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20152023
most citedCan we constrain interior structure of rocky exoplanets from mass and radius measurements?

353 citations · 2.9k across the 46 of their papers we have counts for

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Showing 2021Show all

14 papers · 1 filter

astro-ph.EP2021★ 8 cited

Composition of super-Earths, super-Mercuries, and their host stars

V. Adibekyan, N. C. Santos, C. Dorn +11

Because of their common origin, it was assumed that the composition of planet building blocks should, to a first order, correlate with stellar atmospheric composition, especially f…

astro-ph.EP2021★ 43 cited

An upper limit on late accretion and water delivery in the Trappist-1 exoplanet system

Sean N. Raymond, Andre Izidoro, Emeline Bolmont +9

The Trappist-1 system contains seven roughly Earth-sized planets locked in a multi-resonant orbital configuration, which has enabled precise measurements of the planets' masses and…

astro-ph.EP2021★ 26 cited

The HD 137496 system: A dense, hot super-Mercury and a cold Jupiter

T. Azevedo Silva, O. D. S. Demangeon, S. C. C. Barros +28

Most of the currently known planets are small worlds with radii between that of the Earth and that of Neptune. The characterization of planets in this regime shows a large diversit…

astro-ph.EP2021

Hidden water in magma ocean exoplanets

Caroline Dorn, Tim Lichtenberg

We demonstrate that the deep volatile storage capacity of magma oceans has significant implications for the bulk composition, interior and climate state inferred from exoplanet mas…

astro-ph.EP2021

Compositional Diversity of Rocky Exoplanets

Keith Putirka, Caroline Dorn, Natalie Hinkel +1

Star compositions are essential for examining densities and compositional ranges of rocky exoplanets, testing their similarity to Earth. Stellar elemental abundances and planetary…

astro-ph.EP2021★ 45 cited

TOI-431/HIP 26013: a super-Earth and a sub-Neptune transiting a bright, early K dwarf, with a third RV planet

Ares Osborn, David J. Armstrong, Bryson Cale +125

We present the bright (V), multi-planet system TOI-431, characterised with photometry and radial velocities. We estimate the stellar rotation period to be $30.5 \pm…