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- | mp_category = {{nowrap|[[Trans-Neptunian object|TNO]]<ref name="jpldata" />{{·}}[[Classical Kuiper-belt object|cubew ...{{mp|1999 OJ|4}}''') is a [[trans-Neptunian object]] and [[Binary asteroid|binary system]] from the classical [[Kuiper belt]], located in the outermost regio ...9 KB (1,058 words) - 04:14, 8 February 2025
- {{short description|Binary trans-Neptunian object}} ...nt minor planet|distant]]<ref name="MPC-object" />{{·}}[[minor-planet moon|binary]]<ref name="Leiva2020" /> ...19 KB (2,529 words) - 02:34, 11 December 2024
- ...emi-major axes as objects hop between resonances. The orbital poles of the objects circle that of the Solar System's [[Laplace plane]], which at large semi-ma ...Nine.png|thumb|260px|Secular evolution of eTNOs induced by Planet Nine for objects with semi-major axis of 250 AU.<ref name="Beust_2016" /><ref name="Batygin_ ...38 KB (5,374 words) - 11:55, 22 December 2024
- | spectral_type = moderately [[Trans-Neptunian object#Colors|red]]<ref name="Brown2010"/>{{rp|page=2702}}<br/>V–I = {{val| ...the [[barycenter]] of the Orcus–Vanth system outside of Orcus, forming a [[binary system]] in which the two bodies revolve around the barycenter, much like t ...34 KB (4,469 words) - 21:27, 5 February 2025
- ...[[Scattered disc|SDO]]<ref name="MPC-CEN-SDO-list"/><br />[[Resonant trans-Neptunian object|3:10 res.]]<ref name="Buie"/><ref name="johnstonsarchive-TNO-list"/> | spectral_type = [[Trans-Neptunian object#Colors|B−V]]={{val|1.38|0.03}}<ref name="Boehnhardt-2014"/><ref name ...74 KB (9,249 words) - 11:02, 1 January 2025
- | mp_category = {{ubl|[[Trans-Neptunian object|TNO]]<ref name="jpldata"/>{{·}}[[Classical Kuiper belt object|cubewa | spectral_type = [[Trans-Neptunian object#Colors|IR]] (moderately red)<br/>B–V={{val|0.94|0.01}}<ref name="Teg ...77 KB (9,654 words) - 19:13, 27 January 2025
- ...al biases, resulting from the difficulty of discovering and tracking these objects during much of the year.<ref name=TC-20200525/> ...ypotheses have been proposed to explain the observed clustering of [[trans-Neptunian object]]s (TNOs). ...184 KB (25,307 words) - 08:37, 1 March 2025
- {{short description|Set of gravitationally bound objects in orbit}} ...r system"). Where only one satellite is known, or it is [[double planet|a binary]] with a common centre of gravity, it may be referred to using the hyphenat ...41 KB (5,742 words) - 00:22, 13 September 2024
- Pluto is the only [[trans-Neptunian object]] with a known atmosphere.<ref name=Dias_Oliveira_2015/> Its closest |title =Sub-Arcsecond Scale Imaging of the Pluto/Charon Binary System at 1.4 mm ...59 KB (8,070 words) - 16:25, 19 January 2025
- ...]] (where it mixes with solid [[carbon monoxide]] and [[methane]]) and the Neptunian moon [[Triton (moon)|Triton]]. On Pluto it was directly observed for the fi ...nnotated).png|right|thumb|upright=0.85|Linear N<sub>8</sub>, EEE isomer (''trans''; EZE isomer – not shown – is ''cis'') after Hirschberg ''et al.'' (2 ...50 KB (7,235 words) - 06:23, 11 October 2024
- | semimajor = {{val|−1.2723|0.0001|fmt=none|u=AU}}{{efn|1=Objects on hyperbolic trajectories have negative semimajor axis, giving them a posi ...ed below 27.5 mag (the limit of [[Hubble Space Telescope]] for fast-moving objects) around 1 January 2018. By late 2019, it should have dimmed to 34 mag.}} ...118 KB (15,738 words) - 17:46, 16 February 2025
- ...tational field of the galaxy could influence the orbits of [[Kuiper Belt]] objects through the ''external field effect'', which is unique to MOND.<ref>{{cite ...nments (in the Solar System and on Earth), they have not been verified for objects with extremely low acceleration, such as stars in the outer parts of galaxi ...80 KB (11,265 words) - 22:02, 1 March 2025