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Origin of Water in the Terrestrial Planets: Insights from Meteorite Data and Planet Formation Models
, 2022 International audienceWater condensed as ice beyond the water snowline, the location in the Sun’s natal gaseous disk where temperatures were below 170 K. As the disk evolved and cooled, the snowline moved inwards.
Piani, Laurette, Izidoro, Andre
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Predicting Planets in Known Extrasolar Planetary Systems. III. Forming Terrestrial Planets [PDF]
The Astrophysical Journal, 2006 New coauthor Kaib -- ApJ, in ...
Raymond, Sean N. +2 more
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Tianwen-1 and MAVEN Observations of the Response of Mars to an Interplanetary Coronal Mass Ejection
The Astrophysical Journal, 2023 Interplanetary coronal mass ejections (ICMEs) are solar transients that have significant effects on the upper atmosphere and ionosphere of Mars. The simultaneous spacecraft observations from Tianwen-1/MOMAG in solar wind and multiple instruments on board
Bingkun Yu +24 more
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Main Belt Comets and other “Interlopers” in the Solar System
Universe, 2022 According to traditional ideas about the formation of the Solar System starting from a protoplanetary disk of gas and dust, a well-defined distribution of planets and minor bodies is expected: (a) volatile-poor rocky bodies (terrestrial planets and ...
Vincenzo Orofino
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Exploration of the Atmospheres of the Terrestrial Planets [PDF]
, 2023 In this chapter, we describe the atmospheres of the terrestrial planets of our Solar System. After a brief introduction on the concept of “comparative planetology”, we introduce different theoretical elements which permit us to better grasp the ...
Vandaele, A.C.
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The Astrophysical Journal, 2023 We model the early stages of planet formation in the solar system, including continual planetesimal formation, and planetesimal and pebble accretion onto planetary embryos in an evolving disk driven by a disk wind.
John Chambers
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General circulation modelling of close-in extrasolar giant planets [PDF]
, 2011 PhDA large fraction of the extrasolar planets detected so far are giant planets that have such short orbital periods (a few days) that they are thought to be tidally-synchronised with the host star. Such orbits lead to permanent day/night sides on the
Thrastarson, Heidar Thor
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Frontiers in Astronomy and Space Sciences, 2022 Orbital systems are often self-organized and/or characterized by harmonic relations. Inspired by music theory, we rewrite the Geddes and King-Hele (QJRAS, 24, 10–13, 1983) equations for mirror symmetries among the distances of the planets of the Solar ...
Michael J. Bank, Nicola Scafetta
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A light carbon isotope composition for the Sun
Nature Communications, 2018 The Sun’s light stable isotopes compositions can help us understand how our solar system formed. Here, the authors find that solar C is depleted relative to bulk Earth indicating that the 13C enrichment of the terrestrial planets is from CO self ...
James R. Lyons +2 more
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Космические аппараты и технологии, 2023 Currently, the exploration of the planet Venus is a very relevant and developing direction in space science. The development of rocket and space technologies has expanded the boundaries of accessibility of spacecraft to objects in the Solar System, allow
M. Yu. Yatsenko +2 more
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