{"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":"An external source of CO for Uranus - Thibault Cavali\u00e9","type":"rich","width":600,"height":338,"html":"<blockquote class=\"wp-embedded-content\" data-secret=\"VmuLuxzjjv\"><a href=\"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/en\/2018\/02\/20\/external-source-co-uranus\/\">An external source of CO for Uranus<\/a><\/blockquote><iframe sandbox=\"allow-scripts\" security=\"restricted\" src=\"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/en\/2018\/02\/20\/external-source-co-uranus\/embed\/#?secret=VmuLuxzjjv\" width=\"600\" height=\"338\" title=\"&#8220;An external source of CO for Uranus&#8221; &#8212; Thibault Cavali\u00e9\" data-secret=\"VmuLuxzjjv\" 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":"With the Herschel Space Observatory, my colleagues and I have detected CO (carbon monoxide) in the stratosphere of Uranus. The analysis and interpretation of the data demonstate that it is supplied by an external source. Is this oxygen delivered by comets, as in Jupiter (see this post), or by interplanetary dust particles? Complementary observations (e.g., &hellip; Continue reading \"\"","thumbnail_url":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/files\/2018\/01\/Uranus_CO.png"}