{"id":436,"date":"2016-03-11T23:21:24","date_gmt":"2016-03-11T23:21:24","guid":{"rendered":"http:\/\/www.earth-site.co.uk\/Education\/?page_id=436"},"modified":"2025-09-13T13:42:20","modified_gmt":"2025-09-13T12:42:20","slug":"planet-jupiter","status":"publish","type":"post","link":"https:\/\/www.earth-site.co.uk\/Education\/planet-jupiter\/","title":{"rendered":"Planet Jupiter"},"content":{"rendered":"<div id=\"Content\" align=\"center\" class=\"Body\">\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><em><span style=\"line-height:115%; font-family:'Verdana','sans-serif'; font-size:12.0pt; \">Planet Jupiter is 2.5 times more  massive than all the other planets in our solar system combined, and is believed to have the largest moon system with 67 moons.<\/span><\/em><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"><a href=\"#Overview-of-Planet-Jupiter\">Overview of Planet Jupiter<\/a><\/span><\/p>\n<p class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"><a href=\"#Formation-of-Planet-Jupiter\">Formation of Planet  Jupiter<\/a><\/span><\/p>\n<p class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"><a href=\"#Layers-of-Jupiter\">Layers of Jupiter<\/a><\/span><\/p>\n<p class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"><a href=\"#Jupiters-Magnetosphere\">Jupiter&#8217;s Magnetosphere<\/a><\/span><\/p>\n<p class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"><a href=\"#Jupiters-Rings\">Jupiter&#8217;s Rings <\/a><\/span><\/p>\n<p class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"><a href=\"#Weather-on-Jupiter\">Weather on Jupiter<\/a><\/span><\/p>\n<p class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"><a href=\"#Juno\">Juno<\/a><\/span><\/p>\n<p class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"><a href=\"#Where-in-the-Solar-System\">Where in the Solar System?<\/a><\/span><\/p>\n<p class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"><a href=\"#Quick-Stats\">Quick Stats<\/a><\/span><\/p>\n<p class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"><a href=\"#Real-Time-Data\">Real Time Data<\/a><\/span><\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<h2 class=\"MsoNormal\"><span style=\"line-height:115%; font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><a name=\"Overview-of-Planet-Jupiter\" id=\"Overview-of-Planet-Jupiter\"><\/a>Overview of Planet Jupiter<\/span><\/h2>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><img decoding=\"async\" src=\"\/Education\/Images\/Astronomy\/Jupiter\/Jupiter.gif\" alt=\"Planet Jupiter\" width=\"274\" height=\"243\" hspace=\"12\" align=\"left\" style=\"margin:0px 20px\" loading=\"lazy\" \/><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">Jupiter is named after the King of the roman gods for  very good reason. It is not only the largest planet but its magnetosphere is  the largest object in the solar system. Jupiter and Saturn have the largest  moon systems in the entire solar system Jupiter is known to have at least 67  moon as of 2015 while Saturn is currently known to have at least 62 but more  are being discovered all the time. <\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">Planet Jupiter is 2.5 times more massive than all the other planets in our solar system  combined.<\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">If  Jupiter had become 80 times more massive it would have collapsed in on itself  due to the immense gravity. This immense pressure would have started a thermonuclear  reaction, turning Jupiter into a star. <\/span><\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<h2 class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><a name=\"Formation-of-Planet-Jupiter\" id=\"Formation-of-Planet-Jupiter\"><\/a>Formation of Planet  Jupiter<\/span><\/h2>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" align=\"center\" style=\"text-align:center;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><img decoding=\"async\" src=\"\/Education\/Images\/Astronomy\/Stars\/Birth of Star credit NASA.PNG\" alt=\"Formation of Jupiter\" width=\"618\" height=\"257\" \/><\/span><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"> <\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">When  the solar system was forming and left over material from the sun began to form  the planets, moons and other bodies in our solar system. One planet in  particular got more than 90% of that matter; this planet is the gas giant we  call Jupiter. <\/span><\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">Stars  form when gas clouds begin to clump together and this clump draws in more of  the gas through the gravity it projects. At some point during the stars  creation the gas cloud becomes a disk of matter and, once the star is formed in  the centre, the planets begin to form from clumps in the disk.<\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">There  are different theories as to how the gas giants, Jupiter and Saturn, form. One  model suggests that solid rock clumps creating the core which draws in huge  amounts of gas. While another suggests that the gas clumps and forms the planet  in a single process.<\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">The  true answer as to the formation is not currently known but the primary mission  of NASA&rsquo;s Juno spacecraft (see below) is to find the answer to how gas giants  are formed. Juno is due to reach Jupiter later this year so watch this space. <\/span><\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<h2 class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><a name=\"Layers-of-Jupiter\" id=\"Layers-of-Jupiter\"><\/a>Layers of Jupiter<\/span><\/h2>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" align=\"center\" style=\"text-align:center;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"><img decoding=\"async\" src=\"\/Education\/Images\/Astronomy\/Jupiter\/Layers of Planet Jupiter.png\" alt=\"Layers of Jupiter\" width=\"602\" height=\"343\" \/><\/span><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"> <\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">Jupiter  is mainly made of Hydrogen and <a href=\"https:\/\/www.earth-site.co.uk\/Education\/helium\/\" title=\"The Lighter Side of Science: Exploring the Wonders of Helium (He)\">Helium<\/a>, like our sun, and due to the immense  pressures Jupiter&rsquo;s huge mass creates the Hydrogen can be found in liquid form  below the surface atmosphere. Further into the structure of Jupiter, as the  pressure and temperatures increase, the hydrogen becomes metallic and it is  here that Jupiter&rsquo;s magnetosphere is generated. It is believed that at the  centre of Jupiter there may be a rocky planet similar in size to Earth although  this and many other questions about Jupiter will be answered when NASA&rsquo;s Juno  spacecraft reaches the gas giant in July of 2016.<\/span><\/p>\n<p>&nbsp;<\/p>\n<h2 class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><a name=\"Jupiters-Magnetosphere\" id=\"Jupiters-Magnetosphere\"><\/a>Jupiter&#8217;s Magnetosphere <\/span><\/h2>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" align=\"center\" style=\"text-align:center;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><img decoding=\"async\" src=\"\/Education\/Images\/Astronomy\/Jupiter\/Jupiter's Magnetosphere.png\" alt=\"Jupiter's Magnetosphere\" width=\"602\" height=\"349\" \/><\/span><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"> <\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">Jupiter&rsquo;s  magnetosphere, like Earth&rsquo;s, is created by the spin of the planet and the  metallic layer in its structure. Jupiter&rsquo;s magnetosphere is about than Earth&rsquo;s 20,000  times stronger than Earth&rsquo;s and stretches about 1 billion kilometres (600  million miles) almost reaching Saturn&rsquo;s orbit. If visible it would appear to be  3 times the size of the sun or moon from the Earth&rsquo;s surface. <\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">Earth&rsquo;s  magnetosphere protects us from solar storms and harmful solar radiation while  Jupiter&rsquo;s magnetosphere has trapped radiation within it engulfing its many  moons in harmful radiation.<\/span><\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<h2 class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><a name=\"Jupiters-Rings\" id=\"Jupiters-Rings\"><\/a>Jupiter&#8217;s Rings <\/span><\/h2>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" align=\"center\" style=\"text-align:center;\"><img decoding=\"async\" src=\"\/Education\/Images\/Astronomy\/Jupiter\/NASA Jupiters Rings.PNG\" alt=\"Rings of Jupiter\" width=\"602\" height=\"347\" \/><\/p>\n<p class=\"MsoNormal\" align=\"center\" style=\"text-align:center;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">Image credit: NASA<\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">Jupiter  has got one large ring which can be divided into five segments. Closest to  Jupiter&rsquo;s surface is called the &lsquo;Halo ring&rsquo; and is approximately 10,000km  thick, next is called the &lsquo;Main Ring&rsquo; at approximately 100km thick. The next  sections is called the &lsquo;Inner Gossamer Ring&rsquo; and is 2,600km thick, then the  &lsquo;Outer Gossamer Ring&rsquo; at 8,800km thick and finally the &lsquo;Faint Outer Ring&rsquo; at  8,800km thick.