The article makes this sound related to atmospheric CO2, so not 'carbon' as I had initially hoped from the headline -- carbon like coal, ie, from life.
But atmospheric CO2 and a water cycle may match Earth-like conditions for life?
I did not see a date in the article, ie, how many million years ago this carbon layer was formed.
In the next few hundred millions years after a planet has cooled enough to be covered by liquid water, the water becomes gradually neutralized by leaching mainly potassium, magnesium, sodium and calcium ions from the igneous rocks (smaller amounts of iron(II), manganese(II) and other ions are also leached).
The chemical elements that are required for the appearance of life are ubiquitous.
What is much rarer is to have a planet of the right size, orbiting around a stable star at the right distance and having an adequate source of internal heat that can provide indirectly the source of chemical energy for the first living beings, and also the occurrence at the right place of certain minerals such as Fe-Co-Ni sulfides, that can catalyze the formation of complex organic molecules, before their role is taken by organic enzymes.
https://en.wikipedia.org/wiki/Chemical_formula
https://en.wikipedia.org/wiki/Simplified_Molecular_Input_Lin...
The Simplified Molecular Input Line Entry System (SMILES) is a specification in the form of a line notation for describing the structure of chemical species using short ASCII strings. SMILES strings can be imported by most molecule editors for conversion back into two-dimensional drawings or three-dimensional models of the molecules.
Double, triple, and quadruple bonds are represented by the symbols =, #, and $ respectively as illustrated by the SMILES O=C=O (carbon dioxide...)
These are some of the most abundant substances in the entire Universe. On any medium-size planet without life, the atmosphere is expected to be composed mostly of CO2, together with a smaller amount of dinitrogen, like it is today on Venus. Also the rarefied atmosphere of Mars contains mostly CO2.
Because most rocks containing carbonates and sulfates are formed by precipitation from water, this discovery is just additional evidence that in the past Mars had much more water than today, so that there was some water lake or sea where these rocks are located now.
The atmosphere of the early Earth must have been composed mostly of CO2 too, before algae have appeared and they have reduced most of the CO2 to organic compounds, leaving an atmosphere where N2 is the most abundant component.