Abstract Veins containing carbonates, hydrous silicates, and sulfates that occur within and between grains of augite and olivine in the Nakhla meteorite are good evidence for the former presence of liquid water in the Martian crust. Aqueous solutions gained access to grain interiors via narrow fract...
Highlights, strengths & weaknesses, commercial applications, and societal impact — written for this paper on demand.
No comments yet
Be the first to share your thoughts!