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Both plots
The nodes of the orbits are brought to 270°; and the perihelia to 0° to simplify the comparison of the perihelia and aphelia
Objects plotted: classical in blue, plutions in red.1
Polar view
The aligned orbits are further reclined onto the ecliptic (i.e. rotated around the line of nodes by an angle opposite to the inclination) to allow for easy comparison of perihelia and aphelia.
Polar coordinates
Distance from the Sun (the small gold disk) in AU.
Argument not drawn
Yellow circle: 30AU (~Neptune’s orbit)
Ecliptic view
Projection of the aligned orbits on the plane x,z ((looking at the ecliptic from the edge); the point of view is the ascending node.
Polar coordinates.
Axis: distance form the Sun; perihelia on the left, aphelia on the right.
Angle: orbit inclination [°]
Yellow arc: 30AU (Neptune’s orbit) perihelion
Footnotes
1For roughly a half of known TNO the orbits are not yet known with the precision sufficient for the classification (a particularly delicate task for resonant objects).
Data source
Minor Planet Center Orbit database as of Feb 14th, 2006 except for resonant orbits' classification.
Minor Planet Circular 2005-X77 was used instead.
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Idih kawènèhaké saprelu nyalin, ngedum, lan/utawa ngowah layang iki manut bebaku Palilah Pilayang Bébas GNU, Angka 1.2 utawa angka luwih anyar sing dibabar Yeyasan Piranti Alus Bébas; tanpa Pérangan Invarian, tanpa Tulisan Samak Arep, lan tanpa Tulisan Samak Buri. Salinan palilah dirembug ing pérangan asesirah Palilah Pilayang Bébas GNU.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue
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atribusi – Kowé kudu mènèhi krédhit kang patut, mènèhi pranala lisènsi, lan kandha yèn ana owah-owahan. Kowé bisa tumindak sasenengmu, nanging ora teges kang duwé lisènsi njurung lakumu.
andum mèmper – Manawa kowé nyalin rupa, ngowahi, utawa nggawé karya nganggo bahan karya iki, kowé kudu mbabar karyamu kang wis dadi nganggo lisènsi kang padha utawa kang cocog karo karya asliné..