Invariable plane (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Invariable plane" in English language version.

Last modified: 22:46:24, 8 May 2026 (UTC)

Ref.Un. Ref.Website

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53web.archive.org

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53surewest.net

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31unina.it

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22adsabs.harvard.edu

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22doi.org

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11arxiv.org

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11nasa.gov

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aanda.org (Global: 2,832^nd place; English: 2,956^th place)

Souami, D.; Souchay, J. (2012). "The solar system's invariable plane" (PDF). Astronomy & Astrophysics. 543: A133. Bibcode:2012A&A...543A.133S. doi:10.1051/0004-6361/201219011. ISSN 0004-6361. Retrieved July 15, 2025. We note that for all the bodies (except for the Earth, of course), the inclination with respect to the invariable plane is smaller than the inclination with respect to the ecliptic. This is in particular the case for Jupiter and Saturn, for which the inclinations are 0°.3219 and 0°.9254 instead of 1°.3042 and 2°.4859, respectively.

adsabs.harvard.edu (Global: 14^th place; English: 9^th place)

ui.adsabs.harvard.edu

Tremaine, S.; Touma, J.; Namouni, F. (2009). "Satellite dynamics on the Laplace surface". The Astronomical Journal. 137 (3): 3706–3717. arXiv:0809.0237. Bibcode:2009AJ....137.3706T. doi:10.1088/0004-6256/137/3/3706. S2CID 18901505.
Souami, D.; Souchay, J. (2012). "The solar system's invariable plane" (PDF). Astronomy & Astrophysics. 543: A133. Bibcode:2012A&A...543A.133S. doi:10.1051/0004-6361/201219011. ISSN 0004-6361. Retrieved July 15, 2025. We note that for all the bodies (except for the Earth, of course), the inclination with respect to the invariable plane is smaller than the inclination with respect to the ecliptic. This is in particular the case for Jupiter and Saturn, for which the inclinations are 0°.3219 and 0°.9254 instead of 1°.3042 and 2°.4859, respectively.

arxiv.org (Global: 49^th place; English: 31^st place)

Tremaine, S.; Touma, J.; Namouni, F. (2009). "Satellite dynamics on the Laplace surface". The Astronomical Journal. 137 (3): 3706–3717. arXiv:0809.0237. Bibcode:2009AJ....137.3706T. doi:10.1088/0004-6256/137/3/3706. S2CID 18901505.

books.google.com (Global: 3^rd place; English: 3^rd place)

La Place, P.-S., Marquis de (1829) [1799–1825]. Celestial Mechanics. Translated by Bowditch, Nathaniel. Boston, MA. volume I, chapter V, esp. page 121.{{cite book}}: CS1 maint: multiple names: authors list (link) — English translation published in four volumes, 1829–1839;
originally published as
La Place, P.-S., Marquis de (1799–1825). Traité de mécanique céleste [Treatise on Celestial Mechanics] (in French).{{cite book}}: CS1 maint: multiple names: authors list (link) in five volumes.

doi.org (Global: 2^nd place; English: 2^nd place)

Tremaine, S.; Touma, J.; Namouni, F. (2009). "Satellite dynamics on the Laplace surface". The Astronomical Journal. 137 (3): 3706–3717. arXiv:0809.0237. Bibcode:2009AJ....137.3706T. doi:10.1088/0004-6256/137/3/3706. S2CID 18901505.
Souami, D.; Souchay, J. (2012). "The solar system's invariable plane" (PDF). Astronomy & Astrophysics. 543: A133. Bibcode:2012A&A...543A.133S. doi:10.1051/0004-6361/201219011. ISSN 0004-6361. Retrieved July 15, 2025. We note that for all the bodies (except for the Earth, of course), the inclination with respect to the invariable plane is smaller than the inclination with respect to the ecliptic. This is in particular the case for Jupiter and Saturn, for which the inclinations are 0°.3219 and 0°.9254 instead of 1°.3042 and 2°.4859, respectively.

nasa.gov (Global: 12^th place; English: 73^rd place)

nssdc.gsfc.nasa.gov

Planetary Fact Sheets, at http://nssdc.gsfc.nasa.gov

semanticscholar.org (Global: 15^th place; English: 8^th place)

api.semanticscholar.org

Tremaine, S.; Touma, J.; Namouni, F. (2009). "Satellite dynamics on the Laplace surface". The Astronomical Journal. 137 (3): 3706–3717. arXiv:0809.0237. Bibcode:2009AJ....137.3706T. doi:10.1088/0004-6256/137/3/3706. S2CID 18901505.

surewest.net (Global: low place; English: low place)

home.surewest.net

Heider, K.P. (3 April 2009). "The mean plane (invariable plane) of the Solar System passing through the barycenter". Archived from the original on 3 June 2013. Retrieved 10 April 2009.
produced using
Vitagliano, Aldo. "Solex 10" (computer program). Università degli Studi di Napoli Federico II. Archived from the original on 2015-05-24. Retrieved 2010-11-23.
"MeanPlane (invariable plane) for 142400/01/01". 8 April 2009. Archived from the original on 3 June 2013. Retrieved 10 April 2009. (produced with Solex 10)
"MeanPlane (invariable plane) for 168000/01/01". 6 April 2009. Archived from the original on 3 June 2013. Retrieved 10 April 2009. (produced with Solex 10)

unina.it (Global: 8,909^th place; English: low place)

chemistry.unina.it

Heider, K.P. (3 April 2009). "The mean plane (invariable plane) of the Solar System passing through the barycenter". Archived from the original on 3 June 2013. Retrieved 10 April 2009.
produced using
Vitagliano, Aldo. "Solex 10" (computer program). Università degli Studi di Napoli Federico II. Archived from the original on 2015-05-24. Retrieved 2010-11-23.

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

Heider, K.P. (3 April 2009). "The mean plane (invariable plane) of the Solar System passing through the barycenter". Archived from the original on 3 June 2013. Retrieved 10 April 2009.
produced using
Vitagliano, Aldo. "Solex 10" (computer program). Università degli Studi di Napoli Federico II. Archived from the original on 2015-05-24. Retrieved 2010-11-23.
"MeanPlane (invariable plane) for 142400/01/01". 8 April 2009. Archived from the original on 3 June 2013. Retrieved 10 April 2009. (produced with Solex 10)
"MeanPlane (invariable plane) for 168000/01/01". 6 April 2009. Archived from the original on 3 June 2013. Retrieved 10 April 2009. (produced with Solex 10)

worldcat.org (Global: 4^th place; English: 4^th place)

search.worldcat.org

Souami, D.; Souchay, J. (2012). "The solar system's invariable plane" (PDF). Astronomy & Astrophysics. 543: A133. Bibcode:2012A&A...543A.133S. doi:10.1051/0004-6361/201219011. ISSN 0004-6361. Retrieved July 15, 2025. We note that for all the bodies (except for the Earth, of course), the inclination with respect to the invariable plane is smaller than the inclination with respect to the ecliptic. This is in particular the case for Jupiter and Saturn, for which the inclinations are 0°.3219 and 0°.9254 instead of 1°.3042 and 2°.4859, respectively.

Invariable plane (English Wikipedia)

aanda.org (Global: 2,832nd place; English: 2,956th place)

adsabs.harvard.edu (Global: 14th place; English: 9th place)

ui.adsabs.harvard.edu

arxiv.org (Global: 49th place; English: 31st place)

books.google.com (Global: 3rd place; English: 3rd place)

doi.org (Global: 2nd place; English: 2nd place)

nasa.gov (Global: 12th place; English: 73rd place)