Zobrazeno 1 - 10
of 14 828
pro vyhledávání: '"exoplanet"'
Autor:
Kragh, Helge
Publikováno v:
The Names of Science: Terminology and Language in the History of the Natural Sciences.
Externí odkaz:
https://doi.org/10.1093/9780198917472.003.0007
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
Numerous numerical studies have been carried out in recent years that simulate different aspects of exoplanets’ magnetosphere and stellar winds. These studies have focused primarily on hot Jupiters with sun-like stars. This study addresses the chal
Externí odkaz:
https://doaj.org/article/3a2a9bd585654895a9c95d1e3b7e291c
Publikováno v:
Universe, Vol 10, Iss 9, p 374 (2024)
The distribution of period ratios for 580 known two-planet systems is apparently nonuniform, with several sharp peaks and troughs. In particular, the vicinity of the 2:1 commensurability seems to have a deficit of systems. Using Monte Carlo simulatio
Externí odkaz:
https://doaj.org/article/385a427386e14df2918f14fe922e11de
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
There are several methods for indirectly detecting exoplanets, such as transit, radial velocity, astrometry, and the conventional gravitational microlensing approach. These methods rely on observing the effects of exoplanets on the emission or motion
Externí odkaz:
https://doaj.org/article/af3e13b13d104e898ef3de05cadd5644
Publikováno v:
IEEE Access, Vol 12, Pp 139773-139788 (2024)
Deep learning has been shown to be a valuable tool in astrophysics. In the field of exoplanetary science, deep learning-based approaches are being used extensively to automate the characterization of exoplanet atmospheres, reducing computational cost
Externí odkaz:
https://doaj.org/article/a1d5206cf6564d1c9885c136864e19b4
Publikováno v:
Photonics, Vol 11, Iss 10, p 958 (2024)
The development of astronomy relies heavily on advances in high-resolution imaging techniques. With the growing demand for high-resolution astronomical observations, conventional optical interferometry has gradually revealed various limitations, espe
Externí odkaz:
https://doaj.org/article/76cb939de26043afad1010b7b37b4113
Akademický článek
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Autor:
Amélie Gressier, Néstor Espinoza, Natalie H. Allen, David K. Sing, Agnibha Banerjee, Joanna K. Barstow, Jeff A. Valenti, Nikole K. Lewis, Stephan M. Birkmann, Ryan C. Challener, Elena Manjavacas, Catarina Alves de Oliveira, Nicolas Crouzet, Tracy. L Beck
Publikováno v:
The Astrophysical Journal Letters, Vol 975, Iss 1, p L10 (2024)
Detecting atmospheres around planets with a radius below 1.6 R _⊕ , commonly referred to as rocky planets, has proven to be challenging. However, rocky planets orbiting M dwarfs are ideal candidates due to their favorable planet-to-star radius rati
Externí odkaz:
https://doaj.org/article/723a8b16d5bc4257a72e293aceb8c21a