Uranus and Neptune are reinterpreted as magma-ocean giants with hydrogen-rich interiors rather than traditional ice giants, consistent with observations via three fit parameters each.
Title resolution pending
2 Pith papers cite this work, alongside 219 external citations. Polarity classification is still indexing.
2
Pith papers citing it
219
external citations · OpenAlex
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Ionization rates in the envelopes of NGC-1333 IRAS4A, L1448-C, and L1157 reach 1e-16 to 1e-13 s^{-1}, far above the ISM baseline of 6e-17 s^{-1}.
citing papers explorer
-
Ice Giants Revisited: Uranus and Neptune as Magma Ocean Worlds
Uranus and Neptune are reinterpreted as magma-ocean giants with hydrogen-rich interiors rather than traditional ice giants, consistent with observations via three fit parameters each.
-
Evidence of Enhanced Ionization in Protostellar Envelopes
Ionization rates in the envelopes of NGC-1333 IRAS4A, L1448-C, and L1157 reach 1e-16 to 1e-13 s^{-1}, far above the ISM baseline of 6e-17 s^{-1}.