Hostname: page-component-6bf8c574d5-t27h7 Total loading time: 0 Render date: 2025-02-28T06:00:51.718Z Has data issue: false hasContentIssue false
  • English
  • Français

Asteroid Spectroscopy and Mineralogy

Published online by Cambridge University Press:  19 July 2016

Thomas H. Burbine  and
Richard P. Binzel
Thomas H. Burbine
Affiliation:
Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA 02139, U.S.A. E-mail [email protected] E-mail [email protected]
Richard P. Binzel
Affiliation:
Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA 02139, U.S.A. E-mail [email protected] E-mail [email protected]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Spectroscopic observations of asteroids of smaller sizes and in the near-infrared have led to many exciting discoveries that have increased substantially our knowledge of the mineralogy of asteroids. These discoveries include the identification of hydrated M and E-asteroids, the mineralogical diversity of the S-class, anomalous S-asteroids, a possible source body of the aubrites, Vesta-like objects in the main belt, possible ordinary chondrite-like objects and one of the reddest objects in the solar system.

Type
Physical Observations and Modeling
Information
Symposium - International Astronomical Union , Volume 160: Asteroids, Comets, Meteors 1993 , 1994 , pp. 255 - 270
Copyright
Copyright © Kluwer 1994 

References

Barucci, M. A. and Lazzarin, M.: 1993, “Koronis family: Reflectance spectra of 243 Ida, 1442 Corvina and 2226 Cunitza.” Planet. Space Sci, 41, 641–646.Google Scholar
Barucci, M. A., Capria, M. T., Coradini, A. and Fulchignoni, M.: 1987, “Classification of asteroids using G-mode analysis.” Icarus, 72, 304–324.CrossRefGoogle Scholar
Bell, J. F.: 1986, “Mineralogical evolution of meteorite parent bodies (abstract).” Lunar Planet. Sci., XVII, 985–986.Google Scholar
Bell, J. F.: 1988, “A probable asteroidal parent body for the CV or CO chondrites (abstract). Meteoritics, 23, 256–257.Google Scholar
Bell, J. F., Davis, D. R., Hartmann, W. K. and Gaffey, M. J.: 1989, “Asteroids: The big picture.” In Asteroids II (Binzel, R. P., Gehrels, T. and Matthews, M. S., Eds.), 921–945. University of Arizona Press.Google Scholar
Bell, J. F., Owensby, P. D., Hawke, B. R. and Gaffey, M. J.: 1988, “The 52–color asteroid survey: Final results and interpretation (abstract).” Lunar Planet. Sci., XIX, 57–58.Google Scholar
Binzel, R. P.: 1992, “The optical spectrum of 5145 Pholus.” Icarus, 99, 238–240.Google Scholar
Binzel, R. P. and Xu, S.: 1990, “Asteroid 2965 Surikov: A piece of the missing mantle? (abstract).” Bull. Am. Astron. Soc., 22, 1115–1116.Google Scholar
Binzel, R. P. and Xu, S.: 1993, “Chips off of asteroid 4 Vesta: Evidence for the parent body of basaltic achondrite meteorites.” Science, 260, 186–191.Google Scholar
Binzel, R. P., Xu, S., Bus, S. J., Skrutskie, M. F., Meyer, M. R., Knezek, P. and Barker, E. S.: 1993. “Discovery of a main-belt asteroid resembling ordinary chondrite meteorites.” Science, 262, 1541–1543.Google Scholar
Burbine, T. H. and Bell, J. F.: 1993a, “Asteroid taxonomy: Problems and proposed solutions (abstract).” IAU Symposium 160: Asteroids, Comets, Meteors 1993, 49.Google Scholar
Burbine, T. H. and Bell, J. F.: 1993b, “How diverse is the asteroid belt? (abstract).” Lunar Planet. Sci., XXIV, 223–224.Google Scholar
Burbine, T. H., Gaffey, M. J. and Bell, J. F.: 1992, “S-asteroids 387 Aquitania and 980 Anacostia: Possible fragments of the breakup of a spinel-bearing parent body with CO3/CV3 affinities.” Meteoritics, 27, 424–434.Google Scholar
