Results 111 to 120 of about 171,913 (339)
Ground-based Microlensing Surveys [PDF]
arXiv, 2007 Microlensing is a proven extrasolar planet search method that has already yielded the detection of four exoplanets. These detections have changed our understanding of planet formation ``beyond the snowline'' by demonstrating that Neptune-mass planets with separations of several AU are common.
arxiv
Ejection of Bodies from the Solar System in the Course of the Accumulation of the Giant Planets and the Formation of the Cometary Cloud [PDF]
, 1972 V. S. Safronov
openalex +1 more source
Advanced Materials, EarlyView.A Co‐rich high‐entropy oxide (HEO) catalyst enables efficient electrochemical methane‐to‐ethanol conversion at room temperature. By leveraging elemental enrichment, the catalyst achieves high selectivity and stability, outperforming conventional systems.
Heewon Min +6 more
wiley +1 more source
Chapter 22. Primordial Atmosphere Surrounding a Protoplanet and Formation of Jovian Planets [PDF]
, 1988 Hiroshi Mizuno, Kiyoshi Nakazawa
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Advanced Materials, EarlyView.Laser micropatterning is presented as a promising technology in the search for autonomous dew water harvesting materials. Laser‐grooved metallic surfaces achieve simultaneously high infrared emissivity and superhydrophilicity, which gives them self‐cooling properties under atmospheric radiative deficit and the ability to condense water in an efficient ...
Pablo Pou‐Álvarez +7 more
wiley +1 more source
Disk Evolution, Element Abundances and Cloud Properties of Young Gas Giant Planets
Life, 2014 We discuss the chemical pre-conditions for planet formation, in terms of gas and ice abundances in a protoplanetary disk, as function of time and position, and the resulting chemical composition and cloud properties in the atmosphere when young gas giant
Christiane Helling +5 more
doaj +1 more source
On the properties of free floating planets originating in circumbinary planetary systems [PDF]
arXivFree-floating planets are a new class of planets recently discovered. These planets don't orbit within stellar systems, instead living a nomadic life within the galaxy. How such objects formed remains elusive. Numerous works have explored mechanisms to form such objects, but have not yet provided predictions on their distributions that could ...
arxiv
Formation of Giant Planets: Dependences on Core Accretion Rate and Grain Opacity [PDF]
, 2000 Masahiro Ikoma +2 more
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Challenges and Opportunities of Upconversion Nanoparticles for Emerging NIR Optoelectronic Devices
Advanced Materials, EarlyView.The special photo‐responsiveness of upconversion nanoparticles has opened up a new path for the advancement of near‐infrared (NIR)‐responsive optoelectronics. However, challenges such as low energy‐conversion efficiency and high nonradiative losses still persist.
Sunyingyue Geng +7 more
wiley +1 more source
The Planetary Science JournalErg Chech 002 (EC 002), an andesitic meteorite, has been dated to be the oldest magmatic rock in the solar system. However, controversy has arisen due to inconsistent dating results and isotopic compositions in previous studies, which complicates ...
Bing Yang +5 more
doaj +1 more source