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        <title><![CDATA[Stories by Jatan Mehta on Medium]]></title>
        <description><![CDATA[Stories by Jatan Mehta on Medium]]></description>
        <link>https://medium.com/@uncertainquark?source=rss-7b8fb40c2a02------2</link>
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            <title>Stories by Jatan Mehta on Medium</title>
            <link>https://medium.com/@uncertainquark?source=rss-7b8fb40c2a02------2</link>
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        <lastBuildDate>Mon, 18 Sep 2017 02:54:57 GMT</lastBuildDate>
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        <item>
            <title><![CDATA[The origin of the behaviour of KELT-9b is not known yet.]]></title>
            <link>https://medium.com/@uncertainquark/the-origin-of-the-behaviour-of-kelt-9b-is-not-known-yet-56e260ac942e?source=rss-7b8fb40c2a02------2</link>
            <guid isPermaLink="false">https://medium.com/p/56e260ac942e</guid>
            <dc:creator><![CDATA[Jatan Mehta]]></dc:creator>
            <pubDate>Fri, 15 Sep 2017 07:20:14 GMT</pubDate>
            <atom:updated>2017-09-15T07:20:14.778Z</atom:updated>
            <content:encoded><![CDATA[<p>The origin of the behaviour of KELT-9b is not known yet.</p><img src="https://medium.com/_/stat?event=post.clientViewed&referrerSource=full_rss&postId=56e260ac942e" width="1" height="1">]]></content:encoded>
        </item>
        <item>
            <title><![CDATA[Because the space-time curvature due to gravity as represented in most popular science works is…]]></title>
            <link>https://medium.com/@uncertainquark/because-the-space-time-curvature-due-to-gravity-as-represented-in-most-popular-science-works-is-581bd6e07766?source=rss-7b8fb40c2a02------2</link>
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            <dc:creator><![CDATA[Jatan Mehta]]></dc:creator>
            <pubDate>Mon, 11 Sep 2017 03:37:58 GMT</pubDate>
            <atom:updated>2017-09-11T03:37:58.061Z</atom:updated>
            <content:encoded><![CDATA[<p>Because the space-time curvature due to gravity as represented in most popular science works is only anecdotal. In reality, the curve should be 3d in nature, which is not possible to imagine for us naturally, but we can certainly measure its effects (bending of background star light by foreground object).</p><img src="https://medium.com/_/stat?event=post.clientViewed&referrerSource=full_rss&postId=581bd6e07766" width="1" height="1">]]></content:encoded>
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        <item>
            <title><![CDATA[Rings of Super Saturn — The planet with rings 200 times larger than Saturn’s]]></title>
            <link>https://medium.com/@uncertainquark/rings-of-super-saturn-the-planet-with-rings-200-times-larger-than-saturns-8a72be0b5ecd?source=rss-7b8fb40c2a02------2</link>
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            <category><![CDATA[science]]></category>
            <category><![CDATA[exoplanets]]></category>
            <category><![CDATA[saturn]]></category>
            <category><![CDATA[space]]></category>
            <category><![CDATA[physics]]></category>
            <dc:creator><![CDATA[Jatan Mehta]]></dc:creator>
            <pubDate>Fri, 08 Sep 2017 10:39:58 GMT</pubDate>
            <atom:updated>2017-09-09T16:58:53.953Z</atom:updated>
            <cc:license>https://creativecommons.org/licenses/by-sa/4.0/</cc:license>
            <content:encoded><![CDATA[<h3>Rings of Super Saturn — The planet with rings 200 times larger than Saturn’s</h3><p>About 420 light years away lies a very young planet around a very young sun-like star, with Saturn like rings around it. What is not like Saturn is the truly colossal size of the rings. <a href="https://arxiv.org/abs/1108.4070">Transit observations revealed</a> that this <a href="https://en.wikipedia.org/wiki/Gas_giant">gas giant</a> planet has rings 200 times larger than the rings of Saturn. And so the title of the Lord of the Rings goes to <a href="https://en.wikipedia.org/wiki/1SWASP_J140747.93-394542.6#1SWASP_J140747.93-394542.6_b">J1407b</a> — a Super Saturn at least 20 times more massive than Saturn itself.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/1000/0*K-_iLpaoMAMlFakr.jpg" /><figcaption>Artist’s conception of the giant ring system of the planet J1407b. <a href="https://www.rochester.edu/newscenter/gigantic-ring-system-around-j1407b/">Source: Rochester</a></figcaption></figure><p>Here is how the planet’s ring system size compares to its sun:</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/490/0*e8Si8VVLYWZTfYX7.png" /><figcaption>To scale size comparison of planet J1407b and its rings (left) to its sun (right). <a href="http://www.ctio.noao.edu/noao/content/Eclipsing-Ring-System-J1407">Source: CTIO NOAO</a></figcaption></figure><p>The large ring system was discovered due to it deeply eclipsing the planet’s sun for weeks. The rings have a lot of material in it (containing the mass of an entire Earth), which block the light of the planet’s sun. Here is a video showing the drop in the star’s brightness during the <em>ring-eclipse:</em></p><iframe src="https://cdn.embedly.com/widgets/media.html?src=https%3A%2F%2Fplayer.vimeo.com%2Fvideo%2F117757625&amp;url=https%3A%2F%2Fvimeo.com%2F117757625&amp;image=https%3A%2F%2Fi.vimeocdn.com%2Fvideo%2F504569119_960.jpg&amp;key=a19fcc184b9711e1b4764040d3dc5c07&amp;type=text%2Fhtml&amp;schema=vimeo" width="1000" height="700" frameborder="0" scrolling="no"><a href="https://medium.com/media/29f0b23c022a751e456806a5ec2a5172/href">https://medium.com/media/29f0b23c022a751e456806a5ec2a5172/href</a></iframe><p>Extending ~180 million km in length, the size of the rings beat the Earth-Sun distance. The question is how do such large rings even exist when they should be torn apart by the gravity of the planet’s sun.</p><p><a href="https://arxiv.org/abs/1609.08485">An interesting way this was solved</a> was proposing that the rings were spinning in the opposite direction to that of its planet around its sun. This means that the particles that make up the ring system are never too close to the sun for too long, and thus can stay together in a ring formation in the face of the star’s intense gravitational pull. Here’s an animation:</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/600/0*gIkr86cGCpRK3Hdv.gif" /><figcaption>A simulation of rings spinning in the opposite direction of the planet J1407b (left) vs. in the same direction (right). <a href="https://vimeo.com/184968413">Source: Steven Rieder on Vimeo</a></figcaption></figure><p>The rings stay intact when spinning counter-clockwise as opposed to clockwise spinning with respect to the planet’s spin, hence solving the mystery. Now the question is how do you get rings spinning in the opposite direction in the first place? Well, more answers to find out for Science.</p><p>There is another interesting thing about these rings. Did you notice the ring gap in the above video at 0:09?</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/1024/1*TsHjJDOVTkU2AqxKD2HjTQ.png" /></figure><p>Since the gap is quite substantial and the planetary system quite young, <a href="https://arxiv.org/abs/1501.05652">it is thought that the gap in the rings is cause by a newly formed moon</a> up to 80% the mass of Earth. What we are seeing here is a Jupiter/Saturn like vast moon system being formed. Only larger.</p><p>After the <a href="https://www.nature.com/news/cassini-s-13-years-of-stunning-saturn-science-in-pictures-1.22514">13 years of Stunning Saturn Science</a> that NASA’s <a href="https://en.wikipedia.org/wiki/Cassini%E2%80%93Huygens">Cassini spacecraft</a> has given us, one can only imagine the beautiful imagery and intricate data that will be revealed when (and if) we send a spacecraft to this Lord of the Rings. Meanwhile here’s a simulated version:</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/1024/0*AXWUYHpY3dfhQtT2.png" /><figcaption>J1407b transit seen from its moon, simulated in <a href="https://commons.wikimedia.org/wiki/Celestia">Celestia</a>. <a href="https://commons.wikimedia.org/wiki/File:J1407b_seen_from_its_exomoon.png">Source: Wikipedia</a></figcaption></figure><p>Dreamy. Just to think that there are such <a href="https://medium.com/the-space-perspective/the-most-extreme-exoplanets-ever-found-165144bf3105">extreme worlds out there in the Universe</a> waiting to be discovered, simply boggles my mind.</p><img src="https://medium.com/_/stat?event=post.clientViewed&referrerSource=full_rss&postId=8a72be0b5ecd" width="1" height="1">]]></content:encoded>
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            <title><![CDATA[Hello Brandon, nice to see you writing articles too!]]></title>
            <link>https://medium.com/@uncertainquark/hello-brandon-nice-to-see-you-writing-articles-too-c1487c0c0190?source=rss-7b8fb40c2a02------2</link>
            <guid isPermaLink="false">https://medium.com/p/c1487c0c0190</guid>
            <dc:creator><![CDATA[Jatan Mehta]]></dc:creator>
            <pubDate>Wed, 06 Sep 2017 03:06:01 GMT</pubDate>
            <atom:updated>2017-09-06T03:06:01.494Z</atom:updated>
            <content:encoded><![CDATA[<p>Hello Brandon, nice to see you writing articles too! :D<br>Are you interested in a collaboration? Email me using the ID from my profile.</p><img src="https://medium.com/_/stat?event=post.clientViewed&referrerSource=full_rss&postId=c1487c0c0190" width="1" height="1">]]></content:encoded>
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            <title><![CDATA[The most extreme Exoplanets ever found]]></title>
            <link>https://medium.com/@uncertainquark/the-most-extreme-exoplanets-ever-found-165144bf3105?source=rss-7b8fb40c2a02------2</link>
            <guid isPermaLink="false">https://medium.com/p/165144bf3105</guid>
            <category><![CDATA[science]]></category>
            <category><![CDATA[space]]></category>
            <category><![CDATA[physics]]></category>
            <category><![CDATA[gif]]></category>
            <category><![CDATA[exoplanets]]></category>
            <dc:creator><![CDATA[Jatan Mehta]]></dc:creator>
            <pubDate>Fri, 01 Sep 2017 11:24:01 GMT</pubDate>
            <atom:updated>2017-09-08T10:44:55.164Z</atom:updated>
            <cc:license>https://creativecommons.org/licenses/by-sa/4.0/</cc:license>
