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Part Three - Asteroids as Records of Formation and Differentiation

Published online by Cambridge University Press:  25 February 2017

Edited by
Linda T. Elkins-Tanton  and
Benjamin P. Weiss
Linda T. Elkins-Tanton
Affiliation:
Arizona State University
Benjamin P. Weiss
Affiliation:
Massachusetts Institute of Technology
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Planetesimals
Early Differentiation and Consequences for Planets
 , pp. 267 - 362
Publisher: Cambridge University Press
Print publication year: 2017

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References

References

Abell, P. A., Fernández, Y. R., Pravec, P., et al. 2005. Physical characteristics of comet Nucleus C/2001 OG108 (LONEOS). Icarus, 179, 174–194.CrossRefGoogle Scholar
Abell, P. A., Vilas, F., Jarvis, K. S., et al. 2007. Mineralogical composition of (25143) Itokawa 1998 SF36 from visible and near-infrared reflectance spectroscopy: Evidence for partial melting. Meteoritics & Planetary Science, 42, 2165–2177.CrossRefGoogle Scholar
A’Hearn, M. F., Feaga, L. M., Keller, H. U., et al. 2012. Cometary volatiles and the origin of comets. Astrophysical Journal, 758, A29.CrossRefGoogle Scholar
Barkume, K. M., Brown, M. E., and Schaller, E. L. 2008. Near-infrared spectra of centaurs and Kuiper belt objects. Astronomical Journal, 135, 55–67.CrossRefGoogle Scholar
Barucci, M. A., Cruikshank, D. P., Dotto, E., et al. 2005. Is Sedna another Triton? Astronomy & Astrophysics, 439, L1–L4.CrossRefGoogle Scholar
Barucci, M. A., Merlin, F., Guilbert, A., et al. 2008a. Surface composition and temperature of the TNO Orcus. Astron. Astrophys., 479, L13–L16.CrossRefGoogle Scholar
Barucci, M. A., Brown, M. E., Emery, J. P., and Merlin, F. 2008b. Composition and surface properties of trans-neptunian objects and centaurs. In The Solar System Beyond Neptune, ed. Barucci, M. A., Boehnhardt, H., Cruikshank, D. P., and Morbidelli, A.. Tucson, AZ: University of Arizona Press, 143–160.Google Scholar
Barucci, M.A., Alvarez-Candal, A., Merlin, F., et al. 2011. New insights on ices in centaur and transneptunian populations. Icarus, 214, 297–307.CrossRefGoogle Scholar
Bell, J. F. 1988. A probable asteroidal parent body for the CV or CO chondrites (abstract). Meteoritics, 23, 256–257.Google Scholar
Bennett, C. J., Jamieson, C. S., Osamura, Y., and Kaiser, R. I. 2006. Laboratory studies on the irradiation of methane in interstellar, cometary, and solar system ices. Astrophysical Journal, 653, 792–811.CrossRefGoogle Scholar
Binzel, R. P., Xu, S., Bus, S. J., et al. 1993. Discovery of a main-belt asteroid resembling ordinary chondrite meteorites. Science, 262, 1541–1543.CrossRefGoogle ScholarPubMed
Bockelée-Morvan, D., Crovisier, J., Mumma, M. J., Weaver, H. A. 2004. The composition of cometary volatiles. In Comets II, ed. Festou, M. C., Keller, H. U., and Weaver, H. A.. Tucson, AZ: University of Arizona Press. Tucson, 391–423.CrossRefGoogle Scholar
Bottke, W. F. Jr., Cellino, A., Paolicchi, P., and Binzel, R. P. 2002. An overview of the asteroids: The Asteroids III perspective. In Asteroids III, ed. Bottke, W. F. Jr., Cellino, A., Paolicchi, P., and Binzel, R. P.. Tucson, AZ: University of Arizona Press. Tucson, 3–15.CrossRefGoogle Scholar
Bottke, W. F., Nesvorny, D., Grimm, R. E., Morbidelli, A., and O’Brien, D. P. 2006. Iron meteorites as remnants of planetesimals formed in the terrestrial planet region. Nature, 439, 821–824.CrossRefGoogle ScholarPubMed
Bottke, W. F., Vokrouhlický, D., Minton, D., et al. 2012. An Archaean heavy bombardment from a destabilized extension of the asteroid belt. Nature, 485, 78–81.CrossRefGoogle ScholarPubMed
Brown, M. E. 2000. Near-infrared spectroscopy of Centaurs and irregular satellites. The Astronomical Journal, 119, 977–983.CrossRefGoogle Scholar
Brown, M. E. 2012. The compositions of Kuiper belt objects. Annual Review of Earth and Planetary Sciences, 40, 467–494.CrossRefGoogle Scholar
Brown, M. E. 2013. The density of mid-sized Kuiper belt object 2002 UX25 and the formation of the dwarf planets. Astrophysical Journal Letters, 778, L34.CrossRefGoogle Scholar
Brown, M. E. and Rhoden, A. R. 2014. The 3 μm spectrum of Jupiter’s irregular satellite Himalia. Astrophysical Journal Letters, 793, L44.CrossRefGoogle Scholar
Brown, M. E., Trujillo, C. A., and Rabinowitz, D. L. 2005. Discovery of a planetary-sized object in the scattered Kuiper belt. Astrophysical Journal Letters, 635, L97–L100.CrossRefGoogle Scholar
Brown, M. E., Barkume, K. M., Ragozzine, D., and Schaller, E. L. 2007. A collisional family of icy objects in the Kuiper belt. Nature, 446, 294–296.CrossRefGoogle ScholarPubMed
Brown, M. E., Schaller, E. L., and Fraser, W. C. 2011. A Hypothesis for the color diversity of the Kuiper belt. Astrophysical Journal Letters, 739, L60.CrossRefGoogle Scholar
Brown, M. E., Schaller, E. L., and Fraser, W. C. 2012. Water ice in the Kuiper belt. Astronomical Journal, 143, 7 pp.CrossRefGoogle Scholar
Brownlee, D., Tsou, P., Aléon, J., et al. 2006. Comet 81P/Wild 2 under a microscope. Science, 314, 1711–1716.CrossRefGoogle ScholarPubMed
Brunetto, R., Romano, F., Blanco, A., et al. 2006. Space weathering of silicates simulated by nanosecond pulse UV excimer laser. Icarus, 180, 546–554.CrossRefGoogle Scholar
Burbine, T. H. 1998. Could G-class asteroids be the parent bodies of the CM chondrites? Meteoritics & Planetary Science, 33, 253–258.CrossRefGoogle Scholar
Burbine, T. H. 2014. Asteroids. Planets, asteroids, comets and the solar system. In Treatise on Geochemistry, 2nd edn, ed. Davis, A. M.. Amsterdam: Elsevier, 365–415.CrossRefGoogle Scholar
Burbine, T. H. and O’Brien, K. M. 2004. Determining the possible building blocks of the Earth and Mars. Meteoritics & Planetary Science, 39, 667–681.CrossRefGoogle 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.CrossRefGoogle Scholar
Burbine, T. H., Meibom, A., and Binzel, R. P. 1996. Mantle material in the main belt: Battered to bits? Meteoritics & Planetary Science, 31, 607–620.CrossRefGoogle Scholar
Burbine, T. H., Binzel, R. P., Bus, S. J., and Clark, B. E. 2001. K asteroids and CO3/CV3 chondrites. Meteoritics & Planetary Science, 36, 245–253.CrossRefGoogle Scholar
Burbine, T. H., McCoy, T. J., Meibom, A., et al. 2002a. Meteoritic parent bodies: Their number and identification. In Asteroids III, ed. Bottke, W. F. Jr., Cellino, A., Paolicchi, P., and Binzel, R. P.. Tucson, AZ: University of Arizona Press, 653–667.CrossRefGoogle Scholar
Burbine, T. H., McCoy, T. J., Nittler, L. R., et al. 2002b. Spectra of extremely reduced assemblages: Implications for Mercury. Meteoritics & Planetary Science, 37, 1233–1244.CrossRefGoogle Scholar
Burbine, T. H., McCoy, T. J., Hinrichs, J. L., and Lucey, P. G. 2006. Spectral properties of angrites. Meteoritics & Planetary Science, 41, 1139–1145.CrossRefGoogle Scholar
Burbine, T. H., Duffard, R., Buchanan, P. C., et al. 2011. Spectroscopy of O-type asteroids. Lunar and Planetary Science Conference, 42, 1608.Google Scholar
Bus, S. J. 1999. Compositional structure in the asteroid belt: Results of a spectroscopic survey. Ph.D. thesis, Massachusetts Institute of Technology.Google Scholar
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.CrossRefGoogle Scholar
Campins, H. and Ryan, E. V. 1989. The identification of crystalline olivine in cometary silicates. Astrophysical Journal, 341, 1059–1066.CrossRefGoogle Scholar
Campins, H., Ziffer, J., Licandro, J., et al. 2006. Nuclear spectra of comet 162P/Siding Spring (2004 TU12). Astronomical Journal, 132, 1346–1353.CrossRefGoogle Scholar
