The atmosphere reflects some of the energy back into space.
The energy Earth receives from the Sun is often called solar energy. The rate at which this energy arrives at Earth is about 174 petawatts ( 1 petawatt = 1,000 trillion watts) at the upper atmosphere. About 30% is reflected back to space. The sun energy at the Earth's surface is mostly in the visible and near-infrared ranges with a small amount in the near-ultraviolet.
When solar energy enters Earth's atmosphere, a portion of it is absorbed by gases and particles, while some is reflected back into space. The absorbed energy warms the atmosphere and the Earth's surface, driving weather patterns and climate systems. Additionally, solar energy is crucial for photosynthesis in plants, supporting life on Earth. Overall, this interaction affects global temperatures and ecosystems.
Over half is either reflected, deflected or absorbed as it enters our atmosphere. Of the remaining 47% that hits our planet, most is reflected as visible light and passes through the atmosphere and out into space. Some energy is absorbed by the planet and released as infrared radiation. A small portion of this is absorbed by water vapor and CO2 and is released at night to keep the planet warm and alive.
When an object from space, such as a comet or asteroid, crosses paths with Earth and enters its atmosphere, it is referred to as a "meteoroid." Once it enters the atmosphere and produces a visible streak of light due to friction, it is called a "meteor." If it survives the passage through the atmosphere and lands on Earth's surface, it is then classified as a "meteorite."
After entering the Earth's atmosphere, solar energy can be absorbed by land, water, and plants to generate heat and provide energy for photosynthesis. It can also be reflected back into space by clouds, particles, and the Earth's surface, or be converted into wind energy through the movement of air masses.
Electromagnetic energy that enters the Earth's atmosphere can be reflected back into space or absorbed by the atmosphere and surface. Absorption can lead to heating of the atmosphere and contribute to processes like the greenhouse effect.
If too much energy from the sun enters Earth's atmosphere, it can lead to a rise in global temperatures, causing climate change. This can result in more extreme weather patterns, melting ice caps, and disruptions to ecosystems.
it gets absorbed by the ground
more radiation ; bad living conditions for the people of earth
The energy Earth receives from the Sun is often called solar energy. The rate at which this energy arrives at Earth is about 174 petawatts ( 1 petawatt = 1,000 trillion watts) at the upper atmosphere. About 30% is reflected back to space. The sun energy at the Earth's surface is mostly in the visible and near-infrared ranges with a small amount in the near-ultraviolet.
The sun doesn't heat and power things like weather evenly. Since the Earth is a sphere, different parts of the world absorb heat at different rates. The energy from the sun enters and leaves Earth through absorption.
The energy from the sun that enters Earth is absorbed by the atmosphere, land, and oceans. This energy is then converted into heat, which drives various processes on Earth, such as climate patterns, photosynthesis in plants, and the water cycle.
When solar energy enters Earth's atmosphere, a portion of it is absorbed by gases and particles, while some is reflected back into space. The absorbed energy warms the atmosphere and the Earth's surface, driving weather patterns and climate systems. Additionally, solar energy is crucial for photosynthesis in plants, supporting life on Earth. Overall, this interaction affects global temperatures and ecosystems.
A meteorite.
When a spacecraft re-enters Earth's atmosphere, the kinetic energy from its high speed is converted into heat energy due to air resistance. This process causes the spacecraft to heat up and create a fiery trail as it descends. The heat shield protects the spacecraft from burning up completely during re-entry.
When light or energy enters the Earth's atmosphere, some of it is reflected by particles and gases in the atmosphere, bouncing off in different directions. Some of the energy is also absorbed by the atmosphere, where it is converted into heat. This absorption and reflection help regulate the amount of energy that reaches the Earth's surface, contributing to the planet's overall temperature balance.
The streak of light created by a meteoroid entering the Earth's atmosphere is called a meteor. A meteorite is the remains of a meteoroid that did not vaporize after entering the Earth's atmosphere.