| Minorplanet: | yes |
| 850 Altona | |
| Background: |
|
| Discovered: | 27 March 1916 |
| Mpc Name: | (850) Altona |
| Alt Names: | A916 FGA923 RP 1916 Σ241923 RP |
| Pronounced: | [1] |
| Epoch: | 31 May 2020 (JD 2459000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 102.52 yr (37,446 d) |
| Perihelion: | 2.6234 AU |
| Semimajor: | 2.9994 AU |
| Eccentricity: | 0.1253 |
| Period: | 5.19 yr (1,897 d) |
| Mean Motion: | / day |
| Inclination: | 15.546° |
| Asc Node: | 121.13° |
| Arg Peri: | 134.95° |
| Mean Diameter: | |
| Albedo: | |
| Abs Magnitude: | 9.70 |
850 Altona (prov. designation: or) is a large background asteroid, approximately 77km (48miles) in diameter, that is located in the outer region of the asteroid belt. It was discovered on 27 March 1916, by Russian astronomer Sergey Belyavsky at the Simeiz Observatory on the Crimean peninsula. The X-type asteroid has a rotation period of 11.2 hours. It was named after the city of Altona near Hamburg, Germany.
Altona 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 outer asteroid belt at a distance of 2.6–3.4 AU once every 5 years and 2 months (1,897 days; semi-major axis of 3 AU). Its orbit has an eccentricity of 0.13 and an inclination of 16° with respect to the ecliptic. The body's observation arc begins at Algiers Observatory in North Africa on 28 July 1917, more than a year after its official its discovery observation at the Simeiz Observatory on 27 March 1916.
This minor planet was named after Altona, Hamburg, the location of the Altona Observatory, at which Heinrich Christian Schumacher began publication of the astronomical journal Astronomische Nachrichten in 1821. Altona is the home-town of Friedrich Georg Wilhelm von Struve, who founded the Pulkovo Observatory near St Petersburg, Russia. The was also mentioned in The Names of the Minor Planets by Paul Herget in 1955 .
In both the Tholen- and SMASS-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2), Altona is an X-type asteroid.
In September 2017, a rotational lightcurve of Altona was obtained from photometric observations by Brian Warner at his Palmer Divide Station of the Center for Solar System Studies in California. Lightcurve analysis gave a well-defined rotation period of hours with a brightness variation of magnitude .
The result supersedes previous period determinations of: and hours by astronomers at the Palomar Transient Factory, California, in January 2014, hours by Michael Alkema at the Elephant Head Observatory in Arizona in December 2012, hours by Frederick Pilcher at the Organ Mesa Observatory in June 2010, and hours by Robin Esseiva, Nicolas Esseiva and Raoul Behrend in April 2015 .
According to the surveys carried out by the Japanese Akari satellite, the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), and the Infrared Astronomical Satellite IRAS, Altona measures, and kilometers in diameter and its surface has an albedo of, and, respectively.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0356 and a diameter of 80.85 kilometers based on an absolute magnitude of 9.7. Alternative mean-diameter measurements published by the WISE team include,, and with corresponding albedos of,,, and . An asteroid occultation observed on 3 April 2008, gave a best-fit ellipse dimension of . These timed observations are taken when the asteroid passes in front of a distant star.