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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Modelling the reflective thermal contribution to the acceleration of the Pioneer spacecraft · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1103.5222/</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/1103.5222/feed.xml" rel="self" type="application/rss+xml" /><item><title>Modelling the reflective thermal contribution to the acceleration of the Pioneer spacecraft — mentioned by Jabbles</title><link>https://news.ycombinator.com/item?id=2391801</link><guid isPermaLink="false">urn:hackerpapers:mention:1103.5222:2391801</guid><pubDate>Thu, 31 Mar 2011 14:51:52 GMT</pubDate><description>&lt;p&gt;The key conclusion, with error estimates: We performed 10^4 Monte Carlo iterations, which easily ensures the convergence of the result. The thermal acceleration estimate yielded by the simulation for an instant 26 years after launch, with a 95% probability, is a(t=26) = (5.8 ± 1.3) × 10^−10 ms^-2. ... These results account for between 44% and 96% of the reported value a = (8.74 ± 1.33) × 10^−10 ms^-2 (which, we recall, was obtained under the hypothesis of a constant acceleration) — thus giving a strong indication of the preponderant contribution of thermal eﬀects to the Pioneer anomaly.…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1103.5222/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>physics.space-ph</category></item></channel></rss>
