ABSOLUTE VISUAL MAGNITUDE
* IAU-adopted absolute V magnitude (H)
(MAGNITUDE) |
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 |
---|---|---|---|
12.61 | 0.15 | a | MPC 17264 |
WILLIAMS FAMILY * Family identification according to the Williams analysis | KOZAI FAMILY * Family identification according to the Kozai analysis | CARUSI FAMILY * Family identification according to the Carusi and Massaro analysis | LINDBLAD SOUTHWORTH FAMILY * Family identification according to the Lindblad and Southworth analysis | VAN HOUTEN FAMILY * Family identification according to the van Houten analysis | ARNOLD FAMILY * Family identification according to the Arnold analysis | BROUWER FAMILY * Family identification according to the Brouwer analysis | HIRAYAMA FAMILY * Family identification according to the Hirayama analysis | ZAPPALA FAMILY * Family identification according to the Zappala analysis |
---|---|---|---|---|---|---|---|---|
15 |
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 |
---|---|---|
1973-08-31 | Nauchnyj | Smirnova, T. |
time: 1981-11-25T02:47:20 file: indiv/ast002072/19811125024720_b.tab dataset: Asteroid Photometric Catalog V1.1
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 |
---|---|---|---|
0 | 0 | 0 | Kosmodemyanskaya |
NEOWISE DIAMETER
* NEOWISE best-fit effective spherical diameter, or assumed value if not fitted.
(KILOMETER) |
NEOWISE DIAMETER UNCERTAINTY
* NEOWISE unceratinty in the best-fit effective spherical diameter, or assumed value if not fitted.
(KILOMETER) |
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 |
---|---|---|---|---|---|---|
4.843 | 0.215 | 0.681 | 0.190 | 1.182 | 0.135 | Mas11 |
5.531 | 0.448 | 0.522 | 0.098 | 1.397 | 0.238 | Mas11 |