New Jupiter Satellites and Moon-Moon Collisions
Autor: | Audrey Thirouin, Nicholas Moskovitz, Gareth V. Williams, Dora Fohring, Chadwick A. Trujillo, Robert A. Jacobson, David J. Tholen, Marina Brozovic, Maxime Devogele, Scott S. Sheppard |
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Jazyk: | angličtina |
Rok vydání: | 2018 |
Předmět: |
Earth and Planetary Astrophysics (astro-ph.EP)
Physics Solar System 010504 meteorology & atmospheric sciences FOS: Physical sciences Astronomy General Medicine 01 natural sciences Jupiter Orbit Planet 0103 physical sciences Physics::Space Physics Satellite Astrophysics::Earth and Planetary Astrophysics 010303 astronomy & astrophysics 0105 earth and related environmental sciences Astrophysics - Earth and Planetary Astrophysics |
Popis: | We report the discovery of 12 new satellites of Jupiter, giving Jupiter 79 known satellites. The new finds are between 23rd-24th mag in the r-band and 1-3 km in diameter assuming dark albedos. Nine of the discoveries are in the distant retrograde satellite groupings. Two of the new satellites are in the closer Himalia prograde group near 28 degrees in inclination. S/2016 J2, nicknamed Valetudo, has an orbit unlike any other known outer satellite and is the most distant prograde satellite around any planet at 0.36 Hill radii. Numerical simulations show S/2016 J2 is very stable, with average and range of i=34.2+-3 deg, e=0.216+-0.125, and a=18.9+-0.7 million km over 100 Myrs. Our stability simulations show a S/2016 J2 like orbit would be stable out to a=21.8 million km or 0.41 Hill radii, but no further, unlike more distant and eccentric retrograde satellites. S/2016 J2's large semi-major axis means it significantly overlaps the orbits of the distant retrogrades. A prograde-retrograde moon-moon collision between outer satellites of Jupiter has likely happened over the age of the solar system. Published Research Notes AAS |
Databáze: | OpenAIRE |
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