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2 - Exploring Vesta and Ceres

from Part I - Remote Observations and Exploration of Main Belt Asteroids

Published online by Cambridge University Press:  01 April 2022

Simone Marchi
Affiliation:
Southwest Research Institute, Boulder, Colorado
Carol A. Raymond
Affiliation:
California Institute of Technology
Christopher T. Russell
Affiliation:
University of California, Los Angeles
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Summary

In 1992, NASA’s planetary efforts were invigorated with the launch of the Discovery Program of principal investigator-led missions. Over the next eight years, a group of planetary scientists and engineers gathered regularly to design and propose to NASA solar-electric propulsion missions targeted to various scientifically important bodies. Ultimately, Dawn, a mission to orbit and explore both Vesta and Ceres, was selected for flight in 2001. It launched in 2007, arrived at Vesta in July 2011, and departed in September 2012 for Ceres. Arrival at Ceres occurred in March 2015, where Dawn operated productively until 31 October 2018, when it exhausted its attitude control propellant. Herein, we summarize the history of Dawn and recount the observations and discoveries made by this pioneering mission.

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Chapter
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Vesta and Ceres
Insights from the Dawn Mission for the Origin of the Solar System
, pp. 26 - 38
Publisher: Cambridge University Press
Print publication year: 2022

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References

A’Hearn, M. F., & Feldman, P. D. (1992) Water vaporization on Ceres. Icarus, 98, 5460.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, 5371.Google Scholar
DeSanctis, M. C., Ammannito, E., Capria, M. T., et al. (2012) Spectroscopic characterization of mineralogy and its diversity across Vesta. Science, 336, 697700.Google Scholar
DeSanctis, M. C., Ammannito, E., McSween, H. Y., et al. (2017) Localized aliphatic organic material on the surface of Ceres. Science, 355, 719722.Google Scholar
Hughson, K. H. G., Russell, C. T., Schmidt, B. E., et al. (2018) Normal faults on Ceres: Insights into the mechanical properties and thermal evolution of Nar Sulcus. Geophysical Research Letters, 46.Google Scholar
Jaumann, R., Williams, D. A., Buczkowski, D. L., et al. (2012) Vesta’s shape and morphology. Science, 336, 687690.Google Scholar
Küppers, M., O’Rourke, L., Bockelee-Morvan, D., et al. (2014) Localized sources of water vapour on the dwarf planet (1) Ceres. Nature, 505, 525527.CrossRefGoogle ScholarPubMed
Marchi, S., McSween, H. Y., O’Brien, D. P., et al. (2012) The violent collisional history of asteroid 4 Vesta. Science, 336, 690694.Google Scholar
McCord, T. B., Adams, J. B., & Johnson, T. V. (1970) Asteroid Vesta: Spectral reflectivity and compositional implications. Science, 168, 14451447.Google Scholar
Milliken, R. E., & Rivkin, A. S. (2009) Brucite and carbonate assemblages from altered olivine-rich materials on Ceres. Nature Geoscience, 2, 258261.CrossRefGoogle Scholar
Prettyman, T. H., Yamashita, N., Toplis, M. J., et al. (2017) Extensive water ice within Ceres’ aqueously altered regolith: Evidence from nuclear spectroscopy. Science, 355, 5558.Google Scholar
Rayman, M. D. (2003) The successful conclusion of the Deep Space 1 mission: Important results without a flashy title. Space Technology, 23, 185.Google Scholar
Rayman, M. D. (2019) Dawn at Ceres: The first exploration of the first dwarf planet discovered. Acta Astronautica, doi:10.1016/j.actaastro.2019.12.017.CrossRefGoogle Scholar
Rayman, M. D. (2020) Lessons from the Dawn mission to Ceres and Vesta. Acta Astronautica, 176, 233237.Google Scholar
Rayman, M. D., Fraschetti, T. C., Raymond, C. A., & Russell, C. T. (2007) Coupling of system resource margins through the use of electric propulsion: Implications in preparing for the Dawn mission to Ceres and Vesta. Acta Astronautica, 60, 930938.Google Scholar
Rayman, M. D., & Mase, R. A. (2014) Dawn’s exploration of Vesta. Acta Astronautica, 94, 159167.Google Scholar
Raymond, C. A., Jaumann, R., Nathues, A., et al. (2011) The Dawn topography investigation. Space Science Reviews, 163, 487510.Google Scholar
Rivkin, A. S., Li, J.-Y., Milliken, R. E., et al. (2011) The surface composition of Ceres. Space Science Reviews, 163, 95116.Google Scholar
Rivkin, A. S., & Volquardsen, E. L. (2010) Rotationally-resolved spectra of Ceres in the 3 micron region. Icarus, 206, 327333.CrossRefGoogle Scholar
Ruesch, O., Platz, T., Schenk, P., et al. (2016) Cryovolcanism on Ceres. Science, 353, aaf4286.Google Scholar
Russell, C. T., Coradini, A., Christensen, U., et al. (2004) Dawn: A journey in space and time. Planetary and Space Science, 52, 465489.Google Scholar
Russell, C. T., Coradini, A., Feldman, W. C., et al. (2002) Dawn: A journey to the beginning of the Solar System. Proceedings of Asteroids, Comets, Meteors, July 29–August 2, Technical University Berlin, Berlin, Germany, (ESA-SP-500), pp. 63–66.Google Scholar
Russell, C. T., Raymond, C. A., Ammannito, E., et al. (2016) Dawn arrives at Ceres: Exploration of a small, volatile-rich world. Science, 353, 10081010.Google Scholar
Russell, C. T., Raymond, C. A. Coradini, A., et al. (2012) Dawn at Vesta: Testing the protoplanetary paradigm. Science, 336, 684.Google 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.Google Scholar
Thomas, P. C., Binzel, R. P., Gaffey, M. J., et al. (1997) Impact excavation on asteroid 4 Vesta: Hubble Space Telescope results. Science, 272, 14921495.Google Scholar
Villarreal, M. N., Russell, C. T., Luhmann, J. G., et al. (2017) The dependence of the cerean exosphere on solar energetic particle events. Astrophysical Journal, 838, L8.Google Scholar

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