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Quantum sensing for NASA science missions. [PDF]
Mercer CR +6 more
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The Role of Atmospheric Composition in Defining the Habitable Zone Limits and Supporting E. coli Growth. [PDF]
Kuzucan A +6 more
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Detecting And Characterizing Exoplanets: The Gj 436 And Hd 149026 Systems
Kevin B. Stevenson
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Precise Masses Reveal that TOI-700 c is Low Density and TOI-700 d is Rocky
Gilbert E +35 more
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ExoplanetExplorer: Contextual Visualization of Exoplanet Systems
2023 IEEE Visualization and Visual Analytics (VIS), 2023An exoplanet is a planet outside of our solar system. Researchers study known exoplanets and gather data about them through observations and derived data. Ongoing efforts involve finding planets with an environment that supports life, which likely exists
Emma Broman +6 more
semanticscholar +2 more sources
Exoplanet Systems and Their Stars
Oxford Scholarship Online, 2018This chapter highlights the amazing diversity of exoplanet worlds: planets can orbit neutron stars and giant stars, evaporate in the heat of their stars or have deep oceans, and may suffer from everlasting daysides and nightsides. A few enjoy two or more
K. Schrijver
semanticscholar +2 more sources
The Berlin Exoplanet Search Telescope System
Publications of the Astronomical Society of the Pacific, 2004We describe a small telescope system, the Berlin Exoplanet Search Telescope (BEST), dedicated to the search for planetary transits of Jupiter-sized planets on close-in orbits. This system consists of a commercial 20 cm telescope equipped with a 2048 x2048 pixel CCD.
Rauer, H. +6 more
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Detection of Exoplanet Systems In Kepler Light Curves Using Adaptive Neuro-Fuzzy System
2018 International Conference on Intelligent Systems (IS), 2018The paper investigates the usability of fuzzy inference systems, namely ANFIS to assist in the detection of exoplanet transit events from time-series data of Flux intensity values from host stars.
R. M. A. Amin +6 more
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Solar system, exoplanets, and anthropic principle
Bulletin of the Crimean Astrophysical Observatory, 2009It is shown that the planetary distances of the Solar System are distributed according to the L0 resonance, where L0 = cP0 = 19.24 a.u. is the wavelength of the “cosmological oscillation” of the Universe (whose nature is unknown). Here, c is the speed of light and P0 = 160 min is the period of pulsations of the Sun and the Universe, which turned out to
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