Campins, H., Licandro, J., Pinilla-Alonso, N., et al. 2007. Nuclear spectra of comet 28P Neujmin 1. Astronomical Journal, 134, 1626–1633.CrossRefGoogle Scholar
Campins, H., Hargrove, K., Pinilla-Alonso, N., et al. 2010. Water ice and organics on the surface of the asteroid 24 Themis. Nature, 464, 1320–1321.CrossRefGoogle ScholarPubMed
Capaccioni, F., Coradini, A., Filacchione, G., et al. 2015. The organic-rich surface of comet 67P/Churyumov–Gerasimenko as seen by VIRTIS/Rosetta. Science, 347, 0628.CrossRefGoogle ScholarPubMed
Carry, B. 2012. Density of asteroids. Planetary and Space Science, 73, 98–118.CrossRefGoogle Scholar
Chapman, C. R. and Salisbury, J. W. 1973. Comparisons of meteorite and asteroid spectral reflectivities. Icarus, 19, 507–22.CrossRefGoogle Scholar
Chapman, C.R. 2004. Space weathering of asteroid surfaces. Annual Review of Earth and Planetary Sciences, 32, 539–567.CrossRefGoogle Scholar
Chiang, E. and Youdin, A. N. 2010. Forming planetesimals in solar and extrasolar nebulae. Annual Review of Earth and Planetary Sciences, 38, 493–522.CrossRefGoogle Scholar
Ciesla, F. J. 2007. Outward transport of high-temperature materials around the midplane of the solar nebula. Science, 318, 613–615.CrossRefGoogle ScholarPubMed
Ciesla, F. J., Davison, T. M., Collins, G. S., and O’Brien, D. P. 2013. Thermal consequences of impacts in the early solar system. Meteoritics & Planetary Science, 48, 2559–2576.CrossRefGoogle Scholar
Clark, B. E., Bus, S. J., Rivkin, A. S., et al. 2004a. Spectroscopy of X-type asteroids. Astronomical Journal, 128, 3070–3081.CrossRefGoogle Scholar
Clark, B. E., Bus, S. J., Rivkin, A. S., et al. 2004b. E-type asteroid spectroscopy and compositional modeling. Journal of Geophysical Research, 109, E02001.CrossRefGoogle Scholar
Clark, B. E., Ockert-Bell, M. E., Cloutis, E. A., et al. 2009. Spectroscopy of K-complex asteroids: Parent bodies of carbonaceous meteorites? Icarus, 202, 119–133.CrossRefGoogle Scholar
Clark, R. N., Brown, R. H., Jaumann, R., et al. 2005. Compositional maps of Saturn’s moon Phoebe from imaging spectroscopy. Nature, 435, 66–69.CrossRefGoogle ScholarPubMed
Cloutis, E. A., Gaffey, M. J., Smith, D. G. W., and Lambert, R. St. J. 1990. Reflectance spectra of “featureless” materials and the surface mineralogies of M- and E-class asteroids. Journal of Geophysical Research, 95, 281–293.CrossRefGoogle Scholar
Cloutis, E. A., Binzel, R. P., Burbine, T. H., et al. 2006. Asteroid 3628 Boznemcová: Covered with angrite-like basalts? Meteoritics & Planetary Science, 41, 1147–1161.CrossRefGoogle Scholar
Consolmagno, G. J. and Drake, M. J. 1977. Composition and evolution of the eucrite parent body: Evidence from rare earth elements. Geochimica et Cosmochimica Acta, 41, 1271–1282.CrossRefGoogle Scholar
Consolmagno, G., Britt, D., and Macke, R. 2008. The significance of meteorite density and porosity. Chemie der Erde, 68, 1–29.CrossRefGoogle Scholar
Crovisier, J., Biver, N., Bockelée-Morvan, D., and Colom, P. 2009a. Radio observations of Jupiter-family comets. Planetary and Space Science, 57, 1162–1174.CrossRefGoogle Scholar
Crovisier, J., Biver, N., Bockelée-Morvan, D., et al. 2009b. The chemical diversity of comets: synergies between space exploration and ground-based radio observations. Earth, Moon, and Planets, 105, 267–272.CrossRefGoogle Scholar
Cruikshank, D. P. and Hartmann, W. K. 1984. The meteorite–asteroid connection: Two olivine-rich asteroids. Science, 223, 281–283.CrossRefGoogle ScholarPubMed
Cruikshank, D. P., Roush, T. L., Moore, J. M., et al. 1997. The surfaces of Pluto and Charon. In Pluto and Charon, ed. Stern, S. A. and Tholen, D. J.. Tucson, AZ: University of Arizona Press. 221–267.Google Scholar
Dauphas, N. and Chaussidon, M. 2011. A Perspective from extinct radionuclides on a young stellar object: the sun and its accretion disk. Annual Review of Earth and Planetary Sciences, 39, 351–386.CrossRefGoogle Scholar
De León, J., Licandro, J., Serra-Ricart, M., et al. 2010. Observations, compositional, and physical characterization of near-Earth and Mars-crosser asteroids from a spectroscopic survey. Astronomy & Astrophysics, 517, A23.CrossRefGoogle Scholar
De Luise, F., Dotto, E., Fornasier, S., et al. 2010. A peculiar family of Jupiter Trojans: The Eurybates. Icarus, 209, 586–590.CrossRefGoogle Scholar
DeMeo, F. E., Binzel, R. P., Slivan, S. M., and Bus, S. J. 2009. An extension of the Bus asteroid taxonomy into the near-infrared. Icarus, 202, 160–180.CrossRefGoogle Scholar
DeMeo, F. E. and Carry, B. 2013. The taxonomic distribution of asteroids from multi-filter all sky photometric surveys. Icarus, 226, 723–741.CrossRefGoogle Scholar
DeMeo, F. E. and Carry, B. 2014. Solar system evolution from compositional mapping of the asteroid belt. Nature, 505, 629–634.CrossRefGoogle ScholarPubMed
Dumas, C., Owen, T., and Barucci, M. A. 1998. Near-infrared spectroscopy of low-albedo surfaces of the solar system: search for the spectral signature of dark material. Icarus, 133, 221–232.CrossRefGoogle Scholar
Dunn, T. L., Burbine, T. H., Bottke, W. F., and Clark, J. P. 2013. Mineralogies and source regions of near-Earth asteroids. Icarus, 222, 273–282.CrossRefGoogle Scholar
Emery, J. P. and Brown, R. H. 2003. Constraints on the surface composition of Trojan asteroids from near-infrared (0.8–4.0 μm) spectroscopy. Icarus, 164, 104–121.CrossRefGoogle Scholar
Emery, J.P., Cruikshank, D.P., and van Cleve, J. 2006. Thermal emission spectroscopy (5.2–38 μm) of three Trojan asteroids with the Spitzer Space Telescope: Detection of fine-grained silicates. Icarus, 182, 496–512.CrossRefGoogle Scholar
Emery, J. P., Burr, D. M., and Cruikshank, D. P. 2011. Near-infrared spectroscopy of Trojan asteroids: Evidence for two compositional groups. Astronomical Journal, 141, 25.CrossRefGoogle Scholar
Emery, J. P., Marzari, F. Morbidelli, A., French, L. A., and Grav, T. 2015. The complex history of Trojan asteroids. In Asteroids IV, ed. Michel, P., DeMeo, F., and Bottke, W. F.. Tucson, AZ: University of Arizona Press, 203–220.Google Scholar
Gaffey, M. J., Bell, J. F., and Cruikshank, D. P. 1989. Reflectance spectroscopy and asteroid surface mineralogy. In Asteroids II, ed. Binzel, R. P., Gehrels, T., and Matthews, M. F.. Tucson, AZ: University of Arizona Press, 98–127.Google Scholar
Gaffey, M. J., Bell, J. F., Brown, R. H., et al. 1993. Mineralogic variations within the S-type asteroid class. Icarus, 106, 573–602.CrossRefGoogle Scholar
Gomes, R., Levison, H.F., Tsiganis, K., and Morbidelli, A. 2005. Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets. Nature, 435, 466–469.CrossRefGoogle ScholarPubMed
Gradie, J., and Tedesco, E. 1982. Compositional structure of the asteroid belt. Science, 216, 1405–1407.CrossRefGoogle ScholarPubMed
Grav, T., Holman, M. J., Gladman, B. J., and Aksnes, K. 2003. Photometric survey of the irregular satellites. Icarus, 166, 33–45.CrossRefGoogle Scholar
Grav, T. & Holman, M. J. 2004. Near-infrared photometry of the irregular satellites of Jupiter and Saturn. Astrophysical Journal, 605, L141–L144.CrossRefGoogle Scholar
Hanner, M. S., Lynch, D. K., & Russell, R. W. 1994. The 8–13 micron spectra of comets and the composition of silicate grains. Astrophysical Journal, 425, 274–285.CrossRefGoogle Scholar
Hanner, M. S., Gehrz, R. D., Harker, D. E., et al. 1997. Thermal emission from the dust coma of comet Hale–Bopp and the composition of the silicate grains. Earth Moon and Planets, 79, 247–264.CrossRefGoogle Scholar
Harker, D. E., Woodward, C. E., Kelley, M. S., et al. 2011. Mid-infrared spectrophotometric observations of fragments B and C of comet 73P/Schwassmann–Wachmann 3. Astronomical Journal, 141, 26.CrossRefGoogle Scholar
