標題: Titlebook: Chronology and Evolution of Mars; Proceedings of an IS Reinald Kallenbach,Johannes Geiss,William K. Hartm Conference proceedings 2001 Sprin [打印本頁] 作者: Agoraphobia 時間: 2025-3-21 16:22
書目名稱Chronology and Evolution of Mars影響因子(影響力)
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書目名稱Chronology and Evolution of Mars年度引用學科排名
書目名稱Chronology and Evolution of Mars讀者反饋
書目名稱Chronology and Evolution of Mars讀者反饋學科排名
作者: 松果 時間: 2025-3-21 23:22
https://doi.org/10.1007/978-94-017-1035-0Accretion; Solar System; atmosphere; solar; space science作者: aerobic 時間: 2025-3-22 02:55
978-90-481-5725-9Springer Science+Business Media Dordrecht 2001作者: 弓箭 時間: 2025-3-22 08:38 作者: 整潔漂亮 時間: 2025-3-22 12:04
Steuerbarkeit und Beobachtbarkeit rocks are igneous or sedimentary, but for petrogenetic reasons they could be igneous. We suggest a model in which Mars is covered by about 50% basaltic and 50% andesitic igneous rocks. The soils are a mixture of the two with addition of Mg-sulfate and -chloride plus iron compounds possibly derived from the hematite deposits.作者: 混合物 時間: 2025-3-22 16:46 作者: 混合物 時間: 2025-3-22 17:54 作者: 巨頭 時間: 2025-3-22 23:46 作者: 上釉彩 時間: 2025-3-23 01:50 作者: 沒有希望 時間: 2025-3-23 08:10
Einstellregeln für PI-Mehrgr??enregler (clinopyroxenites), Chassigny (a dunite), and the orthopyroxenite ALH84001. The basaltic shergottites represent surface lava flows, the others magmas that solidified at depth. Shock effects correlate with these compositional types, and, in each case, they can be attributed to a single shock event, 作者: GIDDY 時間: 2025-3-23 10:21
Steuerbarkeit und Beobachtbarkeitdies of Martian meteorites (Nyquist ., 2001) to establish a rough chronology of Martian history. High crater densities in some areas, together with the existence of a 4.5 Gyr rock from Mars (ALH84001), which was weathered at about 4.0 Gyr, affirm that some of the oldest surfaces involve primordial c作者: 膝蓋 時間: 2025-3-23 14:25
Einführung in die digitale Regelungry of the Earth, a planet whose origins have been all but obliterated. Mars is not as depleted in moderately volatile elements as are other terrestrial planets. Judging by the data for Martian meteorites it has Rb/Sr ≈ 0.07 and K/U ≈ 19,000, both of which are roughly twice as high as the values for 作者: 清真寺 時間: 2025-3-23 18:23 作者: Biofeedback 時間: 2025-3-23 23:36 作者: ARCH 時間: 2025-3-24 05:31
Steuerbarkeit und Beobachtbarkeitof its surface features. The determination of Mars surface composition has thus the potential to identify the processes responsible for the entire Mars evolution, from geological timescales to seasonal variations. Due to technical challenges, only few investigations have been performed so far. They 作者: 挑剔小責 時間: 2025-3-24 08:41
Steuerbarkeit und Beobachtbarkeit rocks are igneous or sedimentary, but for petrogenetic reasons they could be igneous. We suggest a model in which Mars is covered by about 50% basaltic and 50% andesitic igneous rocks. The soils are a mixture of the two with addition of Mg-sulfate and -chloride plus iron compounds possibly derived 作者: Pudendal-Nerve 時間: 2025-3-24 12:43 作者: 你正派 時間: 2025-3-24 18:17 作者: flaunt 時間: 2025-3-24 22:05 作者: 脾氣暴躁的人 時間: 2025-3-25 02:20
Steuerbarkeit und Beobachtbarkeit proposed that these aquifers result from geologically recent melting of permafrost ice by sporadic, localized geothermal activity. This is consistent with evidence from crater counts and Martian meteorites that much higher-temperature geothermal activity has produced volcanic activity and lava flow作者: LIMN 時間: 2025-3-25 04:20
Einführung in die Mehrgr??enregelungthe ground and from space. In particular, infrared measurements from the Mariner 9, Viking, Phobos and MGS orbiters have provided information upon the thermal profile, the chemical composition, the stratospheric winds, some isotopic ratios, and the properties of suspended dust. However, further remo作者: Postulate 時間: 2025-3-25 07:31
Introduction: A New Chapter in Mars Researchs of workshops on planetary science at the International Space Science Institute (ISSI), in Bern. The first of these meetings in February, 1999, concentrated on the interdisciplinary assessment of the astronomical, chronological, and geochemical constraints of the formation of the inner solar Esyste作者: LUT 時間: 2025-3-25 14:29 作者: Genistein 時間: 2025-3-25 17:05 作者: Mortar 時間: 2025-3-25 21:13
Ages and Geologic Histories of Martian Meteorites (clinopyroxenites), Chassigny (a dunite), and the orthopyroxenite ALH84001. The basaltic shergottites represent surface lava flows, the others magmas that solidified at depth. Shock effects correlate with these compositional types, and, in each case, they can be attributed to a single shock event, 作者: STEER 時間: 2025-3-26 00:19 作者: Thyroxine 時間: 2025-3-26 06:35 作者: pacifist 時間: 2025-3-26 11:25 作者: Commission 時間: 2025-3-26 16:41
