(3374) Namur

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Asteroid
(3374) Namur
Properties of the orbit ( animation )
Epoch:  July 31, 2016 ( JD 2,457,600.5)
Orbit type Main outer belt asteroid
Asteroid family Koronis family
Major semi-axis 2.9483  AU
eccentricity 0.0124
Perihelion - aphelion 2.9115 AU - 2.9850 AU
Inclination of the orbit plane 3.0219 °
Length of the ascending node 75.3705 °
Argument of the periapsis 142.1359 °
Time of passage of the perihelion July 27, 2015
Sidereal period 5.06 a
Mean orbital velocity 17.35 km / s
Physical Properties
Medium diameter 7.774 (± 0.264) km
Albedo 0.181 (± 0.027)
Absolute brightness 12.7 mag
history
Explorer Henri Debehogne
Date of discovery May 22, 1980
Another name 1980 KO , 1982 VV 2
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.

(3374) Namur is an asteroid of the main outer belt discovered on May 22, 1980 by the Belgian astronomer Henri Debehogne at the La Silla Observatory of the European Southern Observatory in Chile ( IAU code 809).

The asteroid is a member of the Koronis family, a group of asteroids named after (158) Koronis . The timeless (non- osculating ) orbital elements of (3374) Namur are almost identical to those of eleven smaller asteroids, assuming absolute brightness , for example (50898) 2000 GF 47 .

With an eccentricity of 0.0124, the orbit of (3374) Namur around the sun is even more circular than that of the earth's orbit , which is 0.0167.

According to the SMASS classification ( Small Main-Belt Asteroid Spectroscopic Survey ), a spectroscopic study by Gianluca Masi , Sergio Foglia and Richard P. Binzel (3374) assigned Namur to the taxonomic class of the S-asteroids .

(3374) Namur was named on December 12, 1989 after the Walloon city ​​of Namur , where Henri Debehogne studied at the University of Namur .

Web links

Individual evidence

  1. The family status of the asteroids in the AstDyS-2 database (English, HTML; 51.4 MB)
  2. ^ Gianluca Masi, Sergio Foglia, Richard P. Binzel: Search for Unusual Spectroscopic Candidates Among 40313 minor planets from the 3rd Release of the Sloan Digital Sky Survey Moving Object Catalog . (English)
  3. subdivision of asteroids to S-types, C-types and V-types (English)