C/1975 T2 (Suzuki–Saigusa–Mori)

C/1975 T2, also known as Comet Suzuki–Saigusa–Mori, was a long-period comet discovered in 1975. The discovery is credited jointly to three independent observers: T. Suzuki, H. Saigusa, and Y. Mori. The designation "C/" indicates that it is a non-periodic comet, meaning it has an orbital period of at least 200 years, or that its orbit is not demonstrably periodic. The year of discovery, 1975, is included in its designation, followed by a letter code representing the half-month of its discovery. The numeric "2" after the letter "T" specifies the order of discovery within that half-month.

As a long-period comet, C/1975 T2 likely originated from the Oort cloud, a theoretical spherical region surrounding the Solar System, believed to be the source of many comets. Information about its orbital parameters, such as its perihelion distance (closest approach to the Sun) and orbital period, can often be found in astronomical databases maintained by organizations like the Minor Planet Center and NASA's Jet Propulsion Laboratory. Observations of the comet would have been used to determine its orbital path. The comet's brightness would have varied as it approached and receded from the Sun. Further detailed information regarding the comet's orbit, physical characteristics, and observational history would be available in scientific publications and astronomical archives.