Zobrazeno 1 - 10
of 25
pro vyhledávání: '"Mickael Gastineau"'
Autor:
Andrea Di Ruscio, Jacques Laskar, Luciano Iess, Agnes Fienga, Mickael Gastineau, Léo Bernus, Daniele Durante, P. Deram
The accuracy achieved by modern deep space radio tracking systems has dramatically increased the precision of planetary ephemerides in the last decade. This improvement is particularly beneficial to the study of the trans-Neptunian solar system, stil
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ad00c45601bc3bfabde9b359699a0f5d
https://doi.org/10.5194/epsc2020-804
https://doi.org/10.5194/epsc2020-804
Since December 2013, the GAIA spacecraft (ESA) is observing the sky with an unprecedented accuracy. Gaia DR2, released in April 2018, contains the position and epoch of 14099 known solar system objects (SSOs) representing more than 2 million observat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::40649d37ea76d6d0b9400dce0b34a42c
https://doi.org/10.5194/epsc2020-238
https://doi.org/10.5194/epsc2020-238
Publikováno v:
Geophysical Research Letters
Geophysical Research Letters, American Geophysical Union, 2019, 46, pp.7295-7303. ⟨10.1029/2019GL082677⟩
Geophys.Res.Lett.
Geophys.Res.Lett., 2019, 46, pp.7295-7303. ⟨10.1029/2019GL082677⟩
Geophysical Research Letters, American Geophysical Union, 2019, 46, pp.7295-7303. ⟨10.1029/2019GL082677⟩
Geophys.Res.Lett.
Geophys.Res.Lett., 2019, 46, pp.7295-7303. ⟨10.1029/2019GL082677⟩
Lunar laser ranging (LLR) data and Apollo seismic data analyses, revealed independent evidence for the presence of a fluid lunar core. However, the size of the lunar fluid core remained uncertain by $\pm55$ km (encompassing two contrasting 2011 Apoll
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c84e7e6229a25bdb6113f4c827d9110f
https://hal.archives-ouvertes.fr/hal-02088588
https://hal.archives-ouvertes.fr/hal-02088588
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2019, 628, pp.A32. ⟨10.1051/0004-6361/201935786⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 628, pp.A32. ⟨10.1051/0004-6361/201935786⟩
Astronomy and Astrophysics-A&A, 2019, 628, pp.A32. ⟨10.1051/0004-6361/201935786⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 628, pp.A32. ⟨10.1051/0004-6361/201935786⟩
We present a new mixed variable symplectic (MVS) integrator for planetary systems, that fully resolve close encounters. The method is based on a time regularisation that allows keeping the stability properties of the symplectic integrators, while als
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::134d2e859bcd6f281d30481a0f9be37a
https://hal.science/hal-02918712/document
https://hal.science/hal-02918712/document
Autor:
Léo Bernus, Vishnu Viswanathan, Mickael Gastineau, Olivier Minazzoli, Jacques Laskar, Agnes Fienga
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2018, 476 (2), pp.1877-1888. ⟨10.1093/mnras/sty096⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2018, 476 (2), pp.1877-1888. ⟨10.1093/mnras/sty096⟩
Mon.Not.Roy.Astron.Soc., 2018, 476 (2), pp.1877-1888. ⟨10.1093/mnras/sty096⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2018, 476 (2), pp.1877-1888. ⟨10.1093/mnras/sty096⟩
We present here the new INPOP lunar ephemeris, INPOP17a. This ephemeris is obtained through the numerical integration of the equations of motion and of rotation of the Moon, fitted over 48 years of Lunar Laser Ranging (LLR) data. We also include the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9be695f932944424b8876d584e577d1e
https://hal.archives-ouvertes.fr/hal-01833809
https://hal.archives-ouvertes.fr/hal-01833809
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2019, 622, pp.A95. ⟨10.1051/0004-6361/201833342⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 622, pp.A95. ⟨10.1051/0004-6361/201833342⟩
Astronomy and Astrophysics-A&A, 2019, 622, pp.A95. ⟨10.1051/0004-6361/201833342⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 622, pp.A95. ⟨10.1051/0004-6361/201833342⟩