Hayward, T. L., Hanner, M. S., and Sekanina, Z. 2000. Thermal infrared imaging and spectroscopy of comet Hale–Bopp (C/1995 O1). Astrophysical Journal, 538, 428–455.CrossRefGoogle Scholar
Hiroi, T., Pieters, C. M., Zolensky, M. E., and Lipschutz, M. E. 1993. Evidence of thermal metamorphism on the C, G, B, and F asteroids. Science, 261, 1016–1018.CrossRefGoogle Scholar
Hiroi, T. and Sasaki, S. 2001. Importance of space weathering simulation products in compositional modeling of asteroids: 349 Dembowska and 446 Aeternitas as examples. Meteoritics & Planetary Science, 36, 1587–1596.CrossRefGoogle Scholar
Hsieh, H. H. and Jewitt, D. A. 2006. Population of comets in the main asteroid belt. Science, 312, 561–563.CrossRefGoogle ScholarPubMed
Hutchison, R. 2004. Meteorites: A Petrologic, Chemical and Isotopic Synthesis. Cambridge: Cambridge University Press.Google Scholar
Javoy, M., Kaminski, E., Guyot, F., et al. 2010. The chemical composition of the Earth: Enstatite chondrite models. Earth and Planetary Science Letters, 293, 259–268.CrossRefGoogle Scholar
Jewitt, D. (2012). The active asteroids. Astronomical Journal, 143, 66.CrossRefGoogle Scholar
Johansen, A., Oishi, J. S., Mac Low, M.-M., et al. 2007. Rapid planetesimal formation in turbulent circumstellar disks. Nature, 448, 1022–1025.CrossRefGoogle ScholarPubMed
Johansen, A., Klahr, H., and Henning, Th. 2011. High-resolution simulations of planetesimal formation in turbulent protoplanetary discs. Astronomy & Astrophysics, 529, A62.CrossRefGoogle Scholar
Johansen, A., Youdin, A. N., and Lithwick, Y. 2012. Adding particle collisions to the formation of asteroids and Kuiper belt objects via streaming instabilities. Astronomy & Astrophysics, 537, A125.CrossRefGoogle Scholar
Kelley, M. S. and Gaffey, M. J. 2002. High-albedo asteroid 434 Hungaria: Spectrum, composition and genetic connections. Meteoritics & Planetary Science, 37, 1815–1827.CrossRefGoogle Scholar
Kelley, M. S. and Wooden, D. H. 2009. The composition of dust in Jupiter-family comets inferred from infrared spectroscopy. Planetary and Space Science, 57, 1133–1145.CrossRefGoogle Scholar
Küppers, M., O’Rourke, L., Bockelée-Morvan, D., Zakharov, V., Lee, S., et al. 2014. Localized sources of water vapour on the dwarf planet (1) Ceres. Nature, 505, 525–527.CrossRefGoogle ScholarPubMed
Levison, H., Bottke, W.F., Gounelle, M., et al. 2009. Contamination of the asteroid belt by primordial trans-neptunian objects. Nature, 460, 364–366.CrossRefGoogle ScholarPubMed
Licandro, J., Pinilla-Alonso, N., Pedani, M., et al. 2006. The methane ice rich surface of large TNO 2005 FY9: A Pluto-twin in the trans-neptunian belt? Astronomy & Astrophysics, 445, L35–L38.CrossRefGoogle Scholar
Lisse, C. M., VanCleve, J., Adams, A. C., et al. 2006. Spitzer spectral observations of the deep impact ejecta. Science, 313, 635–640.CrossRefGoogle ScholarPubMed
Lynch, D. K., Russell, R. W., and Sitko, M. L. 2002. 3- to 14-μm spectroscopy of comet C/1999 T1 (McNaught–Hartley). Icarus, 159, 234–238.CrossRefGoogle Scholar
Marchi, S., Brunetto, R., Magrin, S., et al. 2005. Space weathering of near-Earth and main belt silicate-rich asteroids: Observations and ion irradiation experiments. Astronomy & Astrophysics, 443, 769–775.CrossRefGoogle Scholar
Marchis, F., Hestroffer, D., Descamps, P., et al. 2006. A low density of 0.8 g cm–3 for the Trojan binary asteroid 617 Patroclus. Nature, 439, 565–567.CrossRefGoogle ScholarPubMed
Marchis, F., Enriquez, J. E., Emery, J. P., et al. 2012. Multiple asteroid systems: Dimensions and thermal properties from Spitzer Space Telescope and ground-based observations. Icarus, 221, 1130–1161.CrossRefGoogle Scholar
Marchis, F., Durech, J., Castillo-Rogez, J., et al. 2014. The puzzling mutual orbit of the binary Trojan asteroid (624) Hektor. Astrophysical Journal Letters, 783, L37.CrossRefGoogle Scholar
Marsset, M., Vernazza, P., Gourgeot, F., et al. 2014. Similar origin for low- and high-albedo Jovian trojans and Hilda asteroids? Astronomy & Astrophysics, 568, L7.CrossRefGoogle Scholar
Merlin, F., Barucci, M.A., de Bergh, C., et al. 2010a. Chemical and physical properties of the variegated Pluto and Charon surfaces. Icarus, 210, 930–943.CrossRefGoogle Scholar
Morbidelli, A., Levison, H. F., Tsiganis, K., and Gomes, R. 2005. Chaotic capture of Jupiter’s Trojan asteroids in the early solar system. Nature, 435, 462–465.CrossRefGoogle ScholarPubMed
Morbidelli, A., Levison, H. F., and Gomes, R. 2008. The dynamical structure of the Kuiper belt and its primordial origin. In The Solar System Beyond Neptune, ed. Barucci, M. A., Boehnhardt, H., Cruikshank, D. P., and Morbidelli, A.. Tucson, AZ: University of Arizona Press, 275–292.Google Scholar
Morbidelli, A., Bottke, W. F., Nesvorny, D., and Levison, H. F. 2009. Asteroids were born big. Icarus, 204, 558–573.CrossRefGoogle Scholar
Mueller, M., Marchis, F., Emery, J.P., et al. 2010. Eclipsing binary Trojan asteroid Patroclus: Thermal inertia from Spitzer observations. Icarus, 205, 505–515.CrossRefGoogle Scholar
Mumma, M. J. and Charnley, S. B. 2011. The chemical composition of comets: Emerging taxonomies and natal heritage. Annual Review of Astronomy & Astrophysics, 49, 471–524.CrossRefGoogle Scholar
Nakamura, T., Noguchi, T., Tanaka, M., et al. 2011. Itokawa dust particles: A direct link between S-type asteroids and ordinary chondrites. Science, 333, 1113–1116.CrossRefGoogle ScholarPubMed
Nakashima, D., Kita, N. T., Ushikubo, T., et al. 2014. Oxygen three-isotope ratios of silicate particles returned from asteroid Itokawa by the Hayabusa spacecraft: A strong link with equilibrated LL chondrites. Earth and Planetary Science Letters, 379, 127–136.CrossRefGoogle Scholar
Peixinho, N., Lacerda, P., and Jewitt, D. 2008. Color–Inclination relation of the classical Kuiper belt objects. Astronomical Journal, 136, 1837–1845.CrossRefGoogle Scholar
Peixinho, N., Delsanti, A., Guilbert-Lepoutre, A., et al. 2012. The bimodal colors of centaurs and small Kuiper belt objects. Astronomy & Astrophysics, 546, A86.CrossRefGoogle Scholar
Rivkin, A. S. 2012. The fraction of hydrated C-complex asteroids in the asteroid belt from SDSS data. Icarus, 221, 744–752.CrossRefGoogle Scholar
Rivkin, A. S. and Emery, J. P. 2010. Detection of ice and organics on an asteroidal surface. Nature, 464, 1322–1323.CrossRefGoogle Scholar
Russell, C. T., Raymond, C. A., Coradini, A., et al. 2012. Dawn at Vesta: Testing the protoplanetary paradigm. Science, 336, 684–686.CrossRefGoogle ScholarPubMed
Sasaki, S., Nakamura, K., Hamabe, Y., et al. 2001. Production of iron nanoparticles by laser irradiation in a simulation of lunar-like space weathering. Nature, 410, 555–557.CrossRefGoogle Scholar
Schaller, E. L. and Brown, M. E. 2007a. Detection of methane on Kuiper belt object (50000) Quaoar. Astrophysical Journal Letters, 670, L49–L51.CrossRefGoogle Scholar
Schaller, E. L. and Brown, M. E. 2007b. Volatile loss and retention on Kuiper belt objects. Astrophysical Journal Letters, 659, L61–L64.CrossRefGoogle Scholar
Shepard, M. K., Taylor, P. A., Nolan, M. C., et al. 2015. A radar survey of M- and X-class asteroids. III. Insights into their composition, hydration state, and structure. Icarus, 245, 38–55.CrossRefGoogle Scholar
Sheppard, S. S. and Trujillo, C. A. 2006. A thick cloud of Neptune Trojans and their colors. Science, 313, 511–514.CrossRefGoogle ScholarPubMed
Sierks, H., Lamy, P., Barbieri, C., et al. 2011. Images of asteroid 21 Lutetia: A remnant planetesimal from the early solar system. Science, 334, 487–490.CrossRefGoogle ScholarPubMed
Sierks, H., Barbieri, C., Lamy, P., et al. 2015. On the nucleus structure and activity of comet 67P/Churyumov-Gerasimenko. Science, 347, aaa1044.CrossRefGoogle ScholarPubMed
