Small Bodies Node

Asteroid 179 Klytaemnestra (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)
11.290	0.022	10.932	0.020	10.900	0.020

Asteroid 179 Klytaemnestra (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
8.15	0.15	a	MPC 17257

Asteroid 179 Klytaemnestra (top)

Asteroid Albedos (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).
0.1609	0.006

Asteroid 179 Klytaemnestra (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.

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
121	46

Asteroid 179 Klytaemnestra (top)

Asteroid Lightcurve Derived Data V16.0 (2 data products)

LC PERIOD FLAG * Flag referring to the sidereal period given in the asteroid lightcurve parameters file, taking the following values: > - less than	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.
	11.173		0.35		3		Harris 1983a
	11.13	0.02	0.55	0.02	2		Ditteon 2007
					.	I	SIMPS
					.	I	Masiero 2012
					.	I	AKARI
					.	I	WISE
S	11.17342	0.00005			.	N	Hanus 2016

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.	LC SPINAXIS QUALITY CODE * The Q value gives our assessment of the quality of the pole solution. 0 Either wrong or very uncertain determination 1 Possible but not certain pole determination. This will most often appear when a limited number of data sets is used, especially if methods other than lightcurve inversion are involved. 2 Good determination, based on large dataset. The solution consists of one or two solutions (and possibly their 180 degree mirrors). If two solutions, they may differ in both longitude and latitude but not by the simple 180 degree mirror. 3 Very good determination, based on large dataset, an ambiguity of about 180 degrees in pole longitude might appear. 4 Excellent determination, pole position confirmed by methods based on independent datasets (for example, lightcurves and radar data, lightcurves and spacecraft fly-by). P A prograde rotation has been determined but no specific pole position has been determined. This will be followed by a 0 or 1, indicating the quality of the determination. R A retrograde rotation has been determined by no specific pole position has been determined. This will be followed by a 0 or 1, indicating the quality of the determination. In some cases, the numerical quality code is 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. If the Q value is blank, the given pole solution has not yet been reviewed under the new rating system.	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 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 SPINAXIS ECLIPTIC LONGITUDE 1 * Ecliptic longitude of the first solution in the spinaxis file of the asteroid derived lightcurve data set (DEGREE)	LC SPINAXIS ECLIPTIC LATITUDE 1 * Ecliptic latitude of the first solution in the spinaxis file of the asteroid derived lightcurve data set (DEGREE)	LC SPINAXIS ECLIPTIC LONGITUDE 2 * Ecliptic longitude of the second solution in the spinaxis file of the asteroid derived lightcurve data set (DEGREE)	LC SPINAXIS ECLIPTIC LATITUDE 2 * Ecliptic latitude of the second solution in the spinaxis file of the asteroid derived lightcurve data set (DEGREE)	LC SPINAXIS ECLIPTIC LONGITUDE 3 * Ecliptic longitude of the third solution in the spinaxis file of the asteroid derived lightcurve data set (DEGREE)	LC SPINAXIS ECLIPTIC LATITUDE 3 * Ecliptic latitude of the third solution in the spinaxis file of the asteroid derived lightcurve data set (DEGREE)	LC SPINAXIS ECLIPTIC LONGITUDE 4 * Ecliptic longitude of the fourth solution in the spinaxis file of the asteroid derived lightcurve data set (DEGREE)	LC SPINAXIS ECLIPTIC LATITUDE 4 * Ecliptic latitude of the fourth solution in the spinaxis file of the asteroid derived lightcurve data set (DEGREE)	LC SPINAXIS SIDEREAL PERIOD * Sidereal period of the spinaxis solution in the spinaxis file of the asteroid derived lightcurve data set. (HOUR)	LC SPINAXIS SHAPE FLAG * Flag for shape model in the spinaxis file of the asteroid derived lightcurve data set: Y = shape model exists
summary	9+	11.173	0.55
Hanus 2016	9+			65.0	-6.0	248.0	-9.0					11.17342

Asteroid 179 Klytaemnestra (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
1877-11-11	Ann Arbor	Watson, J. C.

