{"id":671,"date":"2016-08-12T13:32:50","date_gmt":"2016-08-12T13:32:50","guid":{"rendered":"http:\/\/www.radio-science.eu\/?page_id=671"},"modified":"2023-11-10T14:11:16","modified_gmt":"2023-11-10T14:11:16","slug":"rosetta-mission","status":"publish","type":"page","link":"https:\/\/fip-koeln.de\/en_us\/missionen-und-ziele\/rosetta\/rosetta-mission\/","title":{"rendered":"Rosetta Mission"},"content":{"rendered":"<figure class=\"wp-block-image alignright\"><a href=\"https:\/\/fip-koeln.de\/wp-content\/uploads\/2012\/11\/rosetta01.jpg\"><img loading=\"lazy\" decoding=\"async\" width=\"270\" height=\"203\" src=\"https:\/\/fip-koeln.de\/wp-content\/uploads\/2012\/11\/rosetta01.jpg\" alt=\"Rosetta's Earth-Flyby Quelle: ESA\" class=\"wp-image-94\"\/><\/a><figcaption class=\"wp-element-caption\">Rosetta&#8217;s Earth-Flyby<br>Source: ESA<\/figcaption><\/figure>\n\n\n\n<p>Rosetta is the first mission which will escort a comet from almost aphelion to perhelion and beyond. The ESA spacecraft was launched on 2nd May 2004 by a Ariane-V rocket for a ten year circuit until arrival at 67P\/Churyumov-Gerasimenko in 2014. Rosetta used several flybys at Earth and Mars to gain momentum.<br>Am 2. M\u00e4rz 2004 startete die ESA-Raumsonde ihre zehnj\u00e4hrige Reise zum Kometen Churyumov-Gerasimenko mit einer Ariane-5 Rakete von Kourou, Franz\u00f6sisch-Guayana. Bis zu ihrer Ankunft im Jahr 2014 hat Rosetta mehrere Vorbeifl\u00fcge an Erde und Mars genutzt (sog. &#8222;swing-bys&#8220;), um gen\u00fcgend Schwung zum Erreichen des Kometen zu holen. Es besteht das Ziel, den Kometen Churyumov-Gerasimenko ganz aus der N\u00e4he zu studieren, ihn f\u00fcr viele Monate zu begleiten und mit einem Lander auf der Kometenoberfl\u00e4che zu landen. Da sich der Komet w\u00e4hrend dieser Zeit immer n\u00e4her auf die Sonne zubewegt, wird es somit erstmalig m\u00f6glich sein, die Ver\u00e4nderungen des Kometen bei seiner Reise \u00fcber mehrere Millionen Kilometer durch das All zu untersuchen. Dar\u00fcber hinaus ist Rosetta auf ihrem Weg in das \u00e4u\u00dfere Sonnensystem an zwei Asteroiden, Steins und Lutetia vorbeigeflogen.<\/p>\n\n\n\n<h3 class=\"wp-block-heading\">Rosetta \u2013 Data<\/h3>\n\n\n\n<figure class=\"wp-block-table is-style-stripes\"><table><tbody><tr><th colspan=\"2\"><strong>Mission<\/strong><\/th><\/tr><tr><td>Launch<\/td><td>2nd March 2004, 08:17 am MEZ<\/td><\/tr><tr><td>Launch site<\/td><td>Kourou, French Guayana<\/td><\/tr><tr><td>Launcher rocket<\/td><td>ARIANE 5 G<\/td><\/tr><tr><td>Duration of the mission<\/td><td>In total 12 years, until December 2015<\/td><\/tr><tr><td>Mission Control Center<\/td><td>European Space Operations Center (ESOC), Darmstadt<\/td><\/tr><tr><td>Philae Lander Control Center<\/td><td>DLR MUSC, Cologne<\/td><\/tr><tr><td>ground stations<\/td><td>Perth (Australia), Kourou (French Guayana)<\/td><\/tr><tr><td>Start weight<\/td><td>3,000 kg<\/td><\/tr><tr><td>Fuel<\/td><td>1,670 kg<\/td><\/tr><tr><td>Scientific payload<\/td><td>165 kg<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n<figure class=\"wp-block-table is-style-stripes\"><table><tbody><tr><th colspan=\"2\"><strong>Orbiter<\/strong><\/th><\/tr><tr><td>Dimensions orbiter<\/td><td>2.8 m x 2.1 m x 2.0 m<\/td><\/tr><tr><td>Dimensions solar cell<\/td><td>2 pieces, each with 14 m length, with a total plain of 64 sqm<\/td><\/tr><tr><td>Energy supply \/ Energy production of the solar cells<\/td><td>850 W at 3,4 AU*, 395 W at 5,25 AU*<\/td><\/tr><tr><td>Communication antenna<\/td><td>\n<p style=\"text-align: left;\">High gain antenna, 2,2 m diameter, rotatable<\/p>\n<\/td><\/tr><tr><td colspan=\"2\">*AU = astronomical unit (mean distance between Earth and Sun, approx. 