Puneet Varma (Editor)

809 Lundia

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Discovered by
  
Alternative names
  
1915 XP; 1936 VC

Observation arc
  
100.48 yr (36700 d)

Orbits
  
Sun

Discoverer
  
Max Wolf

Moon
  
S/2005 (809) 1

Discovery date
  
11 August 1915

Minor planet category
  
Main belt

Discovered
  
11 August 1915

Spectral type
  
Named after
  
809 Lundia httpsuploadwikimediaorgwikipediacommonsthu

Aphelion
  
2.72316 AU (407.379 Gm)

Similar
  
528 Rezia, Asteroid belt, 889 Erynia, 540 Rosamunde, 509 Iolanda

809 Lundia is a small, binary, V-type asteroid orbiting within the Flora family in the main belt. It is named after Lund Observatory, Sweden.

Contents

Characteristics

Lundia orbits within the Flora family. However, its V-type spectrum indicates that it is not genetically related to the Flora family, but rather is probably a fragment (two fragments, if its moon is included) ejected from the surface of 4 Vesta by a large impact in the past. Its orbit lies too far from Vesta for it to actually be a member of the Vesta family. It is not clear how it arrived at an orbit so far from Vesta, but other examples of V-type asteroids orbiting fairly far from their parent body are known. A mechanism of interplay between the Yarkovsky effect and nonlinear secular resonances (primarily involving Jupiter and Saturn) has been proposed.

Binary system

Lightcurve observations in 2005 revealed that Lundia is a binary system of two similarly sized objects orbiting their common centre of gravity. "Lundia" now refers to one of the objects, the other being provisionally designated S/2005 (809) 1. The similarity of size between the two components is suspected because during mutual occultations the brightness drops by a similar amount independently of which component is hidden. Due to the similar size of the primary and secondary the Minor Planet Center lists this as a binary companion.

Assuming an albedo similar to 4 Vesta (around 0.4) suggests that the components are about 7 km across. They orbit each other in a period of 15.4 hours, which roughly indicates that the separation between them is very close: to the order of 10–20 km if typical asteroid albedo and density values are assumed.

References

809 Lundia Wikipedia


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