flora asteroid family

Asteroid groups and families. The Flora asteroid family, which resides in the innermost region of the main asteroid belt, has been known for nearly a century. Several years passed before the problem of asteroid fam-ily identification was again taken into consideration by Brouwer (1951), who substantially confirmed the Hirayama families, although he divided Flora into four different groups. 02:24, 4 September 2008 (UTC) Conceptual systems Classification systems Grouping Minor planet groups and families. Based on the Asteroid Lightcurve Database (LCDB), the spin rate distribution of the Flora asteroid family is studied, and a tendency that the spin rates of the small Flora family members concentrate primarily in the range of 3-5 d-1 is found. Florian; FIN: 402; also known as Ariadne family) is a prominent family of stony asteroids located in the inner region of the asteroid belt.It is one of the largest families with more than 13,000 known members, or approximately 3.5% of all main-belt asteroids.

The Flora family (adj. The 1995 work also lists the Polana family as a subgroup of the Nysa family, which seems pretty well accepted now, although there is no page or mention of the Polana family as yet. A prominent example is 1 Ceres, the largest asteroid, which is an interloper in the family once named after it (the Ceres family, now the Gefion family). The ∼ 160 Myr-old Baptistina family is recognized by its V-shape in a vs. H space within the HCM-defined Flora family (Bottke, Vokrouhlický, Nesvorný, 2007, Nesvorný, Brož, Carruba, 2015). Curiously, our understanding of its properties has remained fairly murky even as our knowledge of the asteroid belt has increased. The members of the families are thought to be fragments of past asteroid collisions. The Flora asteroid family members defined by the LCDB are distributed in the semi-major axis interval of a ∈ [2.15, 2.35] au (as shown in Fig. The Flora family (adj. Gefion family, Flora family, Eunomia family, Baptistina family, Augusta family, Alinda asteroid. Florian; FIN: 402; also known as Ariadne family) is a prominent family of stony asteroids located in the inner region of the asteroid belt.It is one of the largest families with more than 13,000 known members, or approximately 3.5% of all main-belt asteroids. Since then, and before 1990, several au- a Flora family member and the first asteroid observed by the Galileo spacecraft. The prominent Flora family in the inner part of the asteroid belt shares the same spectral properties, suggesting that it is a dominant source of near-Earth asteroids. Especially, the orbit and spin characteristics can reflect the influences of the Yarkovsky effect and the Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect on the evolution of the asteroid family, respectively. 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. When applying the synthetic hierarchical clustering method (HCM) by Nesvorný, or the 1995 HCM-analysis by Zappalà, Algunde is a member of the Flora family (), a giant asteroid family and the largest family of stony asteroids in the main-belt. The Flora family (adj. Orbit and classification.

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