Vulcan's Forge by Luca
Giordano (1632-1705)
In 1998, a respected astronomer and physicist turned geologist, Thomas Gold, wrote a highly influential book, The Deep Hot Biosphere, in which he argued that there is abundant microbial life in the water within the pores, cracks and fissures of the rocks beneath our feet. Furthermore, Gold advanced the provocative notion that hydrocarbons within the Earth were not derived from fossils but rather were created early in the life of the planet by chemical and physical processes below the crust, including radiation. (His 1992 paper summarizing some of these ideas is available.) Taken together, these views suggest that there exists an immense and hospitable underground environment for microbes, complete with liquid water, an energy source (hydrocarbons and hydrogen), and livable temperatures (down to about 10 Km at which point it becomes too hot for even the most extreme of thermophiles). Gold postulated that not only is there life in the neighborhood of Vulcan’s furnace, but that there might be as much biomass there as on land and sea combined. Not only would this life not need the sun as an energy source, but unlike the communities thriving around the deep sea vents, it could be independent of all photosynthetically produced products (e.g., oxygen), as well.
But how would one go about studying the deep hot biosphere?