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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.
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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 +4 more sources
Science, 2003
AMERICAN ASTRONOMICAL SOCIETY MEETINGSEATTLE-- Pacific Northwest winter skies cleared for 4 days in early January, welcoming more than 2000 astronomers to their biannual meeting. Announced at the meeting was the latest extrasolar planet to be discovered, which sets three standards: farthest from Earth, tiniest orbit, and the first to be revealed by a ...
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AMERICAN ASTRONOMICAL SOCIETY MEETINGSEATTLE-- Pacific Northwest winter skies cleared for 4 days in early January, welcoming more than 2000 astronomers to their biannual meeting. Announced at the meeting was the latest extrasolar planet to be discovered, which sets three standards: farthest from Earth, tiniest orbit, and the first to be revealed by a ...
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Exoplanets: Atmospheres of Hot Jupiters
2019The history of exoplanetary atmospheres studies is strongly based on the observations and investigations of the gaseous envelopes of hot Jupiters—exoplanet gas giants that have masses comparable to the mass of Jupiter and orbital semi-major axes shorter than 0.1 AU.
P. V. Kaygorodov +2 more
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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
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2019
The atmospheres of hot Jupiters are inherently three dimensional and can be probed through the continuous observation of the planet brightness during it's orbit (aka phase curve). The phase curve amplitude and the offset of the maximum of the phase curve compared to the secondary eclipse is often used as a diagnostic of the day/night temperature ...
Parmentier, Vivien +3 more
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The atmospheres of hot Jupiters are inherently three dimensional and can be probed through the continuous observation of the planet brightness during it's orbit (aka phase curve). The phase curve amplitude and the offset of the maximum of the phase curve compared to the secondary eclipse is often used as a diagnostic of the day/night temperature ...
Parmentier, Vivien +3 more
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Coronal Mass Ejection Effect on Envelopes of Hot Jupiters
Astronomy reports (Print), 2020A. Zhilkin, D. Bisikalo, P. Kaygorodov
semanticscholar +1 more source