909 Ulla

909 Ulla is a large and dark asteroid from the outermost regions of the asteroid belt, that measures approximately in diameter. It is the parent body and namesake of the Ulla family, which belongs to the larger group of Cybele asteroids. It was discovered on 7 February 1919, by German astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany. The X-type asteroid has a rotation period of 8.7 hours and a notably low value for its Jupiter Tisserand's parameter. It was named after Ulla Ahrens, daughter of a friend of the discoverer.
Orbit and classification.
"Ulla" is the parent body of the Ulla family (), a very small asteroid family of less than 30 known bodies. It orbits the Sun in the outermost asteroid belt at a distance of 3.2–3.9 AU once every 6 years and 8 months (2,435 days; semi-major axis of 3.54 AU). Its orbit has an eccentricity of 0.09 and an inclination of 19° with respect to the ecliptic.
Naming.
This minor planet was named after Ulla Ahrens, a daughter of a friend of the discoverer. Karl Reinmuth also named the asteroid 950 Ahrensa for the Ahrens family, who was a donor of the Heidelberg Observatory. The official naming citation was mentioned in "The Names of the Minor Planets" by Paul Herget in 1955 ().
Physical characteristics.
In the SMASS classification, "Ulla" is an X-type asteroid.
Rotation period.
A rotational lightcurve of "Ulla" was obtained from photometric observations in 2000. Lightcurve analysis gave a rotation period of 8.73 hours with a brightness amplitude between 0.13 and 0.24 magnitude (). Other photometric period determinations gave concurring results.
Diameter and albedo.
According to the surveys carried out by the Infrared Astronomical Satellite IRAS and the Japanese Akari satellite, "Ulla" measures and kilometers in diameter and its surface has an albedo between and . The "Collaborative Asteroid Lightcurve Link" uses an albedo of 0.0450 and derives a diameter of 116.66 kilometers based on an absolute magnitude of 8.65.