### Formation of Martian Gullies
Martian gullies are geologically young, sharp-edged channel systems found on steep slopes on Mars. Scientists debate the mechanism responsible for carving these features.
Scientist 1
Martian gullies are formed by the flow of liquid water. Although the Martian surface is cold and has low atmospheric pressure, subsurface liquid water can be released to the surface during warm seasons. When liquid water contains dissolved salts, it forms a brine that has a significantly lower freezing point and a slower evaporation rate than pure water. This allows the salty liquid water to remain stable on the surface long enough to flow downslope, carving the alcoves, channels, and depositional aprons characteristic of water-carved gullies on Earth.
Scientist 2
Martian gullies are formed by dry mass-wasting processes triggered by the seasonal sublimation of carbon dioxide () frost. Under current Martian atmospheric conditions, liquid water is highly unstable and would rapidly freeze or evaporate, preventing it from flowing in quantities sufficient to carve gullies. Instead, winter temperatures allow frost to condense in gully alcoves. In spring, solar heating causes the bottom of the frost layer to sublimate directly into gas. The pressure of this escaping gas fluidizes the overlying dry sand and dust, causing it to flow downslope and erode the gullies without liquid water.
Based on the passage, Scientist 2's explanation of gully formation relies on which of the following assumptions?
- ALiquid water is stable on the Martian surface under current temperature and atmospheric conditions.
- The sublimation of frost can generate sufficient gas pressure to fluidize and transport dry sediments downslope.Answer
- CMartian subsurface water contains a high concentration of dissolved salts that lowers its freezing point.
- Dfrost accumulation only occurs in regions of Mars that have localized high-pressure atmospheric conditions.