Image Details

Choose export citation format:

New Insights into Venus’s Volatile Cycles Revealed by the Formation of Magnesite and Fluoro–Micas

  • Authors: Sara Taeko Port, Maitrayee Bose, Jean-Philippe Harvey, Dorothy Lukco, Tibor Kremic, Gary Hunter

Sara Taeko Port et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 1.

All minerals before and after exposure to simulated Venusian conditions in the GEER for 60 days. The image was acquired by the on-site NASA GRC photographer using a NIKON camera. Most minerals became visibly darker after exposure, except calcite and magnesite. (A) Calcite: CaCO3; (B) Magnesite: MgCO3; (C) Siderite: FeCO3; (D) Phlogopite: KMg3AlSi3O10(F,OH)2; (E) Muscovite: KAl2(AlSi3O10)(F,OH)2; (F) Brucite: Mg(OH)2.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse