標(biāo)題: Titlebook: Geology and Habitability of Terrestrial Planets; Kathryn E. Fishbaugh,Philippe Lognonné,Oleg Korabl Book 2007 Springer-Verlag New York 200 [打印本頁(yè)] 作者: fathom 時(shí)間: 2025-3-21 19:29
書(shū)目名稱Geology and Habitability of Terrestrial Planets影響因子(影響力)
書(shū)目名稱Geology and Habitability of Terrestrial Planets影響因子(影響力)學(xué)科排名
書(shū)目名稱Geology and Habitability of Terrestrial Planets網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Geology and Habitability of Terrestrial Planets網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Geology and Habitability of Terrestrial Planets被引頻次
書(shū)目名稱Geology and Habitability of Terrestrial Planets被引頻次學(xué)科排名
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書(shū)目名稱Geology and Habitability of Terrestrial Planets年度引用學(xué)科排名
書(shū)目名稱Geology and Habitability of Terrestrial Planets讀者反饋
書(shū)目名稱Geology and Habitability of Terrestrial Planets讀者反饋學(xué)科排名
作者: MUTED 時(shí)間: 2025-3-21 20:43
https://doi.org/10.1007/978-3-031-12000-8eductants (e.g. dead organic matter) and oxidants (including waste products). Potential Martian habitats are discussed: by comparison with Earth there are many potential environmental settings on Mars in which life may once have occurred, or may even continue to exist. The long-term evolution of habitability in the Solar System is considered.作者: 委托 時(shí)間: 2025-3-22 01:15
Creating Habitable Zones, at all Scales, from Planets to Mud Micro-Habitats, on Earth and on Mars,eductants (e.g. dead organic matter) and oxidants (including waste products). Potential Martian habitats are discussed: by comparison with Earth there are many potential environmental settings on Mars in which life may once have occurred, or may even continue to exist. The long-term evolution of habitability in the Solar System is considered.作者: 地牢 時(shí)間: 2025-3-22 04:43 作者: Libido 時(shí)間: 2025-3-22 09:47
Three-Level Schemes with Operator Factors,, as well as the presence of a magnetic field, are important factors contributing to the habitability of a planet. This chapter reviews these processes, their mutual interactions, and the role life plays in regulating or modulating them.作者: RACE 時(shí)間: 2025-3-22 13:02 作者: RACE 時(shí)間: 2025-3-22 20:17
Planetary Magnetic Dynamo Effect on Atmospheric Protection of Early Earth and Mars,out 4 Gyr ago), atmospheric escape induced by solar wind began. We consider scenarios which could ultimately lead to a decrease of atmospheric pressure to the presently observed value of 7 mbar: a much weaker early martian magnetic field, a late onset of the dynamo, and high erosion rates of a denser early atmosphere.作者: 橢圓 時(shí)間: 2025-3-22 21:44
Water, Life, and Planetary Geodynamical Evolution,, as well as the presence of a magnetic field, are important factors contributing to the habitability of a planet. This chapter reviews these processes, their mutual interactions, and the role life plays in regulating or modulating them.作者: 潛伏期 時(shí)間: 2025-3-23 01:53 作者: Asparagus 時(shí)間: 2025-3-23 07:17
978-1-4419-2553-4Springer-Verlag New York 2007作者: overshadow 時(shí)間: 2025-3-23 13:20 作者: Malleable 時(shí)間: 2025-3-23 16:30 作者: LUCY 時(shí)間: 2025-3-23 19:41
https://doi.org/10.1007/978-94-011-1763-0cooled and condensed over ～1,000 yrs. As it cooled the Earth degassed its volatiles into the atmosphere. It took another ～2 Myrs for the magma ocean to freeze at the surface. The cooling rate was determined by atmospheric thermal blanketing. Tidal heating by the new Moon was a major energy source to作者: peritonitis 時(shí)間: 2025-3-23 23:29
https://doi.org/10.1007/978-3-031-12000-8s such as habitat linkage. The possibility of habitability first comes about during accretion, as a product of the processes of impact and volatile inventory history. To create habitability water is essential, not only for life but to aid the continual tectonic reworking and erosion that supply key 作者: FRET 時(shí)間: 2025-3-24 04:52 作者: 賄賂 時(shí)間: 2025-3-24 09:06
upper atmospheres, and thermal and non-thermal atmospheric loss processes, the long-time evolution of planetary atmospheres and their water inventories can only be understood within the context of the evolving Sun. We compare the effect of solar induced X-ray and EUV (XUV) heating on the upper atmos作者: –scent 時(shí)間: 2025-3-24 11:14
https://doi.org/10.1057/9780230801424cting the habitability and chances for life to emerge on a planet. The forcing is essentially inversely proportional to the square of the distance to the Sun and, therefore, is most important for the innermost planets in our solar system—the Earth-like planets. The effect of these two forcing terms 作者: Malfunction 時(shí)間: 2025-3-24 18:04 作者: 講個(gè)故事逗他 時(shí)間: 2025-3-24 21:42
Kathryn E. Fishbaugh,Philippe Lognonné,Oleg KorablPresents the combined scientific expertise of researchers studying the conditions of life on other planets作者: Phagocytes 時(shí)間: 2025-3-25 00:02 作者: Nonconformist 時(shí)間: 2025-3-25 06:57 作者: 思想 時(shí)間: 2025-3-25 10:12 作者: 紅潤(rùn) 時(shí)間: 2025-3-25 12:49
