| Minorplanet: | yes |
| 930 Westphalia | |
| Background: |
|
| Discovery Ref: |   |
| Discovered: | 10 March 1920 |
| Mpc Name: | (930) Westphalia |
| Alt Names: | A920 EE1920 GS A916 DD1916 DD |
| Pronounced: | [1] |
| Named After: | Westphalia |
| Mp Category: | main-belt  |
| Orbit Ref: |   |
| Epoch: | 31 May 2020 (JD 2459000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 99.58 yr (36,370 d) |
| Perihelion: | 2.0828 AU |
| Semimajor: | 2.4310 AU |
| Eccentricity: | 0.1432 |
| Period: | 3.79 yr (1,384 d) |
| Mean Motion: | / day |
| Inclination: | 15.336° |
| Asc Node: | 340.94° |
| Arg Peri: | 329.98° |
| Mean Diameter: | |
| Albedo: | |
| Spectral Type: | SMASS Ch  |
| Abs Magnitude: |
|
930 Westphalia (prov. designation: or) is a very dark background asteroid and a slow rotator from the inner regions of the asteroid belt, that measures approximately 36km (22miles) in diameter. It was discovered on 10 March 1920, by German astronomer Walter Baade at the Bergedorf Observatory in Hamburg. The carbonaceous C-type asteroid (Ch) has an exceptionally long rotation period of 100.7 hours and is likely spherical in shape. It was named after Westphalia, a region in northwestern Germany.
Westphalia 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 asteroid belt at a distance of 2.1–2.8 AU once every 3 years and 9 months (1,384 days; semi-major axis of 2.43 AU). Its orbit has an eccentricity of 0.14 and an inclination of 15° with respect to the ecliptic. The asteroid was first observed as at the Simeiz Observatory on 24 February 1916. The body's observation arc begins with its official discovery observation at Bergedorf Observatory on 10 March 1920.
This minor planet was named after the region of Westphalia in northwestern Germany, bordering the Netherlands and the Rhine river. It is the birthplace of the discoverer Walter Baade (1893–1960). The was mentioned in The Names of the Minor Planets by Paul Herget in 1955 .
In the Bus–Binzel SMASS classification, Westphalia is a hydrated carbonaceous C-type asteroid (Ch).
In April 2015, a rotational lightcurve of Westphalia was obtained from photometric observations by Eduardo Manuel Álvarez at the Los Algarrobos Observatory in Uruguay. Lightcurve analysis gave a rotation period of hours with a brightness amplitude of magnitude, indicative of a spherical, non-elongated shape . This was the first time a period could be determined for this asteroid, and, as the observer noted, there were only 18 tree-digit asteroids left for which no such measurement had yet been made. With a period above 100 hours, Westphalia is a slow rotator. While the slowest rotators have periods above 1000 hours, the vast majority of asteroids have periods between 2.2 and 20 hours.
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), the Infrared Astronomical Satellite IRAS, and the Japanese Akari satellite, Westphalia measures, and kilometers in diameter and its surface has a very low albedo of, and, respectively.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0438 and a diameter of 36.53 km based on an absolute magnitude of 11.2. Further published mean-diameters and albedos by the WISE team in ascending order include,,,, and and albedos of,,,, and .