센타우루스자리 프록시마 (Korean Wikipedia)

Analysis of information sources in references of the Wikipedia article "센타우루스자리 프록시마" in Korean language version.

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aanda.org (Global: 5,591st place; Korean: 2,411th place)

archive.org (Global: 6th place; Korean: 18th place)

arxiv.org (Global: 69th place; Korean: 54th place)

books.google.com (Global: 3rd place; Korean: 9th place)

  • 천정보다 남쪽에 있는 항성이 천정과 이루는 각도는 '위도 − 적위'이다. 항성은 천정과 이루는 각도가 90도 이상일 경우 시야에서 사라진다.(지평선 아래로 내려간다는 뜻임) 센타우루스자리 프록시마의 경우 이 별을 볼 수 있는 최고 위도는
    90° + −62.68° = 27.32°이다.
    참고: Campbell, William Wallace (1899). 《The elements of practical astronomy》. London: Macmillan. 109–110쪽. 2008년 8월 12일에 확인함. 

doi.org (Global: 2nd place; Korean: 3rd place)

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eso.org (Global: 3,034th place; Korean: 1,210th place)

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nasa.gov (Global: 75th place; Korean: 67th place)

solarsystem.nasa.gov

  • 밀도(ρ)는 질량을 부피로 나눈 값이다. 따라서 태양의 밀도를 이용하여 구한 프록시마의 밀도는 다음과 같다.
    =
    = 0.122 · 0.154−3 · (1.41 × 103 kg/m3)
    = 33.4 · (1.41 × 103 kg/m3)
    = 4.71 × 104 kg/m3

    이 식에서 는 태양의 평균 밀도이다. 다음 문헌을 참고할 것.

    • Munsell, Kirk; Smith, Harman; Davis, Phil; Harvey, Samantha (2008년 6월 11일). “Sun: facts & figures”. 《Solar system exploration》. NASA. 2008년 1월 2일에 원본 문서에서 보존된 문서. 2008년 7월 12일에 확인함. 

    nssdc.gsfc.nasa.gov

    • Williams, D. R. (2006년 2월 10일). “Moon Fact Sheet”. Lunar & Planetary Science. NASA. 2010년 3월 23일에 원본 문서에서 보존된 문서. 2007년 10월 12일에 확인함. 

    ntrs.nasa.gov

nationalgeographic.com (Global: 344th place; Korean: 269th place)

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  • Adams, Fred C.; Laughlin, Gregory; Graves, Genevieve J. M. 《Red dwarfs and the end of the main sequence》 (PDF). 《Gravitational collapse: from massive stars to planets》 (Revista Mexicana de Astronomía y Astrofísica). 46–49쪽. 2019년 7월 11일에 원본 문서 (PDF)에서 보존된 문서. 2008년 6월 24일에 확인함. 

unizar.es (Global: low place; Korean: low place)

zaguan.unizar.es

  • Anglada, Guillem; Amado, Pedro J; Ortiz, Jose L; Gómez, José F; Macías, Enrique; Alberdi, Antxon; Osorio, Mayra; Gómez, José L; Itziar de Gregorio-Monsalvo; Pérez-Torres, Miguel A; Anglada-Escudé, Guillem; Berdiñas, Zaira M; Jenkins, James S; Jimenez-Serra, Izaskun; Lara, Luisa M; López-González, Maria J; López-Puertas, Manuel; Morales, Nicolas; Ribas, Ignasi; Richards, Anita M. S; Rodríguez-López, Cristina; Rodriguez, Eloy (2017). “ALMA Discovery of Dust Belts Around Proxima Centauri”. 《The Astrophysical Journal》 850 (1): L6. arXiv:1711.00578. Bibcode:2017ApJ...850L...6A. doi:10.3847/2041-8213/aa978b. 

utexas.edu (Global: 916th place; Korean: 819th place)

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washingtonpost.com (Global: 34th place; Korean: 124th place)

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

  • 밀도(ρ)는 질량을 부피로 나눈 값이다. 따라서 태양의 밀도를 이용하여 구한 프록시마의 밀도는 다음과 같다.
    =
    = 0.122 · 0.154−3 · (1.41 × 103 kg/m3)
    = 33.4 · (1.41 × 103 kg/m3)
    = 4.71 × 104 kg/m3

    이 식에서 는 태양의 평균 밀도이다. 다음 문헌을 참고할 것.

worldcat.org (Global: 5th place; Korean: 11th place)

youtube.com (Global: 9th place; Korean: 20th place)

zenodo.org (Global: 621st place; Korean: 732nd place)