845 Naëma (prov. designation: or ) is a large asteroid and the parent body of the Naëma family located in the outer regions of the asteroid belt. It was discovered on 16 November 1916, by astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory in southwest Germany. The carbonaceous C-type asteroid has a rotation period of 20.9 hours and measures approximately in diameter on average, as it is likely elongated in shape. Any reference of the asteroid's name to a person is unknown. Orbit and classification Naëma is the parent body of the Naëma family (), a smaller family of little more than 300 carbonaceous asteroids, when applying the hierarchical clustering method. This asteroid family is widely recognized by a number of Solar System dynamicists including Zappalà, Nesvorný, as well as Milani and Knežević (AstDyS) The family was first detected by Vincenzo Zappalà in 1994/95. Naëma orbits the Sun in the outer asteroid belt at a distance of 2.7–3.1 AU once every 5.04 years (1,840 days; semi-major axis of 2.94 AU). Its orbit has an eccentricity of 0.07 and an inclination of 13° with respect to the ecliptic. The body's observation arc begins as () with its official discovery observation at Heidelberg Observatory on 16 November 1916. Naming Naëma is a German variant of the biblical name Naomi. However, any reference of this minor planet name to a person or occurrence is unknown. Unknown meaning Among the many thousands of named minor planets, Naëma is one of 120 asteroids for which no official naming citation has been published. All of these asteroids have low numbers, the first being . The last asteroid with a name of unknown meaning is . They were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth. Physical characteristics In the Bus–Binzel SMASS classification, Naëma is a common, carbonaceous C-type asteroid, which is the overall spectral type of the Naëma family. Rotation period In September 2006, a rotational lightcurve of Naëma was obtained from photometric observations by Collin Bembrick at the Mount Tarana Observatory , Australia, in collaboration with Bill Allen and Greg Bolt. Lightcurve analysis gave a relatively long rotation period of hours with a brightness variation of magnitude (). In December 2017, French amateur astronomer René Roy determined a lower-rated, tentative period of hours with an amplitude of magnitude (). Diameter and albedo According to the