activity
20052026
most citedA Gas-poor Planetesimal Capture Model for the Formation of Giant Planet Satellite Systems

73 citations · 169 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.EP2026

A Collisional Origin for Ice-rich Iapetus and Titan's Anomalous Eccentricity

Ignacio Mosqueira

We test whether collisions involving Titan can eject enough water-rich material onto sufficiently distant Saturn-bound orbits to form Iapetus, while also accounting for Titan's orb…

astro-ph.EP2026

Satellite Survival through Gas Redistribution in a Low-viscosity Disk

Ignacio Mosqueira

We investigate satellite survival through gas redistribution in a dense circumplanetary disk with a low dimensionless viscosity parameter . The model combines modal…

astro-ph.EP2026

PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation

Ignacio Mosqueira

PDS~70~c and SR~12~c are the only bound planetary-mass objects with secure cold submillimeter disk detections. Together, these systems constrain giant-planet growth and satellite f…

astro-ph.EP2009★ 23 cited

Deciphering the Origin of the Regular Satellites of Gaseous Giants - Iapetus: the Rosetta Ice-Moon

Ignacio Mosqueira, Paul R. Estrada, Sebastien Charnoz

Here we show that Iapetus can serve to discriminate between satellite formation models. Its accretion history can be understood in terms of a two-component gaseous subnebula, with…

astro-ph.EP2009★ 31 cited

Planetesimals and Satellitesimals: Formation of the Satellite Systems

Ignacio Mosqueira, Paul R. Estrada, Diego Turrini

The origin of the regular satellites ties directly to planetary formation in that the satellites form in gas and dust disks around the giant planets and may be viewed as mini-solar…

astro-ph2008★ 12 cited

Formation of Jupiter and Conditions for Accretion of the Galilean Satellites

Paul R. Estrada, Ignacio Mosqueira, Jack J. Lissauer +2

We present an overview of the formation of Jupiter and its associated circumplanetary disk. Jupiter forms via a combination of planetesimal accretion and gravitational accumulation…