            <content:encoded><![CDATA[<p>As of September 2017, <a href="https://exoplanets.nasa.gov/">humans have found 3500+ planets orbiting around stars other than our own</a>, which is a pretty remarkable number. Even more remarkable are some of the most extreme varieties found in the Galaxy.</p><h3>#1: A planet being eaten by its star — Wasp-12b</h3><p>Imagine a planet ~2 times the size of Jupiter. Now imagine it being pulled by the extreme gravitational force of its sun making the planet egg-shaped.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/515/1*QspsmOX3KKv2BRQszcYjoQ.png" /><figcaption>The hot gas giant planet <a href="https://en.wikipedia.org/wiki/WASP-12b">Wasp-12b</a> compared to Jupiter. <a href="https://exoplanets.nasa.gov/alien-worlds/galaxy-of-horrors/">Source: NASA Exoplanets</a></figcaption></figure><figure><img alt="" src="https://cdn-images-1.medium.com/max/670/0*QgZ5BGangjrGPzHY.jpg" /><figcaption>An artist’s impression of the hot gas giant Wasp-12b being devoured by its Sun. <a href="https://www.nasa.gov/mission_pages/hubble/science/planet-eater.html">Source: NASA</a></figcaption></figure><p>In a mere 10 million years of cosmic time, the planet <a href="https://en.wikipedia.org/wiki/WASP-12b">Wasp-12b</a> will be completely destroyed by its sun, becoming a part of it.</p><h3>#2: Planets bathed with excessive radiation — Pulsar Planets</h3><p>Among the very first exoplanets to be discovered, the 3 planets <a href="https://en.wikipedia.org/wiki/PSR_B1257%2B12">PSR B1257+12 A, B and C</a> (discovered in the 1990s) are the last places you want to look for Life. The <a href="https://en.wikipedia.org/wiki/Neutron_star">Neutron star</a> they orbit spins around itself faster than you can blink your eye. It emits excessive radiation pulses from both its poles in the process.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/1024/0*13VoY57O-ap3SBqg.jpg" /><figcaption>An artist’s impression of the exoplanets around the radiation bathing Pulsar PSR B1257+12. <a href="http://PSR B1257+12">Source: Wikipedia</a></figcaption></figure><p>Such intense bathing of radiation from its parent star while extremely hostile to Life, creates <a href="https://www.nasa.gov/mission_pages/chandra/solar-storms-ignite-xray-northern-lights-on-jupiter.html">dazzling auroras</a> on the planets. Makes you wonder how safe the planet from <a href="http://www.imdb.com/title/tt0816692/">Interstellar</a> would be, bombarded by the excessive radiation from around the Black Hole.</p><h3>#3: Rains of molten glass — HD 189733 b</h3><p>Look at this beautiful deep blue planet:</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/784/1*CE_Hygt6WP2sVSJOBY8UoQ.jpeg" /><figcaption>An artist’s impression of <a href="https://en.wikipedia.org/wiki/HD_189733_b">HD 189733 b</a> — a <a href="https://en.wikipedia.org/wiki/Hot_Jupiter">Hot Jupiter</a> orbiting its star every ~2 days. <a href="https://commons.wikimedia.org/wiki/File:Artist%E2%80%99s_impression_of_the_deep_blue_planet_HD_189733b.jpg">Source: Wikipedia</a></figcaption></figure><p>Very Earth-like? Not quite. This Hot Jupiter planet has winds that blow at more than 7000 km/h and is likely to have rains of molten glass, blowing sideways! In fact, the <a href="https://arxiv.org/abs/1101.0059">deep blue color observed</a> is because of scattering of blue light (<a href="https://en.wikipedia.org/wiki/Rayleigh_scattering">Rayleigh scattering</a>) by the silicate particles in its atmosphere.</p><h3>#4: A planet darker than coal — TrES-2b</h3><p>The large Jupiter-sized planet <a href="https://en.wikipedia.org/wiki/TrES-2b">TrES-2b</a> has an atmosphere that absorbs pretty much all of the light of its sun. <a href="https://www.cfa.harvard.edu/news/2011-21">Reflecting less than 1% of sunlight</a> makes it the darkest known planet around any star, darken than coal even.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/466/0*_5Uml-DBIHfHk0kT.jpg" /><figcaption>An artist’s impression of the darkest known planet around any star — TrES-2b. <a href="https://www.nasa.gov/mission_pages/kepler/news/cfa_darkest_exoplanet.html">Source: NASA</a></figcaption></figure><p>This amazing discovery was made using NASA’s <a href="https://en.wikipedia.org/wiki/Kepler_%28spacecraft%29">Kepler telescope</a>. The planet’s exotic atmosphere have been found to contain light-absorbing chemicals like vaporized sodium &amp; potassium and gaseous titanium oxide, yet none of these chemicals fully explain the extreme blackness of TrES-2b. The only faint light that the planet emits is due to it being very hot, a faint red glow the result of its proximity to its sun.</p><h3>#5: A planet hotter than most stars — KELT-9b</h3><p>At more than 4800 degrees Celsius, <a href="https://en.wikipedia.org/wiki/KELT-9b">KELT-9b</a> is hotter than the surface of most stars in the Universe. The planet is even more unusual in that it orbits perpendicular to the spin axis of its star (i.e pole to pole) and <a href="https://arxiv.org/abs/1706.06723">nobody knows why</a>. Imagine a planet ~3x the mass of Jupiter and bring it very close to the Sun, tilt its orbit 90 degrees and let it feel the heat:</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/640/1*4d0qW0Nkowdp9dnO95qklw.gif" /><figcaption>An artist’s concept showing the planet KELT-9b orbiting its host star KELT-9. <a href="https://commons.wikimedia.org/wiki/File:PIA21472_-_Hottest_Hot_Jupiter_Animation_(Artist%27s_Concept).gif">Source: Wikipedia</a></figcaption></figure><p>A polar opposite (pun intended) of this planet would be the planet named <a href="https://en.wikipedia.org/wiki/OGLE-2005-BLG-390Lb"><em>Hoth</em></a><em> </em>after the <a href="https://en.wikipedia.org/wiki/Hoth">Star Wars ice planet</a>. Hoth (in real life) is the coldest planet ever known at -220 degrees Celsius worth of coldness on its surface.