Neptune's resonances in the Scattered Disk. (arXiv:1901.06040v2 [astro-ph.EP] UPDATED) https://t.co/ub3Mv9xpkV
RT @ProfAbelMendez: Neptune's resonances in the Scattered Disk https://t.co/Z47y5egea9
RT @astrokiwi: Scattered disk objects are retained for Gyr by the effects of resonance sticking. Lan & Malhotra find a "second resonance z…
RT @astrokiwi: Scattered disk objects are retained for Gyr by the effects of resonance sticking. Lan & Malhotra find a "second resonance z…
Lan & Malhotra also provide theory for the outer boundary of SDOs at q near 36 au, and data for identifying SDO/resonant orbits just from a/e https://t.co/7czYBUausY https://t.co/8i4Fye8aHu
Scattered disk objects are retained for Gyr by the effects of resonance sticking. Lan & Malhotra find a "second resonance zone" aids SDO stability, and q~30 au distant resonances up to 150 au can be as wide as closer ones. sub'd https://t.co/7czYBUaus
RT @ProfAbelMendez: Neptune's resonances in the Scattered Disk https://t.co/Z47y5egea9
Neptune's resonances in the Scattered Disk https://t.co/Z47y5egea9
Neptune's resonances in the Scattered Disk. https://t.co/SL06m1FMnV
Neptune's resonances in the Scattered Disk. (arXiv:1901.06040v1 [astro-ph.EP]) https://t.co/9gG7vBpwAL
[1901.06040] Neptune's resonances in the Scattered Disk https://t.co/v1k83GawJ6