Pontos de Lagrange (Portuguese Wikipedia)

Analysis of information sources in references of the Wikipedia article "Pontos de Lagrange" in Portuguese language version.

refsWebsite

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10harvard.edu

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8doi.org

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1minorplanetcenter.org

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1mit.edu

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1arizona.edu

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1archives-ouvertes.fr

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1b612foundation.org

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1phys.org

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archive-it.org

wayback.archive-it.org

«L2 Orbit». Space Telescope Science Institute. Consultado em 28 de agosto de 2016. Arquivado do original em 3 de fevereiro de 2014

archives-ouvertes.fr

hal.archives-ouvertes.fr

Tantardini, Marco; Fantino, Elena; Ren, Yuan; Pergola, Pierpaolo; Gómez, Gerard; Masdemont, Josep J. (2010). «Spacecraft trajectories to the L₃ point of the Sun–Earth three-body problem» (PDF). Celestial Mechanics and Dynamical Astronomy. 108 (3): 215–232. Bibcode:2010CeMDA.108..215T. doi:10.1007/s10569-010-9299-x

arizona.edu

math.arizona.edu

Cacolici, Gianna Nicole, et al., "Stability of Lagrange Points: James Webb Space Telescope", University of Arizona. Retrieved 17 Sept. 2018.

arxiv.org

Hui, Man-To; Wiegert, Paul A.; Tholen, David J.; Föhring, Dora (novembro 2021). «The Second Earth Trojan 2020 XL5». The Astrophysical Journal Letters. 922 (2): L25. Bibcode:2021ApJ...922L..25H. arXiv:2111.05058. doi:10.3847/2041-8213/ac37bf
Slíz-Balogh, Judit; Barta, András; Horváth, Gábor (2018). «Celestial mechanics and polarization optics of the Kordylewski dust cloud in the Earth-Moon Lagrange point L5 - Part I. Three-dimensional celestial mechanical modelling of dust cloud formation». Monthly Notices of the Royal Astronomical Society. 480 (4): 5550–5559. Bibcode:2018MNRAS.480.5550S. arXiv:1910.07466. doi:10.1093/mnras/sty2049
Slíz-Balogh, Judit; Barta, András; Horváth, Gábor (2019). «Celestial mechanics and polarization optics of the Kordylewski dust cloud in the Earth-Moon Lagrange point L5. Part II. Imaging polarimetric observation: new evidence for the existence of Kordylewski dust cloud». Monthly Notices of the Royal Astronomical Society. 482 (1): 762–770. Bibcode:2019MNRAS.482..762S. arXiv:1910.07471. doi:10.1093/mnras/sty2630
Belbruno, E.; Gott III, J. Richard (2005). «Where Did The Moon Come From?». The Astronomical Journal. 129 (3): 1724–1745. Bibcode:2005AJ....129.1724B. arXiv:astro-ph/0405372. doi:10.1086/427539
Seidov, Zakir F. (1 de março de 2004). «The Roche Problem: Some Analytics». The Astrophysical Journal. 603 (1): 283–284. Bibcode:2004ApJ...603..283S. arXiv:astro-ph/0311272. doi:10.1086/381315

b612foundation.org

«The Sentinel Mission». B612 Foundation. Consultado em 1 de fevereiro de 2014. Arquivado do original em 30 de junho de 2012

bnf.fr

gallica.bnf.fr

Lagrange, Joseph-Louis (1867–1892). «Tome 6, Chapitre II: Essai sur le problème des trois corps». Œuvres de Lagrange (em francês). [S.l.]: Gauthier-Villars. pp. 229–334

caltech.edu

cds.caltech.edu

Koon, W. S.; Lo, M. W.; Marsden, J. E.; Ross, S. D. (2006). Dynamical Systems, the Three-Body Problem, and Space Mission Design. [S.l.: s.n.] p. 9. Consultado em 9 de junho de 2008. Arquivado do original em 27 de maio de 2008 (16MB)

cornell.edu

math.cornell.edu

Greenspan, Thomas (7 de janeiro de 2014). «Stability of the Lagrange Points, L4 and L5» (PDF). Consultado em 28 de fevereiro de 2018. Arquivado do original (PDF) em 18 de abril de 2018

dartmouth.edu

math.dartmouth.edu

Euler, Leonhard (1765). De motu rectilineo trium corporum se mutuo attrahentium (PDF). [S.l.: s.n.]

