2006 QH181
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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…mehr

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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 further from the Sun are Eris, Sedna, and 2007 OR10. Being so far from the Sun, it only has an apparent magnitude of 23.