Asteroid 143 Adria

Alternate IDs:

1960 WK1

Data sets with data for Asteroid 143 Adria:

2MASS Asteroid and Comet Survey V2.0 (1 data product)
Asteroid Absolute Magnitudes V12.0 (1 data product)
Asteroid Dynamical Families V4.1 (2 data products)
Asteroid Lightcurve Derived Data V16.0 (1 data product)
Asteroid Names and Discovery V12.0 (1 data product)
Asteroid Occultations V14.0 (1 data product)
Asteroid Photometric Catalog V1.1 (15 data products)
Asteroid Taxonomy V6.0 (1 data product)
IRAS Minor Planet Survey V6.0 (1 data product)
IRTF Near-IR Spectroscopy of Asteroids V2.0 (1 data product)
MSX Infrared Minor Planet Survey V1.0 (1 data product)
NEOWISE Diameters and Albedos V1.0 (1 data product)
Small Main-belt Asteroid Spectroscopic Survey, Phase II (1 data product)
UBV Mean Asteroid Colors (1 data product)

Asteroid 143 Adria (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)
12.828	0.018	12.429	0.020	12.232	0.020

Asteroid 143 Adria (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
9.12	0.15	a	MPC 17257

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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.

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
	38

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Asteroid Lightcurve Derived Data V16.0 (1 data product)

LC PERIOD * Rotation period of the asteroid about its axis, in hours, in the asteroid lightcurve parameters file. The period given is synodic unless the S flag (sidereal) is set in P_FLAG. (HOUR)	LC PERIOD ERR * Error in the rotational period given in the asteroid lightcurve parameters file. (HOUR)	LC AMPLITUDE MAXIMUM * Lightcurve amplitude maximum in the asteroid lightcurve parameters file. In cases where a range of amplitudes is given, this field is the upper limit of the range. In cases where a single value is given for the amplitude, this field is that value and a null value is given for AMP_MIN. Both AMP_MIN and AMP_MAX contain a null value if the publication did not include an amplitude. (MAGNITUDE)	LC AMPLITUDE ERR * Error in the lightcurve amplitudes given in the asteroid lightcurve parameters file. (MAGNITUDE)	LC QUALITY CODE * This code describes the reliability of the lightcurve results in the asteroid lightcurve parameters file, and takes the following values: 0 - Result later proven incorrect. This appears only on records of individual observations. 1 - Result based on fragmentary lightcurve(s), may be completely wrong. 2 - Result based on less than full coverage, so that the period may be wrong by 30 percent or so. Also, a quality of 2 is used to note results where an ambiguity exists as to the number of extrema per cycle or the number of elapsed cycles between lightcurves. Hence the result may be wrong by an integer ratio. 3 - Denotes a secure result with no ambiguity and full lightcurve coverage. 4 - In addition to full coverage, denotes that a pole position is reported. In some cases, the numerical quality code may be followed by a plus or minus sign, indicating that the reliability is judged somewhat better (+) or worse (-) than implied by an un-signed number alone. This refinement in scale has been only recently added, and not yet retroactively, so most entries don't have signs, even in some cases where they would be appropriate.	LC NOTES * Notes pertaining to the lightcurve reported in the asteroid lightcurve parameters file. These are one-letter flags, one or more of which may appear in the column. ? - Usually tied with 'T' to indicate uncertainty. 1 - Monomodal curve (one min/max per rotation) 3 - Trimodal curve (three min/max per rotation) 4 - Quadrimodal curve (four min/max per rotation) A - Ambiguous period D - Period determined by us that differs from that given in the original publication E - Occultation observation H - Space telescope observations I - IR/Thermal observations M - Polarimetric observation N - No lightcurve published O - Adaptive optics observation P - Photographic photometry R - Radar observation T - Tumbling (Non-principal axis rotation - see lc_npa.tab for details) V - Visual photometry Additional flags associated with the T flag are as follows: None after the T - The asteroid is definitely tumbling ? : Possible tumbler 0 : The tumbling damping timescale is long enough that tumbling might be expected, but observations are not sufficient to substantiate either tumbling or not tumbling. - : The tumbling damping timescale is long enough that tumbling might be expected, but observations indicate the object is NOT tumbling. + : The tumbling damping timescale is short enough that tumbling would not seem likely, however, observations indicate that it may be tumbling or actually is tumbling.	LC REFERENCE ID * A short version of the reference citation for the published paper in which the values in this entry (in the asteroid lightcurve parameters file) were reported. The full citations may be found in the file lc_references.tab.
11.0	0.1	0.07	0.04	2		Ditteon 2007
22.005	0.001	0.08	0.02	3		Pilcher 2008d
				.	I	SIMPS
21.89	0.02	0.10	0.01	2+		Warner 2007c
21.89		0.05	0.01	1+		Behrend 2005web
11.				1		Lagerkvist 1992b
				.	I	Masiero 2012
				.	I	AKARI
				.	I	WISE
				.	N	Veres 2015

