Lagrange point (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Lagrange point" in English language version.

refsWebsite

Global rank English rank

11harvard.edu

18^th place

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9doi.org

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8web.archive.org

1^st place

6arxiv.org

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6semanticscholar.org

11^th place

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5nasa.gov

75^th place

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2spacenews.com

1,876^th place

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1oeis.org

742^nd place

538^th place

1montana.edu

7,206^th place

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1wolfram.com

513^th place

537^th place

1caltech.edu

887^th place

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1dartmouth.edu

2,242^nd place

1,513^th place

1bnf.fr

124^th place

544^th place

1archive-it.org

910^th place

593^rd place

1stsci.edu

low place

1space.com

936^th place

713^th place

1rfreitas.com

low place

1minorplanetcenter.org

low place

1mit.edu

415^th place

327^th place

1utexas.edu

916^th place

706^th place

1cornell.edu

332^nd place

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1zenodo.org

621^st place

380^th place

1arizona.edu

1,592^nd place

1,119^th place

1archives-ouvertes.fr

1,031^st place

879^th place

1moontoday.net

low place

1ulalaunch.com

low place

1esa.int

1,482^nd place

1,468^th place

1youtube.com

9^th place

13^th place

1b612foundation.org

low place

1phys.org

1,283^rd place

1,130^th place

archive-it.org

wayback.archive-it.org

"L2 Orbit". Space Telescope Science Institute. Archived from the original on 3 February 2014. Retrieved 28 August 2016.

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. S2CID 121179935.

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 (November 2021). "The Second Earth Trojan 2020 XL5". The Astrophysical Journal Letters. 922 (2): L25. arXiv:2111.05058. Bibcode:2021ApJ...922L..25H. doi:10.3847/2041-8213/ac37bf. S2CID 243860678.
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. arXiv:1910.07466. Bibcode:2018MNRAS.480.5550S. 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. arXiv:1910.07471. Bibcode:2019MNRAS.482..762S. doi:10.1093/mnras/sty2630.
Belbruno, Edward; Gott III, J. Richard (2005). "Where Did The Moon Come From?". The Astronomical Journal. 129 (3): 1724–1745. arXiv:astro-ph/0405372. Bibcode:2005AJ....129.1724B. doi:10.1086/427539. S2CID 12983980.
Sepinsky, Jeremy F.; Willems, Bart; Kalogera, Vicky (May 2007). "Equipotential Surfaces and Lagrangian Points in Nonsynchronous, Eccentric Binary and Planetary Systems". The Astrophysical Journal. 660 (2): 1624–1635. arXiv:astro-ph/0612508. Bibcode:2007ApJ...660.1624S. doi:10.1086/513736. S2CID 15519581.
Seidov, Zakir F. (March 1, 2004). "The Roche Problem: Some Analytics". The Astrophysical Journal. 603 (1): 283–284. arXiv:astro-ph/0311272. Bibcode:2004ApJ...603..283S. doi:10.1086/381315. S2CID 16724058.

b612foundation.org

"The Sentinel Mission". B612 Foundation. Archived from the original on 30 June 2012. Retrieved 1 February 2014.

bnf.fr

gallica.bnf.fr

Lagrange, Joseph-Louis (1867–92). "Tome 6, Chapitre II: Essai sur le problème des trois corps". Œuvres de Lagrange (in French). Gauthier-Villars. pp. 229–334.

caltech.edu

cds.caltech.edu

Koon, Wang Sang; Lo, Martin W.; Marsden, Jerrold E.; Ross, Shane D. (2006). Dynamical Systems, the Three-Body Problem, and Space Mission Design. p. 9. Archived from the original on 2008-05-27. Retrieved 2008-06-09. (16MB)

cornell.edu

math.cornell.edu

Greenspan, Thomas (January 7, 2014). "Stability of the Lagrange Points, L4 and L5" (PDF). Archived from the original (PDF) on April 18, 2018. Retrieved February 28, 2018.

dartmouth.edu

math.dartmouth.edu

Euler, Leonhard (1765). De motu rectilineo trium corporum se mutuo attrahentium (PDF).

