Results 71 to 80 of about 44,852 (244)
Coreless Terrestrial Exoplanets [PDF]
Differentiation in terrestrial planets is expected to include the formation of a metallic iron core. We predict the existence of terrestrial planets that have differentiated but have no metallic core--planets that are effectively a giant silicate mantle.
Linda T. Elkins-Tanton, Sara Seager
openaire +3 more sources
X-ray through infrared spectral energy distributions (SEDs) are essential for understanding a star’s effect on exoplanet atmospheric composition and evolution. We present a catalog of panchromatic SEDs, hosted on the Barbara A. Mikulski Archive for Space
Patrick R. Behr+10 more
doaj +1 more source
Mapping out the time-evolution of exoplanet processes [PDF]
There are many competing theories and models describing the formation, migration and evolution of exoplanet systems. As both the precision with which we can characterize exoplanets and their host stars, and the number of systems for which we can make ...
Beichman, Charles+4 more
core +1 more source
The Power of a Name: Toward a Unified Approach to Naming Space Weather Events
Abstract Our increasing reliance on technology vulnerable to space weather effects underscores the urgent need for effective public communication about these phenomena. While scientific research thrives on precise technical language, broader public engagement necessitates a more accessible and memorable approach.
Sophie Chabanski+4 more
wiley +1 more source
The NASA Exoplanet Archive: Data and Tools for Exoplanet Research [PDF]
We describe the contents and functionality of the NASA Exoplanet Archive, a database and tool set funded by NASA to support astronomers in the exoplanet community. The current content of the database includes interactive tables containing properties of all published exoplanets, Kepler planet candidates, threshold-crossing events, data validation ...
Akeson, R. L.+34 more
openaire +4 more sources
ROME. III. The Arecibo Search for Star–Planet Interactions at 5 GHz
After nearly three decades of discovery, many exoplanetary systems have been studied and characterized in detail with one important exception: exoplanet magnetism.
Matthew Route, Alexander Wolszczan
doaj +1 more source
Space Technology for Directly Imaging and Characterizing Exo-Earths
The detection of Earth-like exoplanets in the habitable zone of their stars, and their spectroscopic characterization in a search for biosignatures, requires starlight suppression that exceeds the current best ground-based performance by orders of ...
Crill, Brendan, Siegler, Nicholas
core +1 more source
The Ultraviolet Radiation Environment Around M dwarf Exoplanet Host Stars [PDF]
The spectral and temporal behavior of exoplanet host stars is a critical input to models of the chemistry and evolution of planetary atmospheres. At present, little observational or theoretical basis exists for understanding the ultraviolet spectra of M ...
Bushinsky, Rachel+10 more
core +4 more sources
Abstract We investigate the melt production of planetary impacts as a function of planet size (R/REarth $R/{R}_{\text{Earth}}$ = 0.1–1.5), impactor size (L $L$ = 1–1,000 km), and core size ratio (Rcore/R ${R}_{\text{core}}/R$ = 0.2–0.8) using a combination of parameterized convection models and fully dynamical 2D impact simulations.
Lukas Manske+6 more
wiley +1 more source
Exoplanet Predictions Based on the Generalised Titius-Bode Relation
We evaluate the extent to which newly detected exoplanetary systems containing at least four planets adhere to a generalized Titius-Bode (TB) relation.
Bovaird, Timothy, Lineweaver, Charles H.
core +1 more source