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/800/1*Maix3YIvqIePqVWOT6Pqng.jpeg" /><figcaption>An artist’s impression of the coldest known planet ever found — Hoth. <a href="https://upload.wikimedia.org/wikipedia/commons/thumb/6/6b/OGLE-2005-BLG-390Lb_planet.jpg/1024px-OGLE-2005-BLG-390Lb_planet.jpg">Source: Wikipedia</a></figcaption></figure><h3>#6: Super Saturn J1407b— The largest ring system ever found</h3><p>Saturn’s rings are among the most beautiful sights in the Solar System. Now imagine a planet that is at least 20 times more massive than Saturn with a ring system that is more than 200 times as large. That’s <a href="https://medium.com/the-space-perspective/rings-of-super-saturn-the-planet-with-rings-200-times-larger-than-saturns-8a72be0b5ecd">Super Saturn J1407b</a> for you.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/1000/0*K-_iLpaoMAMlFakr.jpg" /><figcaption>Artist’s conception of the giant ring system of the planet J1407b. <a href="https://www.rochester.edu/newscenter/gigantic-ring-system-around-j1407b/">Source: Rochester</a></figcaption></figure><p>In the image above, the rings of <a href="https://en.wikipedia.org/wiki/1SWASP_J140747.93-394542.6#1SWASP_J140747.93-394542.6_b">J1407b</a> are shown eclipsing the young sun-like star J1407, as they would have appeared in early 2007 when the discovery was made. The rings of this planet are so huge that they stretch 180 million km end to end, larger than the distance between the Earth and the Sun.</p><p>There is also expected to be a large moon of the planet which is almost the same mass as the Earth (<a href="https://arxiv.org/abs/1501.05652">Original Paper</a>). The planet itself is so big its possible that its a <a href="https://en.wikipedia.org/wiki/Brown_dwarf">Brown Dwarf</a> star instead.</p><blockquote>The Galaxy is full of extreme worlds that are born to break the rules, rules that we thought were there. But the more Science we did, we found time and again that Nature finds its ways in curious ways.</blockquote><p>So which one is your favorite? :)</p><img src="https://medium.com/_/stat?event=post.clientViewed&referrerSource=full_rss&postId=165144bf3105" width="1" height="1">]]></content:encoded>
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            <title><![CDATA[Hey Jonathan!]]></title>
            <link>https://medium.com/@uncertainquark/hey-jonathan-71a76ae6b91a?source=rss-7b8fb40c2a02------2</link>
            <guid isPermaLink="false">https://medium.com/p/71a76ae6b91a</guid>
            <dc:creator><![CDATA[Jatan Mehta]]></dc:creator>
            <pubDate>Thu, 31 Aug 2017 13:27:54 GMT</pubDate>
            <atom:updated>2017-08-31T13:27:54.076Z</atom:updated>
            <content:encoded><![CDATA[<p>Hey Jonathan! Your articles are awesome. I noticed that you liked some of my articles. Are you interested in a collaboration? :) Email me using the ID in my profile info.</p><img src="https://medium.com/_/stat?event=post.clientViewed&referrerSource=full_rss&postId=71a76ae6b91a" width="1" height="1">]]></content:encoded>
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            <title><![CDATA[The purpose of the Universe]]></title>
            <link>https://medium.com/@uncertainquark/the-purpose-of-the-universe-c5b2203fd133?source=rss-7b8fb40c2a02------2</link>
            <guid isPermaLink="false">https://medium.com/p/c5b2203fd133</guid>
            <category><![CDATA[physics]]></category>
            <category><![CDATA[life]]></category>
            <category><![CDATA[space]]></category>
            <category><![CDATA[poetry]]></category>
            <category><![CDATA[art]]></category>
            <dc:creator><![CDATA[Jatan Mehta]]></dc:creator>
            <pubDate>Fri, 25 Aug 2017 18:06:02 GMT</pubDate>
            <atom:updated>2017-08-26T05:59:52.582Z</atom:updated>
            <cc:license>https://creativecommons.org/licenses/by-sa/4.0/</cc:license>
