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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Long-Term Stability of Planets in the $α$ Centauri System · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1604.04917/</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/1604.04917/feed.xml" rel="self" type="application/rss+xml" /><item><title>Long-Term Stability of Planets in the $α$ Centauri System — mentioned by devindotcom</title><link>https://news.ycombinator.com/item?id=12687197</link><guid isPermaLink="false">urn:hackerpapers:mention:1604.04917:12687197</guid><pubDate>Tue, 11 Oct 2016 18:31:12 GMT</pubDate><description>&lt;p&gt;Project Blue rep says: Simulations suggest that orbits beyond 2.5 A.U. are unstable, but all the habitable zone orbits are stable: For example, see: https://arxiv.org/abs/1604.04917&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1604.04917/"&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>
