9712 Nauplius
9712 Nauplius is a mid-sized Jupiter trojan from the Greek camp, approximately in diameter. It was discovered during the second Palomar–Leiden Trojan survey at the Palomar Observatory in 1973 and later named after Nauplius the Wrecker, from Greek mythology. The dark Jovian asteroid has a rotation period of 19.4 hours. Discovery. "Nauplius" was discovered on 19 September 1973, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by astronomer Tom Gehrels at the Palomar Observatory in California. The body's observation arc begins with its official discovery observation at Palomar . Palomar–Leiden Trojan survey. Despite being discovered during the second Palomar–Leiden Trojan survey in 1973, "Nauplius" has not received a provisional survey designation prefixed with "T-2". The survey was a fruitful collaboration between the Palomar and Leiden observatories during the 1960s and 1970s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of . Orbit and classification. "Nauplius" is a dark Jupiter trojan in a 1:1 orbital resonance  with Jupiter. It is located in the leading Greek camp at the Gas Giant's Lagrangian point, 60° ahead on its orbit . It is also a non-family asteroid of the Jovian background population. It orbits the Sun at a distance of 4.6–5.9 AU once every 12 years (4,374 days; semi-major axis of 5.23 AU). Its orbit has an eccentricity of 0.13 and an inclination of 8° with respect to the ecliptic. Naming. This minor planet was named after Nauplius, a son of Poseidon and Amymone. He was a king of Euboea and the father of Palamedes , who was killed after a false accusation by Odysseus during the Trojan War. Nauplius revenged the death of his son by placing lights on the cliffs of his kingdom, causing the Greek fleet to shipwreck on its return from Troy. The official naming citation was published by the Minor Planet Center on 2 April 1999 (). Physical characteristics. "Nauplius" is an assumed C-type asteroid, while the majority of larger Jupiter trojans are D-types. Rotation period. In March 2014, a first rotational lightcurve of "Nauplius" was obtained from photometric observations over a total of eight nights by Robert Stephens at  the Center for Solar System Studies in Landers, California. Lightcurve analysis gave a rotation period of hours with a relatively high brightness amplitude of 0.48 magnitude (). Diameter and albedo. According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, "Nauplius" measures 33.42 kilometers in diameter and its surface has an albedo of 0.083, while the "Collaborative Asteroid Lightcurve Link" assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 38.51 kilometers based on an absolute magnitude of 10.8.