activity
20082022
most citedComparing Jupiter interior structure models to Juno gravity measurements and the role of a dilute core

396 citations · 944 across the 16 of their papers we have counts for

collaborators

29 papers

astro-ph.SR20227 cited

X-ray Emission from the Exoplanet Hosting LTT 1445 Triple Star System

Alexander Brown, Cynthia S. Froning, Allison Youngblood +5

JWST will be able to observe the atmospheres of rocky planets transiting nearby M dwarfs. The M dwarf triple star system LTT 1445, at a distance of 6.86 pc, hosts some of the neare…

astro-ph.EP202280 cited

Revelations on Jupiter's Formation, Evolution and Interior: Challenges from Juno Results

Ravit Helled, David J. Stevenson, Jonathan I. Lunine +7

The Juno mission has revolutionized and challenged our understanding of Jupiter. As Juno transitioned to its extended mission, we review the major findings of Jupiter's internal st…

astro-ph.EP202257 cited

Observability of Evaporating Lava Worlds

Mantas Zilinskas, Christiaan van Buchem, Yamila Miguel +4

Lava worlds belong to a class of short orbital period planets reaching dayside temperatures high enough to melt their silicate crust. Theory predicts that the resulting lava oceans…

astro-ph.EP202133 cited

Exploring the link between star and planet formation with Ariel

Diego Turrini, Claudio Codella, Camilla Danielski +22

The goal of the Ariel space mission is to observe a large and diversified population of transiting planets around a range of host star types to collect information on their atmosph…

astro-ph.IM202127 cited

Ariel: Enabling planetary science across light-years

Giovanna Tinetti, Paul Eccleston, Carole Haswell +313

Ariel, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was adopted as the fourth medium-class mission in ESA's Cosmic Vision programme to be launched in 2029. Durin…

astro-ph.IM2021

Ariel Planetary Interiors White Paper

Ravit Helled, Stephanie Werner, Caroline Dorn +10

The recently adopted Ariel ESA mission will measure the atmospheric composition of a large number of exoplanets. This information will then be used to better constrain planetary bu…