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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Orbital Evolution of Binaries in Circumbinary Disks · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2302.01785/</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/2302.01785/feed.xml" rel="self" type="application/rss+xml" /><item><title>Orbital Evolution of Binaries in Circumbinary Disks — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=35186469</link><guid isPermaLink="false">urn:hackerpapers:mention:2302.01785:35186469</guid><pubDate>Thu, 16 Mar 2023 18:46:38 GMT</pubDate><description>&lt;p&gt;&amp;quot;In the planetary system, solar gravity determines the orbits of all bodies larger than dust particles for which other forces become important. But even for dust, gravity is an important factor. Near planets, planetary gravity takes over&amp;quot;, §3.1 of Krüger &amp;amp; Grün&amp;#x27;s Chapter 29 in Encyclopedia of the Solar System (2014) &amp;lt;https://doi.org/10.1016/B978-0-12-415845-0.00029-3&amp;gt; (it&amp;#x27;s on scy hob :) ). See Table 29.4. Where dust is gravitationally interesting at the present age of the solar system is probably in ring/moon interactions, but mostly with the moon acting on the ring dusts as with Saturn&amp;#x27;s…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2302.01785/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.HE</category></item></channel></rss>
