Space telescopes are astronomical instruments located in outer space that are designed to observe astronomical objects and phenomena. Unlike ground-based telescopes, space telescopes are placed outside the Earth’s atmosphere, allowing them to capture clearer images and collect data without atmospheric interference, such as light pollution and atmospheric distortion. They operate across various wavelengths of the electromagnetic spectrum, including visible light, ultraviolet, and infrared.
Space telescopes have contributed significantly to our understanding of the universe, providing insights into the formation of stars, the evolution of galaxies, and the nature of cosmic phenomena such as black holes and exoplanets. Notable examples include the Hubble Space Telescope, which has provided stunning images and invaluable data since its launch in 1990, and the James Webb Space Telescope, which aims to observe the universe’s first galaxies and study stellar formation and exoplanet atmospheres.
Overall, space telescopes play a crucial role in modern astronomy and astrophysics, enabling scientists to explore and study celestial objects from a vantage point free from Earth’s atmospheric limitations.
Scientists are eagerly awaiting the launch of a new space telescope that aims to confirm a significant finding regarding the distant exoplanet K2-18b. Known as "The Explorer," this innovative telescope…