<?xml version="1.0" encoding="UTF-8"?>
<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Kinematics of the Interstellar Vagabond 1I/'Oumuamua (A/2017 U1) · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1710.11364/</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/1710.11364/feed.xml" rel="self" type="application/rss+xml" /><item><title>Kinematics of the Interstellar Vagabond 1I/'Oumuamua (A/2017 U1) — mentioned by kirykl</title><link>https://news.ycombinator.com/item?id=19202540</link><guid isPermaLink="false">urn:hackerpapers:mention:1710.11364:19202540</guid><pubDate>Tue, 19 Feb 2019 20:37:14 GMT</pubDate><description>&lt;p&gt;Weird still is &amp;quot;Oumuamua&amp;#x27;s velocity (being) within 5 km/s of the median Galactic velocity of the stars in the solar neighborhood&amp;quot; (https://arxiv.org/abs/1710.11364) That means the system it originated from if a natural object would need to be coincidentally that close to our median local&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1710.11364/"&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>
