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Atmospheric pressure is an important factor in keeping liquid water on the surface of a planet. With no atmosphere, liquid water would quickly escape into space. It would depend on various factors such as the temperature and escape velocity of the planet of course. Scientists think liquid water existed on Mars in the past when the atmosphere was a lot denser. Water does exist on the surface Mars, but only as ice.
As Mars has cooled, its core has solidified and its geodynamo stopped. The loss of Mars' magnetic field allowed more solar energy to reach the surface. That solar radiation heat dissipated the surface water and atmosphere. Also, because Mars' gravitational field is not as strong as earth's, it was much easier for atoms and molecules at the top of the atmosphere to escape to space. Over millions of years this process led to the loss of most of Mars' atmosphere.
the moon does not have liquid
Rain? precipitation
The hydrosphere is the body of liquid water on the earth, and the atmosphere is the body of gas around the earth.
The continuous movement of water molecules can lead some molecules at the surface to escape in the atmosphere as a gas.
Some molecules from the surface of the liquid gain more energy and are able to escape in the atmosphere.
Evaporation is caused by the continuous Brownian movement of water molecules; several molecules gain sufficient energy to escape in the atmosphere.
When water molecules at the surface gain sufficient energy they can escape in the atmosphere.The energy of water molecules increase by a temperature increase and some molecules at the surface can escape in the atmosphere.
Evaporation is the process of water molecules in liquid water escape into the air as water vapor.
The hydrogen bonds between the water molecules in the liquid are broken.
it becomes easier for the molecules to escape
Atmospheric pressure is an important factor in keeping liquid water on the surface of a planet. With no atmosphere, liquid water would quickly escape into space. It would depend on various factors such as the temperature and escape velocity of the planet of course. Scientists think liquid water existed on Mars in the past when the atmosphere was a lot denser. Water does exist on the surface Mars, but only as ice.
When water molecules at the liquid surface gain sufficient energy they can escape in the atmosphere. Evaporation (not vaporization) occur at any temperature; a higher temperature increase the rate of evaporation.
At higher temperatures waer molecules at the surface of the liquid have more energy and is more simple to escape into atmosphere.
Reducing the air pressure allows the molecules to escape
evaporation