Asteroid 179 Klytaemnestra (top)

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)
2003-06-08	88.4	56.6	-17.8	2	1.4	2.7	3.2
2008-06-29	77.0	77.0	0.0	1	0.0
2009-06-19	77.0	77.0	0.0	1
2009-07-14	77.0	77.0	0.0	1	0.0
2012-04-28	64.0	64.0	0.0	0
2014-07-02	64.0	64.0	0.0	1

Asteroid 179 Klytaemnestra (top)

Asteroid Photometric Catalog V1.1 (4 data products)

000179_19791009030035_V_TAB

time: 1979-10-09T03:00:35 file: indiv/ast000179/19791009030035_v.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.

000179_19791009093415_V_TAB

time: 1979-10-09T09:34:15 file: indiv/ast000179/19791009093415_v.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.

000179_19791009125652_V_TAB

time: 1979-10-09T12:56:52 file: indiv/ast000179/19791009125652_v.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.

000179_19791010040837_V_TAB

time: 1979-10-10T04:08:37 file: indiv/ast000179/19791010040837_v.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.

Asteroid 179 Klytaemnestra (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.
S	S0	S			Sk

Asteroid 179 Klytaemnestra (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)
0.462	25	0.330	20	0.143	16	12.580	12	0.180	15	0.139	21	0.125	16	0.207	30

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)
0.462	25	0.330	20	0.143	16	0.180	15	0.139	21	0.125	16	0.207	30

Asteroid 179 Klytaemnestra (top)

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.
0.1609	0.006	77.69	1.4	0.10

Asteroid 179 Klytaemnestra (top)

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

thumbnail for clarketal2009/179_080311t133408.tab

NEAR_IR SPECTRUM OF ASTEROID 179 KLYTAEMNESTRA

time: 2008-03-11T13:34:08 file: clarketal2009/179_080311t133408.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 179 Klytaemnestra (top)

Mothe-Diniz Asteroid Dynamical Families V1.1 (1 data product)

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	1994 UD8

Asteroid 179 Klytaemnestra (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
69.946	0.518	0.198	0.011	0.907	0.018	Mas14
90.167	1.527	0.119	0.018	1.000	0.000	Mas12
73.813	0.660	0.178	0.018	1.013	0.018	Mas12

Asteroid 179 Klytaemnestra (top)

Nesvorny HCM Asteroid Families V3.0 (1 data product)

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.
614	9506 Telramund

Asteroid 179 Klytaemnestra (top)

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

179 KLYTAEMNESTRA CCD SPECTRUM

time: 1995-12-10T08:01:45 file: data06/179_01.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.

Asteroid 179 Klytaemnestra (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
.408	.034	4	.832	.025	4

Asteroid 179 Klytaemnestra

Data sets with data for Asteroid 179 Klytaemnestra:

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

Asteroid Absolute Magnitudes V12.0 (1 data product)

Asteroid Albedos (1 data product)

Asteroid Dynamical Families V4.1 (2 data products)

Asteroid Lightcurve Derived Data V16.0 (2 data products)

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

Asteroid Occultations V14.0 (1 data product)

Asteroid Photometric Catalog V1.1 (4 data products)

000179_19791009030035_V_TAB

000179_19791009093415_V_TAB

000179_19791009125652_V_TAB

000179_19791010040837_V_TAB

Asteroid Taxonomy V6.0 (1 data product)

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

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

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

NEAR_IR SPECTRUM OF ASTEROID 179 KLYTAEMNESTRA

Mothe-Diniz Asteroid Dynamical Families V1.1 (1 data product)

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

Nesvorny HCM Asteroid Families V3.0 (1 data product)

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

179 KLYTAEMNESTRA CCD SPECTRUM

UBV Mean Asteroid Colors (1 data product)