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Asteroid 2010 Chebyshev

Alternate IDs:
1948 YA, 1969 TL4, 1958 TF1, 1931 VA

Data sets with data for Asteroid 2010 Chebyshev:

Asteroid 2010 Chebyshev (top)

2MASS Asteroid and Comet Survey V2.0 (1 data product)

J MAGNITUDE 2MASS * J band selected magnitude in the 2MASS survey, or if the source is not detected in the J-band, the 95% confidence upper limit derived from a 4 arcsec radius aperture measurement taken at the position of the source on the Atlas Image. (The Atlas Images are quick-look images suitable for deriving positional information but not accurate photometry.) The origin of the magnitude is given by the first character of the rd_flg value.
(MAGNITUDE) 		J MAGNITUDE 2MASS UNC * Corrected photometric uncertainty for the J-band magnitude in the 2MASS survey. If rd_flg[1]=2, this is the measurement error from the profile-fitting procedure, corrected to be consistent with observed repeatability statistics. If rd_flg[1]=1 or 4, this is the RMS of the brightness measured in aperture photometry on the individual frames. If rd_flg=3, the uncertainty is derived from the residuals to the 1-d radial profile fit (averaging over azimuth) to the unsaturated wings of the bright source. If J_MAG_SIG > 8.0, it is a flag value indicating that a meaningful uncertainty could not be determined for the source. This column is null if the magnitude is a 95% confidence upper limit (rd_flg[1]=0 or 6) or if the source is not measurable (rd_flg[1]=9).
(MAGNITUDE) 		H MAGNITUDE 2MASS * H band selected magnitude in the 2MASS survey, or if the source is not detected in the H-band, the 95% confidence upper limit derived from a 4 arcsec radius aperture measurement taken at the position of the source on the Atlas Image. (The Atlas Images are quick-look images suitable for deriving positional information but not accurate photometry.) The origin of the magnitude is given by the second character of the rd_flg value.
(MAGNITUDE) 		H MAGNITUDE 2MASS UNC * Corrected photometric uncertainty for the H-band magnitude in the 2MASS survey. If rd_flg[2]=2, this is the measurement error from the profile-fitting procedure, corrected to be consistent with observed repeatability statistics. If rd_flg[2]=1 or 4, this is the RMS of the brightness measured in aperture photometry on the individual frames. If rd_flg=3, the uncertainty is derived from the residuals to the 1-d radial profile fit (averaging over azimuth) to the unsaturated wings of the bright source. If H_MAG_SIG > 8.0, it is a flag value indicating that a meaningful uncertainty could not be determined for the source. This column is null if the magnitude is a 95% confidence upper limit (rd_flg[2]=0 or 6) or if the source is not measurable (rd_flg[2]=9).
(MAGNITUDE) 		KS MAGNITUDE 2MASS * Ks band selected magnitude in the 2MASS survey, or if the source is not detected in the Ks-band, the 95% confidence upper limit derived from a 4 arcsec radius aperture measurement taken at the position of the source on the Atlas Image. (The Atlas Images are quick-look images suitable for deriving positional information but not accurate photometry.) The origin of the magnitude is given by the third character of the rd_flg value.
(MAGNITUDE) 		KS MAGNITUDE 2MASS UNC * Corrected photometric uncertainty for the Ks-band magnitude in the 2MASS survey. If rd_flg[3]=2, this is the measurement error from the profile-fitting procedure, corrected to be consistent with observed repeatability statistics. If rd_flg[3]=1 or 4, this is the RMS of the brightness measured in aperture photometry on the individual frames. If rd_flg=3, the uncertainty is derived from the residuals to the 1-d radial profile fit (averaging over azimuth) to the unsaturated wings of the bright source. If KS_MAG_SIG > 8.0, it is a flag value indicating that a meaningful uncertainty could not be determined for the source. This column is null if the magnitude is a 95% confidence upper limit (rd_flg[3]=0 or 6) or if the source is not measurable (rd_flg[3]=9).
(MAGNITUDE)
14.471 0.024 14.086 0.030 14.005 0.044
16.464 0.106 15.967 0.174 15.174

Asteroid 2010 Chebyshev (top)

Asteroid Absolute Magnitudes V12.0 (1 data product)

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
11.62 0.15 a MPC 17264

Asteroid 2010 Chebyshev (top)

Asteroid Dynamical Families V4.1 (2 data products)

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.
Themis F 3

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
60 Themis

Asteroid 2010 Chebyshev (top)

Asteroid Names and Discovery V12.0 (1 data product)

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
1969-10-13 Nauchnyj Burnasheva, B.

Asteroid 2010 Chebyshev (top)

Asteroid Taxonomy V6.0 (1 data product)

THOLEN CLASS * Taxonomic classification according to the method of Tholen (1984, 1989). An entry with the value of '***' indicates an object with unusual colors not classifiable into any of the defined classes. BARUCCI CLASS * Taxonomic classification according to the method of Barucci et al. (1987). TEDESCO CLASS * Taxonomic classification according to the method of Tedesco et al. (1989). HOWELL CLASS * Taxonomic classification according to the method of Howell (1994). SMASS CLASS * Taxonomic classification based on the spectra of the SMASS survey (Xu et al. 1995). BUS CLASS * Taxonomic classification based on the spectra of the SMASSII survey (Bus and Binzel 2002). An entry with a value of '***' indicates the object has an unusual spectrum not classifiable into any of the defined classes. S3OS2 CLASS TH * Taxonomic classification based on the spectra of the S3OS2 survey and using the method of Tholen (1984). For details of how the method was applied, see [LAZZAROETAL2004] (Icarus 172, 179-220.) S3OS2 CLASS BB * Taxonomic classification based on the spectra of the S3OS2 survey and using the method of Bus and Binzel (2002). For details of how the method was applied, see [LAZZAROETAL2004] (Icarus 172, 179-220.) BUS DEMEO CLASS * Taxonomic classification from DeMeo et al. (2009). Note that a 'w' following the taxonomic class indicates a slope greater than 0.25, and a ':' indicates a questionable classification because of low quality/questionable data.
BU:

