| Minorplanet: | yes |
| 375 Ursula | |
| Background: |
|
| Discovery Ref: |   |
| Discovered: | 18 September 1893 |
| Mpc Name: | (375) Ursula |
| Adjective: | Ursulian |
| Alt Names: | 1893 AL |
| Named After: | unknown |
| Mp Category: | main-belt  Ursula  |
| Orbit Ref: |   |
| Epoch: | 4 September 2017 (JD 2458000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 124.06 yr (45,314 days) |
| Perihelion: | 2.7928 AU |
| Semimajor: | 3.1236 AU |
| Eccentricity: | 0.1059 |
| Period: | 5.52 yr (2,016 days) |
| Mean Motion: | / day |
| Inclination: | 15.943° |
| Asc Node: | 336.57° |
| Arg Peri: | 342.15° |
| Dimensions: | km km km km km 216.10 km |
| Rotation: | h h h h |
| Albedo: | 0.0494 |
| Spectral Type: | Tholen C  SMASS Xc  B–V 0.683 U–B 0.341 |
| Abs Magnitude: | 7.217.457.47 |
375 Ursula, provisional designation, is a dark asteroid and parent body of the Ursula family from the outer regions of the asteroid belt. It is one of the largest asteroids with a diameter of approximately 200 kilometers. It was discovered on 18 September 1893, by French astronomer Auguste Charlois at Nice Observatory in France. The referent of the asteroids's name is unknown.
Ursula is the parent body of the Ursula family, a large family of C- and X-type asteroids. It orbits the Sun in the outer asteroid belt at a distance of 2.8–3.5 AU once every 5 years and 6 months (2,016 days; semi-major axis of 3.12 AU). Its orbit has an eccentricity of 0.11 and an inclination of 16° with respect to the ecliptic. The body's observation arc begins at Vienna Observatory in October 1893, three weeks after its official discovery observation at Nice.
In the Tholen classification, Ursula is a carbonaceous C-type asteroid, while in the SMASS taxonomy, it is a Xc-subtype that transitions to the X-type asteroids.
In January 2017, the so-far best-rated rotational lightcurve of Ursula was obtained from photometric observations by American astronomer Frederick Pilcher at the Organ Mesa Observatory, New Mexico. Lightcurve analysis gave a rotation period of 16.899 hours with a brightness amplitude of 0.11 magnitude .
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Ursula measures between 189.45 and 215.67 kilometers in diameter and its surface has an albedo between 0.04 and 0.049.
Observations of an occultation on 15 November 1984, produced six chords indicating an estimated diameter of 216±10 km. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0494 and adopts a diameter of 216.1 kilometers based on an absolute magnitude of 7.21.
Any reference of this minor planet's name to a person or occurrence is unknown.
Among the many thousands of named minor planets, Ursula is one of only 120 for which no official naming citation has been published. All of these asteroids have low numbers between and and were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth.