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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Revisiting rho 1 Cancri e: A New Mass Determination Of The Transiting super-Earth · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1208.5709/</link><description>Collected HN comments and submissions linking this paper.</description><language>en</language><lastBuildDate>Mon, 02 Nov 2026 11:16:22 GMT</lastBuildDate><atom:link href="https://hackerpaper.kaipfister.de/p/1208.5709/feed.xml" rel="self" type="application/rss+xml" /><item><title>Revisiting rho 1 Cancri e: A New Mass Determination Of The Transiting super-Earth — mentioned by uvdiv</title><link>https://news.ycombinator.com/item?id=4642234</link><guid isPermaLink="false">urn:hackerpapers:mention:1208.5709:4642234</guid><pubDate>Thu, 11 Oct 2012 19:08:23 GMT</pubDate><description>&lt;p&gt;Here&amp;#x27;s the paper. http://arxiv.org/pdf/1210.2720.pdf It&amp;#x27;s reasoned guess. They know three things about the planet: its mass, its size (radius/volume), and its orbital distance. They also know some of the chemistry of the star it orbits. From the mass and radius, they inferred the density of the planet is a lower than other rock planets. They can explain low density in several ways. One is a thick layer of low-density supercritical water on the surface. Very large, extremely hot &amp;quot;oceans&amp;quot;. An alternative is low-density graphite or diamond inside the mantle. What they show is that a carbon…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1208.5709/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.EP</category></item></channel></rss>
