(astronomy) A naturally occurring solid object, which is smaller than aplanet and adwarf planet, larger than ameteoroid and not acomet, that orbits a star and often has an irregular shape.
(astronomy) In the Solar system, such a body that orbits within the orbit of Jupiter
2007, Hannu Karttunenet al., editors,Fundamental Astronomy, 5th edition, page131:
The orbital planes ofasteroids, minor bodies that circle the Sun mainly between the orbits of Mars and Jupiter, are often more tilted ...
The term "asteroid" has never been precisely defined. It was coined for objects which looked like stars in a telescope but moved like planets. These were known from theasteroid belt between Mars and Jupiter, and were later found co-orbiting with Jupiter (Trojan asteroids) and within the orbit of Mars. They were naturally distinguished fromcomets, which did not look at all starlike. Starting in the 1970s, small non-cometary bodies were found outside the orbit of Jupiter, and usage became divided as to whether to call these "asteroids" as well. Some astronomers restrict the term "asteroid" to rocky or rocky-icy bodies with orbits up to Jupiter. They may retain the termplanetoid for all small bodies, and thus tend to use it for icy or rocky-icy bodies beyond Jupiter, or may use dedicated words such ascentaurs,Kuiper belt objects,transneptunian objects, etc. for the latter. Other astronomers use "asteroid" for all non-cometary bodies smaller than a planet, even large ones such asSedna and (occasionally)Pluto. However, the distinction between asteroid and comet is an artificial one; many outer "asteroids" would become comets if they ventured nearer the Sun. The IAU terminology since 2006 has beensmall Solar System body for any body that orbits the Sun directly and whose shape is not dominated by gravity.
“asteroid”, in[EKSS] Eesti keele seletav sõnaraamat [Descriptive Dictionary of the Estonian Language] (in Estonian) (online version), Tallinn: Eesti Keele Sihtasutus (Estonian Language Foundation),2009