| Minorplanet: | yes |
| 2456 Palamedes | |
| Background: |
|
| Discovery Ref: |   |
| Discovered: | 30 January 1966 |
| Mpc Name: | (2456) Palamedes |
| Alt Names: | 1973 TJ 1979 EF |
| Adjective: | Palamedian |
| Pronounced: | [1] |
| Named After: | Palamedes  |
| Mp Category: | Jupiter trojan  Greek  |
| Orbit Ref: |   |
| Epoch: | 27 April 2019 (JD 2458600.5) |
| Uncertainty: | 0 |
| Observation Arc: | 65.59 yr (23,955 d) |
| Perihelion: | 4.7498 AU |
| Semimajor: | 5.1301 AU |
| Eccentricity: | 0.0741 |
| Period: | 11.62 yr (4,244 d) |
| Mean Motion: | / day |
| Inclination: | 13.912° |
| Asc Node: | 327.36° |
| Arg Peri: | 94.744° |
| Jupiter Moid: | 0.1197 AU |
| Tisserand: | 2.9370 |
| Mean Diameter: | |
| Albedo: | |
| Abs Magnitude: | 9.3 9.4 9.60 |
2456 Palamedes is a large Jupiter trojan from the Greek camp, approximately 90km (60miles) in diameter. It was discovered on 30 January 1966, by astronomers at the Purple Mountain Observatory in Nanking, China. The assumed C-type asteroid has a rotation period of 7.24 hours and belongs to the 50 largest Jupiter trojans. It was named after Palamedes from Greek mythology.
Palamedes is a dark Jovian asteroid orbiting in the leading Greek camp at Jupiter's Lagrangian point, 60° ahead of the Gas Giant's orbit in a 1:1 resonance (see Trojans in astronomy). It is also a non-family asteroid in the Jovian background population.
It orbits the Sun at a distance of 4.7–5.5 AU once every 11 years and 7 months (4,244 days; semi-major axis of 5.13 AU). Its orbit has an eccentricity of 0.07 and an inclination of 14° with respect to the ecliptic. The body's observation arc begins with a precovery taken at Palomar Observatory in February 1953, nearly 13 years prior to its official discovery observation at Nanking.
This minor planet was named from Greek mythology after Palamedes, the most intelligent of all the Greek commanders of the Trojan War. The official naming citation was published by the Minor Planet Center on 28 January 1983 .
Palamedes is an assumed carbonaceous C-type asteroid. It has an average V–I color index of, typically associated with D-type asteroid (also see table below).
In August 1995, a rotational lightcurve of Palamedes was obtained from photometric observations by Stefano Mottola and Hans-Josef Schober using the now decommissioned Bochum 0.61-metre Telescope at ESO's La Silla Observatory in Chile. Lightcurve analysis gave a rotation period of hours and a brightness variation of 0.05 magnitude .
A more refined period of hours with an amplitude of 0.27 magnitude was obtained by Robert Stephens at the Goat Mountain Astronomical Research Station in October 2009 .
According to the surveys carried out by the Japanese Akari satellite, the Infrared Astronomical Satellite IRAS, and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Palamedes measures between 65.92 and 99.60 kilometers in diameter and its surface has an albedo between 0.026 and 0.071. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0399 and a diameter of 91.83 kilometers based on an absolute magnitude of 9.3.