Results 71 to 80 of about 2,912,496 (265)
Photochemistry in Hot H2-dominated Exoplanet Atmospheres [PDF]
Photochemistry has the potential to substantially impact the atmospheric composition of exoplanets with consequences on the radiative transfer, thermal structure, and dynamics of the atmospheres, particularly in UV-rich stellar environments.
B. Fleury +3 more
semanticscholar +1 more source
The Influence of a Stellar Flare on the Dynamical State of the Atmosphere of the Exoplanet HD 209458b [PDF]
7 pages, 5 figures, accepted by Astronomy Reports (2018, v. 62, No. 10)
Luca Fossati +4 more
openaire +3 more sources
The Architectural Design Rules of Solar Systems based on the New Perspective
On the basis of the Lunar Laser Ranging Data released by NASA on the Silver Jubilee Celebration of Man Landing on Moon on 21st July 1969-1994, theoretical formulation of Earth-Moon tidal interaction was carried out and Planetary Satellite Dynamics was ...
A Johnson +33 more
core +1 more source
VIBES: Visual Binary Exoplanet survey with SPHERE [PDF]
Recent surveys indicate that planets in binary systems are more abundant than previously thought, which is in agreement with theoretical work on disc dynamics and planet formation in binaries.
J. Hagelberg +31 more
semanticscholar +1 more source
Neuromorphic Computing with Memcapacitors: Advancements, Challenges, and Future Directions
Neuromorphic computing reduces energy costs by integrating memory and processing in event‐driven architectures, achieving energy usage as low as 10–30 pJ per operation for memcapacitor‐based synapses. Memcapacitors are reviewed as strong contenders for neuromorphic computing, enhancing AI acceleration through charge‐based computations, high resistance,
Nada AbuHamra +4 more
wiley +1 more source
Statistical Distribution Function of Orbital Spacings in Planetary Systems
The minimum orbital separation of planets in long-stable planetary systems is often modeled as a step function, parameterized with a single value ${{\rm{\Delta }}}_{\min }$ (measured in mutual Hill radius of the two neighboring planets).
Jeremy Dietrich +2 more
doaj +1 more source
Photochemical hazes are expected to form in hot Jupiter atmospheres and may explain the strong scattering slopes and muted spectral features observed in the transmission spectra of many hot Jupiters.
Maria E. Steinrueck +7 more
doaj +1 more source
A Dynamic Scheme to Assess Habitability of Exoplanets
In the next few years, the number of catalogued exoplanets will be counted in the thousands and with it the need will arise to prioritize them in regard to habitability and the potential presence of life. Here, we suggest a first attempt of a dynamic scheme for classification based on our current understanding of parameters that are consistent and ...
Schulze-Makuch, D. +7 more
openaire +2 more sources
Formation of Ultra-short-period Planets in Hot Jupiter Systems: Application to WASP-47
The WASP-47 system is notable as the first known system hosting both inner and outer low-mass planetary companions around a hot Jupiter, with an ultra-short-period (USP) planet as the innermost planetary companion.
Su Wang +4 more
doaj +1 more source
The three-body problem, which describes three masses interacting through Newtonian gravity without any restrictions imposed on the initial positions and velocities of these masses, has attracted the attention of many scientists for more than 300 years ...
Musielak, Z. E., Quarles, B.
core +1 more source