doi.org

dx.doi.org

Hui, Man-To; Wiegert, Paul A.; Tholen, David J.; Föhring, Dora (novembro 2021). «The Second Earth Trojan 2020 XL5». The Astrophysical Journal Letters. 922 (2): L25. Bibcode:2021ApJ...922L..25H. arXiv:2111.05058. doi:10.3847/2041-8213/ac37bf
Slíz-Balogh, Judit; Barta, András; Horváth, Gábor (2018). «Celestial mechanics and polarization optics of the Kordylewski dust cloud in the Earth-Moon Lagrange point L5 - Part I. Three-dimensional celestial mechanical modelling of dust cloud formation». Monthly Notices of the Royal Astronomical Society. 480 (4): 5550–5559. Bibcode:2018MNRAS.480.5550S. arXiv:1910.07466. doi:10.1093/mnras/sty2049
Slíz-Balogh, Judit; Barta, András; Horváth, Gábor (2019). «Celestial mechanics and polarization optics of the Kordylewski dust cloud in the Earth-Moon Lagrange point L5. Part II. Imaging polarimetric observation: new evidence for the existence of Kordylewski dust cloud». Monthly Notices of the Royal Astronomical Society. 482 (1): 762–770. Bibcode:2019MNRAS.482..762S. arXiv:1910.07471. doi:10.1093/mnras/sty2630
Freitas, Robert; Valdes, Francisco (1980). «A Search for Natural or Artificial Objects Located at the Earth–Moon Libration Points». Icarus. 42 (3): 442–447. Bibcode:1980Icar...42..442F. doi:10.1016/0019-1035(80)90106-2
Belbruno, E.; Gott III, J. Richard (2005). «Where Did The Moon Come From?». The Astronomical Journal. 129 (3): 1724–1745. Bibcode:2005AJ....129.1724B. arXiv:astro-ph/0405372. doi:10.1086/427539
Seidov, Zakir F. (1 de março de 2004). «The Roche Problem: Some Analytics». The Astrophysical Journal. 603 (1): 283–284. Bibcode:2004ApJ...603..283S. arXiv:astro-ph/0311272. doi:10.1086/381315
Pitjeva, E.V.; Standish, E.M. (1 de abril de 2009). «Proposals for the masses of the three largest asteroids, the Moon-Earth mass ratio and the Astronomical Unit». Celestial Mechanics and Dynamical Astronomy. 103 (4): 365–372. Bibcode:2009CeMDA.103..365P. doi:10.1007/s10569-009-9203-8
Tantardini, Marco; Fantino, Elena; Ren, Yuan; Pergola, Pierpaolo; Gómez, Gerard; Masdemont, Josep J. (2010). «Spacecraft trajectories to the L₃ point of the Sun–Earth three-body problem» (PDF). Celestial Mechanics and Dynamical Astronomy. 108 (3): 215–232. Bibcode:2010CeMDA.108..215T. doi:10.1007/s10569-010-9299-x

esa.int

ideas.esa.int

Hornig, Andreas (1 de maio de 2022). «TYCHO: Supporting Permanently Crewed Lunar Exploration with High-Speed Optical Communication from Everywhere». ESA

