Results 31 to 40 of about 465,389 (352)
The effects of gravity on the climate and circulation of a terrestrial planet [PDF]
Quarterly Journal of the Royal Meteorological Society, 2019 The climate and circulation of a terrestrial planet are governed by, among other things, the distance to its host star, its size, rotation rate, obliquity, atmospheric composition and gravity.
S. Thomson, G. Vallis
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Giant planet effects on terrestrial planet formation and system architecture [PDF]
Monthly notices of the Royal Astronomical Society, 2018 The giant planets of the solar system likely played a large role in shaping the architecture of the terrestrial planets. Using an updated collision model, we conduct a suite of high resolution N-body integrations to probe the relationship between giant ...
Anna C. Childs +3 more
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Two Terrestrial Planet Families with Different Origins [PDF]
Astrophysical Journal, 2018 The potentially important role of stellar irradiation in envelope removal for planets with diameters of ⪅2 R⊕ has been inferred both through theoretical work and the observed bimodal distribution of small planet occurrence as a function of radius.
M. Swain +4 more
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An update on global mining land use
Scientific Data, 2022 Measurement(s) terrestrial mining Technology Type(s) satellite imaging Factor Type(s) area • polygon geometry Sample Characteristic - Environment land Sample Characteristic - Location Earth (planet)
Victor Maus +8 more
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A Terrestrial-mass Rogue Planet Candidate Detected in the Shortest-timescale Microlensing Event [PDF]
Astrophysical Journal Letters, 2020 Some low-mass planets are expected to be ejected from their parent planetary systems during early stages of planetary system formation. According to planet formation theories, such as the core accretion theory, typical masses of ejected planets should be
P. Mróz +29 more
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Simulations for Terrestrial Planets Formation [PDF]
Proceedings of the International Astronomical Union, 2009 AbstractWe investigate the formation of terrestrial planets in the late stage of planetary formation using two-planet model. At that time, the protostar has formed for about 3 Myr and the gas disk has dissipated. In the model, the perturbations from Jupiter and Saturn are considered.
Zhang Niu, Zhang Niu, Ji Jianghui
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EPJ Web of Conferences, 2011 It has been shown that an Earth-size planet or a super-Earth, in resonance with a transiting Jupiter-like body around an M star, can create detectable TTV signals (Kirste & Haghighipour, 2011).
Rastegar S., Haghighipour N.
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Evolution of a Water-rich Atmosphere Formed by a Giant Impact on an Earth-sized Planet
The Astrophysical Journal, 2023 The atmosphere of a terrestrial planet that is replenished with secondary gases should have accumulated hydrogen-rich gas from its protoplanetary disk.
Kenji Kurosaki +3 more
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Numerical simulations for terrestrial planets formation
EPJ Web of Conferences, 2011 We investigate the formation of terrestrial planets in the late stage of planetary formation using two-planet model. At that time, the protostar has formed for about 3 Myr and the gas disk has dissipated.
Ji J., Zhang N.
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The Astronomical Journal, 2023 We present an analysis of a volume-complete sample of 363 mid-to-late M dwarfs within 15 pc of the Sun with masses between 0.1 and 0.3 M _⊙ observed by TESS within sectors 1–42. The median stellar mass of the sample is 0.17 M _⊙ .
Kristo Ment, David Charbonneau
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