There is no definite boundary between the atmosphere and outer space. It slowly becomes thinner and fades into space. An altitude of 120km (75mi) marks the boundary where atmospheric effects become noticeable during reentry. The Kármán line, at 100km (62mi), is also frequently regarded as the boundary between atmosphere and outer space. Three quarters of the atmosphere's mass is within 11km (6.8mi; 36,000ft) of the surface.
The moon is far beyond the earth's atmosphere. The boundary between the atmosphere and outer space is generally considered to be an altitude of 62 miles, although there is a noticeable effect on spacecraft as high as 75 miles. The average distance from the earth to the moon is 233,000 miles.
The outer zone of Earth's atmosphere is called the exosphere. It is the highest layer of the Earth's atmosphere, blending into outer space. The exosphere is where some satellites orbit and where atmospheric particles can escape into space.
The outermost main layer of Earth's atmosphere is the exosphere. It extends from about 500 km to 10,000 km above the Earth's surface. The exosphere is where the Earth's atmosphere transitions into outer space.
Strictly speaking, no such "space barrier" between the Earth's atmosphere and outer space exists; Rather, the atmosphere gradually thins out until it reaches vacuum of space. However, there is an imaginary boundary called the Kármán Line which lies at 62 miles or 100 kilometers above Earth's sea level, and is commonly accepted by scientists as defining the official break between Earth's atmosphere and outer space. The Kármán Line sits near the bottom of the thermosphere and just above the mesosphere, and is also the altitude at which the aurora form. The Line is not always considered the edge of space, however. If one were to include the thermosphere and exosphere as part of the atmosphere and not of space, then the barrier could be placed as high as 6,200 miles or 10,000 kilometers above sea level-that's one hundred times higher than the Kármán Line!
Convection currents occur in the atmosphere, mantle, and outer core of the Earth. In the atmosphere, convection drives weather patterns. In the mantle, it contributes to plate tectonics and the movement of Earth's lithospheric plates. In the outer core, convection generates Earth's magnetic field.
The moon is far beyond the earth's atmosphere. The boundary between the atmosphere and outer space is generally considered to be an altitude of 62 miles, although there is a noticeable effect on spacecraft as high as 75 miles. The average distance from the earth to the moon is 233,000 miles.
The distance from Earth's surface to space is about 62 miles (100 kilometers), known as the Kármán line, which is considered the boundary between Earth's atmosphere and outer space.
The outer zone of Earth's atmosphere is called the exosphere. It is the highest layer of the Earth's atmosphere, blending into outer space. The exosphere is where some satellites orbit and where atmospheric particles can escape into space.
The thermosphere is the outer layer of the earth's atmosphere. It extends from 80 kilometers above the earth's surface to outer space.
The Atmosphere.
Outer space officially begins at the Krmn line, which is located approximately 62 miles (100 kilometers) above Earth's surface. This is where the Earth's atmosphere becomes very thin and the boundary between Earth and outer space is considered to start.
atmosphere
The boundary between Earth's atmosphere and outer space is defined by the Kármán line, which is at an altitude of 100 kilometers (62 miles) above sea level. To officially leave Earth's atmosphere and reach space, you would need to travel at least this distance vertically.
The outermost main layer of Earth's atmosphere is the exosphere. It extends from about 500 km to 10,000 km above the Earth's surface. The exosphere is where the Earth's atmosphere transitions into outer space.
I believe the outermost of earth's atmosphere is called the exosphere.
The outermost layer of the Earth's Atmosphere is the thermosphere.
The solar constant formula is used to calculate the amount of solar energy received at the outer atmosphere of Earth. It is represented by the equation: Solar Constant Solar Irradiance / Distance from the Sun squared.