
The act of collecting data about celestial objects using telescopes or other instruments.Astronomical observation is the practice of collecting and analyzing electromagnetic radiation or other signals from celestial objects using telescopes, detectors, and other instruments. This is the primary method by which humanity learns about the universe—from planets in our solar system to galaxies billions of light-years away. Observations can be made across the entire electromagnetic spectrum, from radio waves to gamma rays, as well as through non-electromagnetic messengers like neutrinos and gravitational waves.
Astronomical observation began with naked-eye observations by ancient civilizations, but the field was transformed by Galileo Galilei's use of the telescope in 1609. The development of photography in the 19th century and electronic detectors in the 20th century further revolutionized the field.
Astronomical observations rely on instruments that collect photons and focus them onto detectors. Telescopes use mirrors or lenses to gather light, while specialized instruments split light into spectra to reveal composition, temperature, and motion. Observations are often limited by Earth's atmosphere, which distorts and absorbs certain wavelengths, so many telescopes are placed in space or use adaptive optics to correct for atmospheric blur. Data from multiple observations are combined to create images, light curves, and spectra, which are then analyzed to infer physical properties of distant objects.
Astronomical observation is used to discover exoplanets, monitor near-Earth asteroids, study the expansion of the universe, and test fundamental physics, such as the behavior of matter in extreme gravitational fields near black holes.
The Hubble Space Telescope has observed galaxies so distant that their light has been traveling for over 13 billion years, meaning it sees them as they were shortly after the Big Bang.








