Evidence of hydrogen−helium immiscibility at Jupiter-interior conditions
Author:
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Link
http://www.nature.com/articles/s41586-021-03516-0.pdf
Reference46 articles.
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2. Salpeter, E. On convection and gravitational layering in Jupiter and in stars of low mass. Astrophys. J. 181, L83–L89 (1973).
3. Fortney, J. J. & Hubbard, W. B. Phase separation in giant planets: inhomogeneous evolution of Saturn. Icarus 164, 228–243 (2003).
4. von Zahn, U. & Hunten, D. M. The helium mass fraction in Jupiter’s atmosphere. Science 272, 849–851 (1996).
5. Wilson, H. F. & Militzer, B. Sequestration of noble gases in giant planet interiors. Phys. Rev. Lett. 104, 121101 (2010).
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