225088 Gonggong: Verskil tussen weergawes
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k Stukkende eksterne skakels vervang met skakels na argiewe Etiket: 2017-bronwysiging |
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Lyn 3:
| name = {{mp|225088|2007 OR|10}}
| symbol =
| image = [[Beeld:EightTNOs af.png|duimnael|260px|senter|
| caption =
| discovery = yes
Lyn 26:
| arg_peri = 206,81° (ω)
| satellites =
| dimensions = {{val|1535|+75|-225|u=km}}<ref name="scida2015">{{cite web| url= https://web.archive.org/web/20160305034458/http://lcogt.net/files/K2SciCon/Robert_Szabo-Szabo_TNOs_web.pdf | title= Pushing the Limits of K2:Observing Trans-Neptunian Objects S3K2: Solar System Studies with K2}}</ref> <br />{{val|1280|+210|-210|u=km}}<ref name=TNOsCool4 /><br />{{val|1200|+300|-200|u=km}}<ref name="Brown2011" />
| mass = ~1,3–6 × 10<sup>21</sup> kg ''(raming)''
| density =
Lyn 66:
|accessdate=31 Januarie 2012
}}</ref> Dit is dus die derde verste bekende liggaam in die Sonnestelsel naas [[V774104]] (103 AE) en [[Eris (dwergplaneet)|Eris]] (96,3 AE) – dit is sedert 2013 verder as [[Sedna]] (85,7 AE).<ref name="Brownblog" /><ref name="horizons" /> Teen 2045 sal dit verder as beide Sedna en Eris wees<ref name=Horizons2076>{{cite web
|url=https://web.archive.org/web/20121109114850/http://home.surewest.net/kheider/astro/Sedna2076.txt
|title=Horizons Output for Sedna 2076/2114
|author=JPL Horizons On-Line Ephemeris System
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