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1887
3717392
Exploring the hypothesis of an inverted Z gradient inside Jupiter
Author(s):
Howard, S.; Guillot, T.; Markham, S.; Helled, R.; Müller, S.; Stevenson, D.J.; Lunine, J.I.; Miguel, Y. (
0000-0002-0747-8862
); Nettelmann, N.
Published
2023
Publication type
Article / Letter to editor
Planets and satellites: interiors
Planets and satellites: gaseous planets
Astrophysics - Earth and Planetary Astrophysics
Date issued
2023
Language
English
Is part of
Astronomy and Astrophysics (2023), L2
hdl
1887/3717392
doi
10.1051/0004-6361/202348129
URL
https://ui.adsabs.harvard.edu/abs/2023A&A...680L...2H
Persistent identifier url
https://hdl.handle.net/1887/3717392
Documents
01 - A_A_680_2023_L2
version: Publisher's Version
Full text at Publisher's site
Open Access