{"id":6656,"date":"2016-10-25T15:58:48","date_gmt":"2016-10-25T12:58:48","guid":{"rendered":"http:\/\/www.inasan.ru\/?p=6656"},"modified":"2018-03-12T13:51:30","modified_gmt":"2018-03-12T10:51:30","slug":"ako_seminar_33","status":"publish","type":"post","link":"http:\/\/www.inasan.ru\/en\/ako_seminar_33\/","title":{"rendered":"Minor bodies of the Solar system  (26.10.2016, 15:00)"},"content":{"rendered":"<p><b>Date: <span style=\"color: #0000ff;\">26.10 2016., 15:00 <\/span><\/b><\/p>\n<p><b><a href=\"http:\/\/www.inasan.rssi.ru\/cgi-bin\/seminar2\/propusk.pl?semno=31\"><span style=\"font-size: small;\">To request a pass to the seminar<\/span><\/a><\/b><\/p>\n<p><strong>Speaker:<\/strong> <i><span style=\"color: #0000ff;\"><span style=\"color: #000000;\"><span style=\"font-family: Times New Roman,serif;\"><span style=\"font-size: medium;\"><span lang=\"en-US\" xml:lang=\"en-US\"><span style=\"color: #0000ff;\">Khamroev Umed, Institute of Astrophysics of the Academy of Sciences of the Republic of Tajikistan.<\/span> <\/span><\/span><\/span><\/span><\/span><\/i><\/p>\n<p><i><\/i><span style=\"color: #0000ff;\"><span style=\"color: #000000;\"><span style=\"font-family: Times New Roman,serif;\"><span style=\"font-size: medium;\"><span lang=\"en-US\" xml:lang=\"en-US\"><strong>Title:<\/strong><em><span style=\"color: #0000ff;\"> Asteroid-meteoro<wbr \/>id complex of Sigma-Capricorni<wbr \/>ds. <\/span><\/em><\/span><\/span><\/span><\/span><\/span><i><span style=\"color: #0000ff;\"><br \/>\n <\/span><\/i><\/p>\n<p><strong><span style=\"color: #000000;\"><span style=\"font-family: Times New Roman,serif;\"><span style=\"font-size: medium;\"><span lang=\"en-US\" xml:lang=\"en-US\">Abstract:<\/span><\/span><\/span><\/span><\/strong><\/p>\n<p><span style=\"color: #000000;\"><span style=\"font-family: Times New Roman,serif;\"><span style=\"font-size: medium;\"><span lang=\"en-US\" xml:lang=\"en-US\"> Investigation of physical and dynamical features of the Sigma-Capricorni<wbr \/>d meteoroids by the results of observations as well the determination of NEAs associated with this stream is the main purpose of this work. Observations of the Sigma-Capricorni<wbr \/>d fireballs were carried out by the fireball network of the IA Ac.Sci. RT. As a result of processing of corresponding fireballs records the trajectories, radiants, velocities, orbits, masses and densities of fireball producing meteoroids of this shower were determined, and their cometary nature was shown. The stream producing this shower is associated with NEA Adonis. Three new NEAs were found among asteroids which were discovered during 2008-13. Investigation of orbital evolution has also shown related link of these NEAs with the Sigma-Capricorni<wbr \/>d stream. A common cometary origin of the objects under consideration was suggested. Thus, asteroid-meteoro<wbr \/>id complex of NEOs Sigma-Capricorni<wbr \/>ds consists of the meteoroid stream producing four meteor showers, and several large sized objects presenting extinct fragments of a comet-progenitor of the stream.<\/span><\/span><\/span><\/span><\/p>\n<p>&nbsp;<\/p>\n<p><span lang=\"EN-US\"><strong>Speaker:<\/strong> <span style=\"color: #0000ff;\">Bakhtigaraev\u00a0N.S., INASAN. <\/span><\/span><\/p>\n<p><span lang=\"EN-US\"><span style=\"color: #0000ff;\"><span style=\"color: #000000;\"><span style=\"font-family: Times New Roman,serif;\"><span style=\"font-size: medium;\"><span lang=\"en-US\" xml:lang=\"en-US\"><strong>Title:<\/strong><\/span><\/span><\/span><\/span><\/span> <span style=\"color: #0000ff;\">On the restoration of the Zeiss-1000 telescope \u00a0in \u00a0Sanglokh \u00a0Observatory (Institute of astrophysics of the Academy of \u00a0Sciences of \u00a0the \u00a0Republic of Tajikistan) \u00a0and plans for joint scientific research.<\/span> <\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Date: 26.10 2016., 15:00 To request a pass to the seminar Speaker: Khamroev Umed, Institute of Astrophysics of the Academy of Sciences of the Republic of Tajikistan. Title: Asteroid-meteoroid complex of Sigma-Capricornids. Abstract: Investigation of physical and dynamical features of the Sigma-Capricornid meteoroids by the results of observations as well the determination of NEAs associated<\/p>\n<div class=\"read-more\"><a href=\"http:\/\/www.inasan.ru\/en\/ako_seminar_33\/\">Continue Reading&rsaquo;&rsaquo;<\/a><\/div>\n","protected":false},"author":7,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[23],"tags":[],"class_list":["post-6656","post","type-post","status-publish","format-standard","hentry","category-akoseminar"],"translation":{"provider":"WPGlobus","version":"3.0.0","language":"en","enabled_languages":["ru","en"],"languages":{"ru":{"title":true,"content":true,"excerpt":false},"en":{"title":true,"content":true,"excerpt":false}}},"_links":{"self":[{"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/posts\/6656","targetHints":{"allow":["GET"]}}],"collection":[{"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/users\/7"}],"replies":[{"embeddable":true,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/comments?post=6656"}],"version-history":[{"count":19,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/posts\/6656\/revisions"}],"predecessor-version":[{"id":8982,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/posts\/6656\/revisions\/8982"}],"wp:attachment":[{"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/media?parent=6656"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/categories?post=6656"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/www.inasan.ru\/en\/wp-json\/wp\/v2\/tags?post=6656"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}