Hot interiors of ice giant planets inferred from electrical conductivity of dense H2O fluid

Documenti analoghi

• On the meaning of the dynamo radius in giant planets with stable layers
  di: Wulff, Paula N., et al.
  Pubblicazione: (2025)
• The influence of interior structure and thermal state on impact melt generation upon large impacts onto terrestrial planets
  di: Manske, Lukas, et al.
  Pubblicazione: (2025)
• The role of interior dynamics and differentiation on the surface and atmosphere of lava planets
  di: Boukaré, Charles-Édouard, et al.
  Pubblicazione: (2023)
• Thermal and magnetic evolution of an Earth-like planet with a basal magma ocean
  di: Lherm, Victor, et al.
  Pubblicazione: (2024)
• Condensate evolution in the solar nebula inferred from combined Cr, Ti, and O isotope analyses of amoeboid olivine aggregates
  di: Jansen, Christian A., et al.
  Pubblicazione: (2024)