Fermi paradox (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Fermi paradox" in English language version.

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archive.org

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astrobiology.com

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berkeley.edu

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britannica.com

  • "Star (astronomy)". Encyclopædia Britannica. Archived from the original on March 1, 2016. Retrieved February 4, 2016. "With regard to mass, size, and intrinsic brightness, the Sun is a typical star." Technically, the sun is near the middle of the main sequence of the Hertzsprung–Russell diagram. This sequence contains 80–90% of the stars of the galaxy. [1] Archived July 16, 2011, at the Wayback Machine

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  • "The Great Silence: the Controversy . . . " (15-page paper), Quarterly J. Royal Astron. Soc., David Brin, 1983, page 301 second-to-last paragraph Archived May 3, 2020, at the Wayback Machine. Brin cites, The Prehistory of Polynesia, edited by J. Jennings, Harvard University Press, 1979. See also Interstellar Migration and the Human Experience, edited by Ben Finney and Eric M. Jones, Ch. 13 "Life (With All Its Problems) in Space" by Alfred W. Crosby, University of California Press, 1985.

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insider.com

  • Woodward, Avlin (September 21, 2019). "A winner of this year's Nobel prize in physics is convinced we'll detect alien life in 100 years. Here are 13 reasons why we haven't made contact yet". Insider Inc. Retrieved September 21, 2019.

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kepler.nasa.gov

  • From "Kepler: About the Mission". NASA. March 31, 2015. Archived from the original on April 20, 2012. Retrieved March 30, 2016. "The Kepler Mission, NASA Discovery mission #10, is specifically designed to survey a portion of our region of the Milky Way galaxy to discover dozens of Earth-size planets in or near the habitable zone and determine how many of the billions of stars in our galaxy have such planets."

acdb-ext.gsfc.nasa.gov

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space.com

springer.com

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techcrunch.com

technologyreview.com

  • Bostrom, Nick (April 22, 2008). "Where Are They?". MIT Technology Review. Retrieved October 5, 2020.

theatlantic.com

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astro.unl.edu

  • "Star (astronomy)". Encyclopædia Britannica. Archived from the original on March 1, 2016. Retrieved February 4, 2016. "With regard to mass, size, and intrinsic brightness, the Sun is a typical star." Technically, the sun is near the middle of the main sequence of the Hertzsprung–Russell diagram. This sequence contains 80–90% of the stars of the galaxy. [1] Archived July 16, 2011, at the Wayback Machine

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