Solar System belts

[6][7] The Grand tack hypothesis is a model of the unique placement of the giant planets and the Solar System belts.

[3][4][8] Most giant planets found outside our Solar System, exoplanets, are inside the snow line, and are called Hot Jupiters.

[5][9] Thus in normal planetary systems giant planets form beyond snow line and then migrated towards the star.

[12][13] [14][15] The asteroid and comet belts orbit the Sun from the inner rocky planets into outer parts of the Solar System, interstellar space.

[16][17][18] An astronomical unit, or AU, is the distance from Earth to the Sun, which is approximately 150 billion meters (93 million miles).

Comparison of the Oort cloud , Kuiper Belt and the Main Asteroid Belt .
The asteroids of the inner Solar System and Jupiter : The main asteroid belt is located between the orbits of Jupiter and Mars .
Sun
Jupiter trojans
Orbits of planets
Asteroid belt
Hilda asteroids (Hildas)
Near-Earth objects (selection)
Known objects in the Kuiper belt beyond the orbit of Neptune. (Scale in AU ; epoch as of January 2015.)
Sun
Jupiter trojans
Giant planets :
Centaurs
Neptune trojans
Resonant Kuiper belt
Classical Kuiper belt
Scattered disc
Solar System planets
The Sun, the planets, their moons, and several trans-Neptunian objects The Sun Mercury Venus The Moon Earth Mars Phobos and Deimos Ceres The main asteroid belt Jupiter Moons of Jupiter Rings of Jupiter Saturn Moons of Saturn Rings of Saturn Uranus Moons of Uranus Rings of Uranus Neptune Moons of Neptune Rings of Neptune Pluto Moons of Pluto Haumea Moons of Haumea Makemake S/2015 (136472) 1 The Kuiper Belt Eris Dysnomia The Scattered Disc The Hills Cloud The Oort Cloud