Results 81 to 90 of about 58,525 (269)
The Detection and Characterization of Extrasolar Planets
Challenges, 2014 We have now confirmed the existence of > 1800 planets orbiting stars other thanthe Sun; known as extrasolar planets or exoplanets. The different methods for detectingsuch planets are sensitive to different regions of parameter space, and so, we are ...
Ken Rice
doaj +1 more source
Health Psychology Review, 2015 Despite its presence in the psychological literature for more than one hundred years, the habit concept, the means by which habit serves to control human behaviour in daily life and the means by wh...
Orbell, Sheina, Verplanken, Bas
openaire +5 more sources
Habitable Zone Lifetime of Exoplanets around Main Sequence Stars [PDF]
, 2013 Funding: Dean's Scholarship at the University of East Anglia.The potential habitability of newly discovered exoplanets is initially assessed by determining whether their orbits fall within the circumstellar habitable zone of their star.
Claire, M. +3 more
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M Dwarf Planet Habitability [PDF]
, 2017 The habitability of M dwarf planets has been debated greatly, as their parent stars possess both beneficial and detrimental qualities for the development of life.
Koenigs, Ben
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The European Physical Journal Special Topics, 2020 Quantification of habitability is a complex task. Previous attempts at measuring habitability are well documented. Classification of exoplanets, on the other hand, is a different approach and depends on quality of training data available in habitable ...
Snehanshu Saha +4 more
semanticscholar +1 more source
The habitability of the Universe through 13 billion years of cosmic time [PDF]
, 2016 The field of astrobiology has made tremendous progress in modelling galactic-scale habitable zones which offer a stable environment for life to form and evolve in complexity.
Cockell, Charles +2 more
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Frontiers in Astronomy and Space Sciences, 2022 We present a new synergic strategy that merges the potential of asteroseismology with solar space weather/climate techniques in order to characterize solar-like stars and their interaction with hosted exoplanets. The method is based on the use of seismic
Raffaele Reda +8 more
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Atmospheric studies of habitability in the Gliese 581 system
, 2011 The M-type star Gliese 581 is orbited by at least one terrestrial planet candidate in the habitable zone, i.e. GL 581 d. Orbital simulations have shown that additional planets inside the habitable zone of GL 581 would be dynamically stable. Recently, two
Gebauer, S. +4 more
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The Carbonate Geochemistry of Enceladus' Ocean
Geophysical Research Letters, 2020 The plume composition at Enceladus contains clues about conditions and processes in the interior. We present new geochemical interpretations of Cassini mass spectrometry data from the plume gas and salt‐rich ice grains.
Christopher R. Glein, J. Hunter Waite
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Habitability of Super-Earth Planets around Other Suns: Models including Red Giant Branch Evolution [PDF]
, 2008 The unexpected diversity of exoplanets includes a growing number of super- Earth planets, i.e., exoplanets with masses of up to several Earth masses and a similar chemical and mineralogical composition as Earth. We present a thermal evolution model for a
Bounama, C. +4 more
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