Results 21 to 30 of about 63,945 (279)
The challenge of forming a fuzzy core in Jupiter [PDF]
Astronomy & Astrophysics, 2020 Recent structure models of Jupiter that match Juno gravity data suggest that the planet harbours an extended region in its deep interior that is enriched with heavy elements: a so-called dilute or fuzzy core.
S. Müller, R. Helled, A. Cumming
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Revealing the source of Jupiter’s x-ray auroral flares
Science Advances, 2021 Jupiter’s unique x-ray aurora is driven by the same processes as Earth’s: Heavy ion scattering by electromagnetic waves. Jupiter’s rapidly rotating, strong magnetic field provides a natural laboratory that is key to understanding the dynamics of high ...
Z. Yao +24 more
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Lumbar Cryptorchidism with Splenogonadal Fusion: The Odd Couple
Journal of Gastrointestinal and Abdominal Radiology, 2022 We present and discuss the clinical, radiological, surgical, and histopathologic findings in a 16-month-old child who presented with bilateral cryptorchidism.
Amol Anil Kulkarni +5 more
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Safety and pharmacokinetics of a highly bioavailable resveratrol preparation (JOTROL TM)
AAPS Open, 2022 Resveratrol exhibits a wide range of biological properties, including anti-glycation, antioxidant, anti-inflammation, neuroprotective (including against advanced dementia and Alzheimer’s disease), anti-cancer, and anti-aging activity in experimental ...
Christopher Kemper +6 more
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How Jupiter’s unusual magnetospheric topology structures its aurora [PDF]
Science Advances, 2020 Jupiter’s slow dayside magnetic merging and fast rotation produce an unusual magnetic topology that can explain its polar aurora. Jupiter’s bright persistent polar aurora and Earth’s dark polar region indicate that the planets’ magnetospheric topologies ...
Binzheng Zhang +12 more
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New Models of Jupiter in the Context of Juno and Galileo [PDF]
Astrophysical Journal, 2019 Observations of Jupiter’s gravity field by Juno have revealed surprisingly low values for the high-order gravitational moments, considering the abundances of heavy elements measured by Galileo 20 years ago. The derivation of recent equations of state for
F. Debras, G. Chabrier
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No large population of unbound or wide-orbit Jupiter-mass planets [PDF]
Nature, 2017 Planet formation theories predict that some planets may be ejected from their parent systems as result of dynamical interactions and other processes. Unbound planets can also be formed through gravitational collapse, in a way similar to that in which ...
P. Mróz +11 more
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The symbol of the crescent Moon with a star on Ancient and Medieval coins [PDF]
Cultural Heritage and Modern TechnologiesThe individual phases of the moon show us this nocturnal satellite subjected to the laws of a cycle of dying and rising. In ancient times different peoples honoured the moon and the stars and felt connected to them in some way.
Štekar A.
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A Kinematical Detection of Two Embedded Jupiter-mass Planets in HD 163296 [PDF]
Astrophysical Journal, 2018 We present the first kinematical detection of embedded protoplanets within a protoplanetary disk. Using archival Atacama Large Millimetre Array (ALMA) observations of HD 163296, we demonstrate a new technique to measure the rotation curves of CO ...
R. Teague +4 more
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Sino-Uralic etymology for 'Jupiter, year' supported by rhyme correspondence [PDF]
Archaeoastronomy and Ancient Technologies, 2020 Using etymological methods, the present study has identified seven Sinitic and Uralic shared etymologies (etyma). Three of them form a rhyme correspondence. Two of them form an onset correspondence. Four of them form another rhyme correspondence.
Gao, J.
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