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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>A giant planet undergoing extreme ultraviolet irradiation by its hot massive-star host · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1706.06723/</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/1706.06723/feed.xml" rel="self" type="application/rss+xml" /><item><title>A giant planet undergoing extreme ultraviolet irradiation by its hot massive-star host — mentioned by jessriedel</title><link>https://news.ycombinator.com/item?id=17800935</link><guid isPermaLink="false">urn:hackerpapers:mention:1706.06723:17800935</guid><pubDate>Mon, 20 Aug 2018 15:52:35 GMT</pubDate><description>&lt;p&gt;You repeated one of my own points back to me and then condescended down to me about not appreciating orders of magnitude. (I&amp;#x27;m a physicist myself.) The whole purpose of my comment is that 25 is not that small of a factor on astronomical scales and it suggests the BB radiation of the planet itself would be detectable. As it turns out, this is the case &amp;gt; As a result, [the planet] has an extremely high equilibrium temperature, assuming zero albedo and perfect heat redistribution, of ∼4050 K. This is as hot as a late K-type star, and thus we expected a large thermal emission signal, which we…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1706.06723/"&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>
