Occurrence and Architecture of Kepler Planetary Systems as Functions of Stellar Mass and Effective Temperature [PDF]
Astronomical Journal, 2020 The Kepler mission has discovered thousands of exoplanets around various stars with different spectral types (M, K, G, and F) and thus different masses and effective temperatures.
Jia-Yi Yang, Jiwei Xie, Ji-lin Zhou
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Kepler Planet Occurrence Rates for Mid-type M Dwarfs as a Function of Spectral Type [PDF]
Astronomical Journal, 2019 Previous studies of planet occurrence rates largely relied on photometric stellar characterizations. In this paper, we present planet occurrence rates for mid-type M dwarfs using spectroscopy, parallaxes, and photometry to determine stellar ...
K. Hardegree-Ullman +3 more
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Experiencia estética y formulación científica: el caso del Harmonices Mundi de Johannes Kepler
Anuario Musical, 2013 La música como modelo explicativo del universo ha estado presente desde el mismo nacimiento de la reflexión filosófica. En el caso de Kepler, la música y la astronomía quedaban homologadas sobre la base de un único arquetipo geométrico, y por ello podían
Carlos Calderón Urreiztieta
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Physica Scripta, 1999 LaTex, 11 pages, 2 PostScript ...
B. Kaulakys, G. Vilutis
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The accelerated Kepler problem [PDF]
Celestial Mechanics and Dynamical Astronomy, 2007 The accelerated Kepler problem is obtained by adding a constant acceleration to the classical two-body Kepler problem. This setting models the dynamics of a jet-sustaining accretion disk and its content of forming planets as the disk loses linear momentum through the asymmetric jet-counterjet system it powers.
NAMOUNI F, GUZZO, MASSIMILIANO
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Elementary Solution of Kepler Problem (and a few other problems)
Revista Brasileira de Ensino de Física, 2022 We present a simple method to obtain the solution of a few orbital problems: the Kepler problem, the modified Kepler problem by the addition of an inverse square potential and linear force.
M. Moriconi
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Re-examining the light curves of Kepler-6b, Kepler-8b and Kepler-40b
AIP Conference Proceedings, 2018 We present a fresh analysis of the light curves of Kepler-6, Kepler-8 and Kepler-40 star-planet systems using similar to 3 years of observations by the Kepler space telescope. Transit light curves were solved usingWinFitter code. The proximity effects (ellipticity and reflection effects) and Doppler beaming effect were also examined using the Fourier ...
Ozturk, O., Erdem, A.
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Identifying Exoplanets with Deep Learning: A Five-planet Resonant Chain around Kepler-80 and an Eighth Planet around Kepler-90 [PDF]
, 2017 NASA’s Kepler Space Telescope was designed to determine the frequency of Earth-sized planets orbiting Sun-like stars, but these planets are on the very edge of the mission’s detection sensitivity.
Christopher J. Shallue, A. Vanderburg
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RR Lyrae Stars as Seen by the Kepler Space Telescope
Frontiers in Astronomy and Space Sciences, 2021 The unprecedented photometric precision along with the quasi-continuous sampling provided by the Kepler space telescope revealed new and unpredicted phenomena that reformed and invigorated RR Lyrae star research.
Emese Plachy +5 more
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Kepler Data Validation I—Architecture, Diagnostic Tests, and Data Products for Vetting Transiting Planet Candidates [PDF]
, 2018 The Kepler Mission was designed to identify and characterize transiting planets in the Kepler Field of View and to determine their occurrence rates. Emphasis was placed on identification of Earth-size planets orbiting in the Habitable Zone of their host ...
J. Twicken +16 more
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