early solar system
râžmân-e xoršidi-ye âqâzin
Fr.: système solaire primordial
A period in the evolution of the → solar system when the planets and satellites were in the process of formation.
small solar system body
jesm-e kucak-e râžmân-e xoršidi
Fr.: petit corps du système solaire
A term introduced by the → International Astronomical Union (August 2006) to name the → solar system bodies other than → planets and → dwarf planets. Small solar system bodies include → asteroids, → comets, and → meteoroids.
Fr.: Système solaire
The collective name for the Sun and all objects gravitationally bound to it. These objects are the eight planets, their 166 known moons, five dwarf planets, and billions of small bodies. The small bodies include asteroids, icy Kuiper belt objects, comets, meteoroids, and interplanetary dust. The solar system is roughly a sphere with a radius greater than 100,000 AU. Planets, satellites, and all interplanetary material together comprise only about 1/750 of the total mass. Geochemical dating methods show that the solar system chemically isolated itself from the rest of the Galaxy (4.7 ± 0.1) × 109 years ago.
solar system abundance
farâvâni-ye râžmân-e xoršidi
Fr.: abondance dans le système solaire
Same as → protosolar abundance.