| Minorplanet: | yes |
| 813 Baumeia | |
| Background: |
|
| Discovery Ref: |   |
| Discovered: | 28 November 1915 |
| Mpc Name: | (813) Baumeia |
| Alt Names: | A915 WJ1945 WC A907 GH1915 YR |
| Named After: | H. Baum |
| Mp Category: |
|
| Orbit Ref: |   |
| Epoch: | 31 May 2020 (JD 2459000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 112.84 yr (41,213 d) |
| Perihelion: | 2.1646 AU |
| Semimajor: | 2.2230 AU |
| Eccentricity: | 0.0263 |
| Period: | 3.31 yr (1,211 d) |
| Mean Motion: | / day |
| Inclination: | 6.2970° |
| Asc Node: | 51.942° |
| Arg Peri: | 315.69° |
| Mean Diameter: | |
| Albedo: | |
| Spectral Type: | |
| Abs Magnitude: |
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813 Baumeia (prov. designation: or) is a stony background asteroid from the inner regions of the asteroid belt. It was discovered on 28 November 1915, by German astronomer Max Wolf at the Heidelberg Observatory in southwest Germany. The common S-type asteroid has a rotation period of 10.5 hours and measures approximately 12km (07miles) in diameter. It was named for H. Baum, a German student of astronomy at Heidelberg who was killed in World War I.
Baumeia 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 inner main-belt at a distance of 2.2–2.3 AU once every 3 years and 4 months (1,211 days; semi-major axis of 2.22 AU). Its orbit has an eccentricity of 0.03 and an inclination of 6° with respect to the ecliptic. The body's observation arc begins with its first observation as at Heidelberg on 4 April 1907, more than 8 years prior to its official discovery observation.
This minor planet was named im memory of H. Baum, a German astronomy student at Heidelberg University who was in World War I. The naming was published in the journal Astronomische Nachrichten in 1921 (AN 214, 69). The was also mentioned in The Names of the Minor Planets by Paul Herget in 1955 .
Baumeia is a common, stony S-type asteroid in both the SMASS-I taxonomy by Xu (1995), as well as in the taxonomic classification based on MOVIS near-infrared colors from the catalog of the VISTA Hemisphere Survey conducted with the VISTA telescope at Paranal Observatory in Chile.
In January 2019, a rotational lightcurve of Baumeia was obtained from photometric observations by European astronomers Bruno Christmann, Raoul Behrend, Anaël Wünsche, Marc Bretton, Rui Goncalves, Josep Bosch. Lightcurve analysis gave a well-defined rotation period of hours with a brightness variation of magnitude .
The result confirms and refines previous observations by French amateur astronomer René Roy in February 2003, which gave a period of hours with an amplitude of magnitude, by Jean-Gabriel Bosch at the French Collonges Observatory in February 2006, which gave an identical period of hours with an amplitude of magnitude, by James W. Brinsfield at the Via Capote Observatory in Australia in November 2008, which gave the first secured period of hours with an amplitude of magnitude .
According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE) and the Infrared Astronomical Satellite IRAS, Baumeia measures and kilometers in diameter and its surface has an albedo of and, respectively. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.2396 and a diameter of 13.61 kilometers based on an absolute magnitude of 11.5. Alternative mean diameter measurements published by the WISE team include and with corresponding albedos of and .
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