activity
20062023
most citedInterior Models of Uranus and Neptune

256 citations · 1.5k across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.EP2023★ 3 cited

About the loss of a primordial atmosphere of super-Earths by planetesimal impacts

Michael Lozovsky, Dina Prialnik, Morris Podolak

We consider planets composed of water ice and rock, located far from a central star. In an earlier study, computing the growth of planets by continuous accretion, we found that a l…

astro-ph.EP2023★ 3 cited

An Equation of State of CO for use in Planetary Modeling

Morris Podolak, Amit Levi, Allona Vazan +1

Although carbon monoxide (CO) is an abundant molecule and may have great importance for planetary interiors, measurements of its properties are difficult due to its extreme volatil…

astro-ph.EP2022★ 2 cited

Detailed Calculations of the Efficiency of Planetesimal Accretion in the Core-Accretion Model -II: The effect of Saturn

Nader Haghighipour, Morris Podolak, Esther Podolak

As part of our ongoing initiative on accurately calculating the accretion rate of planetesimals in the core-accretion model, we demonstrated in a recent article that when the calcu…

astro-ph.EP2022★ 2 cited

The Effect of Accretion Rate and Composition on the Structure of Ice-rich Super-Earths

Michael Lozovsky, Dina Prialnik, Morris Podolak

It is reasonable to assume that the structure of a planet and the interior distribution of its components are determined by its formation history. We thus follow the growth of a pl…

astro-ph.EP2022★ 10 cited

Random Models for Exploring Planet Compositions I: Uranus as an Example

Joshua Podolak, Uri Malamud, Morris Podolak

Modeling the interior of a planet is difficult because the small number of measured parameters is insufficient to constrain the many variables involved in describing the interior s…

astro-ph.EP2022★ 11 cited

On the structure and long-term evolution of ice-rich bodies

Stephan Loveless, Dina Prialnik, Morris Podolak

The interest in the structure of ice-rich planetary bodies, in particular the differentiation between ice and rock, has grown due to the discovery of Kuiper belt objects and exopla…