            <content:encoded><![CDATA[<p>​Does the Universe have a purpose? What is the purpose of Life?</p><p>Through the lens of a Physicist, here is what I think… in the form of a poem!</p><blockquote>Space is vast, near-infinite and empty,<br>But only so much of it we can see..</blockquote><blockquote>Stuck in a direction of time are we,<br>And yet we claim how we came to be..</blockquote><blockquote>Welcome to Space-time’s infinite array,<br>Where everything lies farther and farther away..</blockquote><blockquote>Magnificent Galaxies may be big and bright,<br>But their separation speaks stronger than their light..</blockquote><blockquote>Even the Stars are not as close as they seem,<br>Mere little dots that come and go as they dim..</blockquote><blockquote>Yet, even those tiny dots can be the most violent of all,<br>Massive Supernovae and Gamma ray bursts leading their fall..</blockquote><blockquote>This is a Universe where the stars are born to die,<br>Some form black holes, to space-time they can lie..</blockquote><blockquote>Even the smaller stars are hostile in time,<br>So are the planets that are considered benign..</blockquote><blockquote>Space is cold &amp; time unforgiving,<br>Space is harsh &amp; with time, it defies living..</blockquote><blockquote>Just what is then the purpose of life?<br>Or are we just a roll of dice?</blockquote><blockquote>Life is purposeless and meaningless,<br>Every sentient species alone in the vast space-time emptiness..</blockquote><p>The last bit about the lack of time for two species to communicate is pulled from the Drake equation, which gives an estimate of the number of Intelligent civilizations with whom communication is possible:</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/1024/1*oK6iJFsK3PhskK8oBD6QhA.jpeg" /></figure><p>A part of the argument in the <a href="https://en.wikipedia.org/wiki/Fermi_paradox">Fermi Paradox</a> suggests that the amount of time for which an Intelligent species exists to communicate its existence is quite small and space is quite big.</p><p><a href="https://medium.com/the-space-perspective/is-the-fermi-paradox-really-a-paradox-16b7b55d0b9e">Is the Fermi Paradox really a paradox?</a></p><img src="https://medium.com/_/stat?event=post.clientViewed&referrerSource=full_rss&postId=c5b2203fd133" width="1" height="1">]]></content:encoded>
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            <title><![CDATA[Amazing facts about White Dwarf stars]]></title>
            <link>https://medium.com/@uncertainquark/amazing-facts-about-white-dwarf-stars-1d9d06853b91?source=rss-7b8fb40c2a02------2</link>
            <guid isPermaLink="false">https://medium.com/p/1d9d06853b91</guid>
            <category><![CDATA[nature]]></category>
            <category><![CDATA[science]]></category>
            <category><![CDATA[space]]></category>
            <category><![CDATA[physics]]></category>
            <category><![CDATA[stars]]></category>
            <dc:creator><![CDATA[Jatan Mehta]]></dc:creator>
            <pubDate>Sun, 20 Aug 2017 05:48:15 GMT</pubDate>
            <atom:updated>2017-08-20T06:47:23.610Z</atom:updated>
            <cc:license>https://creativecommons.org/licenses/by-sa/4.0/</cc:license>
            <content:encoded><![CDATA[<p>When our Sun grows old and its size goes down, it will form a little White Dwarf star, the end stage of Sun-like stars. Don’t judge a White Dwarf star by its size though!</p><h3>#1: White Dwarf stars are the size of the Earth, but have the mass of a Sun</h3><p>One of the first White Dwarfs to be found, <a href="https://en.wikipedia.org/wiki/Sirius#Sirius_B">Sirius B</a> is merely the size of the Earth, making it quite small for a star.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/700/1*Big8C5PNb_wNFxo31qDLOA.jpeg" /><figcaption>White Dwarf star Sirius B compared to Earth. <a href="http://www.esa.int/spaceinimages/Images/2005/12/Sirius_B_compared_to_Earth">Source: ESA</a></figcaption></figure><p>And yet it manages to cram about the same mass as our Sun, making it much denser. Sirius B’s powerful gravitational field is 350 000 times greater than Earth’s, meaning that a 68 kg person would weigh 25 million kg on its surface!</p><p>Such high density was thought to be impossible by the scientific community a century ago, paraphrased nicely by <a href="https://en.wikipedia.org/wiki/Arthur_Eddington">Arthur Eddington</a>, after the discovery of such a White Dwarf:</p><blockquote>We learn about the stars by receiving and interpreting the messages which their light brings to us. The message of the Companion of Sirius when it was decoded ran: “I am composed of material 3,000 times denser than anything you have ever come across; a ton of my material would be a little nugget that you could put in a matchbox.” What reply can one make to such a message? The reply which most of us made in 1914 was — “Shut up. Don’t talk nonsense.”</blockquote><h3>#2: More massive a White Dwarf, the less its size!</h3><p>Past the <a href="https://en.wikipedia.org/wiki/Red_giant">Red Giant</a> stage and shedding of all the outer layers of gas, the leftover core of Sun-like stars is not capable of fusing matter to release light and energy. Gravity thus takes over and crams the electrons in such stars to give the high density that they are known for. More the gravity due to higher mass, more the crushing.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/590/0*OdFlQS6Y1MWaEIwM.jpg" /><figcaption>White Dwarf stars imaged by the Hubble Space Telescope. <a href="https://commons.wikimedia.org/wiki/File:White_dwarf-590.jpg">Source: Wikipedia</a></figcaption></figure><p>For gravity to compress a White Dwarf even further, it must force all the electrons to occupy all available spaces (energy state). Beyond that, Quantum Mechanics won’t allow gravity to compress the star any more: <a href="https://en.wikipedia.org/wiki/Pauli_exclusion_principle">Pauli’s Exclusion Principle</a> says that no 2 electrons can occupy the same energy state. This maximum limit for gravity being able to crush a White Dwarf gives the maximum mass it can have, known as the <a href="https://en.wikipedia.org/wiki/Chandrasekhar_Limit">Chandrasekhar limit</a>. <em>The most massive White Dwarf star is thus the smallest one around.