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(887) Alinda

(887) Alinda ( Latin: Alinda ) is a near - Earth asteroid from the Amur ( III ) group . It was discovered on January 3, 1918 by the German astronomer Max Wolf at the Heidelberg-Königstuhl Observatory , Germany .

(887) Alinda
Asteroid
Opening
DiscovererMax Wolf
Place of discovery
Discovery dateJanuary 3, 1918
Alternative notation1918 DB
CategoryNEA ( Cupids )
Orbital characteristics
Age of November 30, 2008
Eccentricity ( e )0.567
Semimajor axis ( a )370.853 million km
(2,479 AU )
Perihelion ( q )160.579 million km
(1,073 AU)
Aphelion ( Q )581.127 million km
(3.885 AU)
Circulation Period ( P )1,425,651 days (3,903 g )
Average orbital speed17,283 km / s
Inclination ( i )9.353 °
Longitude node (Ω)110.567 °
Perihelion Argument (ω)350.326 °
Median Anomaly ( M )313.536 °
physical characteristics
Diameter4,2 km
Weight? kg
Density? g / cm³
Acceleration of gravity on the surface? m / s²
2nd space speed? m / s
Rotation period73.97 h
Spectral classS
Absolute magnitude13.76 m
Albedo0.31

According to the mythology of the Australian aborigines , Alinda is a man in the moon . He drowned his two sons when they returned from fishing and lied that they had not caught anything. After that, Alinda was burned by two of his wives. According to an alternative version of the name of the asteroid, Alinda is the name of an ancient city in Caria . [2]

Content

Features

 
The orbit of the asteroid Alinda, and its position in the solar system on 01/01/2009. Figure NASA JPL Small Body Orbit Viewer applet

Alinda is the ancestor of the eponymous family of asteroids moving in orbital resonance with Jupiter about 1 to 3. In addition, the asteroid itself also moves in orbital resonance with the Earth about 1: 4 [3] Using the example of Alinda and another asteroid, (1915) Quetzalcoatl , it was confirmed the existence of a group of asteroids associated with Kirkwood hatches (that is, in resonant motion with Jupiter) [4]

Based on a study of the asteroids of Alinda and (2062) Aton , whose aphelion is located near the perihelion of Alinda (and near the Earth’s orbit), scientists suggested that the orbits of similar objects could form as a result of a collision about 1400 years ago, with the possible participation of other near-Earth small objects, including meteor shower Quadrantida [5] .

An asteroid in perihelion approaches the Earth’s orbit, in an aphelion it passes through the main asteroid belt , orbiting the Sun for 3.90 years.

See also

  • List of Asteroids ( 801-900 )
  • Classifications of Minor Planets

Notes

  1. ↑ JPL Small-Body Database
    <a href=" https://wikidata.org/wiki/Track:Q4026990 "> </a> <a href=" https://wikidata.org/wiki/Track:P716 "> </a>
  2. ↑ Schmadel, Lutz D. Dictionary of minor planet names . - Springer 2003. (English)
  3. ↑ Gérard Faure Description of the system of asteroids as of May 20, 2004 (unopened) (link not available) . Archived on November 5, 2004. (eng.)
  4. ↑ Simonenko, AN; LM Sherbaum and VG Kruchinenko. On the character of evolution of orbits in the vicinity of the 1: 3 Kirkwood gap (English) // Icarus: journal. - 1979. - Vol. 40 . - P. 335-340 . (eng.)
  5. ↑ A. Rosaev Aten-Alinda orbital evolution: the example of possible interacting orbits (neopr.) . Archived December 10, 2012. FGUP NPC "Nedra"

Links

  • NASA JPL Small Solar System Bodies (887 )
  • Small Solar System MPC Database (887 )
Source - https://ru.wikipedia.org/w/index.php?title=(887)_Alinda&oldid=100067566


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