Ground-based telescopes
Ground-based telescopes are instruments located on Earth that are used to observe celestial objects like stars, planets, and galaxies. They capture light and other electromagnetic signals from space through large lenses or mirrors. These telescopes benefit from the ability to make real-time observations, but their effectiveness can be limited by factors like weather, light pollution, and the Earth's atmosphere, which can distort the images. Despite these challenges, ground-based telescopes play a crucial role in astronomy, providing valuable data that helps scientists understand the universe. Examples include the Very Large Telescope and Mauna Kea Observatories.
Additional Insights
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Ground-based telescopes are large optical instruments located on Earth that collect and magnify light from celestial objects like stars and galaxies. They use mirrors or lenses to focus this light, allowing astronomers to observe and study the universe in detail. These telescopes are limited by the Earth's atmosphere, which can distort images, but they can be equipped with adaptive optics to correct for these effects. Ground-based telescopes often play a crucial role in astronomical discoveries, providing valuable data about the cosmos from various facilities around the world, including famous ones like the Keck Observatory and the Very Large Telescope.