Evolution of the early Earth

There are two possible -- and possibly contradictory -- implications of the faint early Sun paradox and the relevant geologic evidence.

Kasting (1993)

Jim Kasting (Penn State) has proposed that the early Earth (and also the early Mars) had thick atmospheres of CO2 (several hundred times as much atmospheric CO2 as we have now). This allows greenhouse warming of the planet -- we will talk about the greenhouse effect shortly. What effect does having a thick atmosphere of CO2 have on the origin of life? And how does this play into the carbon cycle on the early Earth compared to today?

Note that Chyba et al. also found that a thick (CO2) atmosphere is needed to deliver organic molecules to the early Earth.

We also know from geological evidence that atmospheric oxygen suddenly became very important around 2 billion years ago (we'll talk about that shortly). So two questions are these: What happened to the atmospheric CO2, and where did all this atmospheric oxygen (O2) come from?

Back Next

Back to Lecture 16 outline

Back to lectures page

Back to main course page