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A thousand years old mystery Is the moon made of cheese ? Novel scenarios for the origin and evolution of the moons Hagai Perets, Technion The Solar system have several types of moons Regular satellites of the gas giants ● Irregular satellites of the gas giants ● Moons of Earth and Mars ● Binary planetesimals ● The Solar system have several types of moons Regular satellites of the gas giants ● Irregular satellites of the gas giants ● Moons of Earth and Mars ● Binary planetesimals ● Regular satellites ● ● ● ● Regular satellites lie on co-planar circular orbits aligned with the planet equator Some of them with a few thousands km diameter They orbit the planet at short separations (< few 0.01 the Hill radius) Some are found to be in resonance with each other Mosqueira & Estrada 2003 Irregular satellites are eccentric and/or highly inclined moons Typically at large separations ● Secular Kozai-Lidov evolution play an important role in their evolution Jewitt & Haghighipour (ARAA 2007) Regular satellites likely form very similar to terrestrial planets ● ● ● Start with a gas/dust disk Grow small planetesimals to big ones Migrate, form resonances Ogihara & Ida 2012 Irregular satellites are thought to be captured ● Gas assisted capture -> fine tuned Ćuk & Gladman (2005) ● Pull-down capture during planet growth Heppenheimer & Porco (1977) – ● ● ● > fine tuned Difficulties with Uranus and Neptune Binary disruption (Agnor & Hamilton 2006) ->inefficient, maybe explain Triton Satellite capture during planetary encounters; somewhat fine tuned; Nesvorný, Vokrouhlický & Morbidelli 2007 Jewitt & Haghighipour (ARAA 2007) A new in-situ formation model: Analogy to planetary systems ● Solar system/Kepler multiple systems – ● > Regular satellites Eccentric and/or inclined systems – > Irregular satellites – > Hot Jupiters -> Triton Origin of eccentric/inclined and hot Jupiter planetary systems ● ● ● Planet-planet scattering (e.g. Rasio & Ford 1996) Secular evolution due to third planetary/stellar companions (e.g. Mazeh et al. 1997) Important role for tidal friction (e.g. Wu & Murray 2003) Formation of satellites at the outer regions was not modeled ● The circumplanetary disk should extend up to R_H 2012 ● Where are the external regular satellites ? In-situ formation of irregular moons and the role of moon-moon scattering and secular evolution ● ● Model multiple large moons in the irregular moon separation regime Secular evolution arises naturally due to perturbations by the Sun ● Model evolution in a gaseous disk ● Model tidal friction by the planet ● Model planet asphericity In-situ formation of irregular moons and the role of moon-moon scattering and secular evolution ● ● Model multiple large moons in the irregular moon separation regime Secular evolution arises naturally due to perturbations by the Sun ● Model moons formation in the outer disk ● Model evolution in a gaseous disk ● Model tidal friction by the planet ● Model planet asphericity Perets & Payne, in prep. Moon-moon scattering: Disk heating and satellite growth Perets & Payne, in prep. Moon-moon scattering: Formation of prograde irregulars and runaway moons Moon-moon scattering: Temporary re-capture of irregular moons Moon-moon scattering: Formation of retrograde irregular moons ? Origin of some big Solar system minor-bodies ? ● ● Ejected moons may have survived to this day What kinematic or compositional signature would we expect ? The origin of Earth's moon Earth moon formation theories ● Fission (Darwin) ● Capture (Kuiper) ● Co-accretion ● Giant impact (Hartmann, Canup) Need to explain: lack of Iron, similar isotope composition (titanium, oxygen) as the Earth, inclination,angular momentum Earth moon formation theories ● ● ● ● Fission (angular momentum, inclination problem) Capture (fine tuned, composition) Co-accretion (Iron core depleted, angular momentum) Giant impact (preferred paradigm) Need to explain: lack of Iron, similar isotope composition (titanium oxygen) as the Earth, inclination,angular momentum The Earth moon formed through a giant collision... The Earth-moon composition problem ● ● Most of the material comes from the impactor Material from different planets suggest very different composition of the different planets The fast-spinning Earth solution Is the composition problem really a problem ? Raymond et al. 2009 Is the composition problem really a problem ? Mastrobuono-Battisti & Perets, in prep. ... but the proto-Earth likely had many previous collisions Raymond et al. 2009 Earth's previous moons and the multiple-collisions origin of the moon ● ● ● ● Model a giant impact while a previous moon exists Check if previous moons halts formation of a new moon Model tidal evolution and dynamics of two moons -> SPH Analytic + N-body +tides Model consequent multiple Monte-Carlo collisions and the collisional (use N-body growth of the moon results) Earth's previous moons and the multiple-collisions origin of the moon ● ● ● ● Model a giant impact while a previous moon exists Check if previous moons halts formation of a new moon Model tidal evolution and dynamics of two moons -> SPH Analytic + N-body +tides Model consequent multiple Monte-Carlo collisions and the collisional (use N-body growth of the moon results) New moons can form while previous one exists Citron+Perets+Aharonson, In prep. Few-body simulations results ● ● ● ● Put a newly formed close single moon; evolve for a few Myrs Put a second close moon, and evolve Shorter period moons tidally evolve faster and may over run older ones – > unstable configuration – > Chaotic evolution ~30% of the moons mutually collide, the rest re-collide with the Earth or ejected Summary: Breaking old paradigms of moon formation An in-situ origin for irregular satellites instead of capture scenarios ● Existence of previous moons of Earth, and a multiplecollisions origin for the Moon ●