Water binding energy on silicate grains is twice that on ice, enabling local retention and inheritance for terrestrial planets without outer Solar System delivery.
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3 Pith papers cite this work, alongside 169 external citations. Polarity classification is still indexing.
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astro-ph.EP 3years
2026 3representative citing papers
3I/ATLAS lost roughly 1–7 meters of its surface and ~10^9–10^10 kg of mass during its Solar System passage, based on fits to observed gas production rates.
Evolving protoplanetary disks produce solid C/O and N/O ratios near 1 beyond hypervolatile ice lines, with hypervolatile enhancements up to 100 times higher than static disk models due to drift and advection.
citing papers explorer
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Astrochemical Inheritance of Terrestrial Planets Water from Local Wet Silicates
Water binding energy on silicate grains is twice that on ice, enabling local retention and inheritance for terrestrial planets without outer Solar System delivery.
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Assessment of the Mass Loss and Radius Change of 3I/ATLAS Based on Observed Production Rates
3I/ATLAS lost roughly 1–7 meters of its surface and ~10^9–10^10 kg of mass during its Solar System passage, based on fits to observed gas production rates.
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Icy Volatile Enhancements in Evolving Protoplanetary Disks
Evolving protoplanetary disks produce solid C/O and N/O ratios near 1 beyond hypervolatile ice lines, with hypervolatile enhancements up to 100 times higher than static disk models due to drift and advection.