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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Fractal Signatures in Analogs of Interplanetary Dust Particles · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1402.7132/</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/1402.7132/feed.xml" rel="self" type="application/rss+xml" /><item><title>Fractal Signatures in Analogs of Interplanetary Dust Particles — mentioned by gene-h</title><link>https://news.ycombinator.com/item?id=19203235</link><guid isPermaLink="false">urn:hackerpapers:mention:1402.7132:19203235</guid><pubDate>Tue, 19 Feb 2019 21:55:40 GMT</pubDate><description>&lt;p&gt;It makes more sense to call it a fractal rather than a pile. In the paper they reference, it is suggested that particles can form fractal like structures through a diffusion limited aggregation process[0]. One very important result in planetary science is the observation by the astronaut Donald Pettit of granular materials aggregating together in microgravity[1]* . In the experiment[2], it appears that some of the resulting structures resemble those formed in a diffusion limited aggregation process. *It is also worth noting that this experiment was entirely ad-hoc and came about from Don…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1402.7132/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.SR</category></item></channel></rss>