150 million km)<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n<figure class=\"wp-block-table is-style-stripes\"><table><tbody><tr><th colspan=\"2\"><strong>Philae-Lander<\/strong><\/th><\/tr><tr><td>Weight<\/td><td>100 kg<\/td><\/tr><tr><td>Data transfer<\/td><td>16 kilobytes per second via orbiter<\/td><\/tr><tr><td>Energy supply<\/td><td>Solar generator, 4 W, primary (for the first 60 hours after landing on the comet) and secondary (rechargeable) batteries<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n<figure class=\"wp-block-table is-style-stripes\"><table><tbody><tr><th colspan=\"2\"><strong>Time schedule<\/strong><\/th><\/tr><tr><td>Launch<\/td><td>March 2004<\/td><\/tr><tr><td>1st Earth flyby<\/td><td>March 2005<\/td><\/tr><tr><td>Mars flyby<\/td><td>March 2007<\/td><\/tr><tr><td>2nd Earth flyby<\/td><td>November 2007<\/td><\/tr><tr><td>3rd Earth flyby<\/td><td>November 2009<\/td><\/tr><tr><td>Rendezvous maneuver<\/td><td>May 2014<\/td><\/tr><tr><td>Global mapping of the comet<\/td><td>August 2014<\/td><\/tr><tr><td>Landing on the comet<\/td><td>November 2014<\/td><\/tr><tr><td>Orbit flight<\/td><td>August 2015<\/td><\/tr><tr><td>End of the mission<\/td><td>December 2015<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n<p><strong><em>Primary objectives of the Rosetta mission:<\/em><\/strong><\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>Investigation of the origin of the Solar System through the investigation of the composition of a comet<\/li>\n\n\n\n<li>The exploration of the interaction between comet material and interstellar material<\/li>\n\n\n\n<li>Global characterization of the comet nucleus (dynamical properties, surface morphology, composition)<\/li>\n\n\n\n<li>Chemical, mineralogical and isotopical composition of the volatile and solid substances of the comet nucleus<\/li>\n\n\n\n<li>Physical properties and correlation between the volatile and solid substances of the comet nucleus<\/li>\n\n\n\n<li>Investigation of the evolution of the comet activity and the processes in the crust of the nucleus and the inner coma (dust\/gas interaction)<\/li>\n\n\n\n<li>Investigation of the general characteristics of the asteroids including the investigation of their dynamical properties, surface morphology and composition<\/li>\n<\/ul>\n\n\n\n<p>Die &#8218;Orbiter&#8216;-Nutzlast besteht aus zw\u00f6lf Experimenten, deren Aufgabe es ist, den Kometenkern und die ihn umgebende Gas- und Staubwolke zu untersuchen. Die &#8218;Lander&#8216;-Nutzlast bietet dar\u00fcber hinaus die M\u00f6glichkeit, die Kernoberfl\u00e4che und die darunterliegenden Strukturen aus unmittelbarer N\u00e4he zu analysieren. Die obere Tabelle zeigt die Experimente des Rosetta-Orbiters und die untere Tabelle zeigt die Nutzlast des Landers.