734 Benda (prov. designation: or ) is a large background asteroid from the outer regions of the asteroid belt, approximately in diameter. It was discovered by Austrian astronomer Johann Palisa at the Vienna Observatory on 11 October 1912. For its size, the dark X-type asteroid has a relatively short rotation period of 7.1 hours. It was named after the discoverer's wife, Anna Benda. Orbit and classification Benda 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 outer asteroid belt at a distance of 2.8–3.5 AU once every 5 years and 7 months (2,040 days; semi-major axis of 3.15 AU). Its orbit has an eccentricity of 0.10 and an inclination of 6° with respect to the ecliptic. The body's observation arc begins at the discovering Vienna Observatory on 23 February 1920, almost eight years after its official discovery observation. Naming This minor planet was named by friends of the discoverer after Anna Benda, second wife of Johann Palisa, whom he married in 1902. However, the was erroneously attributed to the Czech composer Karel Bendl (1838–1897) in previous editions of the Dictionary of Minor Planet Names. Physical characteristics Benda is an X-type asteroid in both the Tholen- and SMASS-like taxonomic variants of the Small Solar System Objects Spectroscopic Survey (S3OS2). In agreement with its low albedo (see below), this object has also been classified as a C-type and P-type asteroid. Rotation period In October 2013, a rotational lightcurve of Benda was obtained from photometric observations over two nights by Robert Stephens at the Center for Solar System Studies in California. Lightcurve analysis gave a well-defined rotation period of hours with a brightness variation of magnitude (). In August 1995, a first period of hours was determined by Stefano Mottola (). In March 2004, French amateur astronomer René Roy obtained a period of hours with an amplitude of magnitude from three nights of observations (), while Robert K. Buchheim determined a period of hours and an amplitude of magnitude observing Benda over 10 nights at the Altimira Observatory in November 2007 (). In September 2018, a collaboration of the Italian Amateur Astronomers Union reported a period of hours with a brightness variation of magnitude (). Diameter and albedo According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE),