
Energy-Limited Radiolytic Habitability in the Shallow Martian Subsurface: Implications for ExoMars Rosalind Franklin and Tianwen-3
<a href="https://news.google.com/rss/articles/CBMi-gFBVV95cUxOeEdSQTZZOVNjeFFER0hTdmRveEZIOEUyeXFJdm12blNtcWVvb19RX0k1V2docjBDQ3BMbE5TVVd2NUFGOGxWV28yX0xZUE10MV93VVVSOWk3MGxmYlNLcE41V2xjVTZMbHBnRGlCM09HcXVPN01hMGEzRWNtd0doOG43ek82YjZWb1hJQUZRUDRIZ1hITjdYaEN6NkJ3OTZhUzZ2dmIwMmp1MWpKZ19PcXFPRENRaXpsMmRJMUhqOFFKQW9KSWYtVUlQalhTREFBc1ZwWnZ3QjNTekJ2UTVtMlZWM1R0Zk1LcFpLTU9pejFwd1pBT1NGdnNR?oc=5" target="_blank">Energy-Limited Radiolytic Habitability in the Shallow Martian Subsurface: Implications for ExoMars Rosalind Franklin and Tianwen-3</a>&nbsp;&nbsp;<font color="#6f6f6f">Astrobiology Web</font>

