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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The Flux of Kilogram-Sized Meteoroids from Lunar Impact Monitoring · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1404.6458/</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/1404.6458/feed.xml" rel="self" type="application/rss+xml" /><item><title>The Flux of Kilogram-Sized Meteoroids from Lunar Impact Monitoring — mentioned by azernik</title><link>https://news.ycombinator.com/item?id=19803106</link><guid isPermaLink="false">urn:hackerpapers:mention:1404.6458:19803106</guid><pubDate>Thu, 02 May 2019 00:13:51 GMT</pubDate><description>&lt;p&gt;(Nitpick: those impactors are also meteorites, just big ones; the numbers in the paper I linked numbers are based on probabilities over time of an impactor large enough to get through shielding.) Giant impacts are relatively rare - in the ~13 years of NASA&amp;#x27;s monitoring program, the largest impactor seen on the Earth-facing hemisphere of the moon left a 15m (inner diameter) crater [https://arxiv.org/pdf/1404.6458.pdf], and most have been orders of magnitude smaller. Remember - the Moon has no active tectonics, no atmospheric weathering, and no water or other liquid evaporation/condensation…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1404.6458/"&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>
