Less absorbed solar energy and more internal heat for Jupiter
Radiant energy budgets and internal heat play a key role in the evolution of planets. Here, the authors analyze data from the Cassini mission to show that Jupiter’s radiant energy and internal heat budgets are significantly larger than previous estimates.
Main Authors: | Liming Li, X. Jiang, R. A. West, P. J. Gierasch, S. Perez-Hoyos, A. Sanchez-Lavega, L. N. Fletcher, J. J. Fortney, B. Knowles, C. C. Porco, K. H. Baines, P. M. Fry, A. Mallama, R. K. Achterberg, A. A. Simon, C. A. Nixon, G. S. Orton, U. A. Dyudina, S. P. Ewald, R. W. Schmude |
---|---|
Format: | Article |
Language: | English |
Published: |
Nature Publishing Group
2018-09-01
|
Series: | Nature Communications |
Online Access: | https://doi.org/10.1038/s41467-018-06107-2 |
Similar Items
-
Light Scattering in the Clouds on Jupiter
by: Dyudina, Ulyana Anatolyevna
Published: (2002) -
DOPPLER SIGNATURES OF THE ATMOSPHERIC CIRCULATION ON HOT JUPITERS
by: Showman, Adam P., et al.
Published: (2015) -
TRANSITIONS IN THE CLOUD COMPOSITION OF HOT JUPITERS
by: Parmentier, Vivien, et al.
Published: (2016) -
THREE-DIMENSIONAL ATMOSPHERIC CIRCULATION OF HOT JUPITERS ON HIGHLY ECCENTRIC ORBITS
by: Kataria, T., et al.
Published: (2015) -
ATMOSPHERIC CIRCULATION OF ECCENTRIC HOT JUPITER HAT-P-2B
by: Lewis, Nikole, et al.
Published: (2015)