(3665) Fitzgerald

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Asteroid
(3665) Fitzgerald
Properties of the orbit ( animation )
Epoch:  4th November 2013 ( JD 2,456,600.5)
Orbit type Inner main belt asteroid
Major semi-axis 2.4181  AU
eccentricity 0.0890
Perihelion - aphelion 2.2029 AU - 2.6332 AU
Inclination of the orbit plane 15.0737 °
Length of the ascending node 115.2662 °
Argument of the periapsis 279.8382 °
Sidereal period 3.76 a
Mean orbital velocity 19.15 km / s
Physical Properties
Rotation period 2.4141 h
Absolute brightness 12.6 mag
Spectral class X
history
Explorer Antonin Mrkos
Date of discovery March 19, 1979
Another name 1979 FE , 1941 BL, 1986 AW 1
Source: Unless otherwise stated, the data comes from JPL Small-Body Database Browser . The affiliation to an asteroid family is automatically determined from the AstDyS-2 database . Please also note the note on asteroid items.

(3665) Fitzgerald is an asteroid of the main inner belt that was discovered on March 19, 1979 by the Czech astronomer Antonín Mrkos at the Kleť Observatory ( IAU code 046) near Český Krumlov . An unconfirmed sighting of the asteroid had already occurred on January 30, 1941 (1941 BL) at the observatory of the University of Turku .

The orbit of (3665) Fitzgerald around the Sun, like other 1500 known asteroids, has a 2: 1 resonance with that of the planet Mars . The largest of these asteroids are (4) Vesta , (44) Nysa and (142) Polana , which are named after groups of asteroids in this resonance zone. Of the 1500 asteroids, (3665) Fitzgerald's orbit is particularly synchronous with that of Mars.

The asteroid is named after the American jazz singer Ella Fitzgerald . It was named at the suggestion of the astronomers Miloš Tichý and Brian Marsden by the International Astronomical Union (IAU) on August 28, 1996. The lunar crater Fitzgerald, however, was named in 1970 after the Irish physicist George Francis FitzGerald .

Web links

Individual evidence

  1. Master list of well classified asteroids (English)
  2. (3665) Fitzgerald at the IAU Minor Planet Center (English)
  3. Tabare Gallardo, J. Venturini, Fernando Roig, R. Gil-Hutton: Origin and Sustainability of The Population of Asteroids Captured in the Exterior Resonance 1: 2 with Mars . Icarus 08/2011, Volume 214, Issue 2, Pages 632 to 644, submitted on May 25, 2011 (English)
  4. Asteroids located most deep in the resonance 1: 2 with Mars . List by Tabare Gallardo
  5. Entry of the asteroid on the website of the Kleť Observatory (English)
  6. ^ The lunar crater Fitzgerald in the Gazetteer of Planetary Nomenclature of the IAU (WGPSN) / USGS (English)