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		<summary type="html">&lt;p&gt;Article written and Venn diagram created.&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;== Asteroid vs. Comet ==&lt;br /&gt;
Asteroids and comets are small solar system bodies that are remnants from the formation of the solar system around 4.6 billion years ago.&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt; The primary distinctions between them are their composition and their orbital paths.&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt; Their composition is largely determined by where they originated, with asteroids forming closer to the Sun and comets forming in the colder, outer regions of the solar system.&amp;lt;ref name=&amp;quot;ref3&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Recent discoveries have identified objects with characteristics of both, such as main-belt comets that orbit within the asteroid belt but show comet-like activity.&amp;lt;ref name=&amp;quot;ref4&amp;quot; /&amp;gt; Extinct comets, which have lost most of their volatile ices after many trips near the Sun, can also resemble asteroids.&amp;lt;ref name=&amp;quot;ref4&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Comparison Table ===&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! Category !! Asteroid !! Comet&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;Composition&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
| Primarily made of rock and metals.&amp;lt;ref name=&amp;quot;ref3&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref5&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt;&lt;br /&gt;
| Composed of ice, dust, rock, and organic compounds.&amp;lt;ref name=&amp;quot;ref3&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref5&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;Origin&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
| Mostly from the main asteroid belt between Mars and Jupiter.&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt;&lt;br /&gt;
| Originate in the Kuiper Belt and the more distant Oort Cloud.&amp;lt;ref name=&amp;quot;ref4&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;Orbit Shape&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
| Generally have shorter, more circular orbits.&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt;&lt;br /&gt;
| Typically have long, highly elliptical (egg-shaped) orbits.&amp;lt;ref name=&amp;quot;ref4&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;Orbital Period&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
| Shorter periods, often a few years.&lt;br /&gt;
| Can range from several years to millions of years.&amp;lt;ref name=&amp;quot;ref4&amp;quot; /&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;Appearance&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
| Appear as a point of light; solid and cratered surface.&lt;br /&gt;
| Develops a glowing cloud (coma) and tails when near the Sun.&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;Tails&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
| Do not have tails.&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt;&lt;br /&gt;
| Develops two tails (a dust tail and an ion tail) when solar radiation vaporizes its ice.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File:Venn_diagram_Differences_between_Asteroid_versus_Comet_comparison.png|thumb|center|800px|alt=Venn diagram for Differences between Asteroid and Comet|Venn diagram comparing Differences between Asteroid and Comet]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Formation and Location ===&lt;br /&gt;
Asteroids formed closer to the Sun where the high temperatures would have evaporated any ice.&amp;lt;ref name=&amp;quot;ref3&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt; The majority are found in the asteroid belt, a region between the orbits of Mars and Jupiter. It is believed that the gravitational influence of Jupiter prevented the material in this region from coalescing into a planet.&lt;br /&gt;
&lt;br /&gt;
Comets originated in the colder, outer reaches of the solar system, far enough from the Sun for volatile ices to remain frozen.&amp;lt;ref name=&amp;quot;ref3&amp;quot; /&amp;gt; They are primarily found in two regions: the Kuiper Belt, a disk-like zone beyond Neptune, and the Oort Cloud, a spherical shell at the very edge of the solar system.&amp;lt;ref name=&amp;quot;ref4&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Orbital Characteristics ===&lt;br /&gt;
Most asteroids travel in relatively stable, circular orbits within the main belt.&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt; In contrast, comets have highly eccentric, elongated orbits that take them from the distant outer solar system to a close pass by the Sun.&amp;lt;ref name=&amp;quot;ref4&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;ref2&amp;quot; /&amp;gt; The orbital periods of short-period comets, originating from the Kuiper Belt, are defined as less than 200 years.&amp;lt;ref name=&amp;quot;ref4&amp;quot; /&amp;gt; Long-period comets, from the Oort cloud, can have orbital periods of thousands or even millions of years.&amp;lt;ref name=&amp;quot;ref4&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Physical Appearance ===&lt;br /&gt;
An asteroid typically appears as a rocky, inert body. Its surface is often cratered from collisions with other objects. Comets, on the other hand, are often called &amp;quot;dirty snowballs&amp;quot; due to their icy composition. When a comet&amp;#039;s orbit brings it close to the Sun, the solar heat vaporizes its ices.&amp;lt;ref name=&amp;quot;ref1&amp;quot; /&amp;gt; This process releases gas and dust, forming a large, glowing atmosphere around the nucleus called a coma, and two distinct tails—a dust tail and a gas (ion) tail—that can stretch for millions of kilometers.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&amp;lt;references&amp;gt;&lt;br /&gt;
&amp;lt;ref name=&amp;quot;ref1&amp;quot;&amp;gt;[https://byjus.com/physics/asteroid-and-comet-difference/ &amp;quot;byjus.com&amp;quot;]. Retrieved January 07, 2026.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&amp;lt;ref name=&amp;quot;ref2&amp;quot;&amp;gt;[https://www.britannica.com/science/What-Is-the-Difference-Between-Comets-and-Asteroids &amp;quot;britannica.com&amp;quot;]. Retrieved January 07, 2026.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&amp;lt;ref name=&amp;quot;ref3&amp;quot;&amp;gt;[https://coolcosmos.ipac.caltech.edu/ask/181-What-is-the-difference-between-an-asteroid-and-a-comet- &amp;quot;caltech.edu&amp;quot;]. Retrieved January 07, 2026.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&amp;lt;ref name=&amp;quot;ref4&amp;quot;&amp;gt;[https://en.wikipedia.org/wiki/Comet &amp;quot;wikipedia.org&amp;quot;]. Retrieved January 07, 2026.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&amp;lt;ref name=&amp;quot;ref5&amp;quot;&amp;gt;[https://www.nisenet.org/asteroids &amp;quot;nisenet.org&amp;quot;]. Retrieved January 07, 2026.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&amp;lt;/references&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:Comparisons]]&lt;/div&gt;</summary>
		<author><name>Dwg</name></author>
		
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