Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/1168
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dc.contributor.authorNovaković, Bojanen_US
dc.contributor.authorVokrouhlický, Daviden_US
dc.contributor.authorSpoto, Federicaen_US
dc.contributor.authorNesvorný, Daviden_US
dc.date.accessioned2022-09-23T17:57:44Z-
dc.date.available2022-09-23T17:57:44Z-
dc.date.issued2022-
dc.identifier.issn09232958en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/1168-
dc.description.abstractCollisions are one of the key processes shaping planetary systems. Asteroid families are outcomes of such collision still identifiable across our solar system. The families provide a unique view of catastrophic disruption phenomena and have been in the focus of planetary scientists for more than a century. Most of them are located in the main belt, a ring of asteroids between Mars and Jupiter. Here we review the basic properties of the families, discuss some recent advances, and anticipate future challenges. This review pays more attention to dynamic aspects such as family identification, age determination, and long-term evolution. The text, however, goes beyond that. Especially, we cover the details of young families that see the major advances in the last years, and we anticipate it will develop even faster in the future. We also discuss the relevance of asteroid families for water-ice content in the asteroid belt and our current knowledge on links between families and main-belt comets. query Please check the edit made in the article title.en_US
dc.relation.ispartofCelestial Mechanics and Dynamical Astronomyen
dc.subjectCollisional asteroid familiesen_US
dc.subjectSmall bodiesen_US
dc.subjectSolar systemen_US
dc.titleAsteroid families: properties, recent advances, and future opportunitiesen_US
dc.typeArticleen_US
dc.identifier.doi10.1007/s10569-022-10091-7-
dc.identifier.scopus2-s2.0-85134622500-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85134622500-
dc.contributor.affiliationAstronomyen_US
dc.description.rankM22en_US
dc.relation.volume134en
dc.relation.issue4en
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.grantfulltextnone-
item.openairetypeArticle-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-6349-6881-
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