About: Padua family

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The Padua family (FIN: 507), also known as the Lydia family, is a mid-sized family of asteroids of more than a thousand members. The family is at least 25 million years old. Its members were previously associated to 110 Lydia, and are predominantly X-type asteroids with an albedo of approximately 0.1. Together with the Agnia family, the Padua family is the only other family to have most of its members in a nonlinear secular resonance configuration with more than 75% of its members in a z1 librating state.

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  • The Padua family (FIN: 507), also known as the Lydia family, is a mid-sized family of asteroids of more than a thousand members. The family is at least 25 million years old. Its members were previously associated to 110 Lydia, and are predominantly X-type asteroids with an albedo of approximately 0.1. Together with the Agnia family, the Padua family is the only other family to have most of its members in a nonlinear secular resonance configuration with more than 75% of its members in a z1 librating state. The Paduan (Lydian) asteroids are located in the outer part of the central asteroid belt having a semi-major axis of approximately 2.75. The family's namesake is the asteroid 363 Padua, while 110 Lydia is now a suspected interloper, despite having the same spectral type. (en)
  • La famille de Lydie est une petite famille d'astéroïdes de la ceinture principale à une distance moyenne de 2,75 UA du soleil. Les membres de cette famille ont une composition variable. La famille est nommée d'après l'objet de type M (110) Lydie, le plus grand membre étant l'objet de type T (308) Polyxo. (fr)
  • A família Lydia é uma pequena família de asteroides localizados no cinturão principal. A família foi nomeada devido ao primeiro asteroide que foi classificado neste grupo, o 110 Lydia. (pt)
  • Семейство Лидии — небольшое семейство астероидов, расположенное в главном поясе. Семейство названо в честь первого астероида, классифицированного в эту группу — (110) Лидия. (ru)
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  • La famille de Lydie est une petite famille d'astéroïdes de la ceinture principale à une distance moyenne de 2,75 UA du soleil. Les membres de cette famille ont une composition variable. La famille est nommée d'après l'objet de type M (110) Lydie, le plus grand membre étant l'objet de type T (308) Polyxo. (fr)
  • A família Lydia é uma pequena família de asteroides localizados no cinturão principal. A família foi nomeada devido ao primeiro asteroide que foi classificado neste grupo, o 110 Lydia. (pt)
  • Семейство Лидии — небольшое семейство астероидов, расположенное в главном поясе. Семейство названо в честь первого астероида, классифицированного в эту группу — (110) Лидия. (ru)
  • The Padua family (FIN: 507), also known as the Lydia family, is a mid-sized family of asteroids of more than a thousand members. The family is at least 25 million years old. Its members were previously associated to 110 Lydia, and are predominantly X-type asteroids with an albedo of approximately 0.1. Together with the Agnia family, the Padua family is the only other family to have most of its members in a nonlinear secular resonance configuration with more than 75% of its members in a z1 librating state. (en)
rdfs:label
  • Famille de Lydie (fr)
  • Padua family (en)
  • Família Lydia (pt)
  • Семейство Лидии (ru)
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