The discussion centers on the feasibility of a carbon planet forming in the solar system, particularly questioning if Venus could have been one while maintaining the current structure of the solar system. It is argued that for Venus to be a carbon planet, it would require an unusual distribution of carbon and oxygen, which is not supported by current observations. The composition of Venus is similar to Earth, with a high CO2 atmosphere but a crust lacking in carbon due to the absence of oceans. The conversation also touches on the potential for carbon planets in other stellar systems, particularly those formed in carbon-rich molecular clouds, suggesting that while unusual, such planets could exist elsewhere. Overall, the consensus is that Venus is unlikely to be a carbon planet based on available evidence.