Clark, B. E.: 1993, “Spectral Reflectance Studies and Optical Surface Alteration in the Search for Links Between Meteorites and Asteroids.” Ph. D. Thesis, University of Hawaii.Google Scholar
Cloutis, E. A. and Gaffey, M. J.,: 1993, “The constituent minerals in calcium-aluminum inclusions: Spectral reflectance properties and implications for CO carbonaceous chondrites and asteroids.” Icarus, 105, 568–579.Google Scholar
Cloutis, E. A., Gaffey, M. J., Jackowski, T. L. and Reed, K. L.: 1986, “Calibration of phase abundance, composition, and particle size distribution for olivine-orthopyroxene mixtures from reflectance spectra.” J. Geophys. Res., 91, 11,641–11,653.CrossRefGoogle Scholar
Cruikshank, D. P., Allamandola, L. J., Hartmann, W. K., Tholen, D. J., Brown, R. H., Matthews, C. N. and Bell, J. F.: 1991a, “Solid CN bearing material on outer solar system bodies.” Icarus, 94, 345–353.CrossRefGoogle Scholar
Cruikshank, D. P., Tholen, D. J., Hartmann, W. K., Bell, J. F. and Brown, R. H.: 1991b, “Three basaltic Earth-approaching asteroids and the source of the basaltic meteorites.” Icarus, 89, 1–13.Google Scholar
Davies, J. K. and Sykes, M. V.: 1992, “(5145) 1992 AD.” IAU Circular, 5480.Google Scholar
Farinella, P., Gonczi, R., Froeschlé, Ch. and Froeschlé, C.: 1993, “The injection of asteroid fragments into resonances.” Icarus, 101, 174–187.Google Scholar
Feierberg, M. A. and Drake, M. A.: 1980, “The meteorite-asteroid connection: The infrared spectra of eucrites, shergottites, and Vesta.” Science, 209, 805–807.Google Scholar
Feierberg, M. A., Larson, H. P., Fink, U. and Smith, H. A.: 1980, “Spectroscopic evidence for two achondrite parent bodies: Asteroids 349 Dembowska and 4 Vesta.” journalGeochim. Cosmochim. Acta, 45, 971–981.Google Scholar
Fink, U., Hoffman, M., Grundy, W., Hicks, M. and Sears, W.: 1992, “The steep red spectrum of 1992 AD: An asteroid covered with organic material?” Icarus, 97, 145–149.Google Scholar
Gaffey, M. J.: 1976, “Spectral reflectance characteristics of the meteorite classes.” J. Geophys. Res., 81, 905–920.Google Scholar
Gaffey, M. J.: 1983, “The asteroid (4) Vesta: Rotational spectral variations, surface material heterogeneity, and implications for the origin of the basaltic achondrites (abstract).” Lunar Planet. Sci., XIV, 231–232.Google Scholar
Gaffey, M. J.: 1984. “Rotational spectral variations of asteroid (8) Flora: Implications for the nature of the S-type asteroids and for the parent bodies of the ordinary chondrites.” Icarus, 60, 83–114.Google Scholar
Gaffey, M. J., Bell, J. F., Brown, R. H., Burbine, T. H., Piatek, J. L., Reed, K. L. and Chaky, D. L.: 1993a, “Mineralogic variations within the S-type asteroid class.” Icarus, 106, 573–602.Google Scholar
Gaffey, M. J., Bell, J. F. and Cruikshank, D. P.: 1989, “Reflectance spectroscopy and asteroid surface mineralogy.” In Asteroids II (Binzel, R. P., Gehrels, T. and Matthews, M. S., Eds.), 98–127. University of Arizona Press.Google Scholar
Gaffey, M. J., Burbine, T. H. and Binzel, R. P.: 1993b, “Asteroid spectroscopy: Progress and perspectives.” Meteoritics, 28, 161–187.Google Scholar
Gaffey, M. J., Reed, K. L. and Kelley, M. S.: 1992, “Relationship of E-type Apollo asteroid 3103 (1982 BB) to the enstatite achondrite meteorites and the Hungaria asteroids.” Icarus, 100, 95–109.CrossRefGoogle Scholar
Howell, E. S., Merényi, E. and Lebofsky, L. A.: 1994, “Classification of asteroid spectra using a neural network.” Jour. Geophys. Res., in press.CrossRefGoogle Scholar
