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Exoplanet detection techniques – from astronomy to astrobiology
, 2006 Wolfgang Brandner
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Ozone-like layer in an exoplanet atmosphere [PDF]
Nature, 2017 The nature of exoplanetary atmospheres is hotly debated. The thermal spectrum of an exoplanet called a hot Jupiter reveals the presence of an analogue of Earth's ozone layer, although its composition is unknown. See Letter p.58 Earth's atmosphere consists of layers that are partially defined by ...
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Nature, 2015
Analysis of Kepler data has yielded the smallest known mass for an exoplanet orbiting a normal star. Its mass and size are similar to those of Mars, setting a benchmark for the properties of exoplanets smaller than Earth. See Letter p.321 Kepler-138, a red dwarf in the constellation of Lyra, hosts ...
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Analysis of Kepler data has yielded the smallest known mass for an exoplanet orbiting a normal star. Its mass and size are similar to those of Mars, setting a benchmark for the properties of exoplanets smaller than Earth. See Letter p.321 Kepler-138, a red dwarf in the constellation of Lyra, hosts ...
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Nature, 2014
Spectroscopic observations of a young exoplanet have allowed its spin velocity to be directly measured. Its fast spin is in accord with the extrapolation of the known trend in spin velocity as a function of planet mass. See Letter p.63 Near-infrared spectroscopic observations of the young extrasolar
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Spectroscopic observations of a young exoplanet have allowed its spin velocity to be directly measured. Its fast spin is in accord with the extrapolation of the known trend in spin velocity as a function of planet mass. See Letter p.63 Near-infrared spectroscopic observations of the young extrasolar
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Training on Machine Learning Applied to Space Astronomy Data and Exoplanet Research
IAF Space Exploration SymposiumE. S. Cheng +7 more
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The Lidov-Kozai Effect - Applications in Exoplanet Research and Dynamical Astronomy
, 2016 Ivan I. Shevchenko
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Nature, 2010
The masses of exoplanets have so far been inferred from the tiny gravitational pull they exert on the host stars. It is now possible to measure them from shifts in spectral lines arising from the planets' atmospheres.
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The masses of exoplanets have so far been inferred from the tiny gravitational pull they exert on the host stars. It is now possible to measure them from shifts in spectral lines arising from the planets' atmospheres.
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Surveying the reach and maturity of machine learning and artificial intelligence in astronomy
Wiley Interdisciplinary Reviews: Data Mining and Knowledge Discovery, 2020Christopher Fluke, C Jacobs
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This thesis explores the potential in democratizing and augmenting exoplanet research via citizen science by utilizing a global network of portable image-intensified computerized telescopes, and inquiry-based astronomy instruction. A central objective is to establish that citizen scientists, using exoplanet transit photometry with compact, connected ...
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