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SMASS - Small Main-Belt Asteroid Spectroscopic Survey@import "_stylesheets/smasssite.css";@import "_stylesheets/smass.css";.references {padding: 0.5pc 0 0.5pc 0;}.references ul {list-style: none; padding: 0;}.references ul li ul {padding: 0.5pc 0 0.5pc 0;}.dataproducts {padding: 0.5pc 0 0.5pc 0;}.gotobutton a {font-weight: bold; border: solid 1px black;}.minus {background-color: #C9C;}.busdemeo {background-color: #9CC;}dl dt {padding-top: 2pc;}dl dd {padding-bottom: 2pc;}#FOOTER a img.counter {float: none; border: solid 1px blue;}#FOOTER img.counter {float: none;}Planetary Spectroscopy at MITSMASSSmall Main-Belt Asteroid Spectroscopic SurveyMassachusetts Institute of TechnologyRichard P. Binzel (MIT), Principal InvestigatorCristina A. Thomas (MIT) Andrew S. Rivkin (APL)Thomas H. Burbine (Mt. Holyoke College)Schelte J. (Bobby) Bus (University of Hawaii)Go to Bus-DeMeo taxonomyGo to MIT-UH-IRTF Joint Campaign for NEO ReconnaissanceAvailable SMASS Data SetsSMASS data are organized into sets corresponding to theirpublicationin the refereed literature.Most of these data originally appeared within MIT Ph.D. theses.[9] Near-infrared data for (69230) Hermes, visible and near-infrareddata for (19356) 1997 GH3 and (433) Eros, model spectrum for "spaceweathered" version of 1997 GH3 spectrum. Rivkin, A. S., Binzel, R. P., Sunshine, J., Bus, S. J., Burbine, T. H., and Saxena, A. (2004). "Infrared spectroscopic observations of 69230 Hermes (1937 UB): possible unweathered endmember among ordinary chondrite analogs." Icarus 172, 408-414. Near-infrared spectrum of (69230) Hermes Visible and near-infrared spectrum of (19356) 1997 GH3 Model visible and near-infrared spectrum of (19356) 1997 GH3, with 0.02% smFe Visible and near-infrared spectrum of (433) Eros Gzipped tarfile of all asteroid spectra included in Reference [9]. Asteroid spectra included in Reference [9], available for cherry-picking. The digits after the leading zeroes give the asteroid number. Explanation of columns in asteroid data, same as for data in MIT-IRTF-Hawaii Joint Survey. Model spectrum has wavelength and normalized reflectance only. [8] Visible data and near-infrared data for254 near-Earth and Mars-crossing objects. Binzel, R. P., Rivkin, A. S., Stuart, J. S., Harris, A. W., Bus, S. J., and Burbine, T. H. (2004). "Observed Spectral Properties of Near-Earth Objects: Results for Population Distribution, Source Regions, and Space Weathering Processes." Icarus 170, 259-294. Summary tabulation for 407 near-Earth and Mars-crossing objects. (Table I, from reference [8], in EXCEL format). List of all 254 files of asteroid spectra included in Reference [8] Explanation for Filenames in Set [8] Gzipped tarfile of all asteroid spectra included in Reference [8] Asteroid spectra included in Reference [8], available for cherry-picking. The digits after the leading zeroes give the asteroid number. [7] Visible wavelength spectra of 22near-Earth objects candidates formission targets. Binzel, R. P., Perozzi, E., Rivkin, A. S. , Rossi, A., Harris, A. W., Bus, S. J., Valsecchi, G. B., and Slivan, S. M. (2004). "Dynamical and Compositional Assessment of Near-Earth Object Mission Targets." Meteoritics and Planetary Science 39, 351-366. List of all files of asteroid spectra included in Reference [7] Gzipped tarfile of all asteroid spectra included in Reference [7] Asteroid spectra included in Reference [7], available for cherry-picking. The digits after the leading zeroes give the asteroid number. [6] Combined visible and near-infraredwavelength spectroscopy of fournear-Earth asteroids obtained through remote observing on the NASAIRTF. Binzel, R. P., Birlan, M., Bus, S. J., Harris, A. W., Rivkin, A. S., and Fornasier, S. (2004). "Spectral Observations for Near-Earth Objects Including Potential Target 4660 Nereus: Results from Meudon Remote Observations at the NASA Infrared Telescope Facility (IRTF)." Planetary and Space Science 52, 291-296. Visible and near-infrared spectrum of (1685) Toro. Visible and near-infrared spectrum of (1943) Anteros. Visible and near-infrared spectrum of (4142) Dersu-Uzala. Visible