Aten asteroid


The Aten asteroids are a dynamical group of asteroids whose orbits bring them into proximity with Earth. By definition, Atens are Earth-crossing asteroids. The group is named after 2062 Aten, the first of its kind, discovered on 7 January 1976 by American astronomer Eleanor Helin at Palomar Observatory. As of 2019, 1490 Atens have been discovered, of which 12 are named. Many Atens are classified as potentially hazardous asteroids.

Description

Aten asteroids are defined by having a semi-major axis of less than 1.0 astronomical unit, the roughly average distance from the Earth to the Sun. They also have an aphelion greater than 0.983 AU. This defines them as Earth-crossing asteroids as the orbit of Earth varies between 0.983 and 1.017 AU.
Asteroids' orbits can be highly eccentric. Nearly all known Aten asteroids have an aphelion greater than 1 AU. Observation of objects inferior to the Earth's orbit is difficult, and this difficulty may contribute to sampling bias in the apparent preponderance of eccentric Atens. Aten asteroids account for only about 7.4% of the known near-Earth asteroid population. Many more Apollo-class asteroids are known than Aten-class asteroids, possibly because of the sampling bias.
The shortest semi-major axis for any known Aten asteroid is 0.580 AU, for object. The Aten asteroid with the smallest known perihelion is also the one with the highest known eccentricity: has an orbit with an eccentricity of 0.895, which takes it from a perihelion of 0.092 AU, well within Mercury's orbit, to an aphelion of 1.66 AU, which is greater than the semi-major axis of Mars. For a brief time near the end of 2004, the asteroid 99942 Apophis apparently posed a threat of impacting Earth in 2029 or 2036, but earlier observations were found that eliminated those possibilities.

Atiras

As of 2019 there are 18 known Atira asteroids, traditionally listed as a subgroup of Atens, but often regarded as a separate asteroid class. Unlike Atens, Atiras permanently reside within, and do not cross, Earth's orbit..