Academic literature on the topic 'Gliese 581d'

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Journal articles on the topic "Gliese 581d"

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von Bloh, W., C. Bounama, M. Cuntz, and S. Franck. "Habitability of super-Earths: Gliese 581c & 581d." Proceedings of the International Astronomical Union 3, S249 (2007): 503–6. http://dx.doi.org/10.1017/s1743921308017031.

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AbstractThe unexpected diversity of exoplanets includes a growing number of super-Earth planets, i.e., exoplanets with masses smaller than 10 Earth masses. Unlike the larger exoplanets previously found, these smaller planets are more likely to have similar chemical and mineralogical composition to the Earth. We present a thermal evolution model for super-Earth planets to identify the sources and sinks of atmospheric carbon dioxide. The photosynthesis-sustaining habitable zone (pHZ) is determined by the limits of biological productivity on the planetary surface. We apply our model to calculate
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Hu, Y., and F. Ding. "Radiative constraints on the habitability of exoplanets Gliese 581c and Gliese 581d." Astronomy & Astrophysics 526 (January 12, 2011): A135. http://dx.doi.org/10.1051/0004-6361/201014880.

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Cuntz, Manfred, Scott G. Engle, and Edward F. Guinan. "The Once-canceled Habitable-zone Super-Earth Gliese 581d Might Indeed Exist!" Research Notes of the AAS 8, no. 1 (2024): 20. http://dx.doi.org/10.3847/2515-5172/ad1de4.

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Abstract Recent studies indicate that Gliese 581d, a proposed habitable zone (HZ) super-Earth planet, does not exist, as the respective data denote that the planet is an artifact of stellar activity. Here we report evidence to the contrary considering that those studies were based on inaccurate spectroscopic measurements of the stellar rotation period regarding the planet’s inactive host star (dM3). Gliese 581d, if real, is of particular interest as it constitutes the first planet identified to be in a stellar HZ outside of the solar system based on studies in 2007. If confirmed as a true plan
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von Paris, P., S. Gebauer, M. Godolt, et al. "The extrasolar planet Gliese 581d: a potentially habitable planet?" Astronomy & Astrophysics 522 (October 28, 2010): A23. http://dx.doi.org/10.1051/0004-6361/201015329.

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Wordsworth, R. D., F. Forget, F. Selsis, J. B. Madeleine, E. Millour, and V. Eymet. "Is Gliese 581d habitable? Some constraints from radiative-convective climate modeling." Astronomy & Astrophysics 522 (October 28, 2010): A22. http://dx.doi.org/10.1051/0004-6361/201015053.

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Wordsworth, Robin D., François Forget, Franck Selsis, Ehouarn Millour, Benjamin Charnay, and Jean-Baptiste Madeleine. "GLIESE 581D IS THE FIRST DISCOVERED TERRESTRIAL-MASS EXOPLANET IN THE HABITABLE ZONE." Astrophysical Journal 733, no. 2 (2011): L48. http://dx.doi.org/10.1088/2041-8205/733/2/l48.

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Cuntz, Manfred. "Gliese 581c: Habitability Unlikely—but not Hopeless Either." Research Notes of the AAS 7, no. 6 (2023): 128. http://dx.doi.org/10.3847/2515-5172/acdf52.

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Abstract There is continued interest in the study of habitability for the Gliese 581 system. Previously, for Gliese 581c, a quasi-consensus has been reached that this planet, a super-Earth, is interior to the stellar habitable zone, akin to Venus in the solar system. In this work, I revisit this view considering detailed results about the orbital planetary parameters (including their uncertainties) and previous studies on habitability.
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Pierrehumbert, R. T. "A PALETTE OF CLIMATES FOR GLIESE 581g." Astrophysical Journal 726, no. 1 (2010): L8. http://dx.doi.org/10.1088/2041-8205/726/1/l8.

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Selsis, F., J. F. Kasting, B. Levrard, J. Paillet, I. Ribas, and X. Delfosse. "Habitable planets around the star Gliese 581?" Astronomy & Astrophysics 476, no. 3 (2007): 1373–87. http://dx.doi.org/10.1051/0004-6361:20078091.

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Tóth, Zs, and I. Nagy. "Dynamical stability of the Gliese 581 exoplanetary system." Monthly Notices of the Royal Astronomical Society 442, no. 1 (2014): 454–61. http://dx.doi.org/10.1093/mnras/stu849.

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Dissertations / Theses on the topic "Gliese 581d"

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Silva, Gleidson Gomes da. "Ressonâncias de três corpos: estudo da dinâmica da zona habitável do sistema exoplanetário GJ581." Universidade de São Paulo, 2012. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-24062013-115006/.

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Estudo das ressonâncias de três corpos na zona habitável (ZH), da estrela GJ 581 (Gliese 581), envolvendo dois planetas conhecidos e um terceiro planeta dentro da ZH. Séries de Lie são usadas para obter o Hamiltoniano médio (de segunda ordem nas massas) e teoria de Chirikov é usada para gerar um novo sistema de varáveis canônicas em que os momentos se orientam ao longo e através da ressonância. Um mapa de Hadjidemetriou é construido e permite o cálculo rápido da difusão das órbitas em uma extensa grade de condições iniciais.<br>Study of three-body resonances in the habitable zone (ZH), the sta
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Books on the topic "Gliese 581d"

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First Awakenings: Gliese 581g. Montana Publishing, 2017.

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Command Decision: Gliese 581g. Montana Publishing, 2016.

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Shuck, Christine. Gliese 581: The Departure. Independently Published, 2018.

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Smith, S. E. Command Decision: Project Gliese 581g. Susan E. Smith, 2016.

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Smith, S. E. Survivor Skills: Project Gliese 581g Book 3. Independently Published, 2019.

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Survivor Skills: Project Gliese 581g Book 3. Montana Publishing, 2018.

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Smith, S. E. Survivor Skills: The Project Gliese 581g Series, book 3. Susan E. Smith and Blackstone Audio, 2018.

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Book chapters on the topic "Gliese 581d"

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Stevenson, David S. "Gliese 581d: The First Potentially Habitable Water-World Discovered?" In Astronomers' Universe. Springer New York, 2013. http://dx.doi.org/10.1007/978-1-4614-8133-1_9.

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Haghighipour, Nader. "Gliese 581, the Most Highly Debated Habitable System." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-44185-5_5298.

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Haghighipour, Nader. "Gliese 581, the Most Highly Debated Habitable System." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27833-4_5298-1.

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