Geological Processes and Evolutionaried in time and space. Impact craters and basins shaped the crust in earliest history and as their importance declined, evidence of extensive regional volcanism emerged during the Late Noachian. Regional volcanism characterized the Early Hesperian and subsequent to that time, volcanism was largely作者: Redundant 時間: 2025-3-26 17:58 作者: Intruder 時間: 2025-3-26 21:48 作者: 可憎 時間: 2025-3-27 03:05
Geomorphologic Evidence for Liquid Waterydrologic cycle. However the present-day conditions on Mars are far apart of supporting liquid water on the surface. Although the large-scale morphology of the Martian channels and valleys show remarkable similarities with fluid-eroded features on Earth, there are major differences in their size, sm作者: MILL 時間: 2025-3-27 06:22 作者: 露天歷史劇 時間: 2025-3-27 10:18
Aeolian Processes and Their Effects on Understanding the Chronology of Marsf new landforms, and mantling or burial of surfaces. Erosion of mantling deposits by wind deflation can exhume older surfaces. These processes and their effects on the surface must be taken into account in using impact crater statistics to derive chronologies on Mars. In addition, mapping the locati作者: refine 時間: 2025-3-27 17:06 作者: 紳士 時間: 2025-3-27 21:09 作者: 鳴叫 時間: 2025-3-27 23:15 作者: Terminal 時間: 2025-3-28 02:39
Einführung in die Mehrgr??enregelung3.85 ± 0.02 Gyr (or 3.77 ± 0.02 Gyr) for Imbrium. Our best estimates for the ages of the mare landing areas are: 3.80 ± 0.02 Gyr for Apollo 11 (old surface), 3.75 ± 0.01 Gyr for Apollo 17, 3.58 ± 0.01 Gyr for Apollo 11 (young surface), 3.41 ± 0.04 Gyr for Luna 16, 3.30 ± 0.02 Gyr for Apollo 15, 3.22作者: –吃 時間: 2025-3-28 07:02
Einstellregeln für PI-Mehrgr??enregler a second impact, probably the ejection event..Crystallization ages of shergottites show only two pronounced groups designated S. (~175 Myr), including 4 of 6 dated basalts and all 3 lherzolites, and S. (330 – 475 Myr), including two basaltic shergottites and probably a third according to preliminar作者: plasma 時間: 2025-3-28 14:30 作者: WAX 時間: 2025-3-28 16:48
Einführung in die digitale Regelunged to terrestrial basalts and eucrites may be related to this higher phosphorus content. The highly siderophile element abundance patterns have been interpreted as reflecting strong partitioning during core formation in a magma ocean environment with little if any late veneer. Oxygen isotope data pr作者: BLA 時間: 2025-3-28 21:14
Einführung in die Mehrgr??enregelungickness can be shown to be in agreement with estimates of volcanic production rates from geologic mapping using data from the camera on MGS and previous missions. According to these estimates most of the crust was produced in the Noachian, roughly the first Gyr of evolution. A substantial part of th作者: 尊嚴 時間: 2025-3-28 22:54 作者: ineffectual 時間: 2025-3-29 04:01 作者: Locale 時間: 2025-3-29 08:57
Conference proceedings 2001 cessation of major collisional growth on Mars. Finally, we reevaluate the isotopic evidence that Mars differentiated quickly. Fundamental differences between the composition of Mars and that of other terrestrial planets are apparent from the planet‘s slightly lower density and from the compositions作者: 行為 時間: 2025-3-29 11:37 作者: 開玩笑 時間: 2025-3-29 16:22 作者: commodity 時間: 2025-3-29 20:55 作者: minimal 時間: 2025-3-30 01:37 作者: leniency 時間: 2025-3-30 05:03 作者: DAFT 時間: 2025-3-30 08:35 作者: 小說 時間: 2025-3-30 16:02
Geophysical Constraints on the Evolution of Marsickness can be shown to be in agreement with estimates of volcanic production rates from geologic mapping using data from the camera on MGS and previous missions. According to these estimates most of the crust was produced in the Noachian, roughly the first Gyr of evolution. A substantial part of th作者: synovial-joint 時間: 2025-3-30 17:54 作者: prediabetes 時間: 2025-3-30 23:35 作者: 事與愿違 時間: 2025-3-31 01:00 作者: colloquial 時間: 2025-3-31 08:04 作者: Nebulizer 時間: 2025-3-31 10:39
Conference proceedings 2001on. The fur- ther growth of the Earth was sustained by major collisions with planetesimals and planets such as that which resulted in the formation ofthe Earth‘s moon (Hartmann and Davis, 1975; Cameron and Ward, 1976; Wetherill, 1986; Cameron and Benz, 1991). This late accretionary history, which la作者: lymphoma 時間: 2025-3-31 17:13 作者: CRANK 時間: 2025-3-31 21:13 作者: BOOST 時間: 2025-4-1 00:11
Steuerbarkeit und Beobachtbarkeitir effects on the surface must be taken into account in using impact crater statistics to derive chronologies on Mars. In addition, mapping the locations, relative ages, and orientations of aeolian features can provide insight into Martian weather, climate, and climate history.
