The Earth's atmosphere, this essential gaseous layer surrounding the planet, is structured into five distinct zones: the troposphere, stratosphere, mesosphere, thermosphere, and exosphere. These layers work together to maintain the planet's thermal balance, protect against meteorite impacts, and filter ultraviolet radiation. The primary distinction between them lies in the variation of altitude and temperature, which follows a pattern of decrease, increase, decrease, and new increase across the layers, with each playing vital roles for existence.
The troposphere constitutes the layer closest to the surface, where life develops. Its thickness varies according to latitude and season, situated between 0 and 12-18 km. It houses approximately 80% of the total atmospheric mass and almost all the water vapor. Climatic phenomena, such as storms, winds, and rain, occur in this region due to convection and water vapor. It is also the flight path for helicopters and the point of flight for most commercial aircraft, although temperatures can drop to -60°C at higher altitudes.
Above the troposphere, starting around 8 km and reaching about 18 km, is the stratosphere. Its most notable function is the presence of the ozone layer, located between 15 and 35 km, which absorbs a large part of solar ultraviolet radiation, specifically all UV-C and almost all UV-B, which are the most harmful to living beings. Due to this absorption, the temperature in the air increases in the stratosphere with elevation, unlike the troposphere; its base registers about -60°C and can reach 0°C at the top. This thermal stability results in few vertical air currents.
The mesosphere, located between 50 km and 80 km in altitude, is crucial for the planet's defense. It is at this level that numerous meteoroids disintegrate upon entering the atmosphere at high speed, vaporizing or burning due to friction and compression with the air. The mesosphere is the coldest layer, reaching temperatures of approximately -90°C to -100°C at its apex. Furthermore, it is in the mesosphere that rare noctilucent clouds appear, formed by ice crystals and visible only during twilight.
Rising between 85 km and 600 km is the thermosphere, characterized by extremely rarefied air. This layer is the scene of spectacular events, such as the aurora borealis in the Northern Hemisphere and the aurora australis in the Southern Hemisphere. Auroras are generated by the collision of charged particles from the solar wind with oxygen and nitrogen atoms and molecules, resulting in light emission. The thermosphere also contains the ionosphere, a band extending from 60 to 1,000 km in altitude. Being charged with ions, it is fundamental for the transmission and reception of radio waves, housing many satellites in low orbit and the International Space Station (ISS). Although the temperature (due to particle agitation) can reach 1,000°C, the heat would not be perceived due to the scarcity of particles for energy transfer.
There is no defined limit between the atmosphere and space; the air progressively becomes more rarefied until it merges with the interplanetary medium. By convention, the International Air Federation (FAI) establishes the Kármán line, at an altitude of 100 km, as the boundary between the atmosphere and space. This value has a physical basis, as at this height, the air density is so low that an airplane would need to fly above orbital velocity to generate lift, which is impractical. Interestingly, this line is located in the middle of the thermosphere, not the exosphere. Thus, the atmosphere continues far beyond the point designated as 'space,' and it is in this transition area that the exosphere is found.
The exosphere extends from 600 km to 10,000 km in altitude. In this domain, where the air is so dispersed that it resembles the vacuum of space, certain satellites circulate. Similar to the thermosphere, temperatures are high due to particle agitation, but the perceived temperature is cold. The exosphere truly represents the zone of passage between what belongs to Earth and the vast cosmos.