and near-infrared spectrum of (4660) Nereus. Gzipped tarfile of all asteroid spectra included in Reference [6] [5] Combinedvisible and near-infrared wavelength spectroscopy of asteroid(25143)Itokawa = 1998 SF36, target for the HAYABUSA (MUSES-C)sample return mission. Binzel, R. P., Rivkin, A. S., Bus, S. J., Sunshine, J., and Burbine, T. (2001). "MUSES-C Target Asteroid (25143) 1998 SF36: A Reddened Ordinary Chondrite." Meteoritics and Plan. Sci. 36, 1167-1172. Spectrum of asteroid (25143) Itokawa, original data. (Figure 1, top panel) Spectrum of asteroid (25143) Itokawa, dereddened model. (Figure 1, bottom panel) Gzipped tarfile of all asteroid spectra included in Reference [5] [4] Combined visibleand near-infrared spectroscopy (typically 0.4-1.6 micron) for 48near-Earth objects (NEOs) and select main-belt targets. Binzel, R. P., Harris, A. W., Bus, S. J., and Burbine, T. H. (2001). "Spectral Properties of Near-Earth Objects: Palomar and IRTF Results for 48 Objects Including Spacecraft Targets (9969) Braille and (10302) 1989 ML." Icarus 151, 139-149. List of all files of asteroid spectra included in Reference [4] Explanation for Filenames in Set [4] Explanation for Data Formats in Set [4] Gzipped tarfile of all asteroid spectra included in Reference [4] Asteroid spectra included in Reference [4], available for cherry-picking. The digits after the leading zeroes give the asteroid number. [3] Near-infrared spectroscopy(typically 0.90-1.60 micron) for 241 asteroids from the infrared component ofthe SMASS survey (SMASSIR). Burbine, T. H. (2000). Forging Asteroid-Meteorite Relationships Through Reflectance Spectroscopy. Ph. D. Thesis, Massachusetts Institute of Technology. Burbine, T. H. and Binzel, R. P. (2002). "Small Main-Belt Asteroid Spectroscopic Survey in the Infrared." Icarus 159, 468-499. List of all files of asteroid spectra included in Reference [3] Explanation for Filenames in Set [3] Explanation for Data Formats in Set [3] Gzipped tarfile of all asteroid spectra included in Reference [3] Asteroid spectra included in Reference [3], available for cherry-picking. The digits after the leading zeroes give the asteroid number. [2] Visiblewavelength spectroscopy (0.44-0.92 micron) for 1341 asteroids from thesecond phase of the SMASS survey (SMASS II). Bus, S. J. (1999). Compositional Structure in the Asteroid Belt: Results of a Spectroscopic Survey. Ph. D. Thesis, Massachusetts Institute of Technology. Bus, S. J. and Binzel, R. P. (2002). "Phase II of the Small Main-Belt Asteroid Spectroscopic Survey: The Observations", Icarus 158, 106-145. Bus, S. J. and Binzel, R. P. (2002). "Phase II of the Small Main-Belt Asteroid Spectroscopic Survey: A Feature-Based Taxonomy", Icarus 158, 146-177. Log of asteroids included in Reference [2] Explanation for Filenames in Set [2] Explanation for Data Formats in Set [2] Gzipped tarfile of all asteroid spectra included in Reference [2] Asteroid spectra included in Reference [2], available for cherry-picking. The digits after the leading zeroes give the asteroid number. Taxonomic classifications for 1447 asteroids from the feature-based taxonomy of Bus (1999). [1]Visible wavelength spectroscopy (typically 0.45-0.95 micron) for 316 asteroidsfrom the first phase of the SMASS survey(SMASS I). Xu, S. (1994). CCD Photometry and Spectroscopy of Small Main-Belt Asteroids. Ph. D. Thesis, Massachusetts Institute of Technology. Xu, S., Binzel, R. P., Burbine, T. H., and Bus, S. J. (1995). "Small Main-Belt Asteroid Spectroscopic Survey: Initial Results." Icarus 115, 1-35. Log of asteroids included in Reference [1] Summary table of results from Reference [1] Explanation for Filenames in Set [1] Explanation for Data Formats in Set [1] Gzipped tarfile of all asteroid spectra included in Reference [1] Asteroid spectra included in Reference [1], available for cherry-picking. The digits after the leading zeroes give the asteroid number.  Last modified 2008 Jul 21 Web-tsarina: Cristina Thomas (cathomas@mit.edu) WebCounter visitor number is ![[visitor counter]](http://counter.digits.com/wc/-d/4/SMASSCounter) |
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