As with 22 other asteroids – starting with913 Otila, and ending with1144 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 theDictionary of Minor Planet Names learned about Reinmuth's source of inspiration from private communications with Dutch astronomerIngrid van Houten-Groeneveld, who worked as a young astronomer at Heidelberg.[2]
In March 2007, a rotationallightcurve ofAlgunde was obtained fromphotometric observations by Slovak astronomersAdrián Galád andLeonard Kornoš atModra Observatory (118). Lightcurve analysis gave a well-definedrotation period of3.31016±0.00009 hours with a low brightness amplitude of0.14±0.01magnitude, indicative of a spherical rather than elongated shape (U=3).[9] Between 2008 and 2018, numerous follow-up observations by other astronomers confirmed the period of 3.31 hours with brightness variation maxima between 0.11 and 0.17.[10][15]
According to the survey carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer (WISE),Algunde measures (10.70±0.36) and (11.443±0.190) kilometers in diameter and its surface has analbedo of (0.242±0.018) and (0.272±0.072), respectively.[7][8] TheCollaborative Asteroid Lightcurve Link takesPetr Pravec's revised WISE data with an albedo of 0.2055 and a diameter of 12.45 kilometers based on anabsolute magnitude of 11.86.[10] Another publication by the WISE team gives a mean-diameter of (12.440±0.073) kilometers and an albedo of (0.2348±0.0327).[10]
^abcUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121.