File:TheKuiperBelt Projections 100AU Classical SDO (alternative layout).svg
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Summary
[edit]DescriptionTheKuiperBelt Projections 100AU Classical SDO (alternative layout).svg | Projection of the aligned orbits of the scattered, classical and resonant objects. (See below for more details.) |
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This file was derived from: TheKuiperBelt Projections 100AU Classical SDO.svg: ![]() |
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English: Digital: Македонски: Дигитални: Русский: Цифровые обозначения: English: Alternative layout: Македонски: Алтернативен распоред: Русский: Альтернативная раскладка: |
Summary
[edit]Projection of the aligned orbits of the scattered, classical and resonant objects. Plotted by a program written by Eurocommuter~commonswiki.
Both projections
[edit]- 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, resonant (2:5) in green, classified scattered in black, not formally classified in grey
Polar view
[edit]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
- Red circle: 35AU (perihelion limit; limit of stability with Neptune)
- Yellow circle: 30AU (~Neptune’s orbit)
- Notice how the classical objects are still in primordial, low-eccentricity orbits
Ecliptic view
[edit]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 [°]
- Red arc: 35 AU perihelion limit
- Yellow arc: 30AU (Neptune’s orbit) perihelion
Data source
[edit]Minor Planet Center Orbit database as of Feb 14th, 2006 except for resonant orbits' classification. Minor Planet Circular 2005-X77 was used instead.
Licensing
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Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
Original upload log
[edit]This image is a derivative work of the following images:
- File:TheKuiperBelt_Projections_100AU_Classical_SDO.svg licensed with Cc-by-sa-2.5,2.0,1.0, Cc-by-sa-3.0-migrated, GFDL
- 2006-03-02T09:00:39Z Eurocommuter~commonswiki 480x480 (37611 Bytes) Projection test. By [User:Eurocommuter~commonswiki|Eurocommuter~commonswiki]
- 2006-03-02T08:53:55Z Eurocommuter~commonswiki 480x480 (37611 Bytes) Orbit projections; test. By [User:Eurocommuter~commonswiki|Eurocommuter~commonswiki] [[Category:Astrophysics]][[Category:Asteroids]]
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 12:36, 27 May 2012 | ![]() | 481 × 755 (130 KB) | Grandiose (talk | contribs) | rm white rectangle |
10:34, 27 May 2012 | ![]() | 481 × 755 (130 KB) | Grandiose (talk | contribs) | fix bold | |
09:46, 27 May 2012 | ![]() | 481 × 755 (129 KB) | Grandiose (talk | contribs) | == {{int:filedesc}} == {{Information |Description=Projection of the '''aligned''' orbits of the scattered, classical and resonant objects. (See below for more details.) |Source={{Derived from|TheKuiperBelt_Projections_100AU_Classical_SDO.svg|display=50... |
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- File:TheKuiperBelt Projections 100AU Classical SDO (alternative layout).svg
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