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  1. Asteroid belt - Wikipedia

    en.wikipedia.org/wiki/Main_belt

    Current main belt asteroids that originated as Centaurs or trans-Neptunian objects may lie in the outer belt with short lifetime of less than 4 million years, most likely between 2.8 and 3.2 AU at larger eccentricities than typical of main belt asteroid.

  2. The asteroid belt or main belt is a ring of small and large rocks and dust between the orbits of Mars and Jupiter. The biggest object in the asteroid belt is Ceres , a dwarf planet . The Kirkwood gaps separate the asteroid belt into several groups.

  3. Main-belt comet - Wikipedia

    en.wikipedia.org/wiki/Draft:Active_asteroid

    Main-belt comets (MBCs) are bodies orbiting within the asteroid belt that have shown comet-like activity during part of their orbit. The Jet Propulsion Laboratory defines a main-belt asteroid as an asteroid with a semi-major axis (average distance from the Sun) of more than 2 AU but less than 3.2 AU, and a perihelion (closest approach distance to the Sun) of no less than 1.6 AU.

  4. Ceres (dwarf planet) - Wikipedia

    en.wikipedia.org/wiki/Ceres_(dwarf_planet)

    Ceres (/ ˈ s ɪər iː z /; minor-planet designation: 1 Ceres) is the largest object in the main asteroid belt that lies between the orbits of Mars and Jupiter.With a diameter of 940 km (580 mi), Ceres is both the largest of the asteroids and the only dwarf planet inside Neptune's orbit.

  5. Active asteroid - Wikipedia

    en.wikipedia.org/wiki/Main-belt_comets

    Active asteroids are small Solar System bodies that have asteroid-like orbits but show comet-like visual characteristics.That is, they show comae, tails, or other visual evidence of mass-loss (like a comet), but their orbit remains within Jupiter's orbit (like an asteroid).

  6. Flora family - Simple English Wikipedia, the free encyclopedia

    simple.m.wikipedia.org/wiki/Flora_family

    The Flora family of asteroids is a big group of S-type asteroids in the closer part of the main belt, whose origin and properties are not well understood right now.About 4-5% of all main belt asteroids belong to this family.

  7. Tropical cyclone - Wikipedia

    www.wikipedia.org/search-redirect.php?family=...

    "Tropical" refers to the geographical origin of these systems, which form almost exclusively over tropical seas. "Cyclone" refers to their winds moving in a circle, [5] whirling round their central clear eye , with their winds blowing counterclockwise in the Northern Hemisphere and clockwise in the Southern Hemisphere .

  8. Vesta is the second-most massive body in the asteroid belt. Vesta does have a different interior compared to its surface. It is in the Inner Main Belt, at a distance of about 2.50 AU. It is similar to 2 Pallas in volume (although it is not confirmed), but somewhat more massive.

  9. メインベルト彗星 - Wikipedia

    ja.wikipedia.org/wiki/メインベルト彗星

    メインベルト彗星 (main-belt comet, MBC) は、小惑星帯内を周回し、軌道の一部において彗星のような活動が見られた天体である。 ジェット推進研究所 は、メインベルトの小惑星を、 軌道長半径 が2 天文単位 以上、3.2天文単位未満であって、 近日点 が1.6天文 ...

  10. Felicia - Wikipedia

    en.wikipedia.org/wiki/Felicia

    The name Felicia derives from the Latin adjective felix, meaning "happy, lucky", though in the neuter plural form felicia it literally means "happy things" and often occurred in the phrase tempora felicia, "happy times". The sense of it as a feminine personal name appeared in post-Classical use and is of uncertain origin.