</em></p><h3>#3: White Dwarfs can actually go Supernova!</h3><p>White Dwarf stars are sometimes found in close binary systems where the other star is less massive than our Sun is. Due to the proximity of these stars and the high gravitational pull of the White Dwarf, it pulls in matter from the companion!</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/800/0*Bf9coA-eEMIH13q9.jpg" /><figcaption>A White Dwarf star pulling matter from a companion star and forming an accretion disk. <a href="https://en.wikipedia.org/wiki/File:Accretion_Disk_Binary_System.jpg">Source: Wikipedia</a></figcaption></figure><p>The matter forms an accretion disk around the White Dwarf (due to <a href="https://en.wikipedia.org/wiki/Angular_momentum#Conservation_of_angular_momentum">conservation of angular momentum</a>) before falling on it with tremendous amounts of energy. The in-falling matter increases the density of the White Dwarf. If the density crosses the maximum limit for the stability of a White Dwarf (as discussed above), it results in a runaway <a href="https://en.wikipedia.org/wiki/Carbon_detonation">Carbon fusion detonation</a> that causes the entire star to go <a href="https://en.wikipedia.org/wiki/Supernova">Supernova</a> and <a href="https://arxiv.org/abs/astro-ph/0006305">destroys the entire star in a matter of seconds</a>.</p><h3>#4: White Dwarfs can be Pulsars too!</h3><p>The White Dwarf star <a href="https://astrobites.org/2016/12/23/ar-sco-the-first-white-dwarf-pulsar/">AR Sco</a> has an electromagnetic field 100 million times more powerful than Earth and rotates around itself in a mere 2 minutes. Such a powerful magnetic field produces intense lighthouse-like beams of radiation and particles, which shoot its companion <a href="https://en.wikipedia.org/wiki/Red_Dwarf">Red Dwarf</a> star to generate an enormous electric current in it.</p><iframe src="https://cdn.embedly.com/widgets/media.html?src=https%3A%2F%2Fwww.youtube.com%2Fembed%2FYdFi2qX9Hek%3Ffeature%3Doembed&amp;url=http%3A%2F%2Fwww.youtube.com%2Fwatch%3Fv%3DYdFi2qX9Hek&amp;image=https%3A%2F%2Fi.ytimg.com%2Fvi%2FYdFi2qX9Hek%2Fhqdefault.jpg&amp;key=a19fcc184b9711e1b4764040d3dc5c07&amp;type=text%2Fhtml&amp;schema=youtube" width="854" height="480" frameborder="0" scrolling="no"><a href="https://medium.com/media/21406d7ff4d4c20fb532b1a13ec4b5e1/href">https://medium.com/media/21406d7ff4d4c20fb532b1a13ec4b5e1/href</a></iframe><p>Such highly polarized radiation emission controlled by the star’s magnetic field was only ever seen before in <a href="https://en.wikipedia.org/wiki/Neutron_star">Neutron Stars</a>. Such stars are called <a href="https://en.wikipedia.org/wiki/Pulsar">Pulsars</a> and now White Dwarfs have the claim to that fame too.</p><h3>#5: White Dwarfs as a bright source of gravitational waves</h3><p>1600 Light-years away, 2 dense White Dwarfs are locked in a spiral dance around each other, every orbit a mere 5 minutes. They will eventually collapse together to form an even denser Neutron Star, as the orbit decays continually thanks to laws of <a href="https://en.wikipedia.org/wiki/General_relativity">General Relativity</a>. This releases <em>gravitational waves</em> as visualized here:</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/305/0*I4JdLOwduMnfcvv5.gif" /><figcaption>White Dwarf Stars in the binary systems <a href="https://en.wikipedia.org/wiki/RX_J0806.3%2B1527">RX J0806.3+1527</a> and their ultimate fate. <a href="https://www.nasa.gov/vision/universe/starsgalaxies/collide_whitedwarf.html">Source: NASA</a></figcaption></figure><p>It is expected that this system is one of the brightest sources of gravitational waves known to humans and will be a prime target for the upcoming <a href="https://en.wikipedia.org/wiki/Laser_Interferometer_Space_Antenna">gravitational wave space observatory LISA</a>.</p><h3>#6: White Dwarfs can be used to determine the age of the Universe</h3><p>Even though White Dwarfs no longer fuse matter to generate heat and light, their small surface area implies they cool very slowly, remaining hot for a long time. The cooler a White Dwarf star gets, the more time it takes to cool further, like a cup of coffee. Since <a href="https://en.wikipedia.org/wiki/Age_of_the_universe">the Universe is still quite young</a>, all known White Dwarfs are still quite hot and shine <em>white. </em>It will take billions of years for a White Dwarf to go dim red.