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Brucite and carbonate assemblages from altered olivine-rich materials on Ceres

Nature Geoscience volume 2, pages 258–261 (2009)Cite this article

Abstract

The dwarf planet Ceres is the largest object in the asteroid belt, and is generally thought to be a differentiated body composed primarily of silicate materials and water ice1,2. Some remotely observed features, however, indicate that Ceres may instead have a composition more similar to that of the most common types of carbonaceous meteorite3,4,5,6,7. In particular, Ceres has been shown to have a distinct infrared absorption feature centred at a wavelength of ∼3.06 μm that is superimposed on a broader absorption from ∼2.8 to 3.7 μm (refs 5, 8), which suggests the presence of OH- or H2O-bearing phases. The specific mineral composition of Ceres and its relationship to known meteorite mineral assemblages, however, remains uncertain. Here we show that the spectral features of Ceres can be attributed to the presence of the hydroxide brucite, magnesium carbonates and serpentines, a mineralogy consistent with the aqueous alteration of olivine-rich materials. We therefore suggest that the thermal and aqueous alteration history of Ceres is different from that recorded by carbonaceous meteorites, and that samples from Ceres are not represented in existing meteorite collections.

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Figure 1: Linear mixing model results for the near-infrared reflectance spectrum of Ceres.
Figure 2: Linear mixing model results for the mid-infrared reflectance spectrum of Ceres.
Figure 3: Reflectance spectra of representative C1 and C2 carbonaceous chondrites.

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Acknowledgements

This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA. We also acknowledge support from RELAB at Brown University, the NASA Planetary Astronomy Program and the Infrared Telescope Facility, which is operated by the University of Hawaii under Cooperative Agreement no. NCC 5-538 with the NASA Planetary Astronomy Program.

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Authors and Affiliations

  1. Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, California 91109, USA

    Ralph E. Milliken

  2. Applied Physics Lab, Johns Hopkins University, 11100 Johns Hopkins Rd, Laurel, Maryland 20723, USA

    Andrew S. Rivkin

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  1. Ralph E. Milliken
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  2. Andrew S. Rivkin
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Contributions

R.E.M. was responsible for writing most of the text and the spectral modelling. A.S.R. contributed to the text, acquired and provided the near-infrared spectrum of Ceres and assisted with interpretation of the results.

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Correspondence to Ralph E. Milliken.

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Milliken, R., Rivkin, A. Brucite and carbonate assemblages from altered olivine-rich materials on Ceres. Nature Geosci 2, 258–261 (2009). https://doi.org/10.1038/ngeo478

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