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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
1875-02-23	Pola	Palisa, J.

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Asteroid Occultations V14.0 (1 data product)

OBSERVATION DATE * Date of observation	OCC MAJOR AXIS * Major axis of best-fit ellipse derived from stellar occultation observations (KILOMETER)	OCC MINOR AXIS * Minor axis of best-fit ellipse derived from stellar occultation observations (KILOMETER)	OCC MAJOR AXIS POSITION ANGLE * Position angle of major axis of best-fit ellipse derived from stellar occultation observations (DEGREE)	OCC FIT QUALITY CODE * Quality code for occultation fit: 0 - no fit, no position; 1 - no fit, but observations sufficiently reliable to derive an astrometric position of the asteroid relative to the star; 2 - poor fit; 3 - good fit; 4 - excellent fit	OCC MAJOR AXIS UNC * Standard deviation of major axis of best-fit ellipse derived from stellar occultation observations (KILOMETER)	OCC MINOR AXIS UNC * Standard deviation of minor axis of best-fit ellipse derived from stellar occultation observations (KILOMETER)	OCC MAJOR AXIS POSITION ANGLE UNC * Standard deviation of position angle of major axis of best-fit ellipse derived from stellar occultation observations (DEGREE)
2000-08-21	91.0	91.0	0.0	2	2.3
2014-11-02	92.0	92.0	0.0	1

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Asteroid Photometric Catalog V1.1 (15 data products)

000143_19910801020046_B_TAB

time: 1991-08-01T02:00:46 file: indiv/ast000143/19910801020046_b.tab dataset: Asteroid Photometric Catalog V1.1

The Asteroid Photometric Catalog is intended to be a compilation of all published photometric data on lightcurves of asteroids. This dataset includes the third update to the APC, and is therefore complete through 1992. This file contains a single asteroid lightcurve.

000143_19910801020046_U_TAB

time: 1991-08-01T02:00:46 file: indiv/ast000143/19910801020046_u.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910801020046_V_TAB

time: 1991-08-01T02:00:46 file: indiv/ast000143/19910801020046_v.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910802002519_B_TAB

time: 1991-08-02T00:25:19 file: indiv/ast000143/19910802002519_b.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910802002519_U_TAB

time: 1991-08-02T00:25:19 file: indiv/ast000143/19910802002519_u.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910802002519_V_TAB

time: 1991-08-02T00:25:19 file: indiv/ast000143/19910802002519_v.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910803001458_B_TAB

time: 1991-08-03T00:14:58 file: indiv/ast000143/19910803001458_b.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910803001458_U_TAB

time: 1991-08-03T00:14:58 file: indiv/ast000143/19910803001458_u.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910803001458_V_TAB

time: 1991-08-03T00:14:58 file: indiv/ast000143/19910803001458_v.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910804004246_B_TAB

time: 1991-08-04T00:42:46 file: indiv/ast000143/19910804004246_b.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910804004246_U_TAB

time: 1991-08-04T00:42:46 file: indiv/ast000143/19910804004246_u.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910804004246_V_TAB

time: 1991-08-04T00:42:46 file: indiv/ast000143/19910804004246_v.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910805000749_B_TAB

time: 1991-08-05T00:07:49 file: indiv/ast000143/19910805000749_b.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910805000749_U_TAB

time: 1991-08-05T00:07:49 file: indiv/ast000143/19910805000749_u.tab dataset: Asteroid Photometric Catalog V1.1