</p><iframe src="https://cdn.embedly.com/widgets/media.html?src=https%3A%2F%2Fwww.youtube.com%2Fembed%2FnG1wnarvN8o%3Ffeature%3Doembed&amp;url=http%3A%2F%2Fwww.youtube.com%2Fwatch%3Fv%3DnG1wnarvN8o&amp;image=https%3A%2F%2Fi.ytimg.com%2Fvi%2FnG1wnarvN8o%2Fhqdefault.jpg&amp;key=a19fcc184b9711e1b4764040d3dc5c07&amp;type=text%2Fhtml&amp;schema=youtube" width="640" height="480" frameborder="0" scrolling="no"><a href="https://medium.com/media/5b4b6158a5eadf592d50f000e6355e1b/href">https://medium.com/media/5b4b6158a5eadf592d50f000e6355e1b/href</a></iframe><p>As the cooling takes place slower and slower with time, for a White Dwarf to form a dead <a href="https://en.wikipedia.org/wiki/Black_dwarf">Black Dwarf</a>, <a href="https://arxiv.org/abs/astro-ph/9701131">it will take trillions of years</a>. By looking at the stage of cooling of the oldest White Dwarfs there are, <a href="https://www.jpl.nasa.gov/news/news.php?feature=6430">the Hubble Space Telescope was used to determine the age of the Universe</a>, in agreement with other estimates of 13–14 billions years.</p><blockquote><em>Oh, and </em><a href="https://arxiv.org/abs/astro-ph/0402046"><em>seismological observations of a White Dwarf</em></a><em> suggest that </em><a href="https://arxiv.org/abs/astro-ph/0411199"><em>their cores are crystallized</em></a><em> like diamonds.</em></blockquote><img src="https://medium.com/_/stat?event=post.clientViewed&referrerSource=full_rss&postId=1d9d06853b91" width="1" height="1">]]></content:encoded>
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            <title><![CDATA[How Planets without Stars can possibly host Life on them]]></title>
            <link>https://medium.com/@uncertainquark/how-planets-without-stars-can-possibly-host-life-on-them-98532ac168f7?source=rss-7b8fb40c2a02------2</link>
            <guid isPermaLink="false">https://medium.com/p/98532ac168f7</guid>
            <category><![CDATA[exoplanets]]></category>
            <category><![CDATA[physics]]></category>
            <category><![CDATA[space]]></category>
            <category><![CDATA[life]]></category>
            <category><![CDATA[science]]></category>
            <dc:creator><![CDATA[Jatan Mehta]]></dc:creator>
            <pubDate>Thu, 10 Aug 2017 05:57:28 GMT</pubDate>
            <atom:updated>2017-08-20T06:39:32.976Z</atom:updated>
            <cc:license>https://creativecommons.org/licenses/by-sa/4.0/</cc:license>
            <content:encoded><![CDATA[<p>A look at ways in which starless planets can retain heat.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/1024/0*h4PdFxwRp0s26Idv.jpg" /><figcaption>An artist’s impression of the free-floating planet CFBDSIR J214947.2–040308.9 showing an infrared view of the object. The object appears blueish in this near-infrared view because most of the longer infrared wavelengths is absorbed by methane and other molecules in the planet’s atmosphere. In visible light the object is so cool that it would only shine dimly with a deep red colour when seen close-up. <a href="https://www.eso.org/public/images/eso1245a/">Source: ESO</a></figcaption></figure><p>Rogue planets are planets without stars and thus orbit the galaxy directly. This makes them incredibly difficult to find because they don’t reflect any starlight or are undetectable by common exoplanet detection methods. Yet Science paved the way to <a href="http://www.nbcnews.com/science/astronomers-say-theyve-spotted-lonesome-planet-without-sun-8C11366309">find just one such planet lurking in the dark</a> about 80 light years away. The faint red glow of the rogue planet <a href="https://en.wikipedia.org/wiki/PSO_J318.5-22"><em>PSO J318.5–22</em></a> was directly imaged by the <a href="https://en.wikipedia.org/wiki/Pan-STARRS">Pan-STARRS PS1 telescope</a>. Seeing that such rogue planets are hard to find, it makes sense that one is 6 times more massive than Jupiter, making it relatively easy to spot.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/640/0*F0ZD_gs3XWMIVqvF.png" /><figcaption>A direct image of the first rogue planet to be discovered - PSO J318.5–22. <a href="https://en.wikipedia.org/wiki/File:PSO_J318.5-22_image_from_the_Pan-STARRS1_telescope.png">Source: Wikipedia</a></figcaption></figure><h4>Rogue planets are everywhere</h4><p><a href="https://en.wikipedia.org/wiki/Gravitational_microlensing">Gravitational microlensing</a> observations of 50 million stars in the Milky Way <a href="https://phys.org/news/2011-05-class-planets.html">found 10 Jupiter-sized rogue planets</a>. This helped scientists estimate that there are at least 2 rogue planets for every star in the Galaxy (<a href="https://arxiv.org/abs/1105.3544v1"><em>Paper</em></a>). This means that there are potentially billions of rogue planets out there, lurking silently in the dark. Many of them are likely Earth-sized too.</p><p>A dead and desolate planet with no heat and light from a Sun seems like the last place to look for Life. However, there are ways rogue planets can retain heat and have suitable conditions for Life:</p><h3>#1: Rogue planets with Hydrogen dominated atmosphere can retain heat</h3><p>Not having a Sun has its advantages too, one being that exposure of the planet’s atmosphere to Ultra-Violet (UV) light is minimal. This helps even an Earth-sized rogue planet retain a Hydrogen dominated atmosphere. The paper <a href="http://hoffman.cm.utexas.edu/courses/rogue_planet_nature_letter.pdf"><em>Life-sustaining planets in interstellar space?</em></a> suggests that such an atmosphere can trap the planet’s heat through pressure induced far-infrared radiation. Under the right conditions (like a fully convective atmosphere), liquid water oceans are also possible.