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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Binary YORP and Evolution of Binary Asteroids · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1010.2676/</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/1010.2676/feed.xml" rel="self" type="application/rss+xml" /><item><title>Binary YORP and Evolution of Binary Asteroids — mentioned by dandelany</title><link>https://news.ycombinator.com/item?id=18811705</link><guid isPermaLink="false">urn:hackerpapers:mention:1010.2676:18811705</guid><pubDate>Thu, 03 Jan 2019 00:22:13 GMT</pubDate><description>&lt;p&gt;Tidal forces are one way - either between the two binary components, or from a close encounter with a third, larger body. Another is the &amp;quot;YORP Effect&amp;quot;. Sunlight falling on an asteroid produces a slight thermal radiation pressure (push). If, due to asymmetries in asteroid shape/albedo, the net radiation pressure force is not aligned with the asteroid&amp;#x27;s center of mass, it will produce a torquing force which will cause the asteroid to spin faster (or slower) over time. Applying the idea of YORP Effect to binary asteroids yields the &amp;quot;BYORP [Binary YORP] Effect&amp;quot;, by which the orbital dynamics of…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1010.2676/"&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>
