Hungaria asteroids

"Hungaria asteroid" redirects here. For the namesake asteroid from which the group takes its name, see 434 Hungaria.

A top-down and side view of the positions of Hungaria asteroids outside the orbit of Mars as of 15 May 2026. The box shape of the side view is caused by the high inclination of the group.

The Hungaria asteroids, also known as the Hungaria group, are a dynamical group of asteroids in the asteroid belt which orbit the Sun with a semi-major axis between 1.78 and 2.00 astronomical units (AU). They are the innermost dense concentration of asteroids in the Solar System—the near-Earth asteroids are much more sparse—and derive their name from their largest member 434 Hungaria. The Hungaria group includes the Hungaria family, a collisional asteroid family which dominates its population.