Asteroid 2010 Chebyshev (top)

Eight Color Asteroid Survey V4.0 (2 data products)

ECAS S V * Eight Color Asteroid Survey s-v color
(MAGNITUDE) 		ECAS S V UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey s-v color
(MILLIMAGNITUDE) 		ECAS U V * Eight Color Asteroid Survey u-v color
(MAGNITUDE) 		ECAS U V UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey u-v color
(MILLIMAGNITUDE) 		ECAS B V * Eight Color Asteroid Survey b-v color
(MAGNITUDE) 		ECAS B V UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey b-v color
(MILLIMAGNITUDE) 		ECAS V MAGNITUDE * v magnitude from the Eight Color Asteroid Survey
(MAGNITUDE) 		ECAS V MAG UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey v magnitude
(MILLIMAGNITUDE) 		ECAS V W * Eight Color Asteroid Survey v-w color
(MAGNITUDE) 		ECAS V W UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey v - w color
(MILLIMAGNITUDE) 		ECAS V X * Eight Color Asteroid Survey v-x color
(MAGNITUDE) 		ECAS V X UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey v - x color
(MILLIMAGNITUDE) 		ECAS V P * Eight Color Asteroid Survey v-p color
(MAGNITUDE) 		ECAS V P UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey v - p color
(MILLIMAGNITUDE) 		ECAS V Z * Eight Color Asteroid Survey v-z color
(MAGNITUDE) 		ECAS V Z UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey v - z color
(MILLIMAGNITUDE)
0.133 62 0.159 45 0.032 41 15.584 36 -0.004 46 -0.111 72 -0.172 67 -0.379 101

ECAS MEAN S V * Mean s-v color in the Eight Color Asteroid Survey
(MAGNITUDE) 		ECAS S V UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey s-v color
(MILLIMAGNITUDE) 		ECAS MEAN U V * Mean u-v color in the Eight Color Asteroid Survey
(MAGNITUDE) 		ECAS U V UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey u-v color
(MILLIMAGNITUDE) 		ECAS MEAN B V * Mean b-v color in the Eight Color Asteroid Survey
(MAGNITUDE) 		ECAS B V UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey b-v color
(MILLIMAGNITUDE) 		ECAS MEAN V W * Mean v-w color in the Eight Color Asteroid Survey
(MAGNITUDE) 		ECAS V W UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey v - w color
(MILLIMAGNITUDE) 		ECAS MEAN V X * Mean v-x color in the Eight Color Asteroid Survey
(MAGNITUDE) 		ECAS V X UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey v - x color
(MILLIMAGNITUDE) 		ECAS V P * Eight Color Asteroid Survey v-p color
(MAGNITUDE) 		ECAS V P UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey v - p color
(MILLIMAGNITUDE) 		ECAS V Z * Eight Color Asteroid Survey v-z color
(MAGNITUDE) 		ECAS V Z UNC * Uncertainty (standard deviation) in Eight Color Asteroid Survey v - z color
(MILLIMAGNITUDE)
0.133 62 0.159 45 0.032 41 -0.004 46 -0.111 72 -0.172 67 -0.379 101

Asteroid 2010 Chebyshev (top)

NEOWISE Diameters and Albedos V1.0 (1 data product)

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
24.649 0.194 0.065 0.012 1.035 0.015 Mas11

Asteroid 2010 Chebyshev (top)

NEOWISE Diameters and Albedos V2.0 (1 data product)

ABSOLUTE VISUAL MAGNITUDE * IAU-adopted absolute V magnitude (H)
(magnitudes) 		SLOPE PARAMETER * IAU-adopted slope parameter (G) OBSERVATION DATE * Date of observation
(day) 		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
11.62 +0.15 2455372.9545645 24.649 0.194 0.065 0.012 1.035 0.015 Mas11

Asteroid 2010 Chebyshev (top)

Near-Infrared Photometry of Asteroids From DENIS V1.0 (1 data product)

OBSERVATION DATE * Date of observation
(DAY) 		DENIS I MAGNITUDE * I magnitude in the DENIS (Deep European Near-Infrared southern sky) survey.
(MAGNITUDE) 		DENIS I MAGNITUDE ERROR * Error in the I magnitude in the DENIS (Deep European Near-Infrared southern sky) survey.
(MAGNITUDE) 		DENIS J MAGNITUDE * J magnitude in the DENIS (Deep European Near-Infrared southern sky) survey.
(MAGNITUDE) 		DENIS J MAGNITUDE ERROR * Error in the J magnitude in the DENIS (Deep European Near-Infrared southern sky) survey.
(MAGNITUDE) 		DENIS KS MAGNITUDE * Ks magnitude in the DENIS (Deep European Near-Infrared southern sky) survey.
(MAGNITUDE) 		DENIS KS MAGNITUDE ERROR * Error in the Ks magnitude in the DENIS (Deep European Near-Infrared southern sky) survey.
(MAGNITUDE)
2451752.498646 16.84 0.11 15.89 0.35 99.99 9.99

Asteroid 2010 Chebyshev (top)

UBV Mean Asteroid Colors (1 data product)

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
.339 .065 1 .705 .040 1


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