“…However, carbonaceous dust ablating in the atmosphere of a terrestrial planet could be expected to experience a range of atmospheric compositions, from the current oxygen-nitrogen atmosphere of Earth to its previous oxygen-poor atmosphere, before the accumulation of oxygen around 2.4 Ga, or the carbon dioxide-rich martian atmosphere. Pyrolysis in the presence of reactive fluids is known to alter the nature of the pyrolysis products, as shown by hydrous pyrolysis and hydropyrolysis, in the presence of water and hydrogen, respectively (Sephton et al, 1999;Sephton et al, 2005), and by pyrolysis and gasification in steam and carbon dioxide (e.g., Messenbock et al, 1999;Jamil et al, 2004). The helium atmosphere used here is difficult to relate to the current oxygen-rich atmosphere of Earth, or its previous carbon dioxide-rich atmosphere.…”