harvard.edu

ui.adsabs.harvard.edu

Hui, Man-To; Wiegert, Paul A.; Tholen, David J.; Föhring, Dora (novembro 2021). «The Second Earth Trojan 2020 XL5». The Astrophysical Journal Letters. 922 (2): L25. Bibcode:2021ApJ...922L..25H. arXiv:2111.05058. doi:10.3847/2041-8213/ac37bf
Slíz-Balogh, Judit; Barta, András; Horváth, Gábor (2018). «Celestial mechanics and polarization optics of the Kordylewski dust cloud in the Earth-Moon Lagrange point L5 - Part I. Three-dimensional celestial mechanical modelling of dust cloud formation». Monthly Notices of the Royal Astronomical Society. 480 (4): 5550–5559. Bibcode:2018MNRAS.480.5550S. arXiv:1910.07466. doi:10.1093/mnras/sty2049
Slíz-Balogh, Judit; Barta, András; Horváth, Gábor (2019). «Celestial mechanics and polarization optics of the Kordylewski dust cloud in the Earth-Moon Lagrange point L5. Part II. Imaging polarimetric observation: new evidence for the existence of Kordylewski dust cloud». Monthly Notices of the Royal Astronomical Society. 482 (1): 762–770. Bibcode:2019MNRAS.482..762S. arXiv:1910.07471. doi:10.1093/mnras/sty2630
Freitas, Robert; Valdes, Francisco (1980). «A Search for Natural or Artificial Objects Located at the Earth–Moon Libration Points». Icarus. 42 (3): 442–447. Bibcode:1980Icar...42..442F. doi:10.1016/0019-1035(80)90106-2
Belbruno, E.; Gott III, J. Richard (2005). «Where Did The Moon Come From?». The Astronomical Journal. 129 (3): 1724–1745. Bibcode:2005AJ....129.1724B. arXiv:astro-ph/0405372. doi:10.1086/427539
Seidov, Zakir F. (1 de março de 2004). «The Roche Problem: Some Analytics». The Astrophysical Journal. 603 (1): 283–284. Bibcode:2004ApJ...603..283S. arXiv:astro-ph/0311272. doi:10.1086/381315
Pitjeva, E.V.; Standish, E.M. (1 de abril de 2009). «Proposals for the masses of the three largest asteroids, the Moon-Earth mass ratio and the Astronomical Unit». Celestial Mechanics and Dynamical Astronomy. 103 (4): 365–372. Bibcode:2009CeMDA.103..365P. doi:10.1007/s10569-009-9203-8
Tantardini, Marco; Fantino, Elena; Ren, Yuan; Pergola, Pierpaolo; Gómez, Gerard; Masdemont, Josep J. (2010). «Spacecraft trajectories to the L₃ point of the Sun–Earth three-body problem» (PDF). Celestial Mechanics and Dynamical Astronomy. 108 (3): 215–232. Bibcode:2010CeMDA.108..215T. doi:10.1007/s10569-010-9299-x
Kordylewski, K. (1961). «Photographische Untersuchungen des Librationspunktes L5 im System Erde-Mond». Acta Astronomica, Vol. 11, p.165. 11. p. 165. Bibcode:1961AcA....11..165K

adsabs.harvard.edu

Kordylewski, K. (1961). «Photographische Untersuchungen des Librationspunktes L5 im System Erde-Mond». Acta Astronomica, Vol. 11, p.165. 11. p. 165. Bibcode:1961AcA....11..165K

minorplanetcenter.org

«List Of Neptune Trojans». Minor Planet Center. Consultado em 27 de outubro de 2010. Cópia arquivada em 25 de julho de 2011

mit.edu

ocw.mit.edu

«Widnall, Lecture L18 - Exploring the Neighborhood: the Restricted Three-Body Problem» (PDF)

montana.edu

physics.montana.edu

Cornish, Neil J. (1998). «The Lagrange Points» (PDF). WMAP Education and Outreach. Consultado em 15 de dezembro de 2015. Arquivado do original (PDF) em 7 de setembro de 2015

moontoday.net

SMART-1: On Course for Lunar Capture | Moon Today – Your Daily Source of Moon News Arquivado em 2005-11-02 no Wayback Machine

nasa.gov

solarsystem.nasa.gov

«DSCOVR: In-Depth». NASA Solar System Exploration. NASA. Consultado em 27 de outubro de 2021
«ISEE-3/ICE». Solar System Exploration. NASA. Consultado em 8 de agosto de 2015. Arquivado do original em 20 de julho de 2015

webb.nasa.gov

«About Orbit». NASA. Consultado em 1 de janeiro de 2022

wmap.gsfc.nasa.gov

«The Lagrange Points» (PDF). NASA. 1998 , Neil J. Cornish, with input from Jeremy Goodman

nasa.gov

«NASA - NASA's Wise Mission Finds First Trojan Asteroid Sharing Earth's Orbit». www.nasa.gov

oeis.org

Na verdade (25 + 3√69)/2 ≈ 7001249599357944000♠24.9599357944 (sequência A230242 na OEIS)

phys.org

«NASA proposes a magnetic shield to protect Mars' atmosphere». phys.org

rfreitas.com

Freitas, Robert; Valdes, Francisco (1980). «A Search for Natural or Artificial Objects Located at the Earth–Moon Libration Points». Icarus. 42 (3): 442–447. Bibcode:1980Icar...42..442F. doi:10.1016/0019-1035(80)90106-2

space.com

Choi 2011-07-27T17:06:00Z, Charles Q. (27 de julho de 2011). «First Asteroid Companion of Earth Discovered at Last». Space.com

spacenews.com

Jones, Andrew (14 de junho de 2018). «Chang'e-4 relay satellite enters halo orbit around Earth-Moon L2, microsatellite in lunar orbit». SpaceNews
«B612 studying smallsat missions to search for near Earth objects». SpaceNews.com. 20 de junho de 2017

stsci.edu

«L2 Orbit». Space Telescope Science Institute. Consultado em 28 de agosto de 2016. Arquivado do original em 3 de fevereiro de 2014

ulalaunch.com

Zegler, Frank; Kutter, Bernard (2 de setembro de 2010). «Evolving to a Depot-Based Space Transportation Architecture» (PDF). AIAA SPACE 2010 Conference & Exposition. AIAA. p. 4. Consultado em 25 de janeiro de 2011. Arquivado do original (PDF) em 24 de junho de 2014. L₂ is in deep space far away from any planetary surface and hence the thermal, micrometeoroid, and atomic oxygen environments are vastly superior to those in LEO. Thermodynamic stasis and extended hardware life are far easier to obtain without these punishing conditions seen in LEO. L₂ is not just a great gateway—it is a great place to store propellants. ... L₂ is an ideal location to store propellants and cargos: it is close, high energy, and cold. More importantly, it allows the continuous onward movement of propellants from LEO depots, thus suppressing their size and effectively minimizing the near-Earth boiloff penalties.

utexas.edu

farside.ph.utexas.edu

Fitzpatrick, Richard. «Stability of Lagrange Points». Newtonian Dynamics. University of Texas

web.archive.org

Cornish, Neil J. (1998). «The Lagrange Points» (PDF). WMAP Education and Outreach. Consultado em 15 de dezembro de 2015. Arquivado do original (PDF) em 7 de setembro de 2015
Koon, W. S.; Lo, M. W.; Marsden, J. E.; Ross, S. D. (2006). Dynamical Systems, the Three-Body Problem, and Space Mission Design. [S.l.: s.n.] p. 9. Consultado em 9 de junho de 2008. Arquivado do original em 27 de maio de 2008 (16MB)
«List Of Neptune Trojans». Minor Planet Center. Consultado em 27 de outubro de 2010. Cópia arquivada em 25 de julho de 2011
Greenspan, Thomas (7 de janeiro de 2014). «Stability of the Lagrange Points, L4 and L5» (PDF). Consultado em 28 de fevereiro de 2018. Arquivado do original (PDF) em 18 de abril de 2018
«ISEE-3/ICE». Solar System Exploration. NASA. Consultado em 8 de agosto de 2015. Arquivado do original em 20 de julho de 2015
SMART-1: On Course for Lunar Capture | Moon Today – Your Daily Source of Moon News Arquivado em 2005-11-02 no Wayback Machine
Zegler, Frank; Kutter, Bernard (2 de setembro de 2010). «Evolving to a Depot-Based Space Transportation Architecture» (PDF). AIAA SPACE 2010 Conference & Exposition. AIAA. p. 4. Consultado em 25 de janeiro de 2011. Arquivado do original (PDF) em 24 de junho de 2014. L₂ is in deep space far away from any planetary surface and hence the thermal, micrometeoroid, and atomic oxygen environments are vastly superior to those in LEO. Thermodynamic stasis and extended hardware life are far easier to obtain without these punishing conditions seen in LEO. L₂ is not just a great gateway—it is a great place to store propellants. ... L₂ is an ideal location to store propellants and cargos: it is close, high energy, and cold. More importantly, it allows the continuous onward movement of propellants from LEO depots, thus suppressing their size and effectively minimizing the near-Earth boiloff penalties.
«The Sentinel Mission». B612 Foundation. Consultado em 1 de fevereiro de 2014. Arquivado do original em 30 de junho de 2012

wolfram.com

scienceworld.wolfram.com

Weisstein, Eric. «Lagrange Points». Eric Weisstein's World of Physics

youtube.com

Hornig, Andreas (6 de outubro de 2013). «TYCHO mission to Earth-Moon libration point EML-4 @ IAC 2013». IAC2013

zenodo.org

Pitjeva, E.V.; Standish, E.M. (1 de abril de 2009). «Proposals for the masses of the three largest asteroids, the Moon-Earth mass ratio and the Astronomical Unit». Celestial Mechanics and Dynamical Astronomy. 103 (4): 365–372. Bibcode:2009CeMDA.103..365P. doi:10.1007/s10569-009-9203-8