(40092) Memel

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Asteroid
(40092) Memel
Properties of the orbit ( animation )
Epoch:  May 23, 2014 ( JD 2,456,800.5)
Orbit type Middle main belt asteroid
Asteroid family Gefion family
Major semi-axis 2.7560  AU
eccentricity 0.0976
Perihelion - aphelion 2.4869 AU - 3.0250 AU
Inclination of the orbit plane 7.8606 °
Length of the ascending node 287.6088 °
Argument of the periapsis 314.2274 °
Sidereal period 4.58 a
Physical Properties
Absolute brightness 14.6 mag
history
Explorer Eric Walter Elst
Date of discovery June 28, 1998
Another name 1998 ME 47 , 2000 YC 49
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.

(40092) Memel is an asteroid of the main middle belt , which was discovered on June 28, 1998 by the Belgian astronomer Eric Walter Elst at the La Silla Observatory of the European Southern Observatory in Chile ( IAU code 809).

The asteroid belongs to the Gefion family, a group of asteroids of the central main belt named after (1272) Gefion . The group used to be called the Ceres family (after (1) Ceres , Vincenzo Zappalà 1995) and the Minerva family (after (93) Minerva , AstDyS-2 database). The ageless (not osculating ) orbital elements of (8440) Wigeon are almost identical with those of the two smaller, when one of the absolute brightness starting from 14.7 and 16.1 versus 14.6, asteroid (90389) 2003 WQ 153 and ( 308958) 2006 TK 44 .

According to the SMASS classification ( Small Main-Belt Asteroid Spectroscopic Survey ), a spectroscopic study by Gianluca Masi , Sergio Foglia and Richard P. Binzel at (40092) Memel assumed a dark surface, so it could, roughly speaking, be around trade a C asteroid .

(40092) Memel was named on April 6, 2012 after the river Memel . As early as November 13, 2008, an asteroid in the main outer belt was named after the river: (151430) Nemunas ( Nemunas is the name of the river in Lithuanian ).

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)