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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>On the dynamical evolution of 2002 VE68 · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1208.4444/</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/1208.4444/feed.xml" rel="self" type="application/rss+xml" /><item><title>On the dynamical evolution of 2002 VE68 — mentioned by FooBarBizBazz</title><link>https://news.ycombinator.com/item?id=39152323</link><guid isPermaLink="false">urn:hackerpapers:mention:1208.4444:39152323</guid><pubDate>Sat, 27 Jan 2024 03:48:09 GMT</pubDate><description>&lt;p&gt;The thread is about an object in our solar system, called 2002 VE. Its motion under the influence of gravity isn&amp;#x27;t clearly &amp;quot;an orbit&amp;quot;, but (for now) it sort of follows closed loops when viewed from the moving frame of Venus, so people call it a quasi-moon of Venus. Figure 4 in this paper shows the object&amp;#x27;s trajectory in the frame of Venus: https://arxiv.org/pdf/1208.4444.pdf&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1208.4444/"&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>
