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Spectropolarimetry as a tool for understanding the diversity of planetary atmospheres
The polarization state of starlight reflected by a planetary atmosphere uniquely reveals coverage, particle size, and composition of aerosols as well...
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Formation of rocky super-earths from a narrow ring of planetesimals
The formation of super-Earths, the most abundant planets in the Galaxy, remains elusive. These planets have masses that typically exceed that of the...
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Astronomical Observations in Support of Planetary Entry-Probes to the Outer Planets
A team of Earth-based astronomical observers supporting a giant planet entry-probe event substantially enhances the scientific return of the mission....
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Rotational Dynamics and Evolution of Planetary Satellites in the Solar and Exoplanetary Systems
AbstractIn this review we consider the main rotation regimes that are inherent for planetary satellites of the Solar System, satellites of...
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Map** the structure of the planetary 2:1 mean motion resonance: the TOI-216, K2-24, and HD27894 systems
Mean motion resonances (MMR) are a frequent phenomenon among extrasolar planetary systems. Current observations indicate that many systems have...
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The Effect of the Mode of Heat Treatment and Mechanoactivation of Kaolinite on Mullite Formation
AbstractThe effect of the rate of heating of kaolinite Al 4 [Si 4 O 10 ](OH) 8 on its transformation into mullite 3Al 2 O 3 · 2SiO 2 has been studied. The...
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Chemical evidence for planetary ingestion in a quarter of Sun-like stars
Stellar members of binary systems are formed from the same material, and therefore they should be chemically identical. However, recent studies have...
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Planetary physics research at the Facility for Antiprotons and Ion Research using intense ion beams
Intense particle beams offer a new efficient driver to produce extended samples of high energy density (HED) matter with extreme physical conditions...
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Materials Under Extreme Conditions and Implications for Earth and Planetary Science
In chemistry under extreme conditions, shock compression forces to alter the chemical bonds by densification. A density increase does not always... -
Early terrestrial planet formation by torque-driven convergent migration of planetary embryos
The massive cores of the giant planets are thought to have formed in a gas disk by the accretion of pebble-sized particles whose accretional...
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Application of the Hori–Deprit Method to the Analysis of the Cosmogonic Evolution of Weakly Perturbed Planetary Systems
AbstractThe dynamical evolution of nonresonant two-planet systems whose structure is nearly circular and coplanar is studied by the Hori–Deprit...
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Towards a Planetary Polity: The Formation of Global Identity and State Structures
This article looks into the interconnection between the development of a global identity and a planetary polity from a long-term view. It is argued... -
From the Sun to Jupiter: Evolution of Low Mass Stars and Brown Dwarfs down to Planetary Masses
We present current models for low mass stars and substellar objects down to planetary masses and discuss the success and remaining uncertainties of... -
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Phase behaviours of superionic water at planetary conditions
Most water in the Universe may be superionic, and its thermodynamic and transport properties are crucial for planetary science but difficult to probe...
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Evolution of Planetary Chaotic Zones in Planetesimal Disks
AbstractExtensive numerical experiments on the long-term dynamics of planetesimal disks with planets in systems of single stars have been carried...