2006 QH181
Trans-Neptunian object, Dwarf planet, Scattered disc, Detached object, Apsis, Neptune, Apparent magnitude
Herausgegeben: Hermes, Othniel
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 2006 QH181, also written as 2006 QH181, is a trans-Neptunian object. It is very likely a dwarf planet. It is part of the scattered disc. It may be a detached object since a perihelion of 37.6 AU may place it outside of the direct influence of Neptune, or it could have a 5:1 resonance with Neptune. Further observations of the orbit will be required. It came to perihelion around 1859. It is currently 82 AU from the Sun. The only dwarf-planet-type bodies currently furthe...
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 2006 QH181, also written as 2006 QH181, is a trans-Neptunian object. It is very likely a dwarf planet. It is part of the scattered disc. It may be a detached object since a perihelion of 37.6 AU may place it outside of the direct influence of Neptune, or it could have a 5:1 resonance with Neptune. Further observations of the orbit will be required. It came to perihelion around 1859. It is currently 82 AU from the Sun. The only dwarf-planet-type bodies currently further from the Sun are Eris, Sedna, and 2007 OR10. Being so far from the Sun, it only has an apparent magnitude of 23.
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