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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Tidal obliquity evolution of potentially habitable planets · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1101.2156/</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/1101.2156/feed.xml" rel="self" type="application/rss+xml" /><item><title>Tidal obliquity evolution of potentially habitable planets — mentioned by nabla9</title><link>https://news.ycombinator.com/item?id=17125341</link><guid isPermaLink="false">urn:hackerpapers:mention:1101.2156:17125341</guid><pubDate>Tue, 22 May 2018 12:15:54 GMT</pubDate><description>&lt;p&gt;The background for the article is &amp;#x27;tilt erosion time&amp;#x27; and the large number of tidally locked planets in the habitable zones of numerous low-mass stars. Many new discovered planets are tidally locked: Kepler-438b, Kepler-442b, K2-3d, K2-155d. It was previously assumed that tidally locked planets would not be habitable. New climate modeling seems to change this view. No snowball on habitable tidally locked planets https://arxiv.org/abs/1705.08904 Stabilizing Cloud Feedback Dramatically Expands the Habitable Zone of Tidally Locked Planets https://arxiv.org/abs/1307.0515 Tidal obliquity evolution…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1101.2156/"&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>
