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惑星の居住可能性 (Japanese Wikipedia)

Analysis of information sources in references of the Wikipedia article "惑星の居住可能性" in Japanese language version.

refsWebsite
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5web.archive.org
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5astrobio.net
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4harvard.edu
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3wikipedia.org
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2solstation.com
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2uoregon.edu
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2psu.edu
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2washington.edu
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1nasa.gov
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1arizona.edu
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1calstatela.edu
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1nih.gov
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1nature.com
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1colorado.edu
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1doi.org
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1jmu.edu
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1gsu.edu
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1daviddarling.info
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1cfa-harvard.edu
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1carnegieinstitution.org
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1ucsd.edu
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1unr.edu
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1utexas.edu
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1kencroswell.com
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1upr.edu
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1arxiv.org
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1pnas.org
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arizona.edu (Global: 1,592nd place; Japanese: 3,926th place)

skye.as.arizona.edu

  • Turnbull, Margaret C., and Jill C. Tarter. "Target selection for SETI: A catalog of nearby habitable stellar systems," The Astrophysical Journal Supplement Series, 145: 181-198, March 2003. (Link Archived 2006年11月9日, at the Wayback Machine. (PDF) ). Habitability criteria defined—the foundational source for this article.

arxiv.org (Global: 69th place; Japanese: 227th place)

  • Horner & Jones (2011). “Quantifying Jupiter’s influence on the Earth’s impact flux: Implications for planetary habitability”. arXiv:1202.1314.{{cite arXiv}}: CS1メンテナンス: classが不足 (カテゴリ) 11th annual Australian Space Science Conference

astrobio.net (Global: low place; Japanese: low place)

calstatela.edu (Global: low place; Japanese: low place)

curriculum.calstatela.edu

carnegieinstitution.org (Global: low place; Japanese: low place)

cfa-harvard.edu (Global: low place; Japanese: low place)

colorado.edu (Global: 2,526th place; Japanese: 6,861st place)

origins.colorado.edu

  • Santos, Nuno C., Garik Israelian and Michel Mayor. "Confirming the Metal-Rich Nature of Stars with Giant Planets," Proceedings of 12th Cambridge Workshop on Cool Stars, Stellar Systems, and The Sun, University of Colorado, 2003. (Link (PDF) ). Metallicity and the occurrence of extra-solar planets.

daviddarling.info (Global: 7,061st place; Japanese: 8,237th place)

doi.org (Global: 2nd place; Japanese: 6th place)

gsu.edu (Global: 1,911th place; Japanese: 3,615th place)

hyperphysics.phy-astr.gsu.edu

harvard.edu (Global: 18th place; Japanese: 107th place)

ui.adsabs.harvard.edu

  • Buchhave et al. (2012). “An abundance of small exoplanets around stars with a wide range of metallicities”. Nature 486: pp.375-377. Bibcode: 2012Natur.486..375B. doi:10.1038/nature11121. 
  • Laskar, J., F. Joutel and P. Robutel. "Stabilization of the earth's obliquity by the moon," Nature, 361, 615-617, July 1993. (Link abstract on-line). Necessity of Moon for stable obliquity considered.
  • Raymond et al. (2014). “Terrestrial Planet Formation at Home and Abroad”. Protostars and Planets VI (University of Arizona Press): p.595-618. Bibcode: 2014prpl.conf..595R. 

adsbit.harvard.edu

  • Wiegert, Paul A., and Matt J. Holman. "The stability of planets in the Alpha Centauri system," The Astronomical Journal vol. 113, no. 4, April 1997 (Link). Potentially stable orbits and habitable zones around Alpha Centauri A and B.

jmu.edu (Global: low place; Japanese: low place)

csmres.jmu.edu

kencroswell.com (Global: low place; Japanese: low place)

nasa.gov (Global: 75th place; Japanese: 171st place)

nature.com (Global: 234th place; Japanese: 363rd place)

  • Williams, Darren M., James F. Kasting, and Richard A. Wade. "Habitable moons around extrasolar giant planets," Nature, 385, 234-236, January 1997. (Link abstract on-line). Habitability of moons within the HZ considered.

nih.gov (Global: 4th place; Japanese: 24th place)

ncbi.nlm.nih.gov

  • Kasting, J.F.（英語版）, D.C.B. Whittet, and W.R. Sheldon. "Ultraviolet radiation from F and K stars and implications for planetary habitability," Origins of Life, 27, 413-420, August 1997. (Link abstract on-line). Radiation by spectral type considered.

pnas.org (Global: 1,293rd place; Japanese: 1,250th place)

  • Lunine, Jonathon I. "The occurrence of Jovian planets and the habitability of planetary systems," Proceedings of the National Academy of Science vol. 98, no. 3, 809-814, January 30, 2001 (Link). The role of Jupiter in seeding the early Earth.

psu.edu (Global: 207th place; Japanese: 1,812th place)

geosc.psu.edu

  • Kasting, J.F., D.P. Whitmore, R.T. Reynolds. "Habitable Zones Around Main Sequence Stars," Icarus 101, 108-128, 1993. (Link Archived 2009年3月18日, at the Wayback Machine. (PDF) ). Detailed overview of habitable zone estimates.

psu.edu

solstation.com (Global: low place; Japanese: low place)

ucsd.edu (Global: 1,933rd place; Japanese: 6,680th place)

exobio.ucsd.edu

unr.edu (Global: low place; Japanese: low place)

quake.seismo.unr.edu

  • Joshi, M.M., R. M. Haberle, and R. T. Reynolds. "Simulations of the Atmospheres of Synchronously Rotating Terrestrial Planets Orbiting M Dwarfs: Conditions for Atmospheric Collapse and the Implications for Habitability," Icarus, 129, 450–465, 1997 (Link (PDF) ). Analysis and modelling of atmospheric pressure on planets in Red Dwarf systems.

uoregon.edu (Global: 3,144th place; Japanese: 8,971st place)

zebu.uoregon.edu

upr.edu (Global: low place; Japanese: low place)

phl.upr.edu

utexas.edu (Global: 916th place; Japanese: 2,207th place)

as.utexas.edu

  • Heath, Martin J., Laurance R. Doyle, Manoj M. Joshi, and Robert M. Haberle. "Habitability of Planets Around Red Dwarf Stars," Origins of Life and Evolution of the Biosphere, vol. 29, no. 4, 405-424, 1999 (Link (PDF) ). Water cycle, photosynthetic radiation, and the affect of flares on planets in Red Dwarf systems.

washington.edu (Global: 1,067th place; Japanese: 2,947th place)

atmos.washington.edu

washington.edu

web.archive.org (Global: 1st place; Japanese: 1st place)

wikipedia.org (Global: low place; Japanese: low place)

en.wikipedia.org

  • Evolving the Alienの中で、ジャック・コーエン（英語版）とイアン・スチュアートは、生命が木星型惑星の雲の上で形成されるかもしれない、もっともらしいシナリオを評価した。同様に、カール・セーガンは金星の雲が生命を宿すかもしれないことを示唆した。
  • 近年では、特に、地球上のかつて生命に適さないと考えられていた環境で極限環境微生物が栄えているのが知られるようになってからは、単細胞生物は宇宙の中でありふれた存在であるかもしれない、という認識が少しずつ広まりつつある。複雑な多細胞の生命が発生する可能性については、まだ非常に多くの議論が残っている。ピーター・ウォード（英語版）とドナルド・ブラウンリー（英語版）のRare Earth: Why Complex Life Is Uncommon in the Universeでは、微生物は広範囲に存在するが複雑な生命はとても稀で、おそらく地球特有のものだろうと主張している。地球の歴史に関する現在の知識は、この理論を部分的に支持する。多細胞生物は、生命誕生後30億年以上たった先カンブリア時代の終り頃に現れたと信じられている。地球生命が長い間単細胞のままだったことは、複雑な生物への決定的な一歩は必然的に起こるものではない、ということを強調するものである。近年では、全地球規模の寒冷化が多細胞生物への進化のきっかけになったという説も有力視されつつある。
  • Kasting, J.F.（英語版）, D.C.B. Whittet, and W.R. Sheldon. "Ultraviolet radiation from F and K stars and implications for planetary habitability," Origins of Life, 27, 413-420, August 1997. (Link abstract on-line). Radiation by spectral type considered.