Sitko, M. L., Lynch, D. K., Russell, R. W., and Hanner, M. S. 2004. 3–14 Micron spectroscopy of comets C/2002 O4 (Honig), C/2002 V1 (NEAT), C/2002 X5 (Kudo–Fujikawa), C/2002 Y1 (Juels–Holvorcem), and 69P/Taylor and the relationships among grain temperature, silicate band strength, and structure among comet families. Astrophysical Journal, 612, 576–587.CrossRefGoogle Scholar
Strazzulla, G., Dotto, E., Binzel, R., et al. 2005. Spectral alteration of the meteorite Epinal (H5) induced by heavy ion irradiation: A simulation of space weathering effects on near-Earth asteroids. Icarus, 174, 31–35.CrossRefGoogle Scholar
Sunshine, J. M., Bus, S. J., McCoy, T. J., et al. 2004. High calcium pyroxene as an indicator of igneous differentiation in asteroids and meteorites. Meteoritics & Planetary Science, 39, 1343–1357.CrossRefGoogle Scholar
Sunshine, J. M., Bus, S. J., Corrigan, C. M., et al. 2007. Olivine-dominated asteroids and meteorites: Distinguishing nebular and igneous histories. Meteoritics & Planetary Science, 42, 155–170.CrossRefGoogle Scholar
Sunshine, J. M., Connolly, H. C., McCoy, T. J., et al. 2008. Ancient asteroids enriched in refractory inclusions. Science, 320, 514–516.CrossRefGoogle ScholarPubMed
Takir, D. and Emery, J. P. 2012. Outer main belt asteroids: Identification and distribution of four 3-μm spectral groups. Icarus, 219, 641–654.CrossRefGoogle Scholar
Tegler, S.C., Grundy, W.M., Vilas, F., et al. 2008. Evidence of N2-ice on the surface of the icy dwarf Planet 136472 (2005 FY9). Icarus, 195, 844–850.CrossRefGoogle Scholar
Thomas, P. C. 2010. Sizes, shapes, and derived properties of the saturnian satellites after the Cassini nominal mission. Icarus, 208, 395–401.CrossRefGoogle Scholar
Tsiganis, K., Gomes, R., Morbidelli, A., and Levison, H. F. 2005. Origin of the orbital architecture of the giant planets of the solar system. Nature, 435, 459–461.CrossRefGoogle ScholarPubMed
Tsuchiyama, A., Uesugi, M., Uesugi, K., et al. 2014. Three-dimensional microstructure of samples recovered from asteroid 25143 Itokawa: Comparison with LL5 and LL6 chondrite particles. Meteoritics & Planetary Science, 49, 172–187.CrossRefGoogle Scholar
Vernazza, P., Binzel, R. P., Thomas, C. A., et al. 2008. Compositional differences between meteorites and near-Earth asteroids. Nature, 454, 858–860.CrossRefGoogle ScholarPubMed
Vernazza, P., Binzel, R. P., Rossi, A., Fulchignoni, M., and Birlan, M. 2009a. Solar wind as the origin of rapid weathering of asteroid surfaces. Nature, 458, 993–995.CrossRefGoogle ScholarPubMed
Vernazza, P., Brunetto, R., Binzel, , et al. 2009b. Plausible parent bodies for enstatite chondrites and mesosiderites: Implications for Lutetia’s fly-by. Icarus, 202, 477–486.CrossRefGoogle Scholar
Vernazza, P., Lamy, P., et al. 2011. Asteroid (21) Lutetia as a remnant of Earth’s precursor planetesimals. Icarus, 216, 650–659.CrossRefGoogle Scholar
Vernazza, P., Delbo, M., King, P. L., et al. 2012. High surface porosity as the origin of emissivity features in asteroid spectra. Icarus, 221, 1162–1172.CrossRefGoogle Scholar
Vernazza, P., Zanda, B., Binzel, R. P., et al. 2014. Multiple and fast: The Accretion of ordinary chondrite parent bodies. Astrophysical Journal, 791, L22.CrossRefGoogle Scholar
Vernazza, P., Zanda, B., Nakamura, T., et al. 2015a. The formation and evolution of ordinary chondrite parent bodies. In Asteroids IV, ed. Michel, P., DeMeo, F., and Bottke, W. F.. Tucson, AZ: University of Arizona Press, 618–634.Google Scholar
Vernazza, P., Marsset, B., Beck, P. et al. 2015b. Interplanetary dust particles as samples of icy asteroids. Astrophysical Journal, 806, 204.CrossRefGoogle Scholar
Vilas, F., Lederer, S. M., Gill, S. L., et al. 2006. Aqueous alteration affecting the irregular outer planets satellites: Evidence from spectral reflectance. Icarus, 180, 453–463.CrossRefGoogle Scholar
Walsh, K. J., Morbidelli, A., Raymond, S. N., O’Brien, D. P., and Mandell, A. M. 2011. A low mass for Mars from Jupiter’s early gas-driven migration. Nature, 475, 206–209.CrossRefGoogle ScholarPubMed
Weiss, B. P. and Elkins-Tanton, L. T. 2013. Differentiated planetesimals and the parent bodies of chondrites. Annual Review of Earth and Planetary Sciences, 41, 529–560.CrossRefGoogle Scholar
Westphal, A. J., Fakra, S. C., Gainsforth, Z., et al. 2009. Mixing fraction of inner solar system material in comet 81P/Wild2. Astrophysical Journal, 694, 18–28.CrossRefGoogle Scholar
Wooden, D. H., Woodward, C. E., and Harker, D. E. 2004. Discovery of crystalline silicates in comet C/2001 Q4 (NEAT). Astrophysical Journal Letters, 612, L77–L80.CrossRefGoogle Scholar
Wooden, D. H. 2008. Cometary refractory grains: interstellar and nebular sources. Space Science Reviews, 138, 75–108.CrossRefGoogle Scholar
Woodward, C. E., Jones, T. J., Brown, B., et al. 2011. Dust in comet C/2007 N3 (Lulin). Astronomical Journal, 141, A181.CrossRefGoogle Scholar
Yang, B., Lucey, P., and Glotch, T. 2013. Are large Trojan asteroids salty? An observational, theoretical, and experimental study. Icarus, 223, 359–366.CrossRefGoogle Scholar
Youdin, A. N. 2011. On the formation of planetesimals via secular gravitational instabilities with Turbulent Stirring. Astrophysical Journal, 731, 99.CrossRefGoogle Scholar
Youdin, A. N. and Goodman, J. 2005. Streaming instabilities in protoplanetary disks. Astrophysical Journal, 620, 459–469.CrossRefGoogle Scholar
Yurimoto, H., Abe, K., Abe, M., et al. 2011. Oxygen isotopic compositions of asteroidal materials returned from Itokawa by the Hayabusa mission. Science, 333, 1116–1119.CrossRefGoogle ScholarPubMed
Zellner, B. 1975. 44 Nysa: An iron-depleted asteroid. Astrophysical Journal, 198, L45–L47.CrossRefGoogle Scholar
Zellner, B., Leake, M., Williams, J.G., and Morrison, D. 1977. The E asteroids and the origin of the enstatite achondrites. Geochimica et Cosmochimica Acta, 41, 1759–1767.CrossRefGoogle Scholar
Zolensky, M. E., Zega, T. J., Yano, H., et al. 2006. Mineralogy and petrology of comet 81P/Wild 2 nucleus samples. Science, 314, 1735–1739.CrossRefGoogle Scholar
Zolensky, M. E., Nakamura-Messenger, K., Rietmeijer, F., et al. 2008. Comparing Wild 2 particles to chondrites and IDPs. Meteoritics & Planetary Science, 43, 261–272.CrossRefGoogle Scholar

References

Beck, A. W. and McSween, H. Y. Jr. 2010. Diogenites as polymict breccia composed of orthopyroxenite and harzburgite. Meteoritics & Planetary Science, 45, 850–872.CrossRefGoogle Scholar
Bell, J. F. 1988. A probable asteroidal parent body for the CO or CV chondrites. Meteoritics, 23, 256–257.Google Scholar
Bendjoya, Ph. and Zappalà, V. 2002. Asteroid family identification. In Asteroids III, ed. Bottke, W. F. Jr., Cellino, A., Paolicchi, P., and Binzel, R. P.. Tucson, AZ: University of Arizona Press. Tucson, 613–618.CrossRefGoogle Scholar
Benedix, G. K., Lauretta, D. S., and McCoy, T. J. 2005. Thermodynamic constraints on the formation conditions of winonaites and silicate-bearing IAB irons. Geochimica et Cosmochimica, 69, 5123–5131.CrossRefGoogle 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.CrossRefGoogle ScholarPubMed
Binzel, R. P., Rivkin, A. S., Bus, S. J., et al. 2001. MUSES-C target asteroid (25143) 1998 SF36: A reddened ordinary chondrite. Meteoritics & Planetary Science, 36, 1167–1172.CrossRefGoogle Scholar
Bottke, W. F. Jr., Durda, D. D., Nesvorný, D., et al. 2005. The fossilized size distribution of the main asteroid belt. Icarus, 175, 111–140.CrossRefGoogle Scholar
Brunetto, R., Romano, F., Blanco, A., et al. 2006. Space weathering of silicates simulated by nanosecond pulse UV excimer laser. Icarus, 180, 546–554.CrossRefGoogle Scholar
