Results 41 to 50 of about 2,964,883 (268)
Aerosol dynamics on hot exoplanets: the role of radiation pressure [PDF]
Monthly Notices of the Royal Astronomical SocietyABSTRACT Aerosols appear to be ubiquitous in exoplanetary atmospheres. However, because our understanding of the physical processes that govern aerosols is incomplete, their presence makes the measurement of atmospheric properties, such as molecular abundance ratios, difficult.
James E. Owen, Ruth Murray‐Clay
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Emergent Exoplanet Flux: Review of the Spitzer Results [PDF]
, 2008 Observations using the Spitzer Space Telescope provided the first detections of photons from extrasolar planets. Spitzer observations are allowing us to infer the temperature structure, composition, and dynamics of exoplanet atmospheres.
Bouchy +6 more
core +1 more source
Studying exoplanet orbits & dynamics with allesfitter
, 2022 <p>The orbits and dynamics of exoplanet systems can unveil their tales of formation, migration, star-planet interactions, and atmospheric properties. Kepler, TESS, and soon PLATO deliver an unprecedented wealth of new photometric data on this matter, while ground-based follow-up and radial velocity instruments add valuable insights. Here,
Maximilian N. Günther
openalex +2 more sources
Exoplanet albedo spectra and colors as a function of planet phase, separation, and metallicity [PDF]
, 2010 First generation optical coronagraphic telescopes will obtain images of cool gas and ice giant exoplanets around nearby stars. The albedo spectra of exoplanets at planet-star separations larger than about 1 AU are dominated by reflected light to beyond 1
Ackerman +58 more
core +2 more sources
Secular spin-axis dynamics of exoplanets [PDF]
Astronomy & Astrophysics, 2019 Context. Seasonal variations and climate stability of a planet are very sensitive to the planet obliquity and its evolution. This is of particular interest for the emergence and sustainability of land-based life, but orbital and rotational parameters of exoplanets are still poorly constrained.
Saillenfest, M., Laskar, J., Boué, G.
openaire +4 more sources
TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain
The Astronomical Journal, 2023 Convergent disk migration has long been suspected to be responsible for forming planetary systems with a chain of mean-motion resonances (MMRs). Dynamical evolution over time could disrupt the delicate resonant configuration. We present TOI-1136, a 700 ±
Fei Dai +62 more
doaj +1 more source
Radial velocity eclipse mapping of exoplanets [PDF]
, 2015 Planetary rotation rates and obliquities provide information regarding the history of planet formation, but have not yet been measured for evolved extrasolar planets.
Barnes J. W. +23 more
core +2 more sources
Secular spin-axis dynamics of exoplanets (Corrigendum) [PDF]
Astronomy & Astrophysics, 2019 International ...
Saillenfest, M., Laskar, J., Boué, G.
openaire +3 more sources
On the orbital stability of exoplanet satellites
Publications of the Pulkovo_Observatory, 2022 By calculating the Lyapunov characteristic exponents, an analysis was made of the stability of the secular orbital dynamics of satellites for a number of exoplanets in which the presence of an exomoon is possible.
A. Melnikov
semanticscholar +1 more source
Observations of Extrasolar Planets During the non-Cryogenic Spitzer Space Telescope Mission [PDF]
, 2007 Precision infrared photometry from Spitzer has enabled the first direct studies of light from extrasolar planets, via observations at secondary eclipse in transiting systems.
David Charbonneau +7 more
core +2 more sources