Results 111 to 120 of about 54,418 (256)
The Future of Exoplanet Direct Detection [PDF]
arXiv, 2019 Diffraction fundamentally limits our ability to image and characterize exoplanets. Current and planned coronagraphic searches for exoplanets are making incredible strides but are fundamentally limited by the inner working angle of a few lambda/D.
arxiv
ChemSusChem, Volume 18, Issue 3, February 1, 2025.A novel subclass of graphitic oxynitrides, easily generated from otherwise abundant prebiotic monomers, namely cyanamide and glyoxal, debut in the scenario of sustainable heterogeneous catalysts, as demonstrated through applications to the highly demanding H2 and CO2 agendas.
Nieves Lavado +7 more
wiley +1 more source
Comment: Hans Deeg \S Juan Antonio Belmonte. Handbook of Exoplanets, 2nd Edition, Springer International Publishing AG, part of Springer Nature, In ...
Robutel, Philippe, Leleu, Adrien
openaire +3 more sources
Initial Thermal States of Super‐Earth Exoplanets and Implications for Early Dynamos
Journal of Geophysical Research: Planets, Volume 130, Issue 2, February 2025.Abstract The accretion of Earth and the formation of a metallic core released a large amount of primordial heat and may have enabled its evolution into a habitable world. Metal‐silicate segregation likely occurs in super‐Earth exoplanets as well, but its influence on their initial thermal states has not been fully examined.
Nathaniel I. White, Jie Li
wiley +1 more source
Characterizing Exoplanet Habitability [PDF]
, 2017 A habitable exoplanet is a world that can maintain stable liquid water on its surface. Techniques and approaches to characterizing such worlds are essential, as performing a census of Earth-like planets that may or may not have life will inform our understanding of how frequently life originates and is sustained on worlds other than our own ...
openaire +3 more sources
MARVEL Analysis of High‐Resolution Rovibrational Spectra of 16O13C18O
Journal of Computational Chemistry, Volume 46, Issue 1, January 5, 2025.12348 measured transitions in the wavenumber range 578–9318 cm−1 for carbon dioxide (isotopologue 638) were used° to calculating 3975 empirical rovibrational energy levels with J° up to 82. ABSTRACT A large set of validated experimental transitions and empirical rovibrational energy levels are reported for the fifth most abundant carbon dioxide ...
Ala'a A. A. Azzam +4 more
wiley +1 more source
Atmospheric Retrieval of Exoplanets [PDF]
, 2018 30 pages, 3 figures, Published in Springer Handbook of ...
openaire +3 more sources
Empirical Line Lists in the ExoMol Database
Atoms, 2020 The ExoMol database aims to provide comprehensive molecular line lists for exoplanetary and other hot atmospheres. The data are expanded by inclusion of empirically derived line lists taken from the literature for a series of diatomic molecules, namely ...
Yixin Wang +2 more
doaj +1 more source
Science Fiction Media Representations of Exoplanets: Portrayals of Changing Astronomical Discoveries [PDF]
JCOM Journal of Science Communication 23(1) 2024Interest in science fiction's (SF's) potential science communication use is hindered by concerns about SF misrepresenting science. This study addresses these concerns by asking how SF media reflects scientific findings in exoplanet science. A database of SF exoplanets was analysed using a Bayesian network to find interconnected interactions between ...
arxiv +1 more source
Detectability of Exoplanets in the Beta Pic Moving Group with the Gemini Planet Imager
, 2010 We model the detectability of exoplanets around stars in the Beta Pic Moving Group (BPMG) using the Gemini Planet Imager (GPI), a coronagraphic instrument designed to detect companions by imaging.
Kataria, Tiffany, Simon, Michal
core +1 more source