asteroid belt
(ring of orbiting planetoids/asteroids)
The Asteroid Belt is the torus-shaped region of the solar system
between Mars and Jupiter where many asteroids orbit,
which includes more than 90% of known minor planets.
The term is also used in a more general sense for various
regions of the solar system with smaller populations
of similar bodies, so the above-defined asteroid belt
may be called the main asteroid belt or main belt
and an asteroid within it a main belt asteroid (MBA).
Among the other asteroid populations (called asteroid families):
- Trojan asteroids (or just Trojans), orbiting in the Trojan Points, i.e., the Sun-Jupiter Lagrangian points, L4 and L5. Smaller populations are in the equivalent points for other planets, so they are sometimes distinguished as Jupiter Trojans versus, e.g., Neptune Trojans.
- near Earth asteroids (NEAs), i.e., rocky near-Earth objects (rocky NEOs, as opposed to NEOs that are comets).
(minor planets,solar system,asteroids)
Further reading:
https://en.wikipedia.org/wiki/Asteroid_belt
https://en.wikipedia.org/wiki/Trojan_(astronomy)
https://en.wikipedia.org/wiki/Near-Earth_object#Near-Earth_asteroids_(NEAs)
https://astronomy.swin.edu.au/cosmos/a/asteroid+belt
https://astronomy.swin.edu.au/cosmos/N/Near+Earth+Asteroids
https://astronomy.swin.edu.au/cosmos/T/Trojan+Asteroids
https://en.wiktionary.org/wiki/asteroid_belt
http://www.pas.rochester.edu/~blackman/ast104/afeatures.html
https://wisp.physics.wisc.edu/astro104/lecture19/lec19g.html
https://www.coe.edu/faculty-staff/james-wetzel/astronomy/asteroids
Referenced by pages:
2010 TK7
asteroid
Ceres
circumstellar disk
debris disk
grand tack hypothesis
halo orbit
Kuiper Belt (K Belt)
Lagrangian point
late heavy bombardment (LHB)
Lucy
Nice model
Palomar-Leiden Survey (PLS)
planetoid
Psyche
solar system object (SSO)
Index