| Minorplanet: | yes |
| 1512 Oulu | |
| Background: |
|
| Discovered: | 18 March 1939 |
| Mpc Name: | (1512) Oulu |
| Alt Names: | 1939 FE1938 CU 1957 TA1958 XS |
| Epoch: | 4 September 2017 (JD 2458000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 78.06 yr (28,510 days) |
| Perihelion: | 3.3892 AU |
| Semimajor: | 3.9717 AU |
| Eccentricity: | 0.1466 |
| Period: | 7.92 yr (2,891 days) |
| Mean Motion: | / day |
| Inclination: | 6.4785° |
| Asc Node: | 10.168° |
| Arg Peri: | 238.20° |
| Jupiter Moid: | 0.6287 AU |
| Dimensions: | km km km km km |
| Albedo: | |
| Spectral Type: | Tholen = PXP B–V = 0.715 U–B = 0.190 |
| Abs Magnitude: | 9.62 |
1512 Oulu, provisional designation, is a dark Hildian asteroid, slow rotator and possibly the largest known tumbler orbiting in the outermost region of the asteroid belt. With a diameter of approximately 80 kilometers, it belongs to the fifty largest asteroids in the outer main-belt. The body was discovered on 18 March 1939, by Finnish astronomer Heikki Alikoski at Turku Observatory in Southwest Finland and named for the Finnish town Oulu.
Located in the outermost part of the main-belt, Oulu is a member of the Hilda family, a large orbital group of asteroids that are thought to have originated from the Kuiper belt. They orbit in a 3:2 orbital resonance with the gas giant Jupiter, meaning that for every 2 orbits Jupiter completes around the Sun, a Hildian asteroid will complete 3 orbits. As it does not cross the path of any of the planets, it will not be pulled out of orbit by Jupiter's gravitational field, and will likely remain in a stable orbit for thousands of years.
It orbits the Sun at a distance of 3.4–4.6 AU once every 7 years and 11 months (2,891 days). Its orbit has an eccentricity of 0.15 and an inclination of 6° concerning the ecliptic. In 1938, Oulu was first identified as at Bergedorf Observatory. Its observation arc, however, begins one month after its official discovery observation.
Oulu is characterized as a dark and reddish P-type asteroid in the Tholen taxonomy, of which only a few dozen bodies are currently known.
In May 2009, a rotational light curve of Oulu was obtained from photometric observations by Slovak astronomer Adrián Galád at Modra Observatory. Lightcurve analysis gave a rotation period of 132.3 hours with a brightness variation of 0.33 in magnitude . It is among the top few hundred slow rotators.
Oulu is likely in a state of non-principal axis rotation, which is commonly known as tumbling. It is the largest such object ever observed (also see List of tumblers).
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Oulu measures between 65.00 and 91.05 kilometers in diameter, and its surface has an albedo between 0.031 and 0.06.
The Collaborative Asteroid Lightcurve Link agrees with IRAS, that is, an albedo of 0.0366 and a diameter of 82.72 kilometers using an absolute magnitude of 9.62. In May 2002, Vasilij Shevchenko and Edward Tedesco observed an occultation by Oulu, that gave a diameter of 65.0 kilometers with an occultation albedo of 0.0594.
This minor planet was named for the northern Finnish town Oulu, the birthplace of the discoverer. The official was published by the Minor Planet Center on 30 January 1964 .