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Testing the waters: Analyzing different solid states of water on other planets and moons


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IMAGE: Dissociation pressures of various clathrate hydrates across a range of cryogenic temperatures. The upper regions of each curve indicate stable boundaries of the clathrate hydrates. (Similar colors have been used.
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Credit: 2021 Hideki Tanaka, Okayama Univ.
Just like on Earth, water on other planets, satellites, and even comets comes in a variety of forms depending on multiple factors such as pressure and temperature. Aside from the gaseous, liquid, and solid states we are accustomed to, water can form a different type of crystalline solid called clathrate hydrate. Although they look similar to ice, clathrate hydrates have actually small water-based cages in which smaller molecules are trapped. These trapped guest molecules are essential for preserving the crystalline structure of clathrate hydrates, which would otherwise collapse into regular ice or water. ....

Hideki Tanaka , Okayama University , Planetary Science Journal , Professor Hideki Tanaka , Atomic Molecular Particle Physics , Space Planetary Science , Molecular Physics , ஹைடீகீ தனகா , ஒக்யமா பல்கலைக்கழகம் , கிரகங்கள் அறிவியல் இதழ் , ப்ரொஃபெஸர் ஹைடீகீ தனகா , அணு மூலக்கூறு துகள் இயற்பியல் , இடம் கிரகங்கள் அறிவியல் , மூலக்கூறு இயற்பியல் ,