Órbita da Lua (Portuguese Wikipedia)
Analysis of information sources in references of the Wikipedia article "Órbita da Lua" in Portuguese language version.
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arxiv.org
- Kaveh Pahlevan & Alessandro Morbidelli (26 de novembro de 2015). «Collisionless encounters and the origin of the lunar inclination». Nature. 527 (7579): 492–494. Bibcode:2015Natur.527..492P. PMID 26607544. arXiv:1603.06515
. doi:10.1038/nature16137
books.google.com
- Lang, Kenneth R. (2011), The Cambridge Guide to the Solar System, 2nd ed., Cambridge University Press.
- The reference by H. L. Vacher (2001) (details separately cited in this list) describes this as 'convex outward', whereas older references such as "The Moon's Orbit Around the Sun, Turner, A. B. Journal of the Royal Astronomical Society of Canada, Vol. 6, p. 117, 1912JRASC...6..117T"; and "H Godfray, Elementary Treatise on the Lunar Theory" describe the same geometry by the words concave to the sun.
caltech.edu
media.caltech.edu
doi.org
dx.doi.org
- Martin C. Gutzwiller (1998). «Moon-Earth-Sun: The oldest three-body problem». Reviews of Modern Physics. 70 (2): 589–639. Bibcode:1998RvMP...70..589G. doi:10.1103/RevModPhys.70.589
- Peter Goldreich (novembro de 1966). «History of the Lunar Orbit». Reviews of Geophysics. 4 (4): 411. Bibcode:1966RvGSP...4..411G. doi:10.1029/RG004i004p00411 Jihad Touma & Jack Wisdom (novembro de 1994). «Evolution of the Earth-Moon system». The Astronomical Journal. 108: 1943. Bibcode:1994AJ....108.1943T. doi:10.1086/117209
- Kaveh Pahlevan & Alessandro Morbidelli (26 de novembro de 2015). «Collisionless encounters and the origin of the lunar inclination». Nature. 527 (7579): 492–494. Bibcode:2015Natur.527..492P. PMID 26607544. arXiv:1603.06515. doi:10.1038/nature16137
- Williams, James G.; Boggs, Dale H. (2016). «Secular tidal changes in lunar orbit and Earth rotation». Celestial Mechanics and Dynamical Astronomy (em inglês). 126 (1): 89–129. Bibcode:2016CeMDA.126...89W. ISSN 0923-2958. doi:10.1007/s10569-016-9702-3
- Williams, George E. (2000). «Geological constraints on the Precambrian history of Earth's rotation and the Moon's orbit». Reviews of Geophysics. 38 (1): 37–60. Bibcode:2000RvGeo..38...37W. doi:10.1029/1999RG900016
- Webb, David J. (1982). «Tides and the evolution of the Earth-Moon system». Geophysical Journal of the Royal Astronomical Society. 70 (1): 261–271. Bibcode:1982GeoJ...70..261W. doi:10.1111/j.1365-246X.1982.tb06404.x
harvard.edu
ui.adsabs.harvard.edu
- M. Chapront-Touzé; J. Chapront (1983). «The lunar ephemeris ELP-2000». Astronomy & Astrophysics. 124: 54. Bibcode:1983A&A...124...50C
- M. Chapront-Touzé; J. Chapront (1988). «ELP2000-85: a semi-analytical lunar ephemeris adequate for historical times». Astronomy & Astrophysics. 190: 351. Bibcode:1988A&A...190..342C
- Martin C. Gutzwiller (1998). «Moon-Earth-Sun: The oldest three-body problem». Reviews of Modern Physics. 70 (2): 589–639. Bibcode:1998RvMP...70..589G. doi:10.1103/RevModPhys.70.589
- Peter Goldreich (novembro de 1966). «History of the Lunar Orbit». Reviews of Geophysics. 4 (4): 411. Bibcode:1966RvGSP...4..411G. doi:10.1029/RG004i004p00411 Jihad Touma & Jack Wisdom (novembro de 1994). «Evolution of the Earth-Moon system». The Astronomical Journal. 108: 1943. Bibcode:1994AJ....108.1943T. doi:10.1086/117209
- Kaveh Pahlevan & Alessandro Morbidelli (26 de novembro de 2015). «Collisionless encounters and the origin of the lunar inclination». Nature. 527 (7579): 492–494. Bibcode:2015Natur.527..492P. PMID 26607544. arXiv:1603.06515. doi:10.1038/nature16137
