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Asteroids

The Major Asteroids

Asteroids, also called minor planets, are small rocky bodies that are leftover material from the building of our solar system. Over 250,000 asteroids have been designated to date. Here are the asteroids that can be viewed using a telescope:

Observable Asteroids
      1. Name
      2. Diameter (km) /Mass (kg)
      3. Magnitude
      1. Ceres (dwarf planet)
      2. 975 / 940x1018
      3. 6.8
      1. Pallas
      2. 555 / 210x1018
      3. 7.0
      1. Juno
      2. 267 / 27x1018
      3. 7.6
      1. Vesta
      2. 557 / 260x1018
      3. 5.4
      1. Astraea
      2. 167 / 3x1018
      3. 8.7
      1. Hebe
      2. 185 / 13x1018
      3. 7.7
      1. Iris
      2. 200 / 1.6x1019
      3. 6.8
      1. Flora
      2. 136 / 8.5x1018
      3. 8.5
      1. Metis
      2. 182 / 1.5x1019
      3. 8.4
      1. Hygeia
      2. 407 / 87x1018
      3. 9.1


    Asteroid Groups

    Asteroids are grouped according to their orbit range, as follows:

    Near-Earth Asteroids (NEAs)

    Objects in near-earth orbit. There are about 9,000 objects known ranging from 1 meter to 32 meters in diameter. These asteroids can be further grouped as follows:

    • Atira group: Inside Earth's orbit; semi-major axis less than 1.0 AU
    • Aten group: Cross Earth's orbit; semi-major axis less than 1.0 AU
    • Apollo group: Cross Earth's orbit; semi-major axis greater than 1.0 AU
    • Amor group: Outside Earth's orbit; semi-major axis greater than 1.0 AU

    Main-Belt Asteroids

    The total mass of the asteroid belt is just 4% that of the moon. Millions of asteroids located between the orbits of Mars and Jupiter (1.8 to 4.0 AU) are in the "asteroid belt".

    Trojan Asteroids

    Mainly, two large groups of asteroids located along the orbital path of Jupiter, 60 degrees ahead and behind the planet at the trojan points. There are also eight Mars Trojans and one Earth Trojan known.



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