https://wikimd.org/index.php?action=history&feed=atom&title=SednoidSednoid - Revision history2026-04-25T17:08:53ZRevision history for this page on the wikiMediaWiki 1.44.2https://wikimd.org/index.php?title=Sednoid&diff=5616402&oldid=prevPrab: CSV import2024-04-16T21:09:29Z<p>CSV import</p>
<p><b>New page</b></p><div>[[File:Sednoid_orbits.png|Sednoid orbits|thumb]] [[File:Sednoid_apparent_magnitudes.png|Sednoid apparent magnitudes|thumb|left]] [[File:Sedna-NASA.JPG|Sedna-NASA|thumb|left]] [[File:Distant_object_orbits_and_positions_closeup.png|Distant object orbits and positions closeup|thumb]] '''Sednoids''' are a group of distant [[trans-Neptunian objects]] (TNOs) with similar orbital characteristics, residing in the outermost reaches of the [[Solar System]]. These objects are characterized by their large semi-major axes, high perihelia, and substantial inclination with respect to the ecliptic plane. The most famous member of this group is [[90377 Sedna]], discovered in 2003, which lent its name to the category. Sednoids are of significant interest to astronomers as they provide insights into the processes at play in the distant Solar System and the potential existence of a hypothetical ninth planet, often referred to as [[Planet Nine]] or [[Planet X]].<br />
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==Discovery and Classification==<br />
The discovery of 90377 Sedna by a team led by [[Mike Brown]] at the [[Palomar Observatory]] marked a significant milestone in the study of the outer Solar System. Sedna's discovery was soon followed by the identification of other objects with similar orbital characteristics, leading to the classification of these objects as Sednoids. These objects have semi-major axes greater than 150 [[astronomical unit|astronomical units (AU)]] and perihelia greater than 30 AU, distinguishing them from other known TNOs and [[Kuiper Belt Objects]] (KBOs).<br />
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==Orbital Characteristics==<br />
Sednoids are noted for their extreme orbits, which are highly elongated and take them far beyond the Kuiper Belt, a region of the Solar System populated by icy bodies and dwarf planets. The orbits of Sednoids suggest that they may be influenced by the gravitational pull of unseen celestial objects, possibly a distant, undiscovered planet or the remnants of a star passing near the Solar System in its early history. The dynamics of their orbits are a subject of ongoing research and debate among astronomers.<br />
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==Physical Characteristics==<br />
Little is known about the physical characteristics of Sednoids due to their great distances from Earth. Observations suggest that they are likely composed of a mixture of ice and rock, similar to other TNOs. Their surfaces are believed to be reddish in color, indicating the presence of complex organic molecules known as tholins. The size of Sednoids can vary, with Sedna itself estimated to be about 1,000 kilometers in diameter, making it one of the largest known TNOs.<br />
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==Significance==<br />
The study of Sednoids offers valuable insights into the early Solar System and the processes that shaped its formation and evolution. Their peculiar orbits challenge existing models of Solar System dynamics and suggest the presence of yet-to-be-discovered celestial bodies influencing their paths. Additionally, Sednoids may hold clues about the distribution of mass in the outer Solar System and the potential for life in extreme environments.<br />
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==Future Exploration==<br />
The remote location and faint visibility of Sednoids make them challenging targets for observation and study. Future missions and advances in telescope technology may provide more detailed information about their physical properties and the nature of their orbits. The exploration of Sednoids represents a frontier in Solar System science, offering the potential to unlock mysteries of the distant outer Solar System.<br />
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[[Category:Astronomy]]<br />
[[Category:Trans-Neptunian objects]]<br />
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