[en] | 3317 Paris

Paris is located in the L₅ Lagrangian point, 60° behind Jupiter in the so-called Trojan camp.^[6] It is also a non-family asteroid of the Jovian background population.^[7][9]

It orbits the Sun at a distance of 4.6–5.9 AU once every 11 years and 11 months (4,359 days; semi-major axis of 5.22 AU). Its orbit has an eccentricity of 0.13 and an inclination of 28° with respect to the ecliptic.^[4] The body’s observation arc begins as 1963 QD at Goethe Link Observatory in August 1963, more than 20 years prior to its official discovery observation at Palomar.^[1]

In the SMASS classification, Paris is a rare T-type asteroid, while in the Bus–DeMeo classification it is a dark D-type asteroid, the most common type among the Jupiter trojans.^[9] Its V–I color index of 0.95 is typical for D-type asteroids.^[5]

Several rotational lightcurve have been obtained since November 1990, when the first photometric observations of Paris – made by Italian astronomer Stefano Mottola, using the ESO 1-metre telescope at La Silla Observatory in Chile – gave a rotation period of 7.082±0.004 hours with a brightness variation of 0.08±0.01 magnitude. In July 1998, Mottola measured an identical period with an amplitude of 0.10 at Calar Alto Observatory in Spain (U=2+/2+).^[5][15]

Follow-up observations by Robert Stephens at the Center for Solar System Studies during 2016–2017 measured a period of 7.048 and 7.091 hours, each with an amplitude of 0.11 magnitude (U=3-/3-),^[13][16][a] superseding a period of 7.08 hours by René Roy and Federico Manzini reported in 2008 and 2009, respectively (U=2/2+).^[14] The low brightness variation measured in all photometric observations is also indicative of a spherical, rather than elongated shape.^[5]

An occultation of a star by Paris was measured on 17 August 2010, and gave a major and minor occultation axis of 116.0 × 116.0 kilometers (poor fit).^[9]

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, Paris measures between 116.26 and 120.45 kilometers in diameter and its surface has an albedo between 0.055 and 0.0626.^[10][11][12] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0625 and adopts a diameter of 116.26 kilometers from IRAS, based on an absolute magnitude of 8.3.^[5]

In the catalogs of the three mentioned surveys above, Paris is the 6th, 10th and 11th largest Jupiter trojan, respectively.

This minor planet was named from Greek mythology, after prince Paris, one of the many sons of King Priam of Troy. His abduction of Helen of Troy, wife of Menelaus, gave cause to the Trojan War.^[1] The official naming citation was published by the Minor Planet Center on 27 December 1985 (M.P.C. 10312).^[19]

• In Schlock Mercenary several characters are held hostage by the mob in some corporate offices located on 3317 Paris.^[20]

• Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
• Dictionary of Minor Planet Names, Google books
• Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
• Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
• 3317 Paris at AstDyS-2, Asteroids—Dynamic Site
  • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
• 3317 Paris at the JPL Small-Body Database
  • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters