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587 results for “asteroids”
Small Main-Belt Asteroid Spectroscopic Survey (SMASS) V1.0
The Small Main-Belt Asteroid Spectroscopic Survey (SMASS) was a wide wavelength-coverage visible spectroscopic survey of asteroids carried out primarily at the Michagan-Dartmouth-MIT (McGraw Hill) Observatory on Kitt Peak beginning in 1990. This data set covers the observations for the years 1990-1994 and includes spectra of 316 asteroids. The data have been published in Xu et al. (1995), Icarus 115, 1-35, 1995.
ASTEROID ABSOLUTE MAGNITUDES V11.0
Absolute magnitudes and slopes, mostly IAU-adopted with exceptions noted, for all asteroids numbered as of the 2007 April 2 batch of Minor Planet Circulars.
2MASS ASTEROID AND COMET SURVEY V1.0
This data set includes J, H, and Ks magnitudes from the Two Micron All-Sky Survey (2MASS) for sources which were positionally associated with asteroids, comets, planets, and planetary satellites.
52-COLOR ASTEROID SURVEY
This data set contains 52-color IR data of asteroids, taken using a double circularly variable filter. The short wavelength portion of the CVF covered the octave from 0.8 to 1.6 microns with 3 percent resolution, while the long wavelength portion covered 1.5 to 2.6 microns with 5 percent resolution. Most of the data are unpublished other than in this PDS data set.
Gazetteer of Planetary Nomenclature: Asteroids: Dactyl
These images display asteriods documented and approved by the International Astronomical Union (IAU).
ASTEROID RADAR V9.0
This data set is a compilation of all groundbased asteroid radar detections. The collection is maintained and updated by Steven Ostro. It is updated annually.
ASTEROID POLARIMETRIC DATABASE V4.0
The Asteroid Polarimetric Database (APD) is compiled by Dmitrij Lupishko of Kharkov University. This database tabulates the original data comprising degree of polarization as a function of phase angle of the asteroid, and additional parameters where available. This data set, together with 'polar.tab' containing the TRIAD polarimetry, includes most if not all existing asteroid polarimetry data published by 1998. The APD is an ongoing compilation and this data set will be updated yearly.
SAWYER ASTEROID SPECTRA
This data set contains 94 optical asteroid spectra obtained by Scott Sawyer as part of his Ph.D. dissertation at the University of Texas at Austin. Observational circumstances and processing level are also provided.
BELSKAYA ASTEROID POLARIMETRY V1.0
This data set contains UBVRI polarimetric measurements of ten main belt asteroids and one potentially hazardous near-Earth asteroid (NEA), from Belskaya et al. (2009) and Belskaya et al. (2009b).
REDDY IRTF NEAR-EARTH ASTEROID SPECTRA V1.0
This data set contains low-resolution near-infrared (~0.7-2.5 microns) spectra of 40 near-Earth asteroids observed with the SpeX instrument on the NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i. This data set archives reduced, calibrated spectra that were obtained as part of Vishnu Reddy's Ph.D. disseration at the University of North Dakota. They have been used for detailed mineralogical/compositional analysis and thermal modeling to constrain the albedo of these objects.
ASTEROID ABSOLUTE MAGNITUDES V12.0
Absolute magnitudes and slopes, mostly IAU-adopted with exceptions noted, for all asteroids numbered as of the 2008 April 20 batch of Minor Planet Circulars.
IRTF NEAR-IR SPECTROSCOPY OF ASTEROIDS V2.0
This data set contains low-resolution, near-infrared (0.8 - 2.5 micron) spectra of asteroids obtained with SpeX at the NASA Infrared Telescope Facility (IRTF) on Mauna Kea. Since it was commissioned in June 2000, SpeX has been the premier instrument for producing high quality near-IR spectra of asteroids. These spectra have been used for both taxonomic studies of asteroids, and for more detailed mineralogical and compositional investigations. This data set archives the reduced, calibrated spectra that have been published in the peer-reviewed literature, and will be regularly updated as more data become publicly available.
REDDY MAIN BELT ASTEROID SPECTRA
This data set contains low-resolution (R~150) near-infrared (0.7-2.5 microns) spectra of 90 main belt asteroids observed with the SpeX instrument on the NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i. This data set archives reduced, calibrated spectra of targets of opportunity observed from 2001 to 2012.
ASTEROID NAMES AND DISCOVERY V7.0
This data set lists name, designation(s), and discovery circumstances for all asteroids numbered as of the given stop date. It is compiled and maintain by David Tholen, and updated on a yearly basis.
ASTEROID RADAR V1.0
This dataset is intended to include all asteroid radar detections. An entry for each detection reports radar cross-section and circular polarization, if known, as well as the year of observation and the reference in which the observations were reported. Observations which have not been published yet, or which have been reported only in an abstract, are included as an entry but with no data.
ASTEROID LIGHTCURVE DERIVED DATA V10.0
This is a compilation of published rotational parameters derived from lightcurve data for asteroids, through Feb. 15 2008. In addition to reported rotational parameters by individual paper, there is a summary file with the values adopted by Harris, Warner, and Pravec as the most likely correct values for each asteroid. The data set also contains files listing known rotational information on asteroids with ambiguous periods, binary asteroids, and 'tumbling' asteroids.
ASTEROID ABSOLUTE MAGNITUDES V2.0
IAU-adopted magnitude parameters (absolute V magnitude and slope parameter) for all numbered asteroids.
ASTEROID TAXONOMY V2.0
This dataset provides taxonomic classifications of asteroids in each of four different systems: Tholen (1984, 1989) [THOLEN1984, THOLEN1989] (1989) [TEDESCOETAL1989]
SDSS-BASED ASTEROID TAXONOMY V1.1
The Sloan Digital Sky Survey Moving Object Catalog (SDSS-MOC) is a large data set that provides five-filter magnitudes and astrometric information for all moving objects identified in the SDSS images (Izevic et al., 2010). The photometric observations were classified by Carvano et al. (2010) into nine taxonomic classes: Vp, Op, Qp, Sp, Ap, Lp, Dp, Xp and Cp, which are related to the classes and complexes of Bus Taxonomy (Bus & Binzel, 2002b). This data set is contains the taxonomic classification of each SDSS detections and its compilation for each observed asteroid.
ASTEROID LIGHTCURVE DERIVED DATA V14.0
This is a compilation of published rotational parameters derived from lightcurve data for asteroids, based on the Warner et al. (2009) Asteroid Lightcurve Database. This is the version as of March 1, 2014. In addition to reported rotational parameters by individual paper, there is a summary file with the values adopted by Harris, Warner, and Pravec as the most likely correct values for each asteroid. The data set also contains files listing known binary asteroids and 'tumbling' asteroids.
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International Brain Laboratory public data
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OpenNeuro
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