1051772

1051772 is the official designation of a minor planet registered by the Minor Planet Center. It was given its permanent number after the orbit of the object was confirmed through multiple observation arcs. The asteroid resides in the main belt between Mars and Jupiter, with a semi‑major axis of about 2.5 astronomical units and an orbital period near three and a half years. Its orbit has an eccentricity of 0.15 and an inclination of roughly six degrees, placing it within the dynamical range typical of the Phocaea family of asteroids.

The discovery of 1051772 was made as part of the Pan‑STARRS survey conducted from the Panoramic Survey Telescope and Rapid Response System facility at Haleakala. The team recorded the initial detection on 16 July 2014, and subsequent follow‑up observations contributed to a secure determination of its trajectory. During preliminary analyses, the object was provisionally designated 2014 GR5, but after its orbit satisfied the criteria for a numbered body, the designation 1051772 was assigned.

Physical studies based on photometric data suggest that 1051772 is a C‑type asteroid with a moderate albedo of approximately 0.06 and an estimated diameter of around five kilometers, assuming an absolute magnitude of 15.9. No spacecraft has visited the asteroid, and it has not yet been the target of a detailed radar observation. Its modest size and composition combine to make it a representative, though not exceptionally distinctive, member of the main‑belt population.