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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>A new estimate of the Local Standard of Rest from data on young Galactic objects · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1411.3572/</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/1411.3572/feed.xml" rel="self" type="application/rss+xml" /><item><title>A new estimate of the Local Standard of Rest from data on young Galactic objects — mentioned by maze-le</title><link>https://news.ycombinator.com/item?id=16652441</link><guid isPermaLink="false">urn:hackerpapers:mention:1411.3572:16652441</guid><pubDate>Thu, 22 Mar 2018 20:31:26 GMT</pubDate><description>&lt;p&gt;It seems to be quite fast, but not exceptionally. Lets do a quick calculation, and neglect all aspects of proper stellar kinematics -- Our sun has traveled quite some distance itself during the 70000 years, I don&amp;#x27;t properly described that motion itself, so take everything with a grain of salt: Lets call the speed difference of the star with respect to our sun `Δv` Δv = 20 [ly] / 70 000 [y] = 0.000285714 [ly/y] Now, lets convert the unit `ly/y` into a unit that we can relate to, to get a grasp on it: 1ly = 63241.08AU[1]. Δv = 0.000285714 [ly/y] = 18.0688 [AU/y] 18 AU is about the perihelion of…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1411.3572/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.GA</category></item></channel></rss>
