{"id":492,"date":"2018-10-19T07:52:43","date_gmt":"2018-10-19T07:52:43","guid":{"rendered":"http:\/\/aptog.com\/?p=492"},"modified":"2018-10-19T07:54:19","modified_gmt":"2018-10-19T07:54:19","slug":"binary-asteroid-discovery-iau-announcement-5","status":"publish","type":"post","link":"https:\/\/aptog.com\/?p=492","title":{"rendered":"Binary asteroid discovery IAU announcement"},"content":{"rendered":"<p>IAU CBET\u00a04563<\/p>\n<p>(2178) KAZAKHSTANIA<br \/>\nV. Benishek, Belgrade Astronomical Observatory; P. Pravec, H. Kucakova,<br \/>\nand K. Hornoch, Ondrejov Observatory; V. Chiorny, Kharkiv Observatory; F.<br \/>\nPilcher, Organ Mesa Observatory, Las Cruces, NM, U.S.A.; A. Aznar, Astronomia<br \/>\nPara Todos Observatories Group, Spain; and V. Casanova, Observatorio de Sierra<br \/>\nNevada, Instituto de Astrofisica de Andalucia, Consejo Superior de<br \/>\nInvestigaciones Cientificas, report that photometric observations taken with a<br \/>\n0.35-m telescope at the Sopot Observatory in Serbia, a 0.65-m telescope at the<br \/>\nOndrejov Observatory, a 0.70-m telescope at the Chuguev station of the Kharkiv<br \/>\nObservatory in Ukraine, a 0.35-m telescope at the Organ Mesa Observatory, and<br \/>\na 0.90-m telescope at Sierra Nevada Observatory during Sept. 18-Oct. 15 reveal<br \/>\nthat minor planet (2178) is a binary system with an orbital period of 18.504<br \/>\n\u00b1 0.006 hr. The primary shows a period of 3.0183 \u00b1 0.0002 hr and has a<br \/>\nlight-curve amplitude of 0.31 mag at solar phases 8-11 degrees. Mutual<br \/>\neclipse\/occultation events that are 0.07 to 0.15 magnitude deep indicate a<br \/>\nsecondary-to-primary mean-diameter ratio of 0.26 \u00b1 0.02. The secondary<br \/>\nappears synchronous and has a light-curve amplitude (in the combined primary<br \/>\nplus secondary light curve) of 0.02 mag, suggesting a moderately elongated<br \/>\nshape with the equatorial axis ratio of 1.3 \u00b1 0.1.<\/p>\n<p>http:\/\/www.cbat.eps.harvard.edu\/cbet\/RecentCBETs.html<\/p>\n","protected":false},"excerpt":{"rendered":"<p>IAU CBET\u00a04563 (2178) KAZAKHSTANIA V. Benishek, Belgrade Astronomical Observatory; P. Pravec, H. Kucakova, and K. Hornoch, Ondrejov Observatory; V. Chiorny, Kharkiv Observatory; F. Pilcher, Organ Mesa Observatory, Las Cruces, NM, U.S.A.; A. Aznar, Astronomia Para Todos Observatories Group, Spain; and V. Casanova, Observatorio de Sierra Nevada, Instituto de Astrofisica de Andalucia, Consejo Superior de Investigaciones [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"footnotes":""},"categories":[7],"tags":[],"class_list":["post-492","post","type-post","status-publish","format-standard","hentry","category-papers-and-letters"],"acf":[],"_links":{"self":[{"href":"https:\/\/aptog.com\/index.php?rest_route=\/wp\/v2\/posts\/492","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/aptog.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/aptog.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/aptog.com\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/aptog.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=492"}],"version-history":[{"count":1,"href":"https:\/\/aptog.com\/index.php?rest_route=\/wp\/v2\/posts\/492\/revisions"}],"predecessor-version":[{"id":493,"href":"https:\/\/aptog.com\/index.php?rest_route=\/wp\/v2\/posts\/492\/revisions\/493"}],"wp:attachment":[{"href":"https:\/\/aptog.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=492"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/aptog.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=492"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/aptog.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=492"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}