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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>An orbital window into the ancient Sun's mass · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1811.07135/</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/1811.07135/feed.xml" rel="self" type="application/rss+xml" /><item><title>An orbital window into the ancient Sun's mass — mentioned by zyrxvo</title><link>https://news.ycombinator.com/item?id=35184702</link><guid isPermaLink="false">urn:hackerpapers:mention:1811.07135:35184702</guid><pubDate>Thu, 16 Mar 2023 16:56:33 GMT</pubDate><description>&lt;p&gt;This article by Lhotka &amp;amp; Gale (2019) &amp;lt;https://arxiv.org/abs/1911.02778&amp;gt; is a little beyond my patience for understanding, but they have an excellent parameter space plot in Figure 1 relating a bunch of different effects with respect to dust grain size. Their figure only goes up to grains 1 cm in size though. However, it&amp;#x27;s a detailed paper on the relative &amp;quot;importance of the interplanetary magnetic field on the orbital evolution of dust&amp;quot;. I met Lhotka at a conference where they presented this work. I think this discussion is really fascinating, and it&amp;#x27;s certainly something that I didn&amp;#x27;t…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1811.07135/"&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>
