{"version":"1.0","provider_name":"Thibault Cavali\u00e9","provider_url":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie","author_name":"tcavalie","author_url":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/author\/tcavalie\/","title":"A cometary origin for CO in the stratosphere of Saturn? - Thibault Cavali\u00e9","type":"rich","width":600,"height":338,"html":"<blockquote class=\"wp-embedded-content\" data-secret=\"HLmkiUU3HR\"><a href=\"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/en\/2018\/02\/21\/cometary-origin-co-stratosphere-saturn\/\">A cometary origin for CO in the stratosphere of Saturn?<\/a><\/blockquote><iframe sandbox=\"allow-scripts\" security=\"restricted\" src=\"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/en\/2018\/02\/21\/cometary-origin-co-stratosphere-saturn\/embed\/#?secret=HLmkiUU3HR\" width=\"600\" height=\"338\" title=\"&#8220;A cometary origin for CO in the stratosphere of Saturn?&#8221; &#8212; Thibault Cavali\u00e9\" data-secret=\"HLmkiUU3HR\" frameborder=\"0\" marginwidth=\"0\" marginheight=\"0\" scrolling=\"no\" class=\"wp-embedded-content\"><\/iframe><script>\n\/*! This file is auto-generated *\/\n!function(d,l){\"use strict\";l.querySelector&&d.addEventListener&&\"undefined\"!=typeof URL&&(d.wp=d.wp||{},d.wp.receiveEmbedMessage||(d.wp.receiveEmbedMessage=function(e){var t=e.data;if((t||t.secret||t.message||t.value)&&!\/[^a-zA-Z0-9]\/.test(t.secret)){for(var s,r,n,a=l.querySelectorAll('iframe[data-secret=\"'+t.secret+'\"]'),o=l.querySelectorAll('blockquote[data-secret=\"'+t.secret+'\"]'),c=new RegExp(\"^https?:$\",\"i\"),i=0;i<o.length;i++)o[i].style.display=\"none\";for(i=0;i<a.length;i++)s=a[i],e.source===s.contentWindow&&(s.removeAttribute(\"style\"),\"height\"===t.message?(1e3<(r=parseInt(t.value,10))?r=1e3:~~r<200&&(r=200),s.height=r):\"link\"===t.message&&(r=new URL(s.getAttribute(\"src\")),n=new URL(t.value),c.test(n.protocol))&&n.host===r.host&&l.activeElement===s&&(d.top.location.href=t.value))}},d.addEventListener(\"message\",d.wp.receiveEmbedMessage,!1),l.addEventListener(\"DOMContentLoaded\",function(){for(var e,t,s=l.querySelectorAll(\"iframe.wp-embedded-content\"),r=0;r<s.length;r++)(t=(e=s[r]).getAttribute(\"data-secret\"))||(t=Math.random().toString(36).substring(2,12),e.src+=\"#?secret=\"+t,e.setAttribute(\"data-secret\",t)),e.contentWindow.postMessage({message:\"ready\",secret:t},\"*\")},!1)))}(window,document);\n<\/script>\n","description":"Determining the origin of CO in a giant planet stratosphere is more complex than water as this species does not condense at the tropopauses of these planets and can therefore originate not only for external sources (interplanetary dust particles, comets, icy rings\/satellites), but also from the deep oxygen-rich interiors of these planets. Studying the origin &hellip; Continue reading \"\"","thumbnail_url":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/files\/2018\/02\/Saturn_CO.png"}