<\/span><\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<h2 class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><a name=\"Weather-on-Jupiter\" id=\"Weather-on-Jupiter\"><\/a>Weather on Jupiter <\/span><\/h2>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" align=\"center\" style=\"text-align:center;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><img decoding=\"async\" src=\"\/Education\/Images\/Astronomy\/Jupiter\/NASA Close up of Jupiter.PNG\" alt=\"Planet Jupiter\" width=\"611\" height=\"387\" \/><\/span><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"> <\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">The  giant red spot or Eye on Jupiter is a giant storm system that travels around  Jupiter&rsquo;s surface, just below the equator, making a revolution once every 6  days. It has been observed for over 300 years and is three times wider than  planet Earth. There are many storms on Jupiter, as well as the &lsquo;great red spot&rsquo;  there is also a &lsquo;Little red spot&rsquo; which has been observed giving birth to three  smaller storms recently.<\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">The  dark brown\/red bands that can be seen are formed of warmer gases that are  falling and are actually slightly lower in the atmosphere than the lighter  coloured clouds. These lighter coloured clouds are cooler areas of gas and when  the two come into contact with each other they form great, turbulent storms.<\/span><\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<h2 class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><a name=\"Juno\" id=\"Juno\"><\/a>Juno<\/span><\/h2>\n<p class=\"MsoNormal\" align=\"center\" style=\"text-align:center;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"><img decoding=\"async\" src=\"\/Education\/Images\/Astronomy\/Jupiter\/NASA Juno Space Craft.png\" alt=\"Juno\" width=\"612\" height=\"524\" \/><\/span><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \"> <\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">Although  a lot is known about Jupiter many of its secrets are hidden deep within its  thick layer of stormy gas clouds. Deep beneath the surface, scientists hope to  uncover the mysteries of Jupiter&rsquo;s interior including the true cause of the  storms. <\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">In  order to unlock these and many other secrets about the gas giant, NASA has sent  a space craft called Juno which has been especially designed to carry out this  mission and overcome the harsh conditions such as extreme temperatures and  intense radiation. <\/span><\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" style=\"text-align:justify;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:12.0pt; \">On  the 5th of August 2011 an Atlas V 551 Rocket was launched with the space craft  Juno as the payload. The Rocket is a single use craft whose only role is to get  the Juno into low earth orbit. From there Juno travelled on a flight path  around the sun beyond the orbit of mars, back around Earth. Using our gravity  to shoot it off towards Jupiter (which it should intercept and begin its orbit  on the 5th of July 2016). From there it will use its on-board equipment to scan  the planet relaying all the information back to Earth.<\/span><\/p>\n<p>&nbsp;<\/p>\n<h2 class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><a name=\"Where-in-the-Solar-System\" id=\"Where-in-the-Solar-System\"><\/a>Where in the Solar System?<\/span><\/h2>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\" align=\"center\" style=\"text-align:center;\"><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><img decoding=\"async\" src=\"\/Education\/Images\/Astronomy\/Jupiter\/Where in the Solar System.PNG\" alt=\"Where in the Solar System\" width=\"675\" height=\"406\" \/><\/span><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"> <\/span><\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\"><span style=\"font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><a name=\"Quick-Stats\" id=\"Quick-Stats\"><\/a>Quick Stats<\/span><\/p>\n<p>&nbsp;<\/p>\n<table border=\"0\" cellpadding=\"0\" cellspacing=\"0\" class=\"MsoTableGrid\" style=\"border-collapse:collapse;border:none;\">\n<tr>\n<td valign=\"top\" style=\"width:125.9pt;border:solid white 1.0pt;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\"><a title=\"Jupiter&#8217;s