### Models of the Early Martian Atmosphere
Two models were proposed to explain the presence of liquid water features on early Mars, despite the young Sun being 30% fainter than it is today.
Model 1 (Warm and Wet Greenhouse Model)
Early Mars possessed a thick, stable atmosphere composed primarily of and gas, with a surface pressure of . This thick greenhouse gas envelope was maintained by continuous, global volcanic outgassing. The high surface pressure and potent greenhouse effect raised the average surface temperature above (), allowing for long-term liquid water oceans and a persistent hydrologic cycle. This model assumes that Mars’s magnetic field was strong enough to protect the thick atmosphere from solar wind stripping during its first 500 million years.
Model 2 (Cold and Icy Impact Model)
Early Mars had a thin, dry atmosphere with a surface pressure of less than . The average surface temperature was well below , and the surface water was frozen as planet-wide ice sheets. Large meteoroid impacts, which occurred frequently during the Late Heavy Bombardment, delivered transient heat and vast quantities of water vapor. Each major impact event vaporized local ice sheets and injected and into the atmosphere, creating a temporary, warm greenhouse effect. Surface temperatures rose above for periods of only tens to hundreds of years, causing localized, rapid melting and catastrophic flash floods that carved the valley networks before the atmosphere cooled and froze again.
According to the descriptions of the two models, which of the following statements best contrasts the atmospheric pressures and surface temperature dynamics required by Model 1 and Model 2 to explain the presence of liquid water features on early Mars?
- Model 1 requires a stable surface pressure of with a constant surface temperature above , whereas Model 2 requires a thin atmosphere where surface temperatures only rise above in short, transient intervals.Answer
- BModel 1 requires a thin atmosphere where surface temperatures only rise above in short, transient intervals, whereas Model 2 requires a stable surface pressure of with a constant surface temperature above .
- CBoth models require a stable surface pressure of with surface temperatures constantly maintained above , but Model 1 attributes this to meteoroid impacts and Model 2 to volcanic outgassing.
- DBoth models require a thin atmosphere with surface temperatures below , but Model 1 attributes liquid water features to continuous volcanic outgassing and Model 2 to stable solar radiation.