000143_19910805000749_V_TAB

time: 1991-08-05T00:07:49 file: indiv/ast000143/19910805000749_v.tab dataset: Asteroid Photometric Catalog V1.1

Asteroid 143 Adria (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.
C					Xc

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IRAS Minor Planet Survey V6.0 (1 data product)

SIMPS MEAN ALBEDO * Mean derived geometric albedo on the H,G system from the Supplemental IRAS Minor Planet Survey (SIMPS).	SIMPS MEAN ALBEDO UNC * 1-sigma uncertainty in the mean derived geometric albedo from the Supplemental IRAS Minor Planet Survey (SIMPS), due solely to the precision of the IRAS flux data.	SIMPS MEAN DIAMETER * Mean diameter from the Supplemental IRAS Minor Planet Survey (SIMPS), computed from H and SIMPS_MEAN_ALBEDO (KILOMETERS)	SIMPS MEAN DIAMETER UNC * 1-sigma uncertainty in the mean diameter from the Supplemental IRAS Minor Planet Survey (SIMPS), due solely to the precision of the IRAS flux data.	SIMPS PLC * Probability of lightcurve variation, estimated in the Supplemental IRAS Minor Planet Survey (SIMPS). This quantity is used as a measure of the probability that a lightcurve effect is present in the data. Values are constrained to be between 0.10 and 1.00. Less than significant variation is assigned a value of 0.10.
0.0491	0.002	89.93	1.9	0.10

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IRTF Near-IR Spectroscopy of Asteroids V2.0 (1 data product)

thumbnail for clarketal2009/143_061006t134301.tab

NEAR_IR SPECTRUM OF ASTEROID 143 ADRIA

time: 2006-10-06T13:43:01 file: clarketal2009/143_061006t134301.tab dataset: IRTF Near-IR Spectroscopy of Asteroids V2.0

Asteroid spectrum obtained with SpeX at the NASA Infrared Telescope Facility (IRTF). Preprocessing of the SpeX data, as well as extraction of the 1-D spectrum and wavelength calibration was carried out using various tasks in IRAF. Telluric correction was achieved with IDL code that utilizes model atmospheric transmission spectra generated with ATRAN. Multiple solar-analog stars were used in calibrating this spectrum in units of relative reflectance. Spectrum has been normalized to 1.0 at ~ 1.215 microns (center of the J-band).

Asteroid 143 Adria (top)

MSX Infrared Minor Planet Survey V1.0 (1 data product)

MIMPS ALBEDO * Mean geometric visual albedo on the H,G magnitude system, from the MSX Infrared Minor Planet Survey (MIMPS).	MIMPS ALBEDO UNC * 1-sigma uncertainty in the mean geometric visual albedo from the MSX Infrared Minor Planet Survey (MIMPS).	MIMPS DIAMETER * Mean diameter computed from H and MIMPS_ALBEDO, from the MSX Infrared Minor Planet Survey (MIMPS). (KILOMETERS)	MIMPS DIAMETER UNC * 1-sigma uncertainty in the mean diameter, from the MSX Infrared Minor Planet Survey (MIMPS). (KILOMETERS)
0.0504	0.0027	88.86	2.39

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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
87.337	2.229	0.052	0.009	0.960	0.059	Mas14
95.377	0.698	0.044	0.007	1.000	0.000	Mas12
88.237	19.835	0.054	0.018	0.950	0.144	Nug15
90.919	30.643	0.051	0.037	0.950	0.214	Nug15

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Small Main-belt Asteroid Spectroscopic Survey, Phase II (1 data product)

143 ADRIA AVERAGE CCD SPECTRUM

time: 1996-10-15T03:34:21 file: data04/143_00.tab dataset: Small Main-belt Asteroid Spectroscopic Survey, Phase II

Individual asteroid spectrum obtained during the Phase II Small Main-Belt Asteroid Spectroscopic Survey with the MDM telescopes at Kitt Peak National Observatory.

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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
.336	.021	2	.738	.026	2