First Results from the MIT Optical Rapid Imaging System (MORIS) on the IRTF: A Stellar Occultation by Pluto and a Transit by Exoplanet XO-2b [PDF]
A. A. S. Gulbis +10 more
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It has been suggested that β Pic b has a supersolar metallicity and subsolar C/O ratio. Assuming solar carbon and oxygen abundances for the star β Pic and therefore the planet’s parent protoplanetary disk, β Pic b’s C/O ratio suggests that it formed via ...
Henrique Reggiani +7 more
doaj +1 more source
MESS (multi-purpose exoplanet simulation system) [PDF]
M. Bonavita +7 more
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Gravity darkening and tidally perturbed stellar pulsation in the misaligned exoplanet system WASP-33 [PDF]
Szilárd Kálmán +5 more
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Hic Sunt Dracones: Uncovering Dynamical Perturbers within the Habitable Zone
The continuing exploration of neighboring planetary systems is providing deeper insights into the relative prevalence of various system architectures, particularly with respect to the solar system.
Stephen R. Kane, Jennifer A. Burt
doaj +1 more source
Analyzing light curves to highlight phenomena and trends in planetary systems that house terrestrial exoplanets [PDF]
D. Cao
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Planet formation models suggest that the small exoplanets that migrate from beyond the snowline of the protoplanetary disk likely contain water-ice-rich cores (∼50% by mass), also known as water worlds.
Aritra Chakrabarty, Gijs D. Mulders
doaj +1 more source
Geology and Photometric Variation of Solar System Bodies with Minor Atmospheres: Implications for Solid Exoplanets [PDF]
Yuka Fujii +3 more
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White dwarf systems: The composition of exoplanets
Preprint of a chapter for the 'Encyclopedia of Astrophysics' (Editor-in-Chief Ilya Mandel, Section Editor Dimitri Veras) to be published by Elsevier as a Reference ...
openaire +2 more sources
Comprehensive Parameter Determination of Exoplanets through Asteroseismic Host Star Constraints
This study develops a robust framework for exoplanet characterization by leveraging asteroseismic constraints on host stars. Using precise photometric data from missions such as Kepler and TESS, we derive stellar parameters, including mass, radius, and ...
Wen-Xu Lin +7 more
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