<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Lacerta on 庭 — a journal</title><link>https://www.nichi-doku.de/en/tags/lacerta/</link><description>Recent content in Lacerta on 庭 — a journal</description><generator>Hugo</generator><language>en-US</language><lastBuildDate>Sun, 04 Oct 2026 00:00:00 +0000</lastBuildDate><atom:link href="https://www.nichi-doku.de/en/tags/lacerta/index.xml" rel="self" type="application/rss+xml"/><item><title>Sh2-126 – the Gecko in Lacerta</title><link>https://www.nichi-doku.de/en/astrofotografie/sh2-126-der-gekko-in-der-eidechse/</link><pubDate>Sun, 04 Oct 2026 00:00:00 +0000</pubDate><guid>https://www.nichi-doku.de/en/astrofotografie/sh2-126-der-gekko-in-der-eidechse/</guid><description>&lt;p&gt;Tucked away in the small constellation of Lacerta, the Lizard, lies a sprawling cloud of hydrogen listed as number 126 in Stewart Sharpless&amp;rsquo;s catalogue. Its glow is powered by 10 Lacertae, a hot, bluish O-type star belonging to the young stellar group Lacerta OB1. The star&amp;rsquo;s energetic ultraviolet light excites the surrounding gas, which in turn shines in the characteristic red of hydrogen. Measurements disagree on how far away the region is; most estimates fall somewhere between roughly 1,200 and 1,800 light-years. The nebula cannot be seen through the eyepiece – only long exposures bring out its structure. The shape at the head of the filaments resembles a gecko, a fitting match for its host constellation. Beyond the red bands, grey veils of dust and dark clouds absorb the light from behind.&lt;/p&gt;</description></item></channel></rss>