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Check out the new review paper "The distribution of volatile elements during rocky planet formation" led by Terry-Ann Suer: https://arxiv.org/abs/2311.18262. Very useful for improved models and observations of (hot) rocky exoplanets and atmospheric formation on rocky planets.
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This is great news for using exoplanets surveys to better understand the chemical and physical conditions that may enable prebiotic chemistry on other worlds, and by that give us further clues on the prevalent conditions to kickstart life as we know it – also on our own planet!
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In a magma ocean phase rocky planets glow strongly – they are still hot and molten from the primordial heat of formation – and Lorenzo quantified how much of an advantage this is when searching for these planets.
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This is great news for using exoplanets surveys to better understand the chemical and physical conditions that may enable prebiotic chemistry on other worlds, and by that give us further clues on the prevalent conditions to kickstart life …
He found that the intrinsic heat of transient magma ocean epochs make these planets detectable (and characterisable!) to vast distances (up to ~100 pc). LIFE will be able to find them typically within minutes in both G and M dwarf systems …
In a magma ocean phase rocky planets glow strongly – they are still hot and molten from the primordial heat of formation – and Lorenzo quantified how much of an advantage this is when searching for these planets.
Lorenzo – in his very first paper! 🎉🥳 – now tried to understand if LIFE could find the signature of rocky exoplanets in their early 'magma ocean' phase. From studies of the early Earth we think this phase is critically important in setting…
LIFE (https://life-space-mission.com) is an initiative to develop a space-based nulling interferometer for characterising potentially habitable exoplanets and search for biosignatures. However, LIFE will be capable of doing a lot more, and…
Today on arXiv (https://arxiv.org/abs/2410.13457): Large Interferometer For Exoplanets (LIFE). XIV. Finding terrestrial protoplanets in the galactic neighborhood. A new paper in the LIFE mission series led by Lorenzo Cesario from the Kapte…
A few days ago on arXiv by Joe Eatson: Devolatilization of extrasolar planetesimals by 60Fe and 26Al heating (https://arxiv.org/abs/2402.06476). 26Al the most important desiccating short-lived radionuclide for Solar System analogs, but in …
And now published in ApJL: https://iopscience.iop.org/article/10.3847/2041-8213/ad206e/meta
https://arxiv.org/abs/2401.05864
Check out the new review paper "The distribution of volatile elements during rocky planet formation" led by Terry-Ann Suer: https://arxiv.org/abs/2311.18262. Very useful for improved models and observations of (hot) rocky exoplanets and at…
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