<?xml version="1.0" encoding="UTF-8"?>
<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The MACHO Project: Microlensing Results from 5.7 Years of LMC Observations · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/astro-ph_0001272/</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/astro-ph_0001272/feed.xml" rel="self" type="application/rss+xml" /><item><title>The MACHO Project: Microlensing Results from 5.7 Years of LMC Observations — mentioned by astrosi</title><link>https://news.ycombinator.com/item?id=33053856</link><guid isPermaLink="false">urn:hackerpapers:mention:astro-ph_0001272:33053856</guid><pubDate>Sun, 02 Oct 2022 07:48:29 GMT</pubDate><description>&lt;p&gt;Unlikely, dead dark stars being dark matter candidates is a theory known as MACHOs (massive compact halo objects) If they exist we would expect to detect them as they pass between another star and earth creating a gravitational lens. You can estimate the number of these MACHOs by looking at a bunch of stars for a long period of time and counting the number of microlensing events you see. A team did this in 2000 and found that while there were some events, there weren&amp;#x27;t enough to explain all of the dark matter around the Milky Way. https://arxiv.org/abs/astro-ph/0001272&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/astro-ph_0001272/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph</category></item><item><title>The MACHO Project: Microlensing Results from 5.7 Years of LMC Observations — mentioned by xenophonf</title><link>https://news.ycombinator.com/item?id=19605307</link><guid isPermaLink="false">urn:hackerpapers:mention:astro-ph_0001272:19605307</guid><pubDate>Mon, 08 Apr 2019 14:07:03 GMT</pubDate><description>&lt;p&gt;Are you indirectly asking whether planets can be dark matter candidates? If so, those are called MACHOs (massive compact halo objects). They have been studied via the gravitational microlensing effect. The presence of MACHOs can&amp;#x27;t account for most dark matter. https://arxiv.org/pdf/astro-ph/0001272.pdf https://arxiv.org/pdf/astro-ph/9904401.pdf When you see figures like &amp;quot;1E-7 to 1E-2 M⊙ mass range&amp;quot; (from the above paper&amp;#x27;s introduction), note that a Jupiter mass is about 1E-3 M⊙---one thousandth or 0.1% the mass of the Sun. Earth is 3E-6 M⊙, the Moon is 3.7E-8 M⊙, and Pluto is 6.6E-9 M⊙; or…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/astro-ph_0001272/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph</category></item></channel></rss>