- The periods are calculated from orbital elements, using the rate of change of quantities at the instant J2000. The J2000 rate of change equals the coefficient of the first-degree term of VSOP polynomials. In the original VSOP87 elements, the units are arcseconds(”) and Julian centuries. There are 1,296,000” in a circle, 36525 days in a Julian century. The sidereal month is the time of a revolution of longitude λ with respect to the fixed J2000 equinox. VSOP87 gives 1732559343.7306” or 1336.8513455 revolutions in 36525 days–27.321661547 days per revolution. The tropical month is similar, but the longitude for the equinox of date is used. For the anomalistic year, the mean anomaly (λ−ω) is used (equinox does not matter). For the draconic month, (λ−Ω) is used. For the synodic month, the sidereal period of the mean Sun (or Earth) and the Moon. The period would be 1/(1/m−1/e). VSOP elements from Simon, J.L.; Bretagnon, P.; Chapront, J.; Chapront-Touzé, M.; Francou, G.; Laskar, J. (fevereiro de 1994). «Numerical expressions for precession formulae and mean elements for the Moon and planets». Astronomy and Astrophysics. 282 (2): 669. Bibcode:1994A&A...282..663S
- Williams, James G.; Boggs, Dale H. (2016). «Secular tidal changes in lunar orbit and Earth rotation». Celestial Mechanics and Dynamical Astronomy (em inglês). 126 (1): 89–129. Bibcode:2016CeMDA.126...89W. ISSN 0923-2958. doi:10.1007/s10569-016-9702-3
- Williams, George E. (2000). «Geological constraints on the Precambrian history of Earth's rotation and the Moon's orbit». Reviews of Geophysics. 38 (1): 37–60. Bibcode:2000RvGeo..38...37W. doi:10.1029/1999RG900016
- Webb, David J. (1982). «Tides and the evolution of the Earth-Moon system». Geophysical Journal of the Royal Astronomical Society. 70 (1): 261–271. Bibcode:1982GeoJ...70..261W. doi:10.1111/j.1365-246X.1982.tb06404.x
adsabs.harvard.edu
- The reference by H. L. Vacher (2001) (details separately cited in this list) describes this as 'convex outward', whereas older references such as "The Moon's Orbit Around the Sun, Turner, A. B. Journal of the Royal Astronomical Society of Canada, Vol. 6, p. 117, 1912JRASC...6..117T"; and "H Godfray, Elementary Treatise on the Lunar Theory" describe the same geometry by the words concave to the sun.
mathpages.com
- The Moon Always Veers Toward the Sun at MathPages
newscientist.com
- Jacob Aron (28 de novembro de 2015). «Flying gold knocked the moon off course and ruined eclipses». New Scientist
- «Moonlight helps plankton escape predators during Arctic winters». New Scientist. 16 de janeiro de 2016
nfo.edu
- «View of the Moon». U. of Arkansas at Little Rock. Consultado em 9 de maio de 2016
nih.gov
ncbi.nlm.nih.gov
- Kaveh Pahlevan & Alessandro Morbidelli (26 de novembro de 2015). «Collisionless encounters and the origin of the lunar inclination». Nature. 527 (7579): 492–494. Bibcode:2015Natur.527..492P. PMID 26607544. arXiv:1603.06515. doi:10.1038/nature16137
nus.edu.sg
math.nus.edu.sg
- «The Orbit of the Moon around the Sun is Convex!». Consultado em 14 de abril de 2022. Arquivado do original em 31 de março de 2004
springer.com
link.springer.com
- Williams, James G.; Boggs, Dale H. (2016). «Secular tidal changes in lunar orbit and Earth rotation». Celestial Mechanics and Dynamical Astronomy (em inglês). 126 (1): 89–129. Bibcode:2016CeMDA.126...89W. ISSN 0923-2958. doi:10.1007/s10569-016-9702-3
web.archive.org
- Caltech Scientists Predict Greater Longevity for Planets with Life Arquivado em 2012-03-30 no Wayback Machine
- «The Orbit of the Moon around the Sun is Convex!». Consultado em 14 de abril de 2022. Arquivado do original em 31 de março de 2004
worldcat.org
- Williams, James G.; Boggs, Dale H. (2016). «Secular tidal changes in lunar orbit and Earth rotation». Celestial Mechanics and Dynamical Astronomy (em inglês). 126 (1): 89–129. Bibcode:2016CeMDA.126...89W. ISSN 0923-2958. doi:10.1007/s10569-016-9702-3