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  2. C-type asteroid - Wikipedia

    en.wikipedia.org/wiki/C-type_asteroid

    C-type asteroid. C-type (carbonaceous / ˌkɑːrbəˈneɪʃəs /) asteroids are the most common variety, forming around 75% of known asteroids. [1] They are volatile-rich and distinguished by a very low albedo because their composition includes a large amount of carbon, in addition to rocks and minerals. They have an average density of about 1. ...

  3. Asteroid - Wikipedia

    en.wikipedia.org/wiki/Asteroid

    Sizes are not to scale. An asteroid is a minor planet —an object that is neither a true planet nor an identified comet — that orbits within the inner Solar System. They are rocky, metallic, or icy bodies with no atmosphere, classified as C-type (carbonaceous), M-type (metallic), or S-type (silicaceous). The size and shape of asteroids vary ...

  4. Sierra Nevada Batholith - Wikipedia

    en.wikipedia.org/wiki/Sierra_Nevada_Batholith

    Sierra Nevada Batholith. The Sierra Nevada Batholith is a large batholith that is approximately 400 miles long and 60-80 miles wide which forms the core of the Sierra Nevada mountain range in California, exposed at the surface as granite. [ 1 ]

  5. Asteroid spectral types - Wikipedia

    en.wikipedia.org/wiki/Asteroid_spectral_types

    An asteroid spectral type is assigned to asteroids based on their reflectance spectrum, color, and sometimes albedo. These types are thought to correspond to an asteroid's surface composition. For small bodies that are not internally differentiated, the surface and internal compositions are presumably similar, while large bodies such as Ceres ...

  6. 4 Vesta - Wikipedia

    en.wikipedia.org/wiki/4_Vesta

    Vesta was the fourth asteroid to be discovered, hence the number 4 in its formal designation. The name Vesta, or national variants thereof, is in international use with two exceptions: Greece and China. In Greek, the name adopted was the Hellenic equivalent of Vesta, Hestia (4 Εστία); in English, that name is used for 46 Hestia (Greeks use ...

  7. 511 Davida - Wikipedia

    en.wikipedia.org/wiki/511_Davida

    511 Davida is a large C-type asteroid in the asteroid belt. It is one of the largest asteroids; approximately tied for 7th place, to within measurement uncertainties, and the 5th or 6th most massive. It was discovered by R. S. Dugan in 1903. Davida is named after David Peck Todd, an astronomy professor at Amherst College.

  8. 2015 TC25 - Wikipedia

    en.wikipedia.org/wiki/2015_TC25

    2015 TC25. 2015 TC25 is a near-Earth asteroid, and at only 6 feet (1.8 meters) across and absolute magnitude 29.34 mag, it is thought to be the third smallest asteroid observed over multiple years, after 2021 GM 1 with absolute magnitude 30.4 and 2006 RH 120 with absolute magnitude 29.5. The asteroid is notable for reflecting about 60% of the ...

  9. 7 Iris - Wikipedia

    en.wikipedia.org/wiki/7_Iris

    7 Iris is a large main-belt asteroid and possible remnant planetesimal orbiting the Sun between Mars and Jupiter. It is the fourth-brightest object in the asteroid belt. 7 Iris is classified as an S-type asteroid, meaning that it has a stony composition.