Burbine, T. H., Meibom, A. and Binzel, R. P. 1996. Mantle material in the main belt: Battered to bits? Meteoritics & Planetary Science, 31, 607–620.CrossRefGoogle Scholar
Burbine, T. H., Buchanan, P. C., Binzel, R. P., et al. 2001. Vesta, Vestoids, and the HEDs: Relationships and the origin of spectral differences. Meteoritics & Planetary Science, 36, 761–781.CrossRefGoogle Scholar
Burbine, T. H., McCoy, T. J., Keil, K., et al. 2002a. Meteoritic parent bodies: Their number and identification. In Asteroids III, ed. Bottke, W. F. Jr., Cellino, A., Paolicchi, P., and Binzel, R. P.. Tucson, AZ: University of Arizona Press, 653–667.CrossRefGoogle Scholar
Burbine, T. H., McCoy, T. J., Nittler, L. R., et al. 2002b. Spectra of extremely reduced assemblages: Implications for Mercury. Meteoritics & Planetary Science, 37, 1233–1244.CrossRefGoogle Scholar
Burbine, T. H., McCoy, T. J., Jarosewich, E., et al. 2003. Deriving asteroid mineralogies from reflectance spectra: Implications for the MUSES-C target asteroid. Antarctic Meteorite Research, 16, 185–195.Google Scholar
Bus, S. J. 1999. Compositional structure in the asteroid belt. Results of a spectroscopic survey. Ph.D Thesis, Massachusetts Institute of Technology.Google Scholar
Bus, S. J., ed. 2011. IRTF near-ir spectroscopy of asteroids V2.0. EAR-A-I0046-4-IRTFSPEC-V2.0. NASA Planetary Data System.Google Scholar
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.CrossRefGoogle Scholar
Castillo-Rogez, J. C. and McCord, T. B. 2010. Ceres’ evolution and present state constrained by shape data. Icarus, 205, 443–459.CrossRefGoogle Scholar
Chapman, C. R., 1974. Asteroid size distribution: Implications for the origin of stony-iron and iron meteorites. Geophysical Research Letters, 1, 341–344.CrossRefGoogle Scholar
Chapman, C. R. 1996. S-type asteroids, ordinary chondrites, and space weathering: The evidence from Galileo’s fly-bys of Gaspra and Ida. Meteoritics & Planetary Science, 31, 699–725.CrossRefGoogle Scholar
Clark, B. E., Bus, S. J., Rivkin, A. S., et al. 2004. E-type asteroid spectroscopy and compositional modeling. Journal of Geophysical Research, 109, E02001.CrossRefGoogle Scholar
Clark, B. E., Ockert-Bell, M. E., Cloutis, E. A., et al. 2009. Spectroscopy of K-complex asteroids: Parent bodies of carbonaceous meteorites? Icarus, 202, 119–133.CrossRefGoogle Scholar
Clenet, H., Jutzi, M., Barrat, J.-A., et al. 2014. A deep crust–mantle boundary in the asteroid 4 Vesta. Nature, 511, 303–306.CrossRefGoogle ScholarPubMed
de León, J., Pinilla-Alonso, N., Campins, H., et al. 2012. Near-infrared spectroscopic survey of B-type asteroids: Compositional analysis. Icarus, 218, 196–206.CrossRefGoogle Scholar
DeMeo, F. E., Binzel, R. P., Slivan, S. M., et al. 2009. An extension of the Bus asteroid taxonomy into the near-infrared. Icarus, 202, 160–180.CrossRefGoogle Scholar
de Sanctis, M. C., Migliorini, A., Luzia Jasmim, F., et al. 2011. Spectral and mineralogical characterization of inner main-belt V-type asteroids. Astronomy & Astrophysics, 533, A77.CrossRefGoogle Scholar
Duffard, R. and Roig, F. 2009. Two new V-type asteroids in the outer main belt? Planetary and Space Science, 57, 229–234.CrossRefGoogle Scholar
Gaffey, M. J. 1976. Spectral reflectance characteristics of the meteorite classes. Journal of Geophysical Research, 81, 905–920.CrossRefGoogle 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.CrossRefGoogle Scholar
Gaffey, M. J. 1986. The spectral and physical properties of metal in meteorite assemblages: Implications for asteroid surface materials. Icarus, 66, 468–486.CrossRefGoogle Scholar
Gaffey, M. J., Bell, J. F., Brown, R. H., et al. 1993. Mineralogical variations with the S-type asteroid class. Icarus, 106, 573–602.CrossRefGoogle Scholar
Gardner-Vandy, K. G., Lauretta, D. S., and McCoy, T. J. 2013. A petrologic, thermodynamic and experimental study of brachinites: Partial melt residues of an R chondrite-like precursor. Geochimica et Cosmochimica Acta, 122, 36–37.CrossRefGoogle Scholar
Goodrich, C. A. 1992. Ureilites: A critical review. Meteoritics, 27, 327–352.CrossRefGoogle Scholar
Grady, M. M. 2000. Catalogue of Meteorites, 5th edn. Cambridge: Cambridge University Press.Google Scholar
Granahan, J. C. 1993. Investigations of asteroid family geology. Ph.D Thesis, University of Hawaii.Google Scholar
Granahan, J. C. 2011. Spatially resolved spectral variations of asteroid 951 Gaspra. Icarus, 213, 265–272.CrossRefGoogle Scholar
Granahan, J. C. and Bell, J. F. 1991. On the geologic reality of asteroid families. Lunar and Planetary Science Conference, 22, 477–478.Google Scholar
Greenwood, R. C., Barrat, J.-A., Yamaguchi, A., et al. 2013. The oxygen isotope composition of diogenites: Evidence for early global melting on a single, compositionally diverse, HED parent body. Earth and Planetary Science Letters, 390, 165–174.CrossRefGoogle Scholar
Hardersen, P. S., Gaffey, M. J., and Abell, P. A. 2004. Mineralogy of asteroid 1459 Magnya and implications for its origin. Icarus, 167, 170–177.CrossRefGoogle Scholar
Hardersen, P. S., Reddy, V., Roberts, R., et al. 2014. More chips off of asteroid (4) Vesta: Characterization of eight Vestoids and their HED meteorite analogs. Icarus, 242, 269–282.CrossRefGoogle Scholar
Hasselmann, P. H., Carvano, J. M., and Lazzaro, D., 2012. SDSS-based asteroid taxonomy V1.1. EAR-A-I0035-5-SDSSTAX-V1.1. NASA Planetary Data System.Google Scholar
Hiroi, T., Pieters, C. M., and Takeda, H. 1994. Grain size of the surface regolith of asteroid 4 Vesta estimated from its reflectance spectrum in comparison with HED meteorites. Meteoritics, 29, 394–396.CrossRefGoogle Scholar
Huaman, M. E., Carruba, V., and Domingos, R. C. 2014. Dynamical evolution of V-type photometric candidates. Monthly Notices of the Royal Astronomical Society, 444, 2985–2992.CrossRefGoogle Scholar
Ikeda, Y. and Takeda, H., 1985. A model for the origin of basaltic achondrites based on the Yamato 7308 howardite. Journal of Geophysical Research, 90, C649–C663.CrossRefGoogle Scholar
Isaacson, P. J., Pieters, C. M., Besse, S., et al., 2011. Remote compositional analysis of lunar olivine-rich lithologies with Moon Mineralogy Mapper (M3) spectra. Journal of Geophysical Research, 116, E00G11.CrossRefGoogle Scholar
Ivezić, Ž, Lupton, R. H., Jurić, M., et al. 2002. Color confirmation of asteroid families. Astronomical Journal, 124, 2943–2948.CrossRefGoogle Scholar
Jurewicz, A. J. G., Mittlefehldt, D. W., and Jones, J. H., 1991. Partial melting of the Allende (CV3) meteorite: Implications for origins of basaltic meteorites. Science, 252, 695–698.CrossRefGoogle ScholarPubMed
Keil, K. 2002. Geological history of asteroid 4 Vesta: The “smallest terrestrial planet”. In Asteroids III, ed. Bottke, W. F. Jr., Cellino, A., Paolicchi, P., and Binzel, R. P.. Tucson, AZ: University of Arizona Press, 573–584.CrossRefGoogle Scholar
Keil, K., 2010. Enstatite achondrite meteorites (aubrites) and the histories of their asteroidal parent bodies. Chemie der Erde, 70, 295–317.CrossRefGoogle Scholar
Kelley, M. S. and Gaffey, M. J. 2002. High-albedo asteroid 434 Hungaria: Spectrum, composition, and genetic connections. Meteoritics & Planetary Science, 37, 1815–1827.CrossRefGoogle Scholar
Kelley, M. S., Vilas, F., Gaffey, M. J., et al. 2003. Quantified mineralogical evidence for a common origin of 1929 Kollaa with 4 Vesta and the HED meteorites. Icarus, 165, 215–218.CrossRefGoogle Scholar
Küppers, M., O’Rourke, L., Bockelée, D. 2014. Localized sources of water vapour on the dwarf planet (1) Ceres. Nature, 505, 525–527.CrossRefGoogle ScholarPubMed