Context. The dwarf planet Ceres and the asteroid Vesta have been studied by the Dawn space mission. They are the two heaviest bodies of the main asteroid belt and have different characteristics. Notably, Vesta appears to be dry and inactive with two
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d338549e49261fda946256171e81a376
Autor:
Pierre Gaillard, Mickael Gastineau
Publikováno v:
Communications in Theoretical Physics
Communications in Theoretical Physics, Chinese Physical Society, 2016, 65 (2), pp.136-144. 〈10.1088/0253-6102/65/2/136〉
Communications in Theoretical Physics, Chinese Physical Society, 2016, 65 (2), pp.136-144. ⟨10.1088/0253-6102/65/2/136⟩
Communications in Theoretical Physics, 2016, 65 (2), pp.136-144. ⟨10.1088/0253-6102/65/2/136⟩
Communications in Theoretical Physics, Chinese Physical Society, 2016, 65 (2), pp.136-144. 〈10.1088/0253-6102/65/2/136〉
Communications in Theoretical Physics, Chinese Physical Society, 2016, 65 (2), pp.136-144. ⟨10.1088/0253-6102/65/2/136⟩
Communications in Theoretical Physics, 2016, 65 (2), pp.136-144. ⟨10.1088/0253-6102/65/2/136⟩
International audience; The Peregrine breather of order eleven (P11 breather) solution to the focusing one-dimensional nonlinear Schrödinger equation (NLS) is explicitly constructed here. Deformations of the Peregrine breather of order 11 with 20 re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::959ac0e13caf5ae3f31f3f20fa380542
https://hal.archives-ouvertes.fr/hal-01224526
https://hal.archives-ouvertes.fr/hal-01224526
Autor:
P. Kuchynka, Agnes Fienga, C. Leponcin-Lafitte, Mickael Gastineau, Herve Manche, Jacques Laskar
Publikováno v:
IAU Symposium
Relativity in Fundamental Astronomy-Dynamics, Reference Frames and Data Analysis, IAU Symposium 261
Relativity in Fundamental Astronomy-Dynamics, Reference Frames and Data Analysis, IAU Symposium 261, Apr 2009, Virginia Beach, VA, United States, United States. pp.159-169, ⟨10.1017/S1743921309990330⟩
Relativity in Fundamental Astronomy-Dynamics, Reference Frames and Data Analysis, IAU Symposium 261
Relativity in Fundamental Astronomy-Dynamics, Reference Frames and Data Analysis, IAU Symposium 261, Apr 2009, Virginia Beach, VA, United States, United States. pp.159-169, ⟨10.1017/S1743921309990330⟩
In this paper, we present several gravity tests made in using the last INPOP08 planetary ephemerides. We first propose two methods to estimate the PPN parameter $\beta$ and its correlated value, the Sun J2 and we discuss the correlation between the S
Publikováno v:
Astronomy and Astrophysics Review
Astronomy and Astrophysics Review, Springer Verlag, 2016, 587 (L8), ⟨10.1051/0004-6361/201628227⟩
Astronomy and Astrophysics Review, 2016, 587 (L8), ⟨10.1051/0004-6361/201628227⟩
Astronomy and Astrophysics Review, Springer Verlag, 2016, 587 (L8), ⟨10.1051/0004-6361/201628227⟩
Astronomy and Astrophysics Review, 2016, 587 (L8), ⟨10.1051/0004-6361/201628227⟩
To explain the unusual distribution of Kuiper Belt objects, several authors have advocated the existence of a super-Earth planet in the outer solar system. It has recently been proposed that a 10 M$_{\oplus}$ object with an orbit of 700 AU semi major
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0dd88be444aab713e8a21ca7d2c6b77a
Publikováno v:
Celestial Mechanics and Dynamical Astronomy
Celestial Mechanics and Dynamical Astronomy, Springer Verlag, 2015, 123 (3), pp.325-349. ⟨10.1007/s10569-015-9639-y⟩
Celestial Mechanics and Dynamical Astronomy, 2015, 123 (3), pp.325-349. ⟨10.1007/s10569-015-9639-y⟩
Celestial Mechanics and Dynamical Astronomy, Springer Verlag, 2015, 123 (3), pp.325-349. ⟨10.1007/s10569-015-9639-y⟩
Celestial Mechanics and Dynamical Astronomy, 2015, 123 (3), pp.325-349. ⟨10.1007/s10569-015-9639-y⟩
In this paper, are given numerical estimations of the sensitivity of the latest version of the INPOP planetary ephemerides (INPOP13c) to GR parameters: the PPN parameters $$\beta $$ , $$\gamma $$ , and the oblateness of the Sun J $$_{2}^{\odot }$$ .
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af58d58376d19723feb65cef65edf966
https://hal.archives-ouvertes.fr/hal-01362401
https://hal.archives-ouvertes.fr/hal-01362401