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  1. The Koronis or Koronian family (FIN: 605), also known as the Lacrimosa family,: 16 is a very large asteroid family of stony asteroids, located in the outer region of the asteroid belt. They are thought to have been formed at least two billion years ago in a catastrophic collision between two larger bodies.

  2. La familia de Coronis es una familia de asteroides situada en el cinturón de asteroides. Se cree que son los restos rotos de un solo cuerpo que fue destruido por una colisión. La sonda espacial Galileo visitó a uno de los miembros de esta familia, Ida, en 1993. Pertenecen a este grupo 86 asteroides y están situados a una ...

  3. The Koronis or Koronian family, also known as the Lacrimosa family, is a very large asteroid family of stony asteroids, located in the outer region of the asteroid belt. They are thought to have been formed at least two billion years ago in a catastrophic collision between two larger bodies.

  4. Recently formed family is located within the Themis family (all members are also listed as Themistians). Includes (7968) Elst–Pizarro. [10] : 7, 8, 18 cat: 621: Familia de Koronis: K-2: 246: outer: S: 0.14 (158) Koronis "second family" cat: 622: Familia de Terpsichore: TRP: 138: outer: C: 0.05 (81) Terpsichore: cat: 623: Familia de Fringilla ...

  5. The family is named after 158 Koronis, and the largest known member (208 Lacrimosa) is about 41 km (25 mi) in diameter. The Koronis family travels in a cluster along the same orbit. [1] Over 300 have been found but only about 20 are larger than 20 km in diameter.

  6. en.wikipedia.org › wiki › 243_Ida243 Ida - Wikipedia

    Ida, minor planet designation 243 Ida, is an asteroid in the Koronis family of the asteroid belt. It was discovered on 29 September 1884 by Austrian astronomer Johann Palisa at Vienna Observatory and named after a nymph from Greek mythology.

  7. Some prominent families are the Vesta, Eunomia, Koronis, Eos, and Themis family located in different (colorized) regions of the asteroid belt. An asteroid family is a population of asteroids that share similar proper orbital elements, such as semimajor axis, eccentricity, and orbital inclination.