Temperature: Due to the low density of particles in the exosphere, the temperature can vary widely. In sunlight, the exosphere can reach very high temperatures, while in the shadow of the Earth it can become extremely cold.
Transition to Space: The exosphere gradually transitions into outer space, where the Earth'sgravitational pull becomes weaker and weaker until it can no longer contain the atmospheric gases.
Low Density: The exosphere has an extremely low density, with very few particles per unit volume. This makes it very different from the denser layers of the atmosphere below it.
Interaction with SolarWind: The exosphere interacts with the solarwind, a stream of charged particles emitted by the Sun. This interaction plays a role in processes such as the auroras and the erosion of the Moon'ssurface.
Study Guide for the Exosphere:
To understand the exosphere better, consider the following questions: