{"id":15716,"date":"2018-07-02T18:46:56","date_gmt":"2018-07-02T16:46:56","guid":{"rendered":"http:\/\/karmaka.de\/?p=15716"},"modified":"2018-07-02T18:49:01","modified_gmt":"2018-07-02T16:49:01","slug":"the-common-origin-of-family-and-non-family-asteroids","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=15716","title":{"rendered":"The common origin of family and non-family asteroids"},"content":{"rendered":"<p>Stanley F. Dermott, Apostolos A. Christou, Dan Li, Thomas. J. J. Kehoe &#038; J. Malcolm Robinson <\/p>\n<p>Nature Astronomy (2018) <\/p>\n<p><a href=\"https:\/\/www.nature.com\/articles\/s41550-018-0482-4\" target=\"_blank\"><strong>LINK<\/strong><\/a><\/p>\n<p>&#8220;All asteroids are currently classified as either family, originating from the disruption of known bodies1, or non-family. An outstanding question is the origin of these non-family asteroids. Were they formed individually, or as members of known families but with chaotically evolving orbits, or are they members of old ghost families, that is, asteroids with a common parent body but with orbits that no longer cluster in orbital element space? Here, we show that the sizes of the non-family asteroids in the inner belt are correlated with their orbital eccentricities and anticorrelated with their inclinations, suggesting that both non-family and family asteroids originate from a small number of large primordial planetesimals. We estimate that ~85% of the asteroids in the inner main belt originate from the Flora, Vesta, Nysa, Polana and Eulalia families, with the remaining ~15% originating from either the same families or, more likely, a few ghost families. These new results imply that we must seek explanations for the differing characteristics of the various meteorite groups in the evolutionary histories of a few, large, precursor bodies2. Our findings also support the model that asteroids formed big through the gravitational collapse of material in a protoplanetary disk3.&#8221;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Stanley F. Dermott, Apostolos A. Christou, Dan Li, Thomas. J. J. Kehoe &#038; J. Malcolm Robinson Nature Astronomy (2018) LINK &#8220;All asteroids are currently classified as either family, originating from the disruption of known bodies1,&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[28,77,8,7,137,337,186],"tags":[3433,3514,1854,2932,4606,2071,257,4605,4604,4603,1872],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/15716"}],"collection":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=15716"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/15716\/revisions"}],"predecessor-version":[{"id":15717,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/15716\/revisions\/15717"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=15716"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=15716"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=15716"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}