Larson, H. P. and Fink, U., 1975. Infrared spectral observations of asteroid 4 Vesta. Icarus, 26, 420–427.CrossRefGoogle Scholar
Lazzaro, D., Michtchenko, T., Carvano, J. M., et al. 2000. Discovery of a basaltic asteroid in the outer main belt. Science, 288, 2033–2035.CrossRefGoogle ScholarPubMed
Le Corre, L., Reddy, V., Sanchez, J. A., et al. 2015. Exploring exogenic sources for the olivine on asteroid (4) Vesta. Icarus, 258, 483–499.CrossRefGoogle Scholar
Lucas, M. P. and Emery, J. P. 2014. Asteroid–Meteorite connections in the Hungaria background population: correlations with primitive achondrites? Lunar and Planetary Science Conference, 45, 1766.Google Scholar
Mainzer, A. K., Bauer, J., Grav, T., et al. 2011. Preliminary results from NEOWISE: An enhancement to the Wide-field Infrared Survey Explorer for solar system science. Astrophysical Journal, 731, 53.CrossRefGoogle Scholar
Mandler, B. E. and Elkins-Tanton, L. T. 2013. The origin of eucrites, diogenites, and olivine diogenites: Magma ocean crystallization and shallow magma chamber processes on Vesta. Meteoritics & Planetary Science, 48, 1–17.CrossRefGoogle Scholar
Masiero, J. R., Mainzer, A. K., Grav, T., et al. 2011. Main belt asteroids with WISE/NEOWISE. I. Preliminary albedos and diameters. Astrophysical Journal, 741, 68.CrossRefGoogle Scholar
Masiero, J. R., Mainzer, A. K., Bauer, J. M., et al. 2013. Asteroid family identification using the hierarchical clustering method and WISE/NEOWISE physical properties. Astrophysical Journal, 770, 7.CrossRefGoogle Scholar
Mayne, R. G., Sunshine, J. M., McSween, H. Y., et al. 2011. The origin of Vesta’s crust: Insights from spectroscopy of the Vestoids. Icarus, 214, 147–160.CrossRefGoogle Scholar
McCord, T. B. and Gaffey, M. J. 1974. Asteroids: Surface composition from reflection spectroscopy. Science, 186, 352–355.CrossRefGoogle ScholarPubMed
McCord, T. B. and Sotin, C. 2005. Ceres: Evolution and current state. Journal of Geophysical Research: Planets, 110, E05009.CrossRefGoogle Scholar
McCord, T. B., Adams, J. B., and Johnson, T. V. 1970. Asteroid Vesta: Spectral reflectivity and compositional implications. Science, 168, 1445–1447.CrossRefGoogle ScholarPubMed
McCoy, T. J., Keil, K., Muenow, D. W., et al. 1997. Partial melting and melt migration in the acapulcoite–lodranite parent body. Geochimica et Cosmochimica Acta, 61, 639–650.CrossRefGoogle Scholar
McCoy, T. J., Nittler, L. R., Burbine, T. H., et al. 2000. Anatomy of a partially differentiated asteroid: A “NEAR”-sighted view of acapulcoites and lodranites. Icarus, 148, 29–36.CrossRefGoogle Scholar
McCoy, T. J., Robinson, M. S., Nittler, L. R., et al. 2002. The Near Earth Asteroid Rendezvous mission to asteroid 433 Eros: A milestone in the study of asteroids and their relationship to meteorites. Chemie der Erde, 62, 89–121.CrossRefGoogle Scholar
McSween, H. Y., Ammannito, E., Reddy, V., et al. 2013. Composition of the Rheasilvia basin, a window into Vesta’s interior. Journal of Geophysical Research: Planets, 118, 335–346.CrossRefGoogle Scholar
Michel, P., Tanga, P., Benz, W., et al. 2002. Formation of asteroid families by catastrophic disruption: Simulations with fragmentation and gravitational reaccumulation. Icarus, 160, 10–23.CrossRefGoogle Scholar
Michel, P., Benz, W., and Richardson, D. C. 2003. Disruption of fragmented parent bodies as the origin of asteroid families. Nature, 421, 608–611.CrossRefGoogle ScholarPubMed
Michtchenko, T. A., Lazzaro, D., Ferraz-Mello, S., et al. 2002. Origin of the basaltic asteroid 1459 Magnya: A dynamical and mineralogical study of the outer main belt. Icarus, 158, 343–359.CrossRefGoogle Scholar
Milani, A. and Knežević, V. 2000. http://hamilton.dm.unipi.it/~astdys2/catalogs/allnum.pro.Google Scholar
Milliken, R. E. and Rivkin, A. S. 2009. Brucite and carbonate assemblages from altered olivine-rich materials on Ceres. Nature Geoscience, 2, 258–261.CrossRefGoogle Scholar
Moskovitz, N. A., Willman, M., Burbine, T. H., et al. 2010. A spectroscopic comparison of HED meteorites and V-type asteroids in the inner main belt. Icarus, 208, 773–788.CrossRefGoogle Scholar
Mothé-Diniz, T. and Nesvorný, D. 2008a. Visible spectroscopy of extremely young asteroid families. Astronomy & Astrophysics Letters, 486, L9–L12.CrossRefGoogle Scholar
Mothé-Diniz, T. and Nesvorný, D. 2008b. Tirela: An unusual asteroid family in the outer main belt. Astronomy & Astrophysics, 492, 593–598.CrossRefGoogle Scholar
Mothé-Diniz, T., Roig, F., and Carvano, J. M. 2005. Reanalysis of asteroid families structure through visible spectroscopy. Icarus, 174, 54–80.CrossRefGoogle Scholar
Mothé-Diniz, T., Carvano, J. M., Bus, S. J., et al. 2008. Mineralogical analysis of the Eos family from near-infrared spectra. Icarus, 195, 277–294.CrossRefGoogle Scholar
Nakamura, T., Noguchi, T., Tanaka, M, et al. 2011. Itokawa dust particles: A direct link between S-type asteroids and ordinary chondrites. Science, 333, 1113–115.CrossRefGoogle ScholarPubMed
Nathues, A., Mottola, S., Kaasalainen, M., et al. 2005. Spectral study of the Eunomia asteroid family I. Eunomia. Icarus, 175, 452–463.CrossRefGoogle Scholar
Nathues, A., Hoffmann, M., Schäfer, M., et al. 2014. Distribution of potential olivine sites on the surface of Vesta by Dawn FC. Lunar and Planetary Science Conference, 45, 1740.Google Scholar
Nathues, A., Hoffmann, M., Schäfer, M., et al. 2015. Exogenic olivine from Dawn framing camera color data. Icarus, 258, 467–482.CrossRefGoogle Scholar
Nesvorný, D. 2012. Nesvorny HCM Asteroid Families V2.0. EAR-A-VARGBDET-5-NESVORNYFAM-V2.0. NASA Planetary Data System.Google Scholar
Nesvorný, D., Brož, M., and Carruba, V. 2015. Identification and dynamical properties of asteroid families. In Asteroids IV, ed. Michel, P., DeMeo, F. E., and Bottke, W. F. Jr. Tucson, AZ: University of Arizona Press. Tucson, 297–322.Google Scholar
Neveu, M., Desch, S. J., Shock, E. L., et al. 2015. Prerequisites for explosive cryovolcanism on dwarf planet-class Kuiper belt objects. Icarus, 246, 48–64.CrossRefGoogle Scholar
Noguchi, T., Nakamura, T., Kimura, M., et al. 2011. Incipient space weathering observed on the surface of Itokawa dust particles. Science, 333, 1121–1125.CrossRefGoogle ScholarPubMed
Parker, A., Ivezić, Ž, Jurić, M., et al. 2008. The size distributions of asteroid families in the SDSS Moving Object Catalog 4. Icarus, 198, 138–155.CrossRefGoogle Scholar
Reddy, V., Emery, J. P., Gaffey, M. J., et al. 2009. Composition of 298 Baptistina: Implications for the K/T impactor link. Meteoritics & Planetary Science, 44, 1917–1927.CrossRefGoogle Scholar
Reddy, V., Carvano, J. M., Lazzaro, D., et al. 2011. Mineralogical characterization of Baptistina asteroid family: Implications for K/T impactor source. Icarus, 216, 184–197.CrossRefGoogle Scholar
Reed, K. L., Gaffey, M. J., and Lebofsky, L. A. 1997. Shape and albedo variations of asteroid 15 Eunomia. Icarus, 125, 446–454.CrossRefGoogle Scholar
Righter, K. and Drake, M. J. 1997. A magma ocean on Vesta: Core formation and petrogenesis of eucrites and diogenites. Meteoritics & Planetary Science, 32, 929–944.CrossRefGoogle Scholar
Rivkin, A. S., Asphaug, E., and Bottke, W. F. 2014. The case of the missing Ceres family. Icarus, 243, 429–439.CrossRefGoogle Scholar
Roig, F., Nesvorný, D., Gil-Hutton, R., et al. 2008. V-type asteroids in the middle main belt. Icarus, 194, 125–136.CrossRefGoogle Scholar
Russell, C. T., Raymond, C. A., Coradini, A., et al. 2012. Dawn at Vesta: Testing the protoplanetary paradigm. Science, 336, 684–686.CrossRefGoogle ScholarPubMed
Ruzicka, A., Snyder, G. A., and Taylor, L. A. 1997. Vesta as the HED parent body: Implications for the size of a core and for large-scale differentiation. Meteoritics & Planetary Science, 32, 825–840.CrossRefGoogle Scholar
