Zobrazeno 1 - 10
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pro vyhledávání: '"STEVENSON, D"'
Autor:
Fortney, J. J., Militzer, B., Mankovich, C. R., Helled, R., Wahl, S. M., Nettelmann, N., Hubbard, W. B., Stevenson, D. J., Iess, L., Marley, M. S., Movshovitz, N.
We present a review of Saturn's interior structure and thermal evolution, with a particular focus on work in the past 5 years. Data from the Cassini mission, including a precise determination of the gravity field from the Grand Finale orbits, and the
Externí odkaz:
http://arxiv.org/abs/2304.09215
Autor:
Howard, S., Guillot, T., Bazot, M., Miguel, Y., Stevenson, D. J., Galanti, E., Kaspi, Y., Hubbard, W. B., Militzer, B., Helled, R., Nettelmann, N., Idini, B., Bolton, S.
Publikováno v:
A&A 672, A33 (2023)
The Juno mission has provided measurements of Jupiter s gravity field with an outstanding level of accuracy, leading to better constraints on the interior of the planet. Improving our knowledge of the internal structure of Jupiter is key to understan
Externí odkaz:
http://arxiv.org/abs/2302.09082
Autor:
Miguel, Y., Bazot, M., Guillot, T., Howard, S., Galanti, E., Kaspi, Y., Hubbard, W. B., Militzer, B., Helled, R., Atreya, S. K., Connerney, J. E. P., Durante, D., Kulowski, L., Lunine, J. I., Stevenson, D., Bolton, S.
Publikováno v:
A&A 662, A18 (2022)
While Jupiter's massive gas envelope consists mainly of hydrogen and helium, the key to understanding Jupiter's formation and evolution lies in the distribution of the remaining (heavy) elements. Before the Juno mission, the lack of high-precision gr
Externí odkaz:
http://arxiv.org/abs/2203.01866
Interior models of giant planets traditionally assume that at a given radius (i.e. pressure) the density should be larger than or equal to the one corresponding to a homogeneous, adiabatic stratification throughout the planet (referred to as the 'out
Externí odkaz:
http://arxiv.org/abs/2105.00961
Publikováno v:
A&A, 2011
In order to accurately model giant planets, a whole set of observational constraints is needed. As the conventional constraints for extrasolar planets like mass, radius, and temperature allow for a large number of acceptable models, a new planetary p
Externí odkaz:
http://arxiv.org/abs/1101.0997
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