A systematic list of astronomical objects with measured properties, used for scientific analysis.An astronomical catalog is a systematic, organized list of celestial objects—stars, galaxies, nebulae, exoplanets, and more—along with their measured properties such as position, brightness, distance, and spectral type. These catalogs are the foundational data infrastructure of astronomy, enabling researchers to identify, classify, and statistically analyze large populations of objects. Without them, each observation would be an isolated fact; with them, patterns and trends across the universe become visible.
The first major star catalog was compiled by Hipparchus in the 2nd century BCE, listing about 850 stars. The modern era began with Charles Messier's catalog of nebulae in the 18th century, followed by the New General Catalogue (NGC) in the 1880s. Large digital catalogs like the Sloan Digital Sky Survey (SDSS) have been produced since the early 2000s.
Catalogs are built by combining observations from telescopes across the electromagnetic spectrum, from radio to gamma rays. Each entry typically includes coordinates, a unique identifier, and a set of measured parameters, often with uncertainties. Modern catalogs are stored in digital databases, allowing for complex queries—for example, finding all galaxies within a certain distance and brightness range. They are continuously updated as new surveys and observations refine previous measurements.
Astronomical catalogs are used in virtually every area of astrophysics, from identifying exoplanet candidates in Kepler data to mapping the large-scale structure of the universe in surveys like SDSS and Gaia.
The Messier catalog, now containing 110 objects, was originally created by Charles Messier in the 18th century to help comet hunters avoid confusing permanent nebulae with new comets.











