Spectral properties and geology of bright and dark material on dwarf planet Ceres

G. Thangjam, A. Nathues, T. Platz, M. Hoffmann, E. A. Cloutis, K. Mengel, Matthew Richar Izawa, D. M. Applin

Research output: Contribution to journalArticle

3 Citations (Scopus)

Abstract

Variations and spatial distributions of bright and dark material on dwarf planet Ceres play a key role in understanding the processes that have led to its present surface composition. We define limits for “bright” and “dark” material in order to distinguish them consistently, based on the reflectance of the average surface using Dawn Framing Camera data. A systematic classification of four types of bright material is presented based on their spectral properties, composition, spatial distribution, and association with specific geomorphological features. We found obvious correlations of reflectance with spectral shape (slopes) and age; however, this is not unique throughout the bright spots. Although impact features show generally more extreme reflectance variations, several areas can only be understood in terms of inhomogeneous distribution of composition as inferred from Dawn Visible and Infrared Spectrometer data. Additional material with anomalous composition and spectral properties are rare. The identification of the composition and origin of the dark, particularly the darkest material, remains to be explored. The spectral properties and the morphology of the dark sites suggest an endogenic origin, but it is not clear whether they are more or less primitive surficial exposures or excavated subsurface but localized material. The reflectance, spectral properties, inferred composition, and geologic context collectively suggest that the bright and dark material tends to gradually change toward the average surface over time. This could be because of multiple processes, i.e., impact gardening/space weathering, and lateral mixing, including thermal and aqueous alteration, accompanied by changes in composition and physical properties such as grain size, surface temperature, and porosity (compaction).

Original languageEnglish
Pages (from-to)1961-1982
Number of pages22
JournalMeteoritics and Planetary Science
Volume53
Issue number9
DOIs
Publication statusPublished - Sep 1 2018

Fingerprint

dwarf planets
geology
planet
reflectance
spatial distribution
space weathering
framing cameras
geomorphological feature
spectral reflectance
infrared spectrometers
material
surface temperature
compaction
spectrometer
grain size
weathering
physical property
physical properties
porosity
spectrometers

ASJC Scopus subject areas

  • Geophysics
  • Space and Planetary Science

Cite this

Thangjam, G., Nathues, A., Platz, T., Hoffmann, M., Cloutis, E. A., Mengel, K., ... Applin, D. M. (2018). Spectral properties and geology of bright and dark material on dwarf planet Ceres. Meteoritics and Planetary Science, 53(9), 1961-1982. https://doi.org/10.1111/maps.13044

Spectral properties and geology of bright and dark material on dwarf planet Ceres. / Thangjam, G.; Nathues, A.; Platz, T.; Hoffmann, M.; Cloutis, E. A.; Mengel, K.; Richar Izawa, Matthew; Applin, D. M.

In: Meteoritics and Planetary Science, Vol. 53, No. 9, 01.09.2018, p. 1961-1982.

Research output: Contribution to journalArticle

Thangjam, G, Nathues, A, Platz, T, Hoffmann, M, Cloutis, EA, Mengel, K, Richar Izawa, M & Applin, DM 2018, 'Spectral properties and geology of bright and dark material on dwarf planet Ceres', Meteoritics and Planetary Science, vol. 53, no. 9, pp. 1961-1982. https://doi.org/10.1111/maps.13044
Thangjam G, Nathues A, Platz T, Hoffmann M, Cloutis EA, Mengel K et al. Spectral properties and geology of bright and dark material on dwarf planet Ceres. Meteoritics and Planetary Science. 2018 Sep 1;53(9):1961-1982. https://doi.org/10.1111/maps.13044
Thangjam, G. ; Nathues, A. ; Platz, T. ; Hoffmann, M. ; Cloutis, E. A. ; Mengel, K. ; Richar Izawa, Matthew ; Applin, D. M. / Spectral properties and geology of bright and dark material on dwarf planet Ceres. In: Meteoritics and Planetary Science. 2018 ; Vol. 53, No. 9. pp. 1961-1982.
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