Organic Matter and Associated Minerals on the Dwarf Planet Ceres

• Published in: Minerals (Basel) Vol. 11; no. 8; p. 799
• Main Authors: De Sanctis, Maria Cristina, Ammannito, Eleonora
• Format: Journal Article
• Language: English
• Published: Basel MDPI AG 01.08.2021
• Subjects: aliphatics; Amino acids; Ammonia; Ammonium; Ammonium compounds; Asteroids; Astrobiology; Carbon; Carbon content; Carbonates; Ceres; Ceres asteroid; Coexistence; Dwarf planets; Hydrothermal alteration; Inner solar system; Laboratories; Magnetite; Meteors & meteorites; Mineralogy; Minerals; Organic matter; organics; Salts; Solar system; Water
• ISSN: 2075-163X; 2075-163X
• DOI: 10.3390/min11080799

Ceres is the largest object in the main belt and it is also the most water-rich body in the inner solar system besides the Earth. The discoveries made by the Dawn Mission revealed that the composition of Ceres includes organic material, with a component of carbon globally present and also a high quantity of localized aliphatic organics in specific areas. The inferred mineralogy of Ceres indicates the long-term activity of a large body of liquid water that produced the alteration minerals discovered on its surface, including ammonia-bearing minerals. To explain the presence of ammonium in the phyllosilicates, Ceres must have accreted organic matter, ammonia, water and carbon present in the protoplanetary formation region. It is conceivable that Ceres may have also processed and transformed its own original organic matter that could have been modified by the pervasive hydrothermal alteration. The coexistence of phyllosilicates, magnetite, carbonates, salts, organics and a high carbon content point to rock–water alteration playing an important role in promoting widespread carbon occurrence.