<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>M108 on Suburban Backyard Astro Sights</title><link>https://hgastro.github.io/tags/m108/</link><description>Recent content in M108 on Suburban Backyard Astro Sights</description><generator>Hugo -- gohugo.io</generator><language>en</language><managingEditor>hgastroblog@gmail.com</managingEditor><webMaster>hgastroblog@gmail.com</webMaster><copyright>All images and content on this website © 2025 Howard Grams</copyright><lastBuildDate>Thu, 27 Feb 2020 00:00:00 +0000</lastBuildDate><atom:link href="https://hgastro.github.io/tags/m108/index.xml" rel="self" type="application/rss+xml"/><item><title>The Owl Nebula and Surfboard Galaxy</title><link>https://hgastro.github.io/posts/2020-02-27-m97-and-m108/</link><pubDate>Thu, 27 Feb 2020 00:00:00 +0000</pubDate><author>hgastroblog@gmail.com</author><guid>https://hgastro.github.io/posts/2020-02-27-m97-and-m108/</guid><description>&lt;p>The Owl Nebula (also known Messier 97) is a planetary nebula located approximately 2,030 light years away in the constellation Ursa Major. When William Parsons observed the nebula in 1848, his hand-drawn illustration resembled an owl&amp;rsquo;s head. It has been known as the Owl Nebula ever since. The nebula is approximately 8,000 years old. It is approximately circular in cross-section with a little visible internal structure. The nebula is arranged in three concentric shells, with the outermost shell being about 20–30% larger than the inner shell. The owl-like appearance of the nebula is the result of an inner shell that is not circularly symmetric, but instead forms a barrel-like structure aligned at an angle of 45° to the line of sight.&lt;/p></description></item></channel></rss>