0 ▁Qu ao ar ▁and ▁ 2 0 0 0 0 ▁Var una . ▁ ▁has ▁the ▁most ▁ecc ent ric ▁and ▁incl ined ▁orbit ▁of ▁the ▁three . ▁ ▁A ▁vari ability ▁of ▁the ▁visual ▁bright ness ▁was ▁also ▁detected ▁which ▁could ▁fit ▁to ▁ 7 . 9   h ▁or ▁ 1 5 . 8   h ▁rot ational ▁period ▁( the ▁distinction ▁between ▁single ▁or ▁double - pe aked ▁cur ved ▁could ▁not ▁be ▁made ▁with ▁confidence ). ▁The ▁changes ▁in ▁bright ness ▁are ▁quite ▁close ▁to ▁the ▁error ▁margin ▁and ▁could ▁also ▁be ▁due ▁to ▁an ▁irregular ▁shape . ▁ ▁Or bit ▁▁ ▁The ▁adjacent ▁diag rams ▁show ▁polar ▁and ▁e cli ptic ▁views ▁of ▁the ▁or bits ▁of ▁the ▁two ▁cub ew anos . ▁The ▁peri hel ia ▁( q ) ▁and ▁the ▁a ph elia ▁( Q ) ▁are ▁marked ▁with ▁the ▁dates ▁of ▁passage . ▁The ▁present ▁positions ▁( as ▁of ▁April ▁ 2 0 0 6 ) ▁are ▁marked ▁with ▁the ▁spher es , ▁illustr ating ▁relative ▁sizes ▁and ▁differences ▁in ▁al bed o ▁( both ▁objects ▁appear ▁neutral ▁in ▁the ▁visible ▁spectrum ). ▁▁ ▁is ▁class ified ▁as ▁a ▁classical ▁K ui per ▁bel t ▁object ▁and ▁follows ▁an ▁orbit ▁very ▁similar ▁to ▁that ▁of ▁: ▁highly ▁incl ined ▁( 2 6 ° ) ▁and ▁moder ately ▁ecc ent ric ▁( e ▁~ 0 . 1 2 ), ▁far ▁from ▁Ne pt une ' s ▁perturb ations ▁( per i hel ion ▁at ▁~