Sack, R. O., Azeredo, W. J., and Lipschutz, M. E. 1991. Olivine diogenites: The mantle of the eucrite parent body. Geochimica et Cosmochimica Acta, 55, 1111–1120.CrossRefGoogle Scholar
Sanchez, J. A., Reddy, V., Kelley, M. S., et al. 2014. Olivine-dominated asteroids: Mineralogy and origin. Icarus, 228, 288–300.CrossRefGoogle Scholar
Sasaki, S., Nakamura, K., Hamabe, Y., et al. 2001. Production of iron nanoparticles by laser irradiation in a simulation of lunar-like space weathering. Nature, 410, 555–557.CrossRefGoogle Scholar
Schenck, P., O’Brien, D. P., Marchi, S., et al. 2012. The geologically recent giant impact basins at Vesta’s south pole. Science, 336, 694–697.CrossRefGoogle Scholar
Scott, E. R. D., Greenwood, R. C., Franchi, I. A., et al. 2009. Oxygen isotopic constraints on the origin and parent bodies of eucrites, diogenites, and howardites. Geochimica et Cosmochimica Acta, 73, 5835–5853.CrossRefGoogle Scholar
Singer, R. B. and Roush, T. L. 1985. Effects of temperature on remotely sensed mineral absorption features. Journal of Geophysical Research, 90, 12434–12444.CrossRefGoogle Scholar
Solontoi, M. R., Hammergren, M., Gyuk, G., et al. 2012. AVAST survey 0.4–1.0 μm spectroscopy of igneous asteroids in the inner and middle main belt. Icarus, 220, 577–585.CrossRefGoogle Scholar
Spoto, F., Milani, A., Cellino, A., et al. 2013. Larger classification allows a new interpretation of the Vesta family. American Astronomical Society DPS meeting, 45, 106.07.Google Scholar
Sunshine, J. M., Bus, S. J., and McCoy, T. J., et al. 2004. High-calcium pyroxene as an indicator of igneous differentiation in asteroids and meteorites. Meteoritics & Planetary Science, 39, 1343–1357.CrossRefGoogle Scholar
Sunshine, J. M., Connolly, H. C., McCoy, T. J., et al. 2008. Ancient asteroids enriched in refractory inclusions. Science, 320, 514–517.CrossRefGoogle ScholarPubMed
Tera, F. and Carlson, R. W. 1999. Assessment of the Pb–Pb and U–Pb chronometry of the early solar system. Geochimica et Cosmochimica Acta, 63, 1877–1889.CrossRefGoogle Scholar
Thangjam, G., Nathues, A., Mengel, K., et al. 2014. Olivine-rich exposures at Bellicia and Arruntia craters on (4) Vesta from Dawn FC. Meteoritics & Planetary Science, 49, 1831–1850.CrossRefGoogle Scholar
Tholen, D. J. 1984. Asteroid taxonomy from cluster analysis of photometry. Ph.D Thesis, University of Arizona.Google Scholar
Thomas, P. C., Parker, J. Wm., McFadden, L. A., et al. 2005. Differentiation of the asteroid Ceres as revealed by its shape. Nature, 437, 224–226.CrossRefGoogle ScholarPubMed
Thomas, C. A., Lim, L., Moskovitz, N., et al. 2015. Searching for a differentiated asteroid family: A spectral survey of the Massalia, Merxia, and Agnia families. American Astronomical Society DPS meeting, 47, 308.13.Google Scholar
Vernazza, P., Birlan, M., Rossi, A., et al. 2006. Physical characterization of the Karin family. Astronomy & Astrophysics, 460, 945–951.CrossRefGoogle Scholar
Vernazza, P., Binzel, R. P., Thomas, C. A., et al. 2008. Compositional differences between meteorites and near-Earth asteroids. Nature, 454, 858–860.CrossRefGoogle ScholarPubMed
Warner, B. D., Harris, A. W., Vokrouhlický, D., et al. 2009. Analysis of the Hungaria asteroid population. Icarus, 204, 172–182.CrossRefGoogle Scholar
Warren, P. H. and Kallemeyn, G. W. 1995. Angrites: A volatile-rich variety of asteroidal basalt (except for alkalis and gallium!). Meteoritics, 30, 593.Google Scholar
Watters, T. R. and Prinz, M. 1979. Aubrites: Their origin and relationship to enstatite chondrites. Lunar and Planetary Science Conference, 10, 1073–1093.Google Scholar
Willman, M., Jedicke, R., Nesvorný, D., et al. 2008. Redetermination of the space weathering rate using spectra of Iannini asteroid family members. Icarus, 195, 663–673.CrossRefGoogle Scholar
Yamaguchi, A., Clayton, R. N., Mayeda, T. K., et al. 2002. A new source of basaltic meteorites inferred from Northwest Africa 011. Science, 296, 334–336.CrossRefGoogle ScholarPubMed
Yamaguchi, A., Barrat, J.-A., Ito, M., et al. 2011. Posteucritic magmatism on Vesta: Evidence from the petrology and thermal history of diogenites. Journal of Geophysical Research: Planets, 116, E08009.CrossRefGoogle Scholar
York, D. G., Adelman, J., Anderson, J. E., et al. 2000. The Sloan Digital Sky Survey: Technical summary. Astronomical Journal, 120, 1579–1587.CrossRefGoogle Scholar
Zappalà, V., Cellino, A., Farinella, P., et al. 1990. Asteroid families. I. Identification by hierarchial clustering and reliability assessment. Astronomical Journal, 100, 2030–2046.CrossRefGoogle Scholar
Zellner, B., Leake, M., Williams, J. G., et al. 1977. The E asteroids and the origin of enstatite achondrites. Geochimica et Cosmochimica Acta, 41, 1759–1767.CrossRefGoogle Scholar
Ziffer, J., Campins, H., Licandro, J., et al. 2011. Near-infrared spectroscopy of primitive asteroid families. Icarus, 213, 538–546.CrossRefGoogle Scholar

References

Ammannito, E., De Sanctis, M. C., Capaccioni, F., et al., 2013a. Vestan lithologies mapped by the visual and infrared spectrometer on Dawn. Meteoritics & Planetary Science, 48, 2185–2198.CrossRefGoogle Scholar
Ammannito, E., De Sanctis, M. C., Palomba, E., et al. 2013b. Olivine in an unexpected location on Vesta’s surface. Nature, 504, 122–125.CrossRefGoogle Scholar
Ammannito, E., De Sanctis, M. C., Combe, J. P., et al. 2015. The vestan Rheasilvia basin at high spatial and spectral resolution. Icarus, 259, 194–202.CrossRefGoogle Scholar
Beck, A. W. and McSween, H. Y. 2010. Diogenites as polymict breccias composed of orthopyroxenite and harzburgite. Meteoritics & Planetary Science, 45, 850–872.CrossRefGoogle Scholar
Beck, A. W., McCoy, T. J., Sunshine, J. M., et al., 2013. Challenges in detecting olivine on the surface of 4 Vesta. Meteoritics & Planetary Science, 48, 2155–2165.CrossRefGoogle Scholar
Beck, A. W., Lawrence, D. J., Peplowski, P. N., et al., 2015. Using HED meteorites to interpret neutron and gamma-ray data from asteroid 4 Vesta. Meteoritics & Planetary Science, 50, 1311–1337.CrossRefGoogle Scholar
Binzel, R. P. and Xu, S. 1993. Chips off asteroid 4 Vesta: Evidence for the parent body of basaltic achondrite meteorites. Science, 260, 186–191.CrossRefGoogle ScholarPubMed
Binzel, R. P., Gaffey, M. J., Thomas, P., et al., 1997. Geologic mapping of Vesta from 1994 Hubble Space Telescope images. Icarus, 128, 95–103.CrossRefGoogle Scholar
Buczkowski, D. L., Wyrick, D. Y., Iyer, K. A., et al., 2012. Large-scale troughs on Vesta: A signature of planetary tectonics. Geophysical Research Letters, 39, L18205.CrossRefGoogle Scholar
Buczkowski, D. L. , Wyrick, D. Y., Toplis, M., et al., 2014. The unique geomorphology and physical properties of the Vestalia Terra plateau. Icarus, 244, 89–103.CrossRefGoogle Scholar
Burbine, T. H., Meibom, A., and Binzel, R. P. 1996. Mantle material in the main belt: Battered to bits? Meteoritics & Planetary Science, 31, 607–620.CrossRefGoogle Scholar
Combe, J.-P., McCord, T. B., McFadden, L. A., et al., 2015. Composition of the northern regions of Vesta analyzed by the Dawn mission. Icarus, 259, 53–71.CrossRefGoogle Scholar
Consolmagno, G. J., Golabek, G. J., Turrini, D., et al., 2015. Is Vesta an intact and pristine protoplanet? Icarus, 254, 190–201.CrossRefGoogle Scholar
De Sanctis, M. C., Combe, J.-P., Ammannito, E., et al. 2012. Detection of widespread hydrated materials on Vesta by VIR imaging spectrometer on board the Dawn mission. Astrophysical Journal Letters, 758, L36.CrossRefGoogle Scholar
