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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Swansong Biospheres II: The final signs of life on terrestrial planets near the end of their habitable lifetimes · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1310.4841/</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/1310.4841/feed.xml" rel="self" type="application/rss+xml" /><item><title>Swansong Biospheres II: The final signs of life on terrestrial planets near the end of their habitable lifetimes — mentioned by Retric</title><link>https://news.ycombinator.com/item?id=34385465</link><guid isPermaLink="false">urn:hackerpapers:mention:1310.4841:34385465</guid><pubDate>Sun, 15 Jan 2023 00:20:00 GMT</pubDate><description>&lt;p&gt;Eventually the oceans will boil, but wikipedia links to paper evaluating the atmosphere in “1 Gyr and 2.8 Gyr from present” or 1 to 2.8 billion years not 500. It’s suggesting that life should stick around on earth for ~2.8 billion years though the total number of living cells will noticeably start to decline at 1 billion years. https://arxiv.org/abs/1310.4841 In general it would take a very large change in the suns output to make a noticeable difference on earth. There are critical secondary effects and feedback loops etc, but black body radiation is T^4 so you take the square root of the…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1310.4841/"&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>
