Group of asteroids in the asteroid belt that orbit the Sun between 1.78 and 2.00AU
"Hungaria asteroid" redirects here. For the namesake asteroid from which the group takes its name, see 434 Hungaria.
The Hungaria asteroids, also known as the Hungaria group, are a dynamical group of asteroids in the asteroid belt[1] which orbit the Sun with a semi-major axis (longest radius of an ellipse) between 1.78 and 2.00 astronomical units (AU).[2] 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 (FIN: 003), a collisional asteroid family which dominates its population.[3][4]
^Cite error: The named reference Spratt-1990 was invoked but never defined (see the help page).
^Cite error: The named reference Warner-2009 was invoked but never defined (see the help page).
^Ćuk, Matija; Gladman, Brett J.; Nesvorný, David (2014). "Hungaria asteroid family as the source of aubrite meteorites". Icarus. 239: 154–159. arXiv:1406.0825. Bibcode:2014Icar..239..154C. doi:10.1016/j.icarus.2014.05.048.
^Galiazzo, Mattia A.; Bazsó, Ákos; Dvorak, Rudolf (2013). "Fugitives from the Hungaria region: Close encounters and impacts with terrestrial planets". Planetary and Space Science. 84: 5–13. arXiv:1210.1418. Bibcode:2013P&SS...84....5G. doi:10.1016/j.pss.2013.03.017.
and 23 Related for: Hungaria asteroids information
The Hungariaasteroids, also known as the Hungaria group, are a dynamical group of asteroids in the asteroid belt which orbit the Sun with a semi-major...
asteroid Hungaria group, a group of asteroids named after 434 Hungaria This disambiguation page lists articles associated with the title Hungaria. If an...
The Hungariaasteroids lie closer to the Sun than the 4:1 resonance, but are protected from disruption by their high inclination. When the asteroid belt...
inner asteroid belt. It is an E-type (high-albedo) asteroid. It is the namesake of the Hungariaasteroids, which orbit the Sun on the inside of the 1:4 Kirkwood...
main-belt asteroids with a diameter above 10 km (6.2 mi) have already been discovered, there might be as many as 10 trillion 1 m (3.3 ft)-sized asteroids or...
An asteroid family is a population of asteroids that share similar proper orbital elements, such as semimajor axis, eccentricity, and orbital inclination...
near-Earth asteroids, centaurs, comets, and scattered disc objects. Apollo asteroid Centaur (small Solar System body) Hungariaasteroids List of possible...
their orbits: Main Asteroid belt (main belt), between Mars and Jupiter, in near circular orbit, 2.2 to 3.2 AU Hungariaasteroids, small group, 1.78 to...
Enstatite is thought to be a main component of the E-type asteroids. The Hungariaasteroids are the main examples in the Solar System. A layer of quartz...
1981 LA, is a Hungaria family asteroid from the innermost regions of the asteroid belt, approximately 5 kilometers in diameter. The asteroid was discovered...
Einstein (prov. designation: 1973 EB) is a bright Hungariaasteroid from the innermost region of the asteroid belt. It was discovered by Swiss astronomer Paul...
provisional designation 1938 YG, is a rare-type Hungariaasteroid and binary system from the inner regions of the asteroid belt, approximately 8 kilometers in diameter...
"Relationship of E-type Apollo asteroid 3103 (1982 BB) to the enstatite achondrite meteorites and the Hungariaasteroids". Icarus. 100 (1): 95–109. Bibcode:1992Icar...
of Lithuania. Litva is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. It orbits the Sun...
provisional designation 1994 LE3, is a Hungariaasteroid and synchronous binary system from the inner regions of the asteroid belt, approximately 3 kilometers...
around the asteroid on 27 February 2015. Kenos is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar...
positions, with a remnant remaining as the Hungariaasteroids. Some D-type asteroids are embedded in the inner asteroid belt, within 2.5 au, during encounters...
core member of the Hungaria family (003), a large family of bright asteroids that forms the innermost dense concentration of asteroids in the Solar System...
provisional designation: 1983 EA, is a stony Hungariaasteroid and Mars-crosser from the innermost regions of the asteroid belt, approximately 3.5 kilometers (2...
provisional designation 1935 HE, is a Hungariaasteroid and a suspected contact-binary from the innermost regions of the asteroid belt, approximately 5 kilometers...
order, see List of minor planets. Asteroids are given minor planet numbers, but not all minor planets are asteroids. Minor planet numbers are also given...
not indicate a binary asteroid type, but did add to the data set available for this asteroid; this asteroid is part of the Hungaria group. Nicholas U. Mayall...
provisional designation 1923 NX, is a bright Hungariaasteroid from the innermost regions of the asteroid belt, approximately 5 kilometers in diameter...
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