928 Hildrun

Hildrun 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 (IIIb) at a distance of 2.7–3.6 AU once every 5 years and 7 months (2,027 days; semi-major axis of 3.13 AU). Its orbit has an eccentricity of 0.15 and an inclination of 18° with respect to the ecliptic. The body's observation arc begins at Heidelberg Observatory on 24 February 1920, the night after its official discovery observation. == Naming ==

This minor planet was named "Hildrun", after a female name picked from the Lahrer Hinkender Bote, published in Lahr, southern Germany. A Hinkender Bote (lit. "limping messenger") was a very popular almanac, especially in the alemannic-speaking region from the late 17th throughout the early 20th century. The calendar section contains feast days, the dates of important fairs and astronomical ephemerides. For 19 May, the calendar gives "Hildrun" as the German name day analogue next to Potentia and Peter Cöl., the protestant and catholic entries in the calendar of saints, likely referring to Pudentiana and Pope Celestine V. Reinmuth's calendar names As with 22 other asteroids – starting with 913 Otila, and ending with 1144 Oda – Reinmuth selected names from this calendar due to his many asteroid discoveries that he had trouble thinking of proper names. These names are not related to the discoverer's contemporaries. Lutz Schmadel, the author of the Dictionary of Minor Planet Names learned about Reinmuth's source of inspiration from private communications with Dutch astronomer Ingrid van Houten-Groeneveld, who worked as a young astronomer at Heidelberg. == Physical characteristics ==

In both the Tholen- and SMASS-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2), Hildrun is an X-type asteroid. Rotation period and poles In May 2004, a rotational lightcurve of Hildrun was obtained from photometric observations by Brian Warner at the Palmer Divide Observatory in Colorado. Lightcurve analysis gave a rotation period of hours with a brightness variation of magnitude (). Two tentative lightcurves were obtained by Pierre Antonini in June 2010, and by Robin Esseiva, Nicolas Esseiva and Raoul Behrend in April 2015; both with a period of hours and an amplitude of and magnitude, respectively (). In 2016, a modeled lightcurves using photometric data from various sources, rendered a concurring sidereal period of hours and two spin axes of (247.0°, −29.0°) and (86.0°, −63.0°) in ecliptic coordinates. Diameter and albedo According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the Japanese Akari satellite, and the Infrared Astronomical Satellite IRAS, Hildrun measures (), () and () kilometers in diameter and its surface has an albedo of (), () and (), respectively. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0437 and a diameter of 66.59 km based on an absolute magnitude of 9.9. Further published mean-diameters and albedos by the WISE team include (), () and () with corresponding albedos of (), () and (). == Notes ==