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We present simulations of atmospheres of Earth-like aquaplanets that are tidally locked to their star, that is, planets whose orbital period is equal to the rotation period about their spin axis, so that one side always faces the star and…

Earth and Planetary Astrophysics · Physics 2011-03-11 Timothy M. Merlis , Tapio Schneider

Saturn's northern summertime hemisphere was mapped by JWST/MIRI (4.9-27.9 $\mu$m) in November 2022, tracing the seasonal evolution of temperatures, aerosols, and chemical species in the five years since the end of the Cassini mission. The…

We present an overview of the current status of neutrino oscillation studies at atmospheric neutrino experiments. While the current data gives some tentalising hints regarding the neutrino mass hierarchy, octant of $\theta_{23}$ and…

High Energy Physics - Phenomenology · Physics 2016-06-22 Sandhya Choubey

Considering effects of tidal plus centrifugal stress acting on icy-rocks and the tensile strength thereof, icy-rocks being in the density range (1-2.4) g cm-3 which had come into existence as collisional ejecta (debris) in the vicinity of…

Earth and Planetary Astrophysics · Physics 2011-09-09 J. J. Rawal , Bijan Nikouravan

Planetary rotation rate is a key parameter in determining atmospheric circulation and hence the spatial pattern of clouds. Since clouds can exert a dominant control on planetary radiation balance, rotation rate could be critical for…

Earth and Planetary Astrophysics · Physics 2014-04-29 Jun Yang , Gwenael Boue , Daniel C. Fabrycky , Dorian S. Abbot

Pluto's surface displays a wide variety of geologic units from smooth plains to extremely rugged mountainous expanses. These terrains range in age from young, actively resurfaced regions (no observable craters even in the highest-resolution…

Earth and Planetary Astrophysics · Physics 2025-06-03 Kelsi N. Singer , Oliver L. White , Sarah Greenstreet , Jeffrey M. Moore , David A. Williams , Rosaly M. C. Lopes

Here we describe the observations and the resulting constraints on the upper atmosphere (thermosphere and exosphere) of the "Hot-Jupiters". In particular, observations and theoretical modeling of Hot-Jupiter evaporation are described. The…

Earth and Planetary Astrophysics · Physics 2015-05-13 A. Lecavelier des Etangs

Next year, 2015, the New Horizons spacecraft will have a close encounter with Pluto. In the present study we discuss some possibilities regarding what the spacecraft may encounter during its approach to Pluto. Among them we should include:…

Earth and Planetary Astrophysics · Physics 2015-05-28 Hector Javier Durand-Manterola , Hector Perez-de-Tejada

Pathria(1972) has shown, for a pressureless closed Universe, that it is inside a black (or white) hole. We show now, that the Universe with a cosmic pressure obeying Einstein's field equations, can be inside a white-hole. In the closed…

General Physics · Physics 2008-11-26 Marcelo Samuel Berman

We hereby study the stability of a massless probe orbiting around an oblate central body (planet or planetary satellite) perturbed by a third body, assumed to lie in the equatorial plane (Sun or Jupiter for example) using an Hamiltonian…

Earth and Planetary Astrophysics · Physics 2012-01-11 N. Delsate , P. Robutel , A. Lemaitre , T. Carletti

The TRAPPIST-1 system provides an extraordinary opportunity to study multiple terrestrial extrasolar planets and their atmospheres. Here we use the National Center for Atmospheric Research Community Atmosphere Model version 4 to study the…

Earth and Planetary Astrophysics · Physics 2018-04-03 Eric T. Wolf

Thanks to their short orbital periods and hot extended atmospheres, hot Jupiters are ideal candidates for atmosphere studies with high-resolution spectroscopy. New stable spectrographs help improve our understanding of the evolution and…

For a wide class of spherically symmetric naked singularities there is a sphere within which gravity is effectively repulsive. In such spacetimes accreting matter cannot reach the singularity and will instead form a levitating atmosphere,…

General Relativity and Quantum Cosmology · Physics 2021-09-07 Ronaldo S. S. Vieira , Włodek Kluźniak

This review presents an insight into our current knowledge of the atmospheres of the planets Venus, Mars, Jupiter, Saturn, Uranus and Neptune, the satellite Titan, and those of exoplanets. It deals with the thermal structure, aerosol…

Earth and Planetary Astrophysics · Physics 2023-12-12 Agustín Sánchez-Lavega , Patrick Irwin , Antonio García Muñoz

Detailed characterization of an extrasolar planet's atmosphere provides the best hope for distinguishing the makeup of its outer layers, and the only hope for understanding the interplay between initial composition, chemistry, dynamics &…

Earth and Planetary Astrophysics · Physics 2016-03-09 Ian J. M. Crossfield

A unique feature of Pluto's large satellite Charon is its dark red northern polar cap. Similar colours on Pluto's surface have been attributed to organic macromolecules produced by energetic radiation processing of hydrocarbons. The polar…

The general circulation of the atmosphere determines the long-term variability of weather processes. This circulation is driven by the temperature differences between the poles and the equator, causing air to move along the Earth's surface.…

Atmospheric and Oceanic Physics · Physics 2023-06-21 Alexander V. Kochin

Both Pluto and its satellite Charon have rotation rates synchronous with their orbital mean motion. This is the theoretical end point of tidal evolution where transfer of angular momentum has ceased. Here we follow Pluto's tidal evolution…

Earth and Planetary Astrophysics · Physics 2015-06-18 W. H. Cheng , Man Hoi Lee , S. J. Peale

As a follow-up of a recent study, we challenge the claim that the flow of interstellar helium through the solar system has changed substantially over the last decades. We argue that only the IBEX-Lo 2009-2010 measurements are discrepant…

Solar and Stellar Astrophysics · Physics 2015-06-23 J. L. Bertaux , R. Lallement

With the operation of JWST, atmospheric characterization has now extended to low-mass exoplanets. In compact multiplanetary systems, secular spin-orbital resonance may preserve high obliquities and asynchronous rotation even for…

Earth and Planetary Astrophysics · Physics 2026-01-27 Yanhong Lai , Xianyu Tan , Yubo Su