Ammonia as a Detectable Biosignature on Cold Haber World Exoplanets Around M-Dwarfs
To the point
Sukrit Ranjan and colleagues show that on hydrogen-rich exoplanets around small, cool red dwarfs biology could build up ammonia to detectable levels despite atmospheric sinks, enabling JWST to detect ammonia in about two transits over two months and broadening the search for life beyond oxygen.
Comulytic Note Pro AI Voice Recorder, Unlimited Transcribe & Summarize
The invisible college
Jacques Vallee
The Extraterrestrial Species Almanac: The Ultimate Guide to Greys, Reptilians, Hybrids, and Nordics (MUFON)
Craig Campobasso
Exploring the Cosmos with James Webb
Steeven Cadel
Our recommendations from Amazon