Jones, T. D., Lebofsky, L. A., Lewis, J. S. and Marley, M. S.: 1990, “The composition and origin of the C, P, and D asteroids: Water as a tracer of thermal evolution in the outer belt.” Icarus, 88, 172–192.Google Scholar
Keil, K.: 1989, “Enstatite meteorites and their parent bodies.” Meteoritics, 24, 195–208.Google Scholar
Luu, J. X. and Jewitt, D. C.: 1990, “Charge-coupled device spectra of asteroids. I. Near-Earth and 3: 1 resonance asteroids.” Astron. J., 99, 1985–2011.Google Scholar
McCord, T. B., Adams, J. B. and Johnson, T. V.: 1970, “Asteroid Vesta: Spectral reflectivity and compositional implications.” Science, 168, 1445–1447.CrossRefGoogle Scholar
Meteorite Working Group,: 1993. Antarctic Meteorite Newsletter (Score, R. and Lindstrom, M., Eds.), 16, 15.Google Scholar
Mueller, B. E. A., Tholen, D. J., Hartmann, W. K. and Cruikshank, D.: 1992, “Extraordinary colors of asteroidal object (5145) 1992 AD.” Icarus, 97, 150–154.Google Scholar
Ostro, S. J., Campbell, D. J. and Shapiro, I. I.: 1985, “Mainbelt asteroids: Dual-polarization radar observations.” Science, 229, 442–446.Google Scholar
Pieters, C. M. and McFadden, L. A.: 1994, “Meteorite and asteroid reflectance spectroscopy: Clues to early solar system processes.” Ann. Rev. of Earth and Plan. Science, in press.Google Scholar
Rivkin, A. S., Britt, D. T., Howell, E. S. and Lebofsky, L. A.: 1994, “Hydrated E-class and M-class asteroids (abstract).” Lunar Planet. Sci., XXV, in press.Google Scholar
Scotti, J. V.: 1992, “1992 AD.” IAU Circular, 5434.Google Scholar
Takeda, H., Saika, K., Otsuki, M. and Hiroi, T.: 1993, “A new Antarctic meteorite with chromite, orthopyroxene and metal with reference to a formation model of S asteroids (abstract).” Lunar Planet. Sci., XXIV, 1395–1396.Google Scholar
Tedesco, E. F., Matson, D. L., Veeder, G. J., Gradie, J. C. and Lebofsky, L. A.: 1989, “A three-parameter asteroid taxonomy.” Astron. J., 97, 580–606.CrossRefGoogle Scholar
Tholen, D. J.: 1984, “Asteroid Taxonomy from Cluster Analysis of Photometry.” Ph. D. Thesis, University of Arizona.Google Scholar
Veeder, G. J., Hanner, M. S., Matson, D. L., Tedesco, E. F., Lebofsky, L. A. and Tokunaga, A. T.: 1989, “Radiometry of near-Earth asteroids.” Astron. J., 97, 1211–1219.Google Scholar
Vilas, F. and McFadden, L. A.: 1993, “CCD reflectance spectra of selected asteroids. I. Presentation and data analysis considerations.” Icarus, 100, 85–94.Google Scholar
Wetherill, G. W.: 1987, “Dynamical relations between asteroids, meteorites and Apollo-Amor objects.” Phil. Trans. R. Soc. Lond. A, 323, 323–337.Google Scholar
Wisniewski, W. Z.: 1987, “Photometry of six radar target asteroids.”, Icarus, 90, 117–122.CrossRefGoogle Scholar
Xu, S.: 1994, “CCD Photometry and Spectroscopy of Small Main-Belt Asteroids.” Ph. D. Thesis, Massachusetts Institute of Technology.Google Scholar
Xu, S., Binzel, R. P., Burbine, T. H. and Bus, S. J.: 1993, “Small main-belt asteroid spectroscopic survey (abstract).” Bull. Am. Astron. Soc., 25, 1135.Google Scholar
Zappalà, V., Cellino, P., Farinella, P. and Kneževi$cG, Z.: 1990, “Asteroid families. 1. Identification by hierarchical clustering and reliability assessment.” Astron. J., 100, 2030–2046.CrossRefGoogle Scholar
Zellner, B., Leake, M., Morrison, D. and Williams, J. G.: 1977, “The E asteroids and the origin of the enstatite chondrites.” Geochim. Cosmochim. Acta, 41, 1759–1767.Google Scholar
Zellner, B., Tholen, D. J. and Tedesco, E. F.: 1985, “The eight-color asteroid survey: Results for 589 minor planets.” Icarus, 61, 355–416.Google Scholar