doi.org

Hui, Man-To; Wiegert, Paul A.; Tholen, David J.; Föhring, Dora (November 2021). "The Second Earth Trojan 2020 XL5". The Astrophysical Journal Letters. 922 (2): L25. arXiv:2111.05058. Bibcode:2021ApJ...922L..25H. doi:10.3847/2041-8213/ac37bf. S2CID 243860678.
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. arXiv:1910.07466. Bibcode:2018MNRAS.480.5550S. 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. arXiv:1910.07471. Bibcode:2019MNRAS.482..762S. 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, Edward; Gott III, J. Richard (2005). "Where Did The Moon Come From?". The Astronomical Journal. 129 (3): 1724–1745. arXiv:astro-ph/0405372. Bibcode:2005AJ....129.1724B. doi:10.1086/427539. S2CID 12983980.
Sepinsky, Jeremy F.; Willems, Bart; Kalogera, Vicky (May 2007). "Equipotential Surfaces and Lagrangian Points in Nonsynchronous, Eccentric Binary and Planetary Systems". The Astrophysical Journal. 660 (2): 1624–1635. arXiv:astro-ph/0612508. Bibcode:2007ApJ...660.1624S. doi:10.1086/513736. S2CID 15519581.
Seidov, Zakir F. (March 1, 2004). "The Roche Problem: Some Analytics". The Astrophysical Journal. 603 (1): 283–284. arXiv:astro-ph/0311272. Bibcode:2004ApJ...603..283S. doi:10.1086/381315. S2CID 16724058.
Pitjeva, Elena V.; Standish, E. Myles (2009-04-01). "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. S2CID 121374703.
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. S2CID 121179935.

esa.int

ideas.esa.int

Hornig, Andreas (2022-05-01). "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 (November 2021). "The Second Earth Trojan 2020 XL5". The Astrophysical Journal Letters. 922 (2): L25. arXiv:2111.05058. Bibcode:2021ApJ...922L..25H. doi:10.3847/2041-8213/ac37bf. S2CID 243860678.
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. arXiv:1910.07466. Bibcode:2018MNRAS.480.5550S. 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. arXiv:1910.07471. Bibcode:2019MNRAS.482..762S. 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, Edward; Gott III, J. Richard (2005). "Where Did The Moon Come From?". The Astronomical Journal. 129 (3): 1724–1745. arXiv:astro-ph/0405372. Bibcode:2005AJ....129.1724B. doi:10.1086/427539. S2CID 12983980.
Sepinsky, Jeremy F.; Willems, Bart; Kalogera, Vicky (May 2007). "Equipotential Surfaces and Lagrangian Points in Nonsynchronous, Eccentric Binary and Planetary Systems". The Astrophysical Journal. 660 (2): 1624–1635. arXiv:astro-ph/0612508. Bibcode:2007ApJ...660.1624S. doi:10.1086/513736. S2CID 15519581.
Seidov, Zakir F. (March 1, 2004). "The Roche Problem: Some Analytics". The Astrophysical Journal. 603 (1): 283–284. arXiv:astro-ph/0311272. Bibcode:2004ApJ...603..283S. doi:10.1086/381315. S2CID 16724058.
Pitjeva, Elena V.; Standish, E. Myles (2009-04-01). "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. S2CID 121374703.
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. S2CID 121179935.
Kordylewski, Kazimierz (1961). "Photographische Untersuchungen des Librationspunktes L₅ im System Erde-Mond". Acta Astronomica, Vol. 11, p.165. Vol. 11. p. 165. Bibcode:1961AcA....11..165K.

adsabs.harvard.edu

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

minorplanetcenter.org

"List Of Neptune Trojans". Minor Planet Center. Archived from the original on 2011-07-25. Retrieved 2010-10-27.

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. Archived from the original (PDF) on September 7, 2015. Retrieved 15 Dec 2015.

moontoday.net

SMART-1: On Course for Lunar Capture | Moon Today – Your Daily Source of Moon News Archived 2 November 2005 at the Wayback Machine

nasa.gov

solarsystem.nasa.gov

"DSCOVR: In-Depth". NASA Solar System Exploration. NASA. Retrieved 2021-10-27.
"ISEE-3/ICE". Solar System Exploration. NASA. Archived from the original on July 20, 2015. Retrieved August 8, 2015.

webb.nasa.gov

"About Orbit". NASA. Retrieved 2022-01-01.

