90377 Sedna

Rerum orbitalium ratio epochae  constitit. Qua epocha 90377  per dies  circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum  et eccentricitatem , distans igitur a sole quam minime unitatibus , quam maxime unitatibus . Inclinatio orbitalis ° reperiebatur, anomalia media °.

 Notae 

 Bibliographia 
 M. A. Barucci et al., "Is Sedna another Triton?" in Astronomy and Astrophysics vol. 439 no. 2 (2005) pp. L1-L4
 M. A. Barucci et al., "(90377) Sedna: Investigation of surface compositional variation" in Astronomical Journal vol. 140 no. 6 (2010)
 J. P. Emery et al., "Ices on (90377) Sedna: confirmation and compositional constraints" in Astronomy and Astrophysics vol. 466 (2007) pp. 395-398
 Lucie Jílková et al., "How Sedna and family were captured in a close encounter with a solar sibling" in Monthly Notices of the Royal Astronomical Society vol. 453 (2015) pp. 3157–3162
 A. Pál et al., "“TNOs are Cool”: A survey of the trans-Neptunian region. VII. Size and surface characteristics of (90377) Sedna and 2010 EK139" in Astronomy and Astrophysics vol. 541 (2012) L6
 Vladislav Zubko et al., "Analysis of Mission Opportunities to Sedna in 2029-2034" in Advances in Space Research (Iunii 2021) Textus praeliminaris apud arXiv

 Nexus externi 

Categoria:Asteroides anno  reperti
Categoria:Corpora Ultraneptuniana