Results 61 to 70 of about 13,291 (174)
HARPS-N @ TNG, two year harvesting data : performances and results
, 2014 The planet hunter HARPS-N[1], in operation at the Telescopio Nazionale Galileo (TNG)[13] from April 2012 is a highresolution spectrograph designed to achieve a very high radial velocity precision measurement thanks to an ultra stable environment and in a
Latham, D.W. +39 more
core +1 more source
Molecular opacities for exoplanets [PDF]
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2014 Spectroscopic observations of exoplanets are now possible by transit methods and direct emission. Spectroscopic requirements for exoplanets are reviewed based on existing measurements and model predictions for hot Jupiters and super-Earths.
openaire +3 more sources
Implications of Tides for Life on Exoplanets [PDF]
Astrobiology, 2018 As evident from the nearby examples of Proxima Centauri and TRAPPIST-1, Earth-sized planets in the habitable zone of low-mass stars are common. Here, we focus on such planetary systems and argue that their (oceanic) tides could be more prominent due to stronger tidal forces.
Lingam, Manasvi, Loeb, Abraham
openaire +3 more sources
Modeling the Seasonality of Wind‐Driven Hydrocarbon Waves in Titan's Polar Lakes
Journal of Geophysical Research: Planets, Volume 131, Issue 5, May 2026.Abstract Titan, the only body in the solar system aside from Earth with standing liquids on its surface, has high‐latitude hydrocarbon lakes and seas. As Titan's atmosphere generates light winds, there should be waves on the surface of these lakes and seas, yet, direct wave observations are scant.
Charlene E. Detelich +8 more
wiley +1 more source
Volcanism at Piton de la Fournaise as an Analog for Chloris Mons, Venus
Journal of Geophysical Research: Planets, Volume 131, Issue 5, May 2026.Abstract Identifying and investigating terrestrial analogs for Venus volcanic activity is necessary to prepare for the planned upcoming missions to Venus. We propose volcanism at Piton de la Fournaise, a frequently active oceanic shield volcano, as an analog to volcanism at Chloris Mons, Venus.
Evan G. K. Cooper +5 more
wiley +1 more source
Impacts of Carbon Dioxide Deposition on Martian Near‐Surface Wave Activity
Geophysical Research Letters, Volume 53, Issue 7, 16 April 2026.Abstract A prominent feature of Mars' winter atmosphere is near‐surface baroclinic wave activity. These waves exert strong control on dust storm variability and contribute to transport of heat, momentum, and dust. Using a suite of Mars general circulation model simulations, we investigate an underexplored connection between near‐surface wave activity ...
Hung Kwan Fok +2 more
wiley +1 more source
OF “COCKTAIL PARTIES” AND EXOPLANETS [PDF]
The Astrophysical Journal, 2012 ApJ ...
openaire +2 more sources
exoplanet-dev/jaxoplanet: Astronomical time series analysis with JAX
<h2>What's Changed</h2> <ul> <li>Updating and applying pre-commit by @dfm in https://github.com/exoplanet-dev/jaxoplanet/pull/16</li> <li>Adding interface for arbitrary order limb darkening by @dfm in https://github ...
Degen, David +6 more
core +1 more source
, 2014 A unique short-period (P = 0.65356(1) d) Mercury-size Kepler exoplanet candidate KIC012557548b has been discovered recently by Rappaport et al. (2012).
Zhou, Guyin (George) +6 more
core +1 more source
Journal of Geophysical Research: Planets, Volume 131, Issue 4, April 2026.Abstract Xenon (Xe) is a heavy noble gas with intriguing chemical properties, such as having several stable isotopes and the ability to form compounds under extreme conditions. Despite the predictions based on cosmochemical models that suggest xenon should be relatively abundant in planetary reservoirs, empirical data indicate a significant depletion ...
Avinash Kumar Both +2 more
wiley +1 more source