Moons\" href=\"https:\/\/www.earth-site.co.uk\/Education\/jupiters-moons\/\">Moons<\/a><\/p>\n<\/td>\n<td valign=\"top\" style=\"width:127.6pt;border:solid white 1.0pt;border-left:none;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">67<\/p>\n<\/td>\n<\/tr>\n<tr>\n<td valign=\"top\" style=\"width:125.9pt;border:solid white 1.0pt;border-top:none;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">Rings<\/p>\n<\/td>\n<td valign=\"top\" style=\"width:127.6pt;border-top:none;border-left:none;border-bottom:solid white 1.0pt;border-right:solid white 1.0pt;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">1<\/p>\n<\/td>\n<\/tr>\n<tr>\n<td valign=\"top\" style=\"width:125.9pt;border:solid white 1.0pt;border-top:none;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">Orbit period<\/p>\n<\/td>\n<td valign=\"top\" style=\"width:127.6pt;border-top:none;border-left:none;border-bottom:solid white 1.0pt;border-right:solid white 1.0pt;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">483.68 million  Earth Days<\/p>\n<\/td>\n<\/tr>\n<tr>\n<td valign=\"top\" style=\"width:125.9pt;border:solid white 1.0pt;border-top:none;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">Rotation Period<\/p>\n<\/td>\n<td valign=\"top\" style=\"width:127.6pt;border-top:none;border-left:none;border-bottom:solid white 1.0pt;border-right:solid white 1.0pt;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">9.92 hours <\/p>\n<\/td>\n<\/tr>\n<tr>\n<td valign=\"top\" style=\"width:125.9pt;border:solid white 1.0pt;border-top:none;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">Equatorial Radius <\/p>\n<\/td>\n<td valign=\"top\" style=\"width:127.6pt;border-top:none;border-left:none;border-bottom:solid white 1.0pt;border-right:solid white 1.0pt;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">71,492 km (44,423 miles)<\/p>\n<\/td>\n<\/tr>\n<tr>\n<td valign=\"top\" style=\"width:125.9pt;border:solid white 1.0pt;border-top:none;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">Overall Density<\/p>\n<\/td>\n<td valign=\"top\" style=\"width:127.6pt;border-top:none;border-left:none;border-bottom:solid white 1.0pt;border-right:solid white 1.0pt;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">1.33 g\/cm<sup>3<\/sup><\/p>\n<\/td>\n<\/tr>\n<tr>\n<td valign=\"top\" style=\"width:125.9pt;border:solid white 1.0pt;border-top:none;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">Mass (Earth = 1)<\/p>\n<\/td>\n<td valign=\"top\" style=\"width:127.6pt;border-top:none;border-left:none;border-bottom:solid white 1.0pt;border-right:solid white 1.0pt;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">317.82<\/p>\n<\/td>\n<\/tr>\n<tr>\n<td valign=\"top\" style=\"width:125.9pt;border:solid white 1.0pt;border-top:none;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">Gravity (Earth = 1)<\/p>\n<\/td>\n<td valign=\"top\" style=\"width:127.6pt;border-top:none;border-left:none;border-bottom:solid white 1.0pt;border-right:solid white 1.0pt;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">2.36<\/p>\n<\/td>\n<\/tr>\n<tr>\n<td valign=\"top\" style=\"width:125.9pt;border:solid white 1.0pt;border-top:none;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\"> Temperature<\/p>\n<\/td>\n<td valign=\"top\" style=\"width:127.6pt;border-top:none;border-left:none;border-bottom:solid white 1.0pt;border-right:solid white 1.0pt;padding:0cm 5.4pt 0cm 5.4pt;\">\n<p class=\"MsoNormal style95 style1\" style=\"margin-bottom:.0001pt;line-height:normal;\">-148&deg;C (-234&deg;F or 125 &deg;K)<\/p>\n<\/td>\n<\/tr>\n<\/table>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<h2 class=\"MsoNormal\"><span style=\"line-height:115%; font-family:'Verdana','sans-serif'; font-size:14.0pt; \"><a name=\"Real-Time-Data\" id=\"Real-Time-Data\"><\/a>Real Time Data<\/span><\/h2>\n<p>&nbsp;<\/p>\n<p class=\"MsoNormal\"><span style=\"line-height:115%; font-family:'Verdana','sans-serif'; font-size:12.0pt; \">Data was correct at the time the page was loaded. If you require an update hit F5 on your keyboard to refresh the page.<\/span><\/p>\n<p>&nbsp;<\/p>\n<p><script type=\"text\/javascript\" id=\"WolframAlphaScriptb270a720f6ac2e8a8c53d968243d5971\" src=\"\/\/www.wolframalpha.com\/widget\/widget.jsp?id=b270a720f6ac2e8a8c53d968243d5971&#038;theme=blue&#038;output=iframeOpen&#038;width=600&#038;height=700\"><\/script><\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>Planet Jupiter is 2.5 times more massive than all the other planets in our solar system combined, and is believed 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