ABSOLUTE VISUAL MAGNITUDE
* IAU-adopted absolute V magnitude (H)
|SLOPE PARAMETER * IAU-adopted slope parameter (G)||SLOPE PARAMETER ORIGIN FLAG * Those slope parameters that were determined by fitting the IAU-adopted phase function to data are given an origin code letter of 'f' (for 'fitted'); all others are given a code letter of 'a' (for 'assumed').||MPC REFERENCE * Minor Planet Circular (MPC) or Minor Planet Orbit Supplement (MPO) reference|
|ZAPPALA FAMILY NAME * Familiy name in the family analysis of Zappala et al. (1995)||ZAPPALA CLUMP FLAG * Indicates whether the Zappala family designation is a clump or a family, as defined in Zappala et al. (1995). F = family, C = clump.||ZAPPALA FAMILY CONFIDENCE LEVEL * Confidence level of Zappala family membership, defined as quality code (QC) in Zappala et al. 1995.|
|DISCOVERY DATE * Date of discovery of an object||DISCOVERY LOCATION * Location where the discovery observation of an object was made||DISCOVERER NAMES * The name(s) of the discoverer(s) of an object|
|1984-02-23||La Silla||Debehogne, H.|
|MK RESONANCE FLAG * Resonance flag as defined in Milani and Knesevic 1994, Icarus 107, 219.||MK MEAN ELEMENTS QUALITY CODE * Mean elements quality code as defined in Milani and Knesevic 1994, Icarus 107, 219.||MK OSCULATING ELEMENTS QUALITY CODE * Osculating elements quality code as defined in Milani and Knesevic 1994, Icarus 107, 219.||MOTHEFAM CLUSTER MEMBERSHIP * The cluster membership as defined in the Mothe-Diniz et al. asteroid family data set, based on the name or provisional designation of the lowest-numbered asteroid in the cluster|
* NEOWISE best-fit effective spherical diameter, or assumed value if not fitted.
NEOWISE DIAMETER UNCERTAINTY
* NEOWISE unceratinty in the best-fit effective spherical diameter, or assumed value if not fitted.
|NEOWISE V ALBEDO * NEOWISE best-fit visible geometric albedo, or assumed value if not fitted.||NEOWISE V ALBEDO UNCERTAINTY * NEOWISE uncertainty of the best-fit visible geometric albedo, or assumed value if not fitted.||NEOWISE THERMAL BEAMING PARAMETER * NEOWISE best-fit NEATM thermal beaming parameter, or assumed value if not fitted.||NEOWISE THERMAL BEAMING PARAMETER UNCERTAINTY * NEOWISE uncertainty of the best-fit NEATM thermal beaming parameter, or assumed value if not fitted.||NEOWISE REFERENCE CODE * NEOWISE reference code to the original publication of fitted parameters. See the refrence.tab in the dataset for the full reference|
|NESVORNY SYNTHETIC FAMILY NUMBER * Family number assigned for the purpose of the Nesvorny family analysis based on synthetic proper elements. Family numbers in the 400's refer to inner belt families, in the 500's to central belt families, and in the 600's to outer belt families. High inclination families from synthetic proper elements have family numbers in the 700's for the inner belt, the 800's for the central belt, and the 900's for the outer belt.||NESVORNY SYNTHETIC FAMILY NAME * The name of the asteroid family in the Nesvorny family analysis based on synthetic proper elements. The family name is based on the name or provisional designation of the largest member of the family.|