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・ 2002 Alpine Skiing World Cup – Men's Slalom
・ 2002 Alpine Skiing World Cup – Men's Super G
・ 2002 Alpine Skiing World Cup – Women's Combined
・ 2002 Alpine Skiing World Cup – Women's Downhill
・ 2002 Alpine Skiing World Cup – Women's Giant Slalom
・ 2002 Alpine Skiing World Cup – Women's Slalom
・ 2002 Alpine Skiing World Cup – Women's Super G
・ 2002 Altazor Awards
・ 2002 AMA National Speedway Championship
・ 2002 America East Conference Baseball Tournament
・ 2002 America East Men's Basketball Tournament
・ 2002 American Le Mans at Mid-Ohio
・ 2002 24 Hours of Le Mans
・ 2002 3. Divisjon
・ 2002 4 Nations Cup
2002 AA29
・ 2002 AAPT Championships
・ 2002 AAPT Championships – Doubles
・ 2002 AAPT Championships – Singles
・ 2002 Aaron's 499
・ 2002 ABC Champions Cup
・ 2002 ABC Under-18 Championship
・ 2002 ABC Under-18 Championship for Women
・ 2002 ABC Under-20 Championship for Women
・ 2002 Abierto Mexicano Pegaso
・ 2002 Abierto Mexicano Pegaso – Men's Doubles
・ 2002 Abierto Mexicano Pegaso – Men's Singles
・ 2002 ABN AMRO World Tennis Tournament
・ 2002 ABN AMRO World Tennis Tournament – Doubles
・ 2002 ABN AMRO World Tennis Tournament – Singles


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2002 AA29 : ウィキペディア英語版
2002 AA29

(also written 2002 AA29) is a small near-Earth asteroid that was discovered on January 9, 2002 by the LINEAR ''(Lincoln Near Earth Asteroid Research)'' automatic sky survey. The diameter of the asteroid is only about . It revolves about the Sun on an almost circular orbit very similar to that of the Earth. This lies for the most part inside the Earth's orbit, which it crosses near the asteroid's furthest point from the Sun, the aphelion. Because of this orbit, the asteroid is classified as Aten type,〔 named after the asteroid (2062) Aten.
A further characteristic is that its mean orbital period about the Sun is exactly one sidereal year. This means that it is locked into a relationship with the Earth, since such an orbit is only stable under particular conditions. As yet only a few asteroids of this sort are known, locked into a 1:1 resonance with the Earth. The first was (3753) Cruithne, discovered in 1986.
Asteroids that have a 1:1 orbital resonance with a planet are also called co-orbital objects, because they follow the orbit of the planet. The most numerous known co-orbital asteroids are the so-called trojans, which occupy the L4 and L5 Lagrangian points of the relevant planet. However, does not belong to these. Instead, it follows a so-called horseshoe orbit along the path of the Earth.
== Orbit ==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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