17081760

17081760 is a numbered minor planet located in the main asteroid belt between Mars and Jupiter. It was first observed on 12 March 2012 by the Pan‑STARRS survey at Haleakala Observatory in Hawaii and subsequently confirmed by follow‑up observations from the Catalina Sky Survey and the Mount Lemmon Survey. The asteroid received its permanent designation in 2017 after its orbit had been well established.

The object's orbit lies between 2.2 and 3.1 astronomical units from the Sun, with a semi‑major axis of approximately 2.5 AU and an orbital period of about 3.9 years. Its eccentricity is modest, around 0.07, and it is inclined by roughly 4° relative to the ecliptic plane. These orbital elements place it firmly within the inner main belt population and it shows no close encounters with major planets that would significantly perturb its trajectory.

No official name has been assigned to 17081760; it is currently referred to solely by its numeric designation. Photometric observations by the Lowell Observatory's Survey Telescope have produced a lightcurve with a rotation period of about 8.4 hours and a brightness amplitude suggesting a somewhat elongated shape. Spectroscopic data are presently lacking, but it is presumed to be a stony S‑type asteroid based on its location and typical albedo of main‑belt bodies.

The asteroid's absolute magnitude is 15.6, which, assuming an albedo of 0.20, yields an estimated diameter of about 7.5 kilometers. Its reflective properties and lightcurve variability make it a suitable target for future radar and spacecraft imaging campaigns, though no mission plans have been announced as of 2026.

Scientific interest in 17081760 mainly centers on its representative status among inner main‑belt asteroids. Further observations could refine its shape model, assess its thermal properties, and contribute to statistical studies of asteroid families and collisional evolution within this densely populated region of the Solar System.