Results 181 to 190 of about 10,242 (205)
Some of the next articles are maybe not open access.
Science, 1965
On the evenings of 26 October and 15 December 1962, while the disk of Jupiter was being scanned for thermal emission in the 8- to 14-micron wavelength region, a large enhancement was discovered in the emission from shadows cast on Jupiter by the Jovian satellites Ganymede and Europa.
openaire +3 more sources
On the evenings of 26 October and 15 December 1962, while the disk of Jupiter was being scanned for thermal emission in the 8- to 14-micron wavelength region, a large enhancement was discovered in the emission from shadows cast on Jupiter by the Jovian satellites Ganymede and Europa.
openaire +3 more sources
Gas envelopes of exoplanets—hot Jupiters
Uspekhi Fizicheskih Nauk, 2020Abstract We consider the physical characteristics and dynamics of the gaseous envelopes of hot Jupiters (HJs) — gas giants with a mass comparable to Jupiter’s and a semi-major axis of less than 0.1 a.u. Although HJs were discovered almost a quarter of a century ago, many issues about their origin remain open. There are two reasons for
D V Bisikalo +3 more
openaire +1 more source
A solar C/O and sub-solar metallicity in a hot Jupiter atmosphere
Nature, 2021Michael R Line +2 more
exaly
Are hot Neptunes partially evaporated hot Jupiters?
2011The detection of short period planets (hot Jupiters and their lower mass counterparts, hot Neptunes and super-Earths) still defies the models of planet formation and evolution. Several possibilities have been proposed to explain the nature and formation process of the lower mass population, including in situ formation, disk migration, planet-planet ...
Boué, Gwenaël +3 more
openaire +1 more source
Hot Jupiters: Origins, Structure, Atmospheres
Journal of Geophysical Research E: Planets, 2021Jonathan J Fortney +2 more
exaly
Risk factors, pathophysiology, and treatment of hot flashes in cancer
Ca-A Cancer Journal for Clinicians, 2013Janet Carpenter +2 more
exaly