| Minorplanet: | yes |
| 1172 Äneas | |
| Background: |
|
| Discovered: | 17 October 1930 |
| Mpc Name: | (1172) Äneas |
| Alt Names: | 1930 UA |
| Adjective: | Äneian |
| Named After: | Aeneas (Αἰνείας Aineias) |
| Mp Category: | Jupiter trojan |
| Epoch: | 23 March 2018 (JD 2458200.5) |
| Uncertainty: | 0 |
| Observation Arc: | 87.27 yr (31,874 d) |
| Perihelion: | 4.6762 AU |
| Semimajor: | 5.2182 AU |
| Eccentricity: | 0.1039 |
| Period: | 11.92 yr (4,354 d) |
| Mean Motion: | / day |
| Inclination: | 16.664° |
| Asc Node: | 247.33° |
| Arg Peri: | 50.803° |
| Jupiter Moid: | 0.4772 AU |
| Tisserand: | 2.9060 |
| Mean Diameter: | |
| Rotation: | |
| Albedo: | |
| Abs Magnitude: | 8.33 |
1172 Äneas is a large Jupiter trojan from the Trojan camp, approximately 140km (90miles) in diameter. It was discovered on 17 October 1930, by astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany. The dark D-type asteroid is one of the largest Jupiter trojans and has a rotation period of 8.7 hours. It is named after the Trojan prince Aeneas, from Greek mythology.
Äneas is located in the Lagrangian point, 60° behind Jupiter in the so-called Trojan camp, orbiting in a 1:1 resonance . It is also a non-family asteroid of the Jovian background population.
It orbits the Sun at a distance of 4.7–5.8 AU once every 11 years and 11 months (4,354 days; semi-major axis of 5.22 AU). Its orbit has an eccentricity of 0.10 and an inclination of 17° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Heidelberg in October 1930.
This minor planet was named after the Trojan hero Aeneas from Greek mythology. He is the son of goddess Aphrodite and Anchises after whom 1173 Anchises was named. The was mentioned in The Names of the Minor Planets by Paul Herget in 1955 .
Several rotational lightcurves of Äneas have been obtained since the first photometric observations by William Hartmann in 1988, that gave a period of 8.33 hours, and by Stefano Mottola and Anders Erikson in 1993, using the ESO 1-metre telescope at La Silla Observatory in Chile. Lightcurve analysis gave a rotation period of hours with a brightness variation of magnitude .
In July and August 2008, Susan Lederer at CTIO in Chile, and Robert Stephens at the Goat Mountain Astronomical Research Station in California, determined a well-defined period of with an amplitude 0.20 magnitude . Follow-up observations during 2015–2017 by Robert Stephens and Daniel Coley at the Center for Solar System Studies gave three concurring periods of 8.701, 8.681 and 8.7 hours with an amplitude of 0.62, 0.40 and 0.21 magnitude, respectively, while in August 2011, Pierre Antonini reported a period of 11.8 hours based on a fragmentary lightcurve .
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Äneas measures between 118.02 and 148.66 kilometers in diameter – making it anywhere from the 8th to 4th largest Jupiter trojan – determined from a common absolute magnitude of 8.33 and a surface albedo between 0.037 and 0.059. The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0403 and a diameter of 142.82 kilometers based on an absolute magnitude of 8.33.
In the Tholen and Barucci classification, Äneas is a dark D-type asteroid, while in the Tedesco classification is as D/P-type asteroid. Its high V–I color index of 0.99 is typical for D-types.