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Assigning a family to a minor planet is challenging. Depending on different models (HCM), cut-off limits, and new insights, the results can vary significantly. This project page summarizes the current status. For each notable family, a subpage lists all members (grouped into existing and non-existing minor-planet object pages). Based on the used source(s), approximately 100,000 numbered minor planets (out of 500k numbered bodies) have been assigned to one of 100+ families.

The systematic listing of all sourced family members in the sub-pages of this summary page may be used to evaluate the feasibility and value for changes in categorization and catalog-listing of minor planet on wikipedia.

• Rfassbind/Minor planet family members atESA–space situational awareness
  • Summary · Orbit · Physical Properties · Observations · Ephemerides
• Rfassbind/Minor planet family members atESA–space situational awareness
  • Summary · Orbit · Physical Properties · Observations · Ephemerides
• Rfassbind/Minor planet family members atESA–space situational awareness
  • Summary · Orbit · Physical Properties · Observations · Ephemerides
• Rfassbind/Minor planet family members atESA–space situational awareness
  • Summary · Orbit · Physical Properties · Observations · Ephemerides
• Rfassbind/Minor planet family members atESA–space situational awareness
  • Summary · Orbit · Physical Properties · Observations · Ephemerides

Based on the notable asteroid families list by"Identification and Dynamical Properties of Asteroid Families",D. Nesvorny, M. Broz, V. Carrubaall (2014), Table 2 on page 23:Brož et al., (2013)

• Referenced sourceSmall Bodies Data Ferret
• Access WebTool
• Similar source:project data, slightly older/outdated: Broz (2013), cite listed below
• AsteroidFamiliesPortal website maintained by the Department of Astronomy at the Faculty of Mathematics of the University of Belgrade

• Interlopers

• ADS: Broz-2013

<ref name="Broz-2013">{{Cite journal  |first1     = M. |last1 = Broz  |first2     = A. |last2 = Morbidelli  |first3     = W. F. |last3 = Bottke  |first4     = J. |last4 = Rozehnal  |first5     = D. |last5 = Vokrouhlický  |first6     = D. |last6 = Nesvorný  |date       = March 2013  |title      = Constraining the cometary flux through the asteroid belt during the late heavy bombardment  |url        = https://arxiv.org/pdf/1301.6221.pdf  |journal    = Astronomy and Astrophysics  |volume     = 551  |page       = 16  |bibcode    = 2013A&A...551A.117B  |doi        = 10.1051/0004-6361/201219296  |arxiv      = 1301.6221  |access-date= 23 June 2017}}</ref>

• ADS: Nesvorny-2014,PDF

<ref name="Nesvorny-2014">{{Cite journal  |first1     = D. |last1 = Nesvorný  |first2     = M. |last2 = Broz  |first3     = V. |last3 = Carruba  |date       = December 2014  |title      = Identification and Dynamical Properties of Asteroid Families  |url        = https://arxiv.org/pdf/1502.01628.pdf  |journal    = Asteroids IV  |pages      = 297–321  |bibcode    = 2015aste.book..297N   |doi        = 10.2458/azu_uapress_9780816532131-ch016  |arxiv      = 1502.01628  |access-date= 23 June 2017}}</ref>{{rp|23}}<ref name="Ferret">{{cite web  |title      = Small Bodies Data Ferret  |work       = Nesvorny HCM Asteroid Families V3.0  |url        = http://sbntools.psi.edu/ferret/PropertySearch/familyForm.action  |accessdate = 22 July 2017}}</ref>

• ADS: Nesvorny-2014,PDF, 23–26