File:Neso orbital evolution - Brozovic & Jacobson 2022 Fig 5.png
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Summary
| Description |
English: Plots showing Neso's osculating eccentricity (e), inclination (i), and argument of pericenter (w) over a 5,000-year time period. These orbital elements oscillate periodically due to the Kozai–Lidov resonance (which causes Neso's argument of pericenter, w, to permanently oscillate around 90 degrees). The reference plane for inclination is the orbital plane of Uranus around the Sun, α = 273.48 deg and δ = 67.70 deg. These are mean orbital poles at 2000 January 1, 12:00:00 TDB, which we obtained by fitting a precessing ellipse to DE441 planetary ephemeris. |
| Date | |
| Source | Cropped from Figure 5 of https://iopscience.iop.org/article/10.3847/1538-3881/ac617f#ajac617ff5 |
| Author | Marina Brozović and Robert A. Jacobson 2022 AJ 163 241 |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 07:33, 1 July 2026 | | 610 × 875 (214 KB) | wikimediacommons>Nrco0e | Uploaded a work by Marina Brozović and Robert A. Jacobson 2022 AJ 163 241 from Cropped from Figure 5 of https://iopscience.iop.org/article/10.3847/1538-3881/ac617f#ajac617ff5 with UploadWizard |
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