Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Giacomo Lari"'
Publikováno v:
Aerospace, Vol 11, Iss 2, p 124 (2024)
The extreme accuracy of Juno radio science data allows us to perform very precise orbit determination experiments. While previous works focused on the estimation of the gravitational field of Jupiter, in this article, we aim to accurately determine t
Externí odkaz:
https://doaj.org/article/a5bf2d6ed66b4978933763d72155105d
Autor:
Daniele Durante, Tristan Guillot, Luciano Iess, David J. Stevenson, Christopher R. Mankovich, Steve Markham, Eli Galanti, Yohai Kaspi, Marco Zannoni, Luis Gomez Casajus, Giacomo Lari, Marzia Parisi, Dustin R. Buccino, Ryan S. Park, Scott J. Bolton
Publikováno v:
Nature Communications, Vol 13, Iss 1, Pp 1-8 (2022)
Juno spacecraft experienced unknown accelerations near the closest approach to Jupiter. Here, the authors show that Jupiter’s axially symmetric, north-south asymmetric gravity field measured by Juno is perturbed by a time-variable component, associ
Externí odkaz:
https://doaj.org/article/b82ea36e2b554861b641a436db72891d
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2023, 518 (2), pp.3023-3035. ⟨10.1093/mnras/stac3299⟩
Monthly Notices of the Royal Astronomical Society, 2023, 518 (2), pp.3023-3035. ⟨10.1093/mnras/stac3299⟩
The dynamics of the innermost Galilean satellites (Io, Europa and Ganymede) is characterised by a chain of mean motion resonances, called Laplace resonance, and by a strong tidal dissipation that causes wide variations of their semi-major axes over l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f0aaad72184f41686bbe0df7d94d0f5
https://hal.science/hal-03879278
https://hal.science/hal-03879278
Orbit determination methods for interplanetary missions: development and use of the Orbit14 software
Publikováno v:
Experimental Astronomy. 53:159-208
In the last years, a new generation of interplanetary space missions have been designed for the exploration of the solar system. At the same time, radio-science instrumentation has reached an unprecedented level of accuracy, leading to a significant
Publikováno v:
Nature Astronomy
Nature Astronomy, 2021, 5, pp.345-349. ⟨10.1038/s41550-020-01284-x⟩
Nature Astronomy, Nature Publishing Group, 2021, 5, pp.345-349. ⟨10.1038/s41550-020-01284-x⟩
Nature Astronomy, 2021, 5, pp.345-349. ⟨10.1038/s41550-020-01284-x⟩
Nature Astronomy, Nature Publishing Group, 2021, 5, pp.345-349. ⟨10.1038/s41550-020-01284-x⟩
The obliquity of a planet is the tilt between its equator and its orbital plane. Giant planets are expected to form with near-zero obliquities. After its formation, some dynamical mechanism must therefore have tilted Saturn up to its current obliquit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::115aeef43ab7e655f80cebd0acb132a5
http://arxiv.org/abs/2110.04104
http://arxiv.org/abs/2110.04104
Autor:
Melaine Saillenfest, Giacomo Lari
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 654, pp.A83. ⟨10.1051/0004-6361/202141467⟩
Astronomy and Astrophysics-A&A, 2021, 654, pp.A83. ⟨10.1051/0004-6361/202141467⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 654, pp.A83. ⟨10.1051/0004-6361/202141467⟩
Astronomy and Astrophysics-A&A, 2021, 654, pp.A83. ⟨10.1051/0004-6361/202141467⟩
Context: As a result of Titan's migration and Saturn's probable capture in secular spin-orbit resonance, recent works show that Saturn's obliquity could be steadily increasing today and may reach large values in the next billions of years. Satellites
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::93beabbfb5ce85bec92ba04170e3f51b
https://hal.archives-ouvertes.fr/hal-03375960/file/aa41467-21.pdf
https://hal.archives-ouvertes.fr/hal-03375960/file/aa41467-21.pdf
Autor:
Melaine Saillenfest, Zeeve Rogoszinski, Giacomo Lari, Kevin Baillié, Gwenaël Boué, Aurélien Crida, Valéry Lainey
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 668, pp.A108. ⟨10.1051/0004-6361/202243953⟩
Astronomy and Astrophysics-A&A, 2022, 668, pp.A108. ⟨10.1051/0004-6361/202243953⟩
Context. The 98{\deg}-obliquity of Uranus is commonly attributed to giant impacts that occurred at the end of the planetary formation. This picture, however, is not devoid of weaknesses. Aims. On a billion-year timescale, the tidal migration of the s
Publikováno v:
Geoscientific Model Development, Vol 12, Pp 581-595 (2019)
Pyroclastic avalanches are a type of granular flow generated at active volcanoes by different mechanisms, including the collapse of steep pyroclastic deposits (e.g., scoria and ash cones), fountaining during moderately explosive eruptions, and crumbl
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 647, pp.A92. ⟨10.1051/0004-6361/202039891⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 647, pp.A92. ⟨10.1051/0004-6361/202039891⟩
Astronomy and Astrophysics-A&A, 2021, 647, pp.A92. ⟨10.1051/0004-6361/202039891⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 647, pp.A92. ⟨10.1051/0004-6361/202039891⟩
Aims: It has recently been shown that the fast migration of Titan could be responsible for the current 26.7{\deg}-tilt of Saturn's spin axis. We aim to quantify the level of generality of this result and to measure the most likely sets of parameters.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b75741094bd3d4075528253bf795d097
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A40. ⟨10.1051/0004-6361/202037445⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, 2020, 639, pp.A40. ⟨10.1051/0004-6361/202037445⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A40. ⟨10.1051/0004-6361/202037445⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, 2020, 639, pp.A40. ⟨10.1051/0004-6361/202037445⟩
Context. The strong tidal dissipation in the couple Jupiter-Io is spread to all the moons involved in the Laplace resonance (Io, Europa, and Ganymede), leading to a migration of their orbits. Aims. We aim to characterize the future behavior of the Ga
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::65eee6f26c14951b4423e1c6cb249946
https://hal.archives-ouvertes.fr/hal-02987249
https://hal.archives-ouvertes.fr/hal-02987249