</p><h3>#2: Rogue planets can be geologically active</h3><p>A large natural satellite like our Moon generates tidal forces on Earth that cause significant heating due to friction. This heating increases geological activity of the planet.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/1024/0*6SycqvrhxxtI0YmD.jpg" /><figcaption>The tidal force of the Moon on the Earth (shown by the bulges) is a result of the centripetal force caused by the rotation around a common center of mass (yellow arrows) and the gravitational force caused by the Moon (red arrows). <a href="https://commons.wikimedia.org/wiki/File:Tidal_force.jpg">Source: Wikipedia</a></figcaption></figure><p>Early on after planetary formation, terrestrial planets with a large satellite (like the Earth-Moon system) can interact with Jupiter-sized bodies and get kicked out of the star system. <a href="https://arxiv.org/abs/0709.0945">Simulations of the same</a> suggest that about 5% of such terrestrial planets retain their satellite even after being pushed out of the system. The tidal heating caused by such a moon provides a longer span for geological activity for such rogue planets, giving a chance for Life to arise.</p><h3>#3: Moon of rogue planets can potentially harbour Life</h3><p>Free floating planetary-mass objects can eventually form a mini planetary system around them, much like the Jupiter mini-system. The <a href="https://en.wikipedia.org/wiki/Sub-brown_dwarf">sub-brown dwarf</a> <a href="https://en.wikipedia.org/wiki/OTS_44"><em>OTS-44</em></a> is <a href="https://arxiv.org/abs/1310.1936">known to be surrounded by a disk of at least 10 Earth masses</a>. OTS-44 can thus have a set of moons going around it in the future.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/1024/0*NQCsSgKWVzZtdw-K.png" /><figcaption>An artist’s impression of the sub-brown dwarf OTS 44 showing the disk of at least 10 Earth masses, which might evolve into a set of moons around the rogue planet. <a href="https://commons.wikimedia.org/wiki/File:Brown_Dwarf_11_0600.png">Source: Wikipedia</a></figcaption></figure><p>Just like how the tidal forces of Jupiter are responsible for its moon <a href="https://en.wikipedia.org/wiki/Europa_(moon)#Subsurface_ocean">Europa’s subsurface ocean</a>, moons around such rogue planets can have subsurface liquid water oceans too by the very same mechanism.</p><figure><img alt="" src="https://cdn-images-1.medium.com/max/1024/1*MZY8BnMsDJ57H8ovh612WQ.jpeg" /><figcaption>An artist’s illustration showing the internal structure of Jupiter’s moon Europa. Beneath the thick ice covering, lies an ocean of liquid water caused by the tidal heating effects of Jupiter’s gravity. Source: <a href="https://photojournal.jpl.nasa.gov/catalog/PIA01669">Source: NASA</a></figcaption></figure><p>Coupled this with possible sea floor volcanism and <a href="https://en.wikipedia.org/wiki/Hydrothermal_vent">hydrothermal vents</a> (that are considered to have been the birthplace of Life on Earth), such exomoons of these rogue exoplanets stand a chance at producing Life, even if bacterial.</p><p>In 2013, a possible discovery of an exomoon around a rogue planet was announced <a href="https://arxiv.org/abs/1312.3951">in this paper</a>.</p><h3>The Future</h3><p>The possibilities of Life existing on rogue planets is thus not as tiny as we think at first go. Our current capabilities of finding rogue planets is not so good but NASA’s upcoming <a href="https://en.wikipedia.org/wiki/Wide_Field_Infrared_Survey_Telescope">Wide Field InfraRed Survey Telescope</a> (WFIRST) is expected to expand our search significantly. Only then with significantly more data, can we even begin to contemplate the real possibilities of Life on such dark worlds.</p><blockquote>If we find any form of Life (however primeval) on dark and desolate exoplanets that have no Sun of their own, it would be clear that Nature still has a gazillion mysteries of its inner workings hidden from us, waiting to be understood.</blockquote><img src="https://medium.com/_/stat?event=post.clientViewed&referrerSource=full_rss&postId=98532ac168f7" width="1" height="1">]]></content:encoded>
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            <title><![CDATA[Haumea is actually ellipsoidal in shape, which doesn’t qualify as an irregular body: https://en…]]></title>
            <link>https://medium.com/@uncertainquark/haumea-is-actually-ellipsoidal-in-shape-which-doesnt-qualify-as-an-irregular-body-https-en-f5e5a928768a?source=rss-7b8fb40c2a02------2</link>
            <guid isPermaLink="false">https://medium.com/p/f5e5a928768a</guid>
            <dc:creator><![CDATA[Jatan Mehta]]></dc:creator>
            <pubDate>Sat, 29 Jul 2017 15:43:26 GMT</pubDate>
            <atom:updated>2017-07-29T15:43:26.154Z</atom:updated>
            <content:encoded><![CDATA[<p>Haumea is actually ellipsoidal in shape, which doesn’t qualify as an irregular body: <a href="https://en.wikipedia.org/wiki/Haumea#Size.2C_shape.2C_and_composition">https://en.wikipedia.org/wiki/Haumea#Size.2C_shape.2C_and_composition</a></p><img src="https://medium.com/_/stat?event=post.clientViewed&referrerSource=full_rss&postId=f5e5a928768a" width="1" height="1">]]></content:encoded>
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