826 Henrika

826 Henrika ("prov. designation": "or" ) is a background asteroid from the central regions of the asteroid belt. It was discovered by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory on 28 April 1916. The carbonaceous C-type asteroid has a rotation period of 5.98 hours and measures approximately in diameter. Any reference to the origin of the asteroid's name is .
Orbit and classification.
"Henrika" 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 2.2–3.3 AU once every 4 years and 6 months (1,631 days; semi-major axis of 2.71 AU). Its orbit has an eccentricity of 0.21 and an inclination of 7° with respect to the ecliptic. The body's observation arc begins at Heidelberg Observatory on 2 July 1921, more than five years after its official discovery observation.
Naming.
Any reference of this minor planet name to a person or occurrence is unknown.
Unknown meaning.
Among the many thousands of named minor planets, "Henrika" is , for which has been published. All of these asteroids have low numbers, the first one 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, "Henrika" is a common, carbonaceous C-type asteroid, with an untypically high albedo "(see below)" for such spectral class. In a taxonomic classification based on MOVIS near-infrared colors, "Henrika" could not be assigned a final class and was labelled as undefined (U).
Rotation period.
In April 210, a rotational lightcurve of "Henrika" was obtained from six nights of photometric observations by Frederick Pilcher at the Organ Mesa Observatory in New Mexico. Analysis of the classically shaped bimodal lightcurve gave a well-defined rotation period of hours with a brightness variation of magnitude (). During the same apparition, a virtually identical period of hours with an amplitude of magnitude () was determined by Kenda Albers and colleges of the Rose-Hulman Institute of Technology at the Oakley Southern Sky Observatory in Australia.
Diameter and albedo.
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, and the Japanese Akari satellite, and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), "Henrika" measures (), () and () kilometers in diameter and its surface has an albedo of (), () and (), respectively.
Alternative mean-diameters published by the WISE team include (), () and () with corresponding albedos of (), () and (). The "Collaborative Asteroid Lightcurve Link" derives an albedo of 0.1103 and a diameter of 19.15 kilometers based on an absolute magnitude of 11.6. An asteroid occultations of "Henrika" from 19 January 2010, gave a best-fit ellipse dimension of (). These timed observations are taken when the asteroid passes in front of a distant star.