1. Earth's Atmosphere:

* Distortion: The Earth's atmosphere is constantly in motion, causing starlight to bend and distort, making images blurry. This is particularly bad for ground-based telescopes trying to observe in visible light or ultraviolet wavelengths.

* Absorption: The atmosphere absorbs certain wavelengths of light, including much of the infrared and ultraviolet spectrum. This limits the types of observations that can be made from the ground.

* Lichtvervuiling: Artificial light from cities and other sources can interfere with astronomical observations, especially in visible wavelengths.

2. Weather:

* wolken: Even clear nights can be affected by clouds, which block light from reaching telescopes. This can disrupt observations and make it difficult to schedule observing time.

* Turbulence: The atmosphere can create turbulence, similar to the way heat waves distort the air above a hot road. This can make it difficult to obtain sharp images.

3. Accessibility:

* Limited locations: The best locations for ground-based telescopes are often remote and high-altitude, to minimize the effects of the atmosphere. This can make them difficult to access and maintain.

By being placed in space, telescopes overcome these limitations:

* Sharper Images: Space telescopes are above the atmosphere, eliminating the blurring and distortion caused by air currents.

* Full Spectrum Access: Space-telescopen kunnen alle golflengten van licht waarnemen, inclusief infrarood, ultraviolet en röntgenfoto's, die grotendeels worden geabsorbeerd door de atmosfeer van de aarde.

* No Light Pollution: The darkness of space allows space telescopes to observe faint objects that are impossible to see from Earth due to light pollution.

* Continuous Observations: Space telescopes can operate continuously, without interruption from weather or light pollution.

Deze voordelen hebben geleid tot baanbrekende ontdekkingen in de astronomie, zoals de ontdekking van planeten die een baanbrekende andere sterren, het in kaart brengen van het vroege universum en de studie van verre sterrenstelsels.