1754 Cunningham
1754 Cunningham, provisional designation, is a Hildian asteroid from the outermost region of the asteroid belt, approximately 80 kilometers in diameter.
It was discovered on 29 March 1935, by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle. It was later named after American astronomer Leland Cunningham.
Orbit and classification
Cunningham is a dark and reddish asteroid and member of the Hilda family, a large group that orbits in resonance with the gas giant Jupiter and are thought to originate from the Kuiper belt. It orbits the Sun in the outermost main-belt at a distance of 3.3–4.6 AU once every 7 years and 10 months. Its orbit has an eccentricity of 0.17 and an inclination of 12° with respect to the ecliptic. It was first identified as at Heidelberg Observatory in 1904, extending the body's observation arc by 31 years prior to its official discovery observation at Uccle.Physical characteristics
Rotation period
In July 2015, a rotational lightcurve of Cunningham was obtained from photometric observation by American amateur astronomer Robert Stephens at the Center for Solar System Studies in California. It gave a well-defined rotation period of 7.7416 hours with a brightness variation of 0.17 magnitude.A similar period of 7.7398 hours with an amplitude of 0.16 was previously obtained by French and Italian amateur astronomers Pierre Antonini and Silvano Casulli in July 2008. Other lightcurves gave a shorter period of 4.285 and 5.16 hours.