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The atmosphere of the planet Mars is \(95.3 \%\) carbon dioxide \(\left(\mathrm{CO}_{2}\right)\) and about \(0.03 \%\) water vapor. The atmospheric pressure is only about \(600 \mathrm{~Pa}\), and the surface temperature varies from \(-30^{\circ} \mathrm{C}\) to \(-100^{\circ} \mathrm{C}\). The polar ice caps contain both \(\mathrm{CO}_{2}\) ice and water ice. Could there be liquid \(\mathrm{CO}_{2}\) on the surface of Mars? Could there be liquid water? Why or why not?

Short Answer

Expert verified
No, neither liquid CO2 nor liquid water can exist on Mars due to low pressure.

Step by step solution

01

Understand the Conditions on Mars

To determine if liquid CO2 or water could exist on Mars, note that the atmospheric pressure is 600 Pa, and the temperature ranges from -30°C to -100°C.
02

Check CO2 Phase Diagram

Under normal circumstances, CO2 sublimates directly from a solid to a gas at 1 atm (101325 Pa) at -78°C. At 600 Pa, the pressure is too low to have liquid CO2 at any temperature.
03

Check Water Phase Diagram

For water, the triple point is 0.01°C at 611.657 Pa. Below this pressure, water cannot exist as a liquid, so at 600 Pa and below 0°C, water can only exist as ice or vapor.
04

Analyze Mars Conditions

Given Mars’ pressures and temperature range, neither liquid CO2 nor liquid water can exist because conditions fall outside the necessary pressure and temperature ranges for their liquid states.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

CO2 Phase Diagram
The CO2 phase diagram describes how carbon dioxide exists in different phases (solid, liquid, gas) under varying temperatures and pressures. On Earth, at standard atmospheric pressure (1 atm or 101325 Pa), CO2 transitions directly from a solid state to a gaseous state at temperatures above -78°C through a process called sublimation. This means there is no liquid state under these conditions.

On Mars, the atmospheric pressure is only 600 Pa, significantly lower than Earth's standard pressure. Under Mars' conditions, CO2 sublimates directly from a solid (dry ice) to a gas without forming a liquid. This is because the pressure on Mars is below the triple point of CO2, indicating that liquid CO2 cannot exist on the Martian surface. Consequently, while CO2 ice and vapor may be present, the phase diagram confirms that liquid CO2 is not possible under Martian conditions.
Water Phase Diagram
The water phase diagram helps us understand how water can exist as ice, liquid, or vapor depending on temperature and pressure. On Earth, water transitions between these states at specific pressures and temperatures; the most familiar transition being from ice to liquid at 0°C under 101325 Pa (1 atm).

However, on Mars, with a much lower atmospheric pressure of 600 Pa, conditions are below the triple point of water. The triple point marks the specific condition (0.01°C, 611.657 Pa) where water can coexist in all three states. Since Mars' typical conditions do not allow for pressures above the triple point, liquid water cannot naturally occur. Thus, on Mars, water is present either as vapor or as ice due to the exceedingly low pressures.
Mars Atmospheric Conditions
Mars has an extremely thin atmosphere, composed mostly of carbon dioxide (95.3%) and traces of water vapor (0.03%). The atmospheric pressure is about 600 Pa, which is much lower than Earth's atmospheric pressure. This low pressure profoundly affects the phase states of materials, like CO2 and water, found on Mars.

The surface temperature on Mars varies greatly, ranging from -30°C to -100°C. These temperatures and the low atmospheric pressure mean that neither CO2 nor water can exist in their liquid states. Both substances bypass the liquid state under these Martian conditions, remaining as solids or gases (for CO2) and as vapors or ice (for water). Consequently, Mars is an environment with extreme conditions that limit the existence of liquids on its surface.
Triple Point of Water
The triple point of water is a fundamental concept in understanding the states of water under varying conditions. It refers to the exact temperature and pressure where water can exist simultaneously as a solid, liquid, and gas. This occurs at a temperature of 0.01°C and a pressure of 611.657 Pa.

The triple point is critical in scientific experiments and calibrations because it represents a stable point where all three phases coexist in equilibrium. In the context of Mars, the atmospheric pressure of 600 Pa falls just below this essential point.
  • Below this pressure, water cannot maintain a liquid state.
  • On Mars, this means that water can only exist as ice or vapor, never as a liquid due to its atmospheric conditions.
  • Understanding the triple point of water helps in determining the possible state of water under diverse extraterrestrial conditions.
Thus, on Mars, the triple point highlights the limitations posed by its unique pressures in sustaining liquid water.

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Most popular questions from this chapter

Initially at a temperature of \(80.0^{\circ} \mathrm{C}, 0.28 \mathrm{~m}^{3}\) of air expands at a constant gauge pressure of \(1.38 \times 10^{5} \mathrm{~Pa}\) to a volume of \(1.42 \mathrm{~m}^{3}\) and then expands further adiabatically to a final volume of \(2.27 \mathrm{~m}^{3}\) and a final gauge pressure of \(2.29 \times 10^{4} \mathrm{~Pa}\). Draw a \(p V\) diagram for this sequence of processes, and compute the total work done by the air. \(C_{Y}\) for air is \(20.8 \mathrm{~J} /(\mathrm{mol} \cdot \mathrm{K})\).

Three moles of an ideal gas are in a rigid cubical box with sides of length \(0.200 \mathrm{~m}\). (a) What is the force that the gas exerts on each of the six sides of the box when the gas temperature is \(20.0^{\circ} \mathrm{C} ?\) (b) What is the force when the temperature of the gas is increased to \(100.0^{\circ} \mathrm{C} ?\)

Calculate the volume of \(1.00 \mathrm{~mol}\) of liquid water at a temperature of \(20^{\circ} \mathrm{C}\) (at which its density is \(998 \mathrm{~kg} / \mathrm{m}^{3}\) ), and compare this volume with the volume occupied by \(1.00 \mathrm{~mol}\) of steam at \(200^{\circ} \mathrm{C}\). Assume the steam is at atmospheric pressure and can be treated as an ideal gas.

A diver observes a bubble of air rising from the bottom of a lake (where the absolute pressure is 3.50 atm) to the surface (where the pressure is \(1.00 \mathrm{~atm}\) ). The temperature at the bottom is \(4.0^{\circ} \mathrm{C}\) and the temperature at the surface is \(23.0^{\circ} \mathrm{C}\). (a) What is the ratio of the volume of the bubble as it reaches the surface to its volume at the bottom? (b) Would it be safe for the diver to hold his breath while ascending from the bottom of the lake to the surface? Why or why not?

The conditions of standard temperature and pressure (STP) are a temperature of \(0.00^{\circ} \mathrm{C}\) and a pressure of 1.00 atm. (a) How many liters does 1.00 mol of any ideal gas occupy at STP? (b) For a scientist on Venus, an absolute pressure of 1 Venusian-atmosphere is 92 earth-atmospheres. Of course she would use the Venusianatmosphere to define STP. Assuming she kept the same temperature, how many liters would 1 mole of ideal gas occupy on Venus?

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