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Mary Anning, Alfred Nicholson Leeds and Steve Etches form part of a long line of individuals who furnished a substantial addition to our understanding of marine and terrestrial ecosystems through collecting significant numbers of superb fossils. For all three collectors, fossils became a factor that dominated their lives, and their fossil collecting led to the discovery of numerous taxa new to science. Extensive collecting was made possible by the fortunate circumstances of living ‘in the right place at the right time’, close to fine-grained UK Jurassic deposits (Lagerstätten) with well-preserved large Jurassic marine reptiles. All three were highly-motivated and developed a considerable skill sets for discovering, collecting, preparing, conserving and displaying fossils. They developed personal and professional interactions with family and friends, and university and museum professionals, although their collecting resulted in variable recognition of their work. Each collector can be considered a complex mix of amateur and professional: Mary Anning, a professional fossil collector and amateur palaeontologist; Alfred Leeds transitioned from amateur to professional fossil collector, but remained an amateur palaeontologist; and Steve Etches has remained an amateur fossil collector and palaeontologist. However, all three exhibited an entirely professional outlook to collecting, and should be considered professionals of the highest degree. The impact of Mary Anning, Alfred Nicholson Leeds and Steve Etches has been critical for the development of Palaeontology as a science, and without whom palaeontology, with all its associated benefits to a wide scientific and non-scientific audience, would not be as rich as we currently know it.  相似文献   
2.
Gas phase transport according to chemical fluid transport (CFT) in Earth's crust as well as in the solar nebula is characterized by very high transport efficiency. Systematic investigations of mobilization, transport and deposition of gaseous MeX (Me = metal, X = F or Cl) compounds by solid gas equilibrium reactions are suitable to explain numerous extensive accumulations of minerals and ores. More than 40 of the considered chemical elements form volatile MeX compounds. Some elements tend to form MeF compounds, whereas others are more likely to form MeCl compounds. Silicon reacts with HF to form SiF4 and replaces other elements to form MeF compounds at low temperature ranges. Accumulations caused by SiF4 transport explain the formation of numerous quartz varieties and silicate minerals in Earth's crust. Iron most likely reacts with HCl to form FeCl2 as well as FeCl3 and explain the formation of iron or iron compounds. Thermodynamically directed transport from cool to hot areas in connection with cyclic processes increases the transport efficiency of MeX-species. Such species are SiF4, Al2F6, POF3, Cu3Cl3, SnCl4, BF3, GeF4, GeCl4, Ga2Cl6, ZrF4, NbF5 and TiF4. The transport gases SiF4 and POF3 often react with environmental compounds forming pneumatolytic and metasomatical mineral accumulations. CFT is the “motor” of pneumatolytic and metasomatical processes.  相似文献   
3.
The common or similar elements of faunas shared by the Early Cambrian Chengjiang fauna and the Middle Cambrian Burgess Shale fauna are listed in a generic level so as to have a better understanding of the palaeogeographic relationship between the South China Block and Laurentia. The Burgess Shale-type faunas probably had a worldwide distribution during the interval ranging from the Late Tommotian to Atdabanian. The geographic and biological contributions to the cosmopolitan geographic distribution of the Burgess Shale-type faunas are discussed. However, newly developed pelagic larvae in many phyla, which probably acquired their first bloom in the Cambrian, might have promoted the dispersal.  相似文献   
4.
The final assembly of the supercontinent Gondwana during the Pan-African orogenic episodes (ca. 550–520 Ma) almost simultaneously took place with the Cambrian explosion that is best manifested by a number of Cambrian Burgess Shale-type Lagerstätten in South China. The relationship between South China and Gondwana during the Cambrian is far from consensus. Burgess Shale-type Lagerstätten may have potential importance for the paleogeographic reconstruction. However, such Lagerstätten have been known in large number only in Laurentia and South China, far less common in Gondwana and other continents. Burgess Shale-type Lagerstätten in South China are not evenly spaced through the Cambrian. They appear to be concentrated in the Lower Cambrian, particularly in the Canglangpuian and Qiongzhusian stages, much reduced in number from the uppermost Lower Cambrian. Of ten reported such Lagerstätten, only the Kaili biota (basal Middle Cambrian) is known to be younger than Early Cambrian. This reduction could be explained by the fact that vast areas of siliciclastic facies in both the western plate interior (platform) and the eastern slope basin during most time of Early Cambrian (Meishucunian to Canglangpuian) is evolved into carbonate facies at the very end of Early Cambrian (Longwangmiaoian). It has been known from this study that both siliciclastic platform facies and slope basin facies (shale basin) could preserve soft-bodied fossils. Cambrian Burgess Shale-type Lagerstätten in South China are of great significance for providing a sequences of exceptionally preserved biota in a chronological succession. Comparison of such Lagerstätten in a chronological framework may give us more details on the Cambrian explosion events.  相似文献   
5