270 citations · 709 across the 23 of their papers we have counts for
6 papers · 1 filter
Most High-density Exoplanets Are Unlikely to Be Remnant Giant-planet Cores
Zifan Lin, Saverio Cambioni, Sara Seager
Some exoplanets have much higher densities than expected from stellar abundances of planet-forming elements. There are two theories - metal-rich formation hypothesis and naked core…
Surface properties of the Kalliope-Linus system from ALMA and VLA data
Katherine de Kleer, Saverio Cambioni, Bryan Butler +1
The abundance and distribution of metal in asteroid surfaces can be constrained from thermal emission measurements at radio wavelengths, informing our understanding of planetesimal…
Can metal-rich worlds form by giant impacts?
Saverio Cambioni, Benjamin P. Weiss, Erik Asphaug +5
Planets and stars are expected to be compositionally linked because they accrete from the same material reservoir. However, astronomical observations revealed the existence of exop…
Estimate of water and hydroxyl abundance on asteroid (16) Psyche from JWST data
Stephanie G. Jarmak, Tracy M. Becker, Charles E. Woodward +10
Our understanding of Solar System evolution is closely tied to interpretations of asteroid composition, particularly the M-class asteroids. These asteroids were initially thought t…
The Heterogeneous Surface of Asteroid (16) Psyche
Saverio Cambioni, Katherine de Kleer, Michael Shepard
Main-belt asteroid (16) Psyche is the largest M-type asteroid, a class of object classically thought to be the metal cores of differentiated planetesimals and the parent bodies of…
A New Database of Giant Impacts over a Wide Range of Masses and with Material Strength: A First Analysis of Outcomes
Alexandre Emsenhuber, Erik Asphaug, Saverio Cambioni +4
In the late stage of terrestrial planet formation, planets are predicted to undergo pairwise collisions known as giant impacts. Here we present a high-resolution database of giant…