<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom" xmlns:content="http://purl.org/rss/1.0/modules/content/"><channel><title>Collimation on Startgaze — Astronomy, Stargazing &amp; Space Science</title><link>https://www.startgaze.com/tags/collimation/</link><description>Recent content in Collimation on Startgaze — Astronomy, Stargazing &amp; Space Science</description><generator>Hugo</generator><language>en-us</language><lastBuildDate>Wed, 09 Sep 2026 07:37:57 +0000</lastBuildDate><atom:link href="https://www.startgaze.com/tags/collimation/index.xml" rel="self" type="application/rss+xml"/><item><title>Collimating a Dobsonian after the drive: the two tools that matter</title><link>https://www.startgaze.com/posts/2026-09-09-collimate-dobsonian-after-the-drive/</link><pubDate>Wed, 09 Sep 2026 07:37:57 +0000</pubDate><guid>https://www.startgaze.com/posts/2026-09-09-collimate-dobsonian-after-the-drive/</guid><description>A Dobsonian arrives at the dark site out of collimation every time. Here&amp;#39;s the two-minute field routine, the two tools worth owning, and the star test that proves it.</description></item></channel></rss>