Transition metal abundance as a key parameter for the search of Life in the Universe
The search for Life in the Universe generally assumes three basic life's needs: I) building block elements (i.e., CHNOPS), II) a solvent to life's reactions (generally, liquid water) and III) a thermodynamic disequilibrium. It is assumed that similar requirements might be universal in the...
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| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Maynooth Academic Publishing
2025-08-01
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| Series: | The Open Journal of Astrophysics |
| Online Access: | https://doi.org/10.33232/001c.143246 |
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