De Sanctis, M. C., Ammannito, E., Capria, M. T., et al. 2013. Vesta’s mineralogical composition as revealed by the visible and infrared spectrometer on Dawn. Meteoritics & Planetary Science, 48, 2166–2184.CrossRefGoogle Scholar
Denevi, B. W., Blewett, D. T., Buczkowski, D. L., et al. 2012. Pitted terrain on Vesta and implications for the presence of volatiles. Science, 338, 246–249.CrossRefGoogle ScholarPubMed
Ermakov, A. I., Zuber, M. T., Smith, D. E., et al. 2014. Constraints on Vesta’s interior structure using gravity and shape models from the Dawn mission. Icarus, 240, 146–160.CrossRefGoogle Scholar
Jaumann, R. J., Williams, D. A., Buczkowski, D. L., et al. 2012. Vesta’s shape and morphology. Science, 336, 687–690.CrossRefGoogle ScholarPubMed
Jutzi, M., Asphaug, E., Gillet, P., et al. 2013. The structure of asteroid 4 Vesta as revealed by models of planet-scale collisions. Nature, 494, 207–210.CrossRefGoogle ScholarPubMed
Konopliv, A. S., Asmar, S. W., Park, R. S. et al. 2014. The Vesta gravity field, spin pole and rotation period, landmark positions and ephemeris from the Dawn tracking and optical data. Icarus, 240, 103–117.CrossRefGoogle Scholar
Li, S. and Milliken, R. E. 2015. Quantitative mapping of minerals on Vesta using Dawn VIR data. Lunar and Planetary Science Conference, 46, 2179.Google Scholar
Lunning, N. G., McSween, H. Y., Tenner, T. J., et al. 2015. Insights into the mantle of asteroid 4 Vesta from mineral fragments in meteorite breccias. Earth and Planetary Science Letters, 418, 126–135.CrossRefGoogle Scholar
Macke, R. J., Britt, D. T., and Consolmagno, G. J. 2011. Density, porosity, and magnetic susceptibility of achondritic meteorites. Meteoritics & Planetary Science, 46, 311–326.CrossRefGoogle Scholar
Marchi, S., McSween, H. Y., O’Brien, D. P., et al. 2012. The violent collisional history of asteroid 4 Vesta. Science, 336, 690–694.CrossRefGoogle ScholarPubMed
Mandler, B. E. and Elkins-Tanton, L. T. 2013. The origin of eucrites, diogenites, and olivine diogenites: Magma ocean crystallization and shallow magma chamber processes on Vesta. Meteoritics & Planetary Science, 48, 2333–2349.CrossRefGoogle Scholar
Marzari, F., Farinella, P., and Davis, D. R. 1999. Origin, aging, and death of asteroid families. Icarus, 142, 63–77.CrossRefGoogle Scholar
McCord, T. B., Adams, J. B., and Johnson, T. V. 1970. Asteroid Vesta: Spectral reflectivity and compositional implications. Science, 168, 1445–1447.CrossRefGoogle ScholarPubMed
McCord, T. B., Li, J-Y., Combe, J-P., et al. 2012. Dark material on Vesta from the infall of carbonaceous volatile-rich material. Nature, 291, 83–86.CrossRefGoogle Scholar
McSween, H. Y., Mittlefehdlt, D. W., Beck, A. W., et al. 2011. HED meteorites and their relationship to the geology of Vesta. Space Science Reviews, 163, 141–174.CrossRefGoogle Scholar
McSween, H. Y. Jr., Binzel, R. P., De Sanctis, M. C., et al. 2013a. Dawn; the Vesta–HED connection; and the geologic context for eucrites, diogenites, and howardites. Meteoritics & Planetary Science, 48, 2090–2014.CrossRefGoogle Scholar
McSween, H. Y. Jr., Ammannito, E., Reddy, V., et al. 2013b. Composition of the Rheasilvia basin, a window into Vesta’s interior. Journal of Geophysical Research, 118, 335–346.CrossRefGoogle Scholar
Mizzon, H., Monnereau, M., Toplis, M., et al. 2015. A numerical model of the physical and chemical evolution of Vesta based on compaction equations and the olivine-anorthite-silica ternary diagram. Lunar and Planetary Science Conference, 46, 1832.Google Scholar
Neumann, W., Breuer, D., and Spohn, T. 2014. Differentiation of Vesta: Implications for a shallow magma ocean. Earth and Planetary Science Letters, 395, 267–280.CrossRefGoogle Scholar
Noguchi, T., Nakamura, T., Kimura, M., et al. 2011. Incipient space weathering observed on the surface of Itokawa dust particles. Science, 333, 1121–1125.CrossRefGoogle ScholarPubMed
O’Brien, D. P., Marchi, S., Morbidelli, A., et al. 2015. Constraining the cratering chronology of Vesta. Planetary and Space Science, 103, 131–142.CrossRefGoogle Scholar
Park, R. S., Konopliv, A. S., Asmar, S. W., et al. 2014. Gravity field expansion in ellipsoidal harmonic and polyhedral internal representations applied to Vesta. Icarus, 240, 118–132.CrossRefGoogle Scholar
Pieters, C. M., Ammannito, E., Blewett, D. P., et al. 2012. Distinctive space weathering on Vesta from regolith mixing processes. Nature, 491, 79–82.CrossRefGoogle ScholarPubMed
Prettyman, T. H., Mittlefehldt, D. W., Yamashita, N., et al. 2012. Elemental mapping by Dawn reveals exogenic H in Vesta’s regolith. Science, 338, 242–246.CrossRefGoogle Scholar
Prettyman, T. H., Mittlefehldt, D. W., Yamashita, N., et al. 2013. Neutron absorption constraints on the composition of 4 Vesta. Meteoritics & Planetary Science, 48, 2211–2236.CrossRefGoogle Scholar
Prettyman, T. H., Yamashita, N., Reedy, R. C., et al. 2015. Concentrations of potassium and thorium within Vesta’s regolith. Icarus, 259, 39–52.CrossRefGoogle Scholar
Preusker, F., Scholten, F., Matz, K.-D., et al. 2014. Global Shape of (4) Vesta from Dawn FC stereo images. Lunar and Planetary Science Conference, 45, 2027.Google Scholar
Reddy, V., Le Corre, L., and O’Brien, D. P., et al. 2012. Delivery of dark material to Vesta via carbonaceous chondritic impacts. Icarus, 221, 544–559.CrossRefGoogle Scholar
Righter, K. and Drake, M. J. 1997. A magma ocean on Vesta: Core formation and petrogenesis of eucrites and diogenites. Meteoritics & Planetary Science, 32, 929–944.CrossRefGoogle Scholar
Ruesch, O., Hiesinger, H., De Sanctis, M. C., et al. 2014. Detections and geologic context of local enrichments of olivine on Vesta with VIR/Dawn data. Journal of Geophysical Research, 119, 2078–2108.CrossRefGoogle Scholar
Russell, C. T. and Raymond, C. A. 2011. The Dawn mission to Vesta and Ceres. Space Science Reviews Special Issue on Dawn Mission, 163, 3–23.CrossRefGoogle Scholar
Russell, C. T., Raymond, C. A., Coradini, A., et al. 2012. Dawn at Vesta: Testing the protoplanetary paradigm. Science, 336, 684–686.CrossRefGoogle ScholarPubMed
Ruzicka, A., Snyder, G. A., and Taylor, L. A. 1997. Vesta as the howardite, eucrite and diogenite parent body: Implications for the size of a core and for large-scale differentiation. Meteoritics & Planetary Science, 32, 825–840.CrossRefGoogle Scholar
Sarafian, A. R., Roden, M.F., and Patino-Douce, A. E. 2013. The volatile content of Vesta: Clues from apatite in eucrites. Meteoritics & Planetary Science, 48, 2135–2154.CrossRefGoogle Scholar
Schenk, P., O’Brien, D. P., Marchi, S., et al. 2012. The geologically recent giant impact basins at Vesta’s south pole. Science, 336, 694–697.CrossRefGoogle ScholarPubMed
Schiller, M., Baker, J., Creech, J., et al. 2011. Rapid timescales for magma ocean crystallization on the howardite–eucrite–diogenite parent body. Astrophysical Journal Letters, 740, L22.CrossRefGoogle Scholar
Schmedemann, N., Kneissl, T., Ivanov, B. A., et al. 2015. The cratering record, chronology and surface ages of (4) Vesta in comparison to smaller asteroids and ages of HED meteorites. Planetary and Space Science, 103, 104–130.CrossRefGoogle Scholar
Scully, J.E.C., Russell, C.T., Yin, A., et al. 2015. Geomorphological evidence for transient water flow on Vesta. Earth and Planetary Science Letters, 411, 151–163.CrossRefGoogle Scholar
Srinivasan, G., Goswami, J. N., and Bhandari, N. 1999. 26Al in eucrite Piplia Kalan: Plausible heat source and formation chronology. Science, 284, 1348–1350.CrossRefGoogle ScholarPubMed
Thangjam, G., Reddy, V., Le Corre, L., et al. 2013. Lithologic mapping of HED terrains on Vesta using Dawn framing camera color data. Meteoritics & Planetary Science, 48, 2199–2210.CrossRefGoogle Scholar