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	<title>Planet Nine - Revision history</title>
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	<updated>2026-04-26T13:38:59Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<id>https://wikimd.org/index.php?title=Planet_Nine&amp;diff=5655555&amp;oldid=prev</id>
		<title>Prab: CSV import</title>
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		<updated>2024-04-24T03:29:13Z</updated>

		<summary type="html">&lt;p&gt;CSV import&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[[File:Planet_nine_artistic_plain.png|Planet nine artistic plain|thumb]] &amp;#039;&amp;#039;&amp;#039;Planet Nine&amp;#039;&amp;#039;&amp;#039; is a hypothetical [[planet]] in the outer region of the [[Solar System]]. Its existence was first proposed by [[astronomers]] [[Konstantin Batygin]] and [[Michael E. Brown]] in 2016, based on the unusual clustering of six objects in the [[Kuiper Belt]], a region beyond [[Neptune]] filled with [[dwarf planets]], [[comets]], and other small [[solar system bodies]]. The gravitational effects on these objects suggest the presence of a large, unseen planet. Planet Nine is theorized to be a [[gas giant]] with a mass approximately ten times that of [[Earth]], orbiting the Sun at a distance of 400 to 800 [[astronomical units]] (AU).&lt;br /&gt;
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==Discovery and Evidence==&lt;br /&gt;
The evidence for Planet Nine comes from the analysis of the orbits of distant Kuiper Belt objects (KBOs). These KBOs exhibit orbits that are aligned in a way that cannot be explained by the presence of the known planets alone. Simulations run by Batygin and Brown showed that a massive outer planet would naturally cause the observed orbital alignment. Despite extensive searches, Planet Nine has not yet been directly observed, and its existence remains theoretical.&lt;br /&gt;
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==Characteristics==&lt;br /&gt;
Based on mathematical models and computer simulations, Planet Nine is believed to be a gas giant, similar in composition to [[Uranus]] and [[Neptune]]. Its estimated mass makes it significant enough to influence the orbits of objects in the outer Solar System, yet it remains elusive due to its great distance from the Sun and dim visibility.&lt;br /&gt;
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==Orbit==&lt;br /&gt;
The hypothesized orbit of Planet Nine is highly elliptical, taking it far beyond the known planets and into the depths of the outer Solar System. Its orbital period is speculated to be between 10,000 and 20,000 [[Earth]] years, making a complete journey around the Sun a rare event in human timescales.&lt;br /&gt;
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==Implications for the Solar System==&lt;br /&gt;
The existence of Planet Nine could explain several mysteries of the Solar System, including the peculiar orbits of some distant objects and the overall architecture of the outer regions. It could also provide insights into the formation and evolution of the Solar System, suggesting that there are still major discoveries to be made about our cosmic neighborhood.&lt;br /&gt;
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==Search Efforts==&lt;br /&gt;
Astronomers worldwide are engaged in the search for Planet Nine, using some of the most powerful telescopes available. The search involves scanning the skies for faint objects moving slowly against the backdrop of stars. Despite the challenges, the discovery of Planet Nine would be a monumental achievement in astronomy, offering new understanding of the Solar System&amp;#039;s boundaries and the potential for more unseen planets.&lt;br /&gt;
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==Controversy and Alternative Theories==&lt;br /&gt;
While the hypothesis of Planet Nine has gained significant attention, it is not without its critics. Some scientists propose alternative explanations for the observed orbital anomalies, such as the collective gravitational effects of numerous smaller objects in the Kuiper Belt, rather than a single massive planet. The debate continues as more data is collected and analyzed.&lt;br /&gt;
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[[Category:Astronomy]]&lt;br /&gt;
[[Category:Solar System]]&lt;br /&gt;
[[Category:Hypothetical planets]]&lt;br /&gt;
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{{Astronomy-stub}}&lt;/div&gt;</summary>
		<author><name>Prab</name></author>
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