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	<id>https://www.conservapedia.com/index.php?action=history&amp;feed=atom&amp;title=Hubble_sequence</id>
	<title>Hubble sequence - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://www.conservapedia.com/index.php?action=history&amp;feed=atom&amp;title=Hubble_sequence"/>
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	<updated>2026-10-23T14:01:47Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>https://www.conservapedia.com/index.php?title=Hubble_sequence&amp;diff=1377265&amp;oldid=prev</id>
		<title>FredericBernard: Added image</title>
		<link rel="alternate" type="text/html" href="https://www.conservapedia.com/index.php?title=Hubble_sequence&amp;diff=1377265&amp;oldid=prev"/>
		<updated>2017-09-27T14:12:36Z</updated>

		<summary type="html">&lt;p&gt;Added image&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 14:12, September 27, 2017&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot; &gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;[[File:HubbleTuningFork.jpg|thumb|right|295px|Classification into [[Spiral galaxy|spirals]] and [[Elliptical galaxy|ellipticals]].]]&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The '''Hubble sequence''' is a scheme for classifying [[galaxies]].&amp;lt;ref name=spacetelescope&amp;gt;[https://www.spacetelescope.org/images/heic9902o/ The Hubble tuning fork diagram] from spacetelescope.org&amp;lt;/ref&amp;gt; Developed in 1926 by [[Edwin Hubble]], it splits galaxies into two major groups: [[elliptical galaxy|elliptical galaxies]] and [[spiral galaxy|spiral galaxies]]. Nowadays, it is understood to be too simple a classification scheme. It is sometimes called the &amp;quot;Hubble tuning fork diagram&amp;quot; due to its resemblance to a tuning fork.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The '''Hubble sequence''' is a scheme for classifying [[galaxies]].&amp;lt;ref name=spacetelescope&amp;gt;[https://www.spacetelescope.org/images/heic9902o/ The Hubble tuning fork diagram] from spacetelescope.org&amp;lt;/ref&amp;gt; Developed in 1926 by [[Edwin Hubble]], it splits galaxies into two major groups: [[elliptical galaxy|elliptical galaxies]] and [[spiral galaxy|spiral galaxies]]. Nowadays, it is understood to be too simple a classification scheme. It is sometimes called the &amp;quot;Hubble tuning fork diagram&amp;quot; due to its resemblance to a tuning fork.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
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		<author><name>FredericBernard</name></author>
	</entry>
	<entry>
		<id>https://www.conservapedia.com/index.php?title=Hubble_sequence&amp;diff=1375632&amp;oldid=prev</id>
		<title>FredericBernard: Create page with explanation of the Hubble classification scheme for galaxies</title>
		<link rel="alternate" type="text/html" href="https://www.conservapedia.com/index.php?title=Hubble_sequence&amp;diff=1375632&amp;oldid=prev"/>
		<updated>2017-09-21T16:47:24Z</updated>

		<summary type="html">&lt;p&gt;Create page with explanation of the Hubble classification scheme for galaxies&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;The '''Hubble sequence''' is a scheme for classifying [[galaxies]].&amp;lt;ref name=spacetelescope&amp;gt;[https://www.spacetelescope.org/images/heic9902o/ The Hubble tuning fork diagram] from spacetelescope.org&amp;lt;/ref&amp;gt; Developed in 1926 by [[Edwin Hubble]], it splits galaxies into two major groups: [[elliptical galaxy|elliptical galaxies]] and [[spiral galaxy|spiral galaxies]]. Nowadays, it is understood to be too simple a classification scheme. It is sometimes called the &amp;quot;Hubble tuning fork diagram&amp;quot; due to its resemblance to a tuning fork.&lt;br /&gt;
&lt;br /&gt;
==Galaxy Types==&lt;br /&gt;
===Elliptical Galaxies===&lt;br /&gt;
[[Elliptical galaxy|Elliptical galaxies]] are shaped like an [[ellipse]] and are classified as &amp;quot;En&amp;quot; where n is an [[integer]] between 0 and 7 relating to the galaxies eccentricity. A galaxy with a higher n is more eccentric, so that an E0 galaxy is circular while and E7 galaxy is very elongated. Elliptical galaxies are called &amp;quot;early-type&amp;quot; as Hubble originally believed that galaxies evolved from ellipticals into spiral galaxies.&amp;lt;ref name=sdss&amp;gt;[http://skyserver.sdss.org/dr1/en/proj/advanced/galaxies/tuningfork.asp Hubble tuning fork] from skyserver.sdss.org&amp;lt;/ref&amp;gt; This is not thought to be true now but the name still sticks. Elliptical galaxies form the handle of the tuning fork.&lt;br /&gt;
&lt;br /&gt;
===Spiral Galaxies===&lt;br /&gt;
These are galaxies that are shaped like a disk and contain spiral arms. They are split into two categories depending on whether the bulge contains a bar or not and form the prongs of the tuning fork. If a bar is present, they are labelled &amp;quot;SB&amp;quot;, otherwise just &amp;quot;S&amp;quot;.&amp;lt;ref name=spacetelescope/&amp;gt; They are further classified by assigning the letters &amp;quot;a&amp;quot;, &amp;quot;b&amp;quot; and &amp;quot;c&amp;quot;, depending on how tightly wound their spiral arms are. The letter &amp;quot;a&amp;quot; is assigned to those with the tightest winding and &amp;quot;c&amp;quot; to the least tightly wound. Type b is located in between. The size of the bulge also appears to follow a pattern, with type a galaxies containing a large bulge and type c a small bulge.&amp;lt;ref name=spacetelescope/&amp;gt; They are called &amp;quot;late-types&amp;quot; as Hubble believed they evolved from elliptical galaxies but this is known not to be the case.&amp;lt;ref name=sdss/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Lenticular Galaxies===&lt;br /&gt;
[[Lenticular galaxy|Lenticular galaxies]] occur where the handle joins the two prongs of the tuning fork. They are classified as &amp;quot;S0&amp;quot; and bridge the two main types.&amp;lt;ref name=spacetelescope/&amp;gt; These galaxies have the bulge and disk present in spiral galaxies, but do not have spiral arms.&amp;lt;ref name=sdss/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Irregular Galaxies===&lt;br /&gt;
Some galaxies do not fit into the above types and are called [[irregular galaxy|irregular galaxies]].&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
{{Galaxies}}&lt;br /&gt;
&lt;br /&gt;
[[Category:Astronomy]]&lt;/div&gt;</summary>
		<author><name>FredericBernard</name></author>
	</entry>
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