<\/p>\n\n\n\n<h3 class=\"wp-block-heading\">Experiments<\/h3>\n\n\n\n<p class=\"translation-block\"><strong>Remote Sensing<\/strong> Rosetta Lander Philae Payload\nFor more information, visit the <a href=\"http:\/\/rosetta.esa.int\/science-e\/www\/area\/index.cfm?fareaid=13\" target=\"_self\">ESA page<\/a><\/p>\n\n\n\n<figure class=\"wp-block-table is-style-stripes\"><table><tbody><tr><th colspan=\"2\"><strong>Rosetta Lander &#8211; Philae<\/strong><\/th><\/tr><tr><td>APX<\/td><td>\u03b1-particles and X-ray detector<\/td><\/tr><tr><td>Probe-<br>drawing<\/td><td>&#8211;<\/td><\/tr><tr><td>COSAC<\/td><td>Gas analysis and elementary, molecular composition, respectively<\/td><\/tr><tr><td>MODULUS Ptolemy<\/td><td>Gas analysis and isotope composition<\/td><\/tr><tr><td>\u00c7IVA<br>ROLIS<\/td><td>Rosetta lander cameras<\/td><\/tr><tr><td>SESAME<\/td><td>Material analysis<\/td><\/tr><tr><td>MUPUS<\/td><td>Material analysis<\/td><\/tr><tr><td>ROMAP<\/td><td>Magnetometer and plasma analysis<\/td><\/tr><tr><td>CONSERT<\/td><td>Tomography of the core<\/td><\/tr><\/tbody><\/table><\/figure>","protected":false},"excerpt":{"rendered":"<p>Rosetta ist die erste Mission, deren Ziel es ist, einen Kometen \u00fcber einen l\u00e4ngeren Zeitraum hinweg zu begleiten und zu beobachten.Am 2. M\u00e4rz 2004 startete die ESA-Raumsonde ihre zehnj\u00e4hrige Reise zum Kometen Churyumov-Gerasimenko mit einer Ariane-5 Rakete von Kourou, Franz\u00f6sisch-Guayana. Bis zu ihrer Ankunft im Jahr 2014 hat Rosetta mehrere Vorbeifl\u00fcge an Erde und Mars [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":90,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_uag_custom_page_level_css":"","site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"default","site-content-style":"default","site-sidebar-style":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","ast-disable-related-posts":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":"","astra-migrate-meta-layouts":"default","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"ast-content-background-meta":{"desktop":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"footnotes":""},"class_list":["post-671","page","type-page","status-publish","hentry"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.4 - 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Bis zu ihrer Ankunft im Jahr 2014 hat Rosetta mehrere Vorbeifl\u00fcge an Erde und Mars&hellip;","_links":{"self":[{"href":"https:\/\/fip-koeln.de\/en_us\/wp-json\/wp\/v2\/pages\/671","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/fip-koeln.de\/en_us\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/fip-koeln.de\/en_us\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/fip-koeln.de\/en_us\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/fip-koeln.de\/en_us\/wp-json\/wp\/v2\/comments?post=671"}],"version-history":[{"count":53,"href":"https:\/\/fip-koeln.de\/en_us\/wp-json\/wp\/v2\/pages\/671\/revisions"}],"predecessor-version":[{"id":1753,"href":"https:\/\/fip-koeln.de\/en_us\/wp-json\/wp\/v2\/pages\/671\/revisions\/1753"}],"up":[{"embeddable":true,"href":"https:\/\/fip-koeln.de\/en_us\/wp-json\/wp\/v2\/pages\/90"}],"wp:attachment":[{"href":"https:\/\/fip-koeln.de\/en_us\/wp-json\/wp\/v2\/media?parent=671"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}