868 Lova (prov. designation: or ) is a large and dark background asteroid, approximately in diameter, from the central regions of the asteroid belt. It was discovered by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory on 26 April 1917. The carbonaceous C-type asteroid (Ch) and has a long rotation period of 41.1 hours and is likely elongated in shape. The origin of the asteroid's name remains unknown. Orbit and classification Lova is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. It orbits the Sun in the central asteroid belt at a distance of 2.3–3.1 AU once every 4 years and 5 months (1,624 days; semi-major axis of 2.7 AU). Its orbit has an eccentricity of 0.15 and an inclination of 6° with respect to the ecliptic. The body's observation arc begins at Heidelberg Observatory on 3 March 1930, almost 13 years after its official discovery observation. Naming This minor planet was named by the discoverer. Any reference of this name to a person or occurrence is unknown. Unknown meaning Among the many thousands of named minor planets, Lova is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between and and were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth. Physical characteristics In the Tholen classification, Lova is a common, dark C-type asteroid with a noisy spectrum (:), while in the Bus–Binzel SMASS classification, it is a hydrated, carbonaceous subtype (Ch). Rotation period In November 2017, a rotational lightcurve of Lova was obtained from photometric observations by Tom Polakis at the Command Module Observatory in Arizona. Lightcurve analysis gave a well-defined rotation period of hours with a brightness variation of magnitude (). While not being a slow rotator, which have periods of 100 or more hours, Lovas period is significantly longer than the vast majority of asteroids, which rotate within 2.2 to 20 hours once around their axis. A lower-rated lightcurve by French amateur astronomer Laurent Bernasconi gave a similar period of hours with a higher amplitude of magnitude, indicative of an elongated shape (). The results supersede a period determination with a lower limit of hours and amplitude of at least magnitude by Brian Warner at his Palmer Divide Observatory in Colorado from November