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 |
---|---|---|---|
13.60 | 0.15 | a | MPC 17266 |
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. |
---|---|---|
Polana (nysa) | F | 3 |
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 |
---|---|---|
1978-08-31 | Nauchnyj | Chernykh, N. |
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 FAMILY MEMBERSHIP * The family membership as defined in the Mothe-Diniz et al. asteroid family data set. |
---|---|---|---|
0 | 0 | 0 | Nysa |
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 |
---|---|---|---|---|---|---|
12.014 | 0.068 | 0.037 | 0.005 | 0.947 | 0.011 | Mas11 |
time: 1993-08-23T06:40:26 file: data11/2809_01.tab dataset: Small Main-belt Asteroid Spectroscopic Survey, Phase II
U B COLOR
* Unweighted mean of accepted U-B color values
(MAGNITUDE) |
U B COLOR UNC
* Standard deviation of mean U-B color values
(MAGNITUDE) |
U B OBS COUNT * Number of accepted observations used to compute the mean U-B color |
B V COLOR
* Unweighted mean of accepted B-V color values
(MAGNITUDE) |
B V COLOR UNC
* Standard deviation of mean B-V color values
(MAGNITUDE) |
B V OBS COUNT * Number of accepted observations used to compute the mean B-V color |
---|---|---|---|---|---|
.243 | .054 | 1 | .648 | .030 | 1 |