How is the weather on land formed?

As we know, Venus and Mars have weather. Venus lacks seasonal variation because its axis is hardly tilted: it is hot at all times. 95% of the atmosphere is carbon dioxide, which heats the surface of Venus through the greenhouse effect, with an average temperature of 885 degrees Fahrenheit (457 degrees Celsius).

The surface pressure of Venus is 90 standard atmospheric pressure (9 1, 192 mbar), while the surface pressure of the earth is 1 standard atmospheric pressure (10 13 mbar), and the violent easterly wind is traveling at a speed of 200 miles (322 kilometers) per hour. Light poured out through the thick sulfuric acid cloud, making Venus shine in the night sky.

The atmosphere of Mars contains 95% carbon dioxide, but its gravity is relatively small. Most of its original gas has been blown away by the solar wind. The average pressure on the surface of Mars is 0008 standard atmospheric pressure (8 mbar). Low air pressure, coupled with extreme dryness, prevented the formation and accumulation of water. This means that there are almost no clouds on Mars, and the thin atmosphere makes Mars very sensitive to the heat of the sun: for example, the temperature at the equator varies from-193 F to+72 F (-125 C to+22 C) all year round. Ice covers the poles of Mars. Their melting and freezing are affected by the distance between Mars and the sun, and also by the wind with a speed of 125 miles (200 kilometers) per hour. It produces powerful dust clouds, blocks sunlight and slows down the melting of ice. These dust storms often attack the whole star.