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The Apollo asteroids are a group of near-Earth asteroids named after 1862 Apollo, discovered by German astronomer Karl Reinmuth in the 1930s. They have an orbital semi-major axis greater than that of the Earth (a > 1 AU) but perihelion distances less than the Earth's aphelion distance (q < 1.017 AU).
List[]
Designation | Year | Discovered/First Observed | Reference |
---|---|---|---|
2019 SU 3 | 2019 | ATLAS-HKO | N/A |
2016 WF 9 | 2016 | NEOWISE | N/A |
2014 JO 25 | 2014 | CSS | N/A |
Small Solar System Bodies including comets | ||
---|---|---|
Cis-Neptunian | NEO | ꞌAylóꞌchaxnim • Atrias • Apollos • Arjunas • Amors • Venus Trojan • Earth Trojans • Mars Trojans • Quasi-Satellites |
Main Belt/Jupiter Trojans | Asteroids • Various Collisional Families • Ceres/Vesta Trojans • Hilda • Jupiter Trojans • Quasi-Satellites | |
Distant/Centaur | Centaur • Damocloid • Saturn Trojan • Uranus Trojans • Neptune Trojans | |
TNO | Kuiper Belt/KBO | Classical (Cold • Hot) • Resonant (Plutino • Twotino) |
Scattered disc/SDO | Resonant | |
ETNO | ESDO | |
EDDO | Sednoid → Oort Cloud Objects | |
Comets | NEC • Sungrazing/Kreutz Sungrazing • Remnant • Extinct • Lost • Jupiter • Quasi-Hilda • Halley-type |