Emergence of a Habitable Planet,cooled and condensed over ～1,000 yrs. As it cooled the Earth degassed its volatiles into the atmosphere. It took another ～2 Myrs for the magma ocean to freeze at the surface. The cooling rate was determined by atmospheric thermal blanketing. Tidal heating by the new Moon was a major energy source to作者: mitral-valve 時(shí)間: 2025-3-25 18:13
Creating Habitable Zones, at all Scales, from Planets to Mud Micro-Habitats, on Earth and on Mars,s such as habitat linkage. The possibility of habitability first comes about during accretion, as a product of the processes of impact and volatile inventory history. To create habitability water is essential, not only for life but to aid the continual tectonic reworking and erosion that supply key 作者: tympanometry 時(shí)間: 2025-3-25 21:48
Water, Life, and Planetary Geodynamical Evolution,rely a substrate on which life may develop. Large-scale exchange of heat and volatile species between planetary interiors and hydrospheres/atmospheres, as well as the presence of a magnetic field, are important factors contributing to the habitability of a planet. This chapter reviews these processe作者: mechanism 時(shí)間: 2025-3-26 01:14
A Comparative Study of the Influence of the Active Young Sun on the Early Atmospheres of Earth, Venupper atmospheres, and thermal and non-thermal atmospheric loss processes, the long-time evolution of planetary atmospheres and their water inventories can only be understood within the context of the evolving Sun. We compare the effect of solar induced X-ray and EUV (XUV) heating on the upper atmos作者: preservative 時(shí)間: 2025-3-26 05:38
Planetary Magnetic Fields and Solar Forcing: Implications for Atmospheric Evolution,cting the habitability and chances for life to emerge on a planet. The forcing is essentially inversely proportional to the square of the distance to the Sun and, therefore, is most important for the innermost planets in our solar system—the Earth-like planets. The effect of these two forcing terms 作者: chapel 時(shí)間: 2025-3-26 09:49
Planetary Magnetic Dynamo Effect on Atmospheric Protection of Early Earth and Mars,osphere is protected from erosion by solar wind. The magnetic field ensures the maintenance of a dense atmosphere, necessary for liquid water to exist on the surface of Mars. We also examine the impact of the rotation of Mars on the magnetic field. When the magnetic field of Mars ceased to exist (ab作者: Bricklayer 時(shí)間: 2025-3-26 15:04 作者: 立即 時(shí)間: 2025-3-26 17:59 作者: enchant 時(shí)間: 2025-3-27 00:55
Epilogue: The Origins of Life in the Solar System and Future Exploration,作者: Accomplish 時(shí)間: 2025-3-27 02:22
Kindergarten und Musikprobelokal,understanding of the habitats that can sustain or have sustained life has grown tremendously with the characterisation of extremophiles. In this chapter, we highlight the range of environments that are known to harbour life on Earth, describe the environments that existed during the period of time w作者: 規(guī)范要多 時(shí)間: 2025-3-27 05:26 作者: 致詞 時(shí)間: 2025-3-27 10:59 作者: 染色體 時(shí)間: 2025-3-27 16:41 作者: FLUSH 時(shí)間: 2025-3-27 19:54 作者: 小歌劇 時(shí)間: 2025-3-27 23:49
Emergence of a Habitable Planet,d and its oceans white with ice. But if carbonate subduction were inefficient the CO. would have mostly stayed in the atmosphere, which would have kept the surface near ～500?K for many tens of millions of years. Hydrous minerals are harder to subduct than carbonates and there is a good chance that t作者: 使熄滅 時(shí)間: 2025-3-28 05:27
A Comparative Study of the Influence of the Active Young Sun on the Early Atmospheres of Earth, Venarly Earth, Venus and Mars. The exospheric temperatures obtained for all the three planets during this time period lead to diffusion-limited hydrodynamic escape of atomic hydrogen and high Jeans’ escape rates for heavier species like H., He, C, N, O, etc. The duration of this blow-off phase for atom作者: Hyperopia 時(shí)間: 2025-3-28 07:49 作者: verdict 時(shí)間: 2025-3-28 10:30 作者: 突襲 時(shí)間: 2025-3-28 18:17 作者: SEED 時(shí)間: 2025-3-28 20:50 作者: Antarctic 時(shí)間: 2025-3-29 00:43
Shama Siddiqui,Anwar Ahmed Khane outcomes. Methods of assessing everyday functioning include self- and informant-report as well as performance-based measures of everyday tasks that provide more objective assessment facilitated by standardized coding schemes. Everyday action research has revealed relations between cognitive/neurop作者: 魯莽 時(shí)間: 2025-3-29 05:18 作者: COST 時(shí)間: 2025-3-29 08:58 作者: Diastole 時(shí)間: 2025-3-29 14:04
Garside and Quadratic Normalisation: A Survey,ain how it extends to the more general framework of Garside families. Extending the viewpoint even more, we then consider general quadratic normalisation procedures and characterise Garside normalisation among them.作者: 一加就噴出 時(shí)間: 2025-3-29 16:11 作者: Anticlimax 時(shí)間: 2025-3-29 22:21
