astrophysical
Observatory under the auspices of Division III of the International
Astronomical Union (IAU).
The MPC Orbit database contains orbital elements of minor
planets that have been published in the Minor Planet Circulars,
the Minor Planet Orbit Supplement and the Minor Planet
Electronic Circulars.1200000designationAsteroid number or provisional designation.meta.id;meta.maincharnullablemagAbsolute Magnitude of the asteroid, i.e., the magnitude of the asteroid at a distance of 1 AU when viewed at a phase angle of 0°.magphys.magAbsfloatindexednullableslopeSlope Parameter G. It describes how the magnitude of the asteroid varies as a function of changing illumination (phase angle)src.morph.paramfloatnullableorb_epochEpoch of the orbit (julian years)atime.epochdoublenullablemean_anomalyMean anomaly at the epochdegsrc.orbital.meanAnomalyfloatnullablearg_perihelArgument of Perihelion, J2000.0degsrc.orbital.periastronfloatnullablelong_ascLongitude of ascending node, J2000.0degsrc.orbital.nodefloatnullableinclinationInclination of the orbit to the ecliptic, J2000.0degsrc.orbital.inclinationfloatnullableeccentricityEccentricity of the orbitsrc.orbital.eccentricityfloatnullablemean_motionMean Daily Motiondeg/dpos.pm;arith.diff;phys.velocfloatnullablesemimaj_axOrbital semimajor axisAUphys.size.smajAxisfloatindexednullableuncertainty_parameterQuality code (0 is best) as per http://www.minorplanetcenter.org/iau/info/UValue.html. Or: E -- the orbital eccentricity was assumed; D -- for one-opposition orbits this means a double (or multiple) designation is involved; F -- an e-assumed double (or multiple) designation is involved.meta.code.errorcharnullablebib_referenceOrigin of the datameta.bibcharnullablen_obsNumber of Observationsmeta.number;obsintnullablen_oppNumber of Oppositionsmeta.numberintarc_lengthLength of observed arcs for single-opposition orbits.dtime.intervalshortnullablefirst_obsDiscovery year for multi-opposition orbits.atime.epochshortnullablerms_fitRMS Residual of orbital fitarcsecstat.fit.residualfloatnullableperturbersInformation on orbit perturbers; see table note.meta.notecharnullablecomputerIdentifies the computer of the orbitmeta.notecharnullableorbit_classOrbit family this object belongs to (note that the classification is based on cuts in osculating element space and is not 100% reliable.src.classcharnullableorbit_flagsAdditional classification flag(s) as comma-separated human-readable phrasessrc.classcharnullablenameHuman-readable designation of the Asteroid.meta.idunicodeCharindexednullablelast_obsDate of last observationatime.epoch;obsfloatnullable