User:Exoplanetaryscience/OrbitalResonances
A list of possible orbital resonances created using a guess-and-check method created for the specific task.
Graph[edit]
| Object name | Object name #2 | Object name #3 | period (days) [e] | semimajor axis [e] | perihelion [e] | aphelion [e] | eccentricity [e] | resonance to Neptune | resonance residual[1] |
|---|---|---|---|---|---|---|---|---|---|
| 2013 BL76 | 162,100,000 [91,675] | 1253.5 [4.7] | 8.37360 [0.000037] | 2498.7 [9.4] | 0.99332 [0.000025] | 3:808 | 0.0418 | ||
| 2013 BL76 | 162,100,000 [91,675] | 1253.5 [4.7] | 8.37360 [0.000037] | 2498.7 [9.4] | 0.99332 [0.000025] | 22:5925 | 0.0268 | ||
| 2005 VX3 | 22,120,000 [69,287,000] | 1542 [322] | 4.1343 [0.00027] | 3080 [643] | 0.9973 [0.00056] | 2:735 | 0.0556 | ||
| 2005 VX3 | 22,120,000 [69,287,000] | 1542 [322] | 4.1343 [0.00027] | 3080 [643] | 0.9973 [0.00056] | 17:6247 | 0.0274 |
^ the maximum value is 5, best is 0. It's a measure of how far from the true resonance the object is. 0 Would be a perfect value, and any value greater than 5 denotes that the given resonance is much less likely than a similar resonance to it.
Planetary orbital resonances[edit]
| Axis location (AU) | period (years) | Planet | resonance (A:P) | objects within 0.01 years |
|---|---|---|---|---|
| 0.396850 | 0.25 | Earth | 4:1 | 0 |
| 0.480750 | 0.333333 | Earth | 3:1 | 0 |
| 0.629961 | 0.5 | Earth | 2:1 | 3 |
| 1.0 | 1.0 | Earth | 1:1 | 31 |
| 1.310371 | 1.5 | Earth | 2:3 | 67 |
| 1.587401 | 2.0 | Earth | 1:2 | 55 |