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

Actually 25 + 3√69/2 ≈ 24.9599357944 (sequence A230242 in the 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.

semanticscholar.org

api.semanticscholar.org

Hui, Man-To; Wiegert, Paul A.; Tholen, David J.; Föhring, Dora (November 2021). "The Second Earth Trojan 2020 XL5". The Astrophysical Journal Letters. 922 (2): L25. arXiv:2111.05058. Bibcode:2021ApJ...922L..25H. doi:10.3847/2041-8213/ac37bf. S2CID 243860678.
Belbruno, Edward; Gott III, J. Richard (2005). "Where Did The Moon Come From?". The Astronomical Journal. 129 (3): 1724–1745. arXiv:astro-ph/0405372. Bibcode:2005AJ....129.1724B. doi:10.1086/427539. S2CID 12983980.
Sepinsky, Jeremy F.; Willems, Bart; Kalogera, Vicky (May 2007). "Equipotential Surfaces and Lagrangian Points in Nonsynchronous, Eccentric Binary and Planetary Systems". The Astrophysical Journal. 660 (2): 1624–1635. arXiv:astro-ph/0612508. Bibcode:2007ApJ...660.1624S. doi:10.1086/513736. S2CID 15519581.
Seidov, Zakir F. (March 1, 2004). "The Roche Problem: Some Analytics". The Astrophysical Journal. 603 (1): 283–284. arXiv:astro-ph/0311272. Bibcode:2004ApJ...603..283S. doi:10.1086/381315. S2CID 16724058.
Pitjeva, Elena V.; Standish, E. Myles (2009-04-01). "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. S2CID 121374703.
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. S2CID 121179935.

space.com

Choi, Charles Q. (27 July 2011). "First Asteroid Companion of Earth Discovered at Last". Space.com.

spacenews.com

Jones, Andrew (2018-06-14). "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. June 20, 2017.

stsci.edu

"L2 Orbit". Space Telescope Science Institute. Archived from the original on 3 February 2014. Retrieved 28 August 2016.

ulalaunch.com

Zegler, Frank; Kutter, Bernard (2010-09-02). "Evolving to a Depot-Based Space Transportation Architecture" (PDF). AIAA SPACE 2010 Conference & Exposition. AIAA. p. 4. Archived from the original (PDF) on 2014-06-24. Retrieved 2011-01-25. 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. Archived from the original (PDF) on September 7, 2015. Retrieved 15 Dec 2015.
Koon, Wang Sang; Lo, Martin W.; Marsden, Jerrold E.; Ross, Shane D. (2006). Dynamical Systems, the Three-Body Problem, and Space Mission Design. p. 9. Archived from the original on 2008-05-27. Retrieved 2008-06-09. (16MB)
"List Of Neptune Trojans". Minor Planet Center. Archived from the original on 2011-07-25. Retrieved 2010-10-27.
Greenspan, Thomas (January 7, 2014). "Stability of the Lagrange Points, L4 and L5" (PDF). Archived from the original (PDF) on April 18, 2018. Retrieved February 28, 2018.
"ISEE-3/ICE". Solar System Exploration. NASA. Archived from the original on July 20, 2015. Retrieved August 8, 2015.
SMART-1: On Course for Lunar Capture | Moon Today – Your Daily Source of Moon News Archived 2 November 2005 at the Wayback Machine
Zegler, Frank; Kutter, Bernard (2010-09-02). "Evolving to a Depot-Based Space Transportation Architecture" (PDF). AIAA SPACE 2010 Conference & Exposition. AIAA. p. 4. Archived from the original (PDF) on 2014-06-24. Retrieved 2011-01-25. 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. Archived from the original on 30 June 2012. Retrieved 1 February 2014.

wolfram.com

scienceworld.wolfram.com

Weisstein, Eric W. "Lagrange Points". Eric Weisstein's World of Physics.

youtube.com

Hornig, Andreas (2013-10-06). "TYCHO mission to Earth-Moon libration point EML-4 @ IAC 2013". IAC2013.

zenodo.org

Pitjeva, Elena V.; Standish, E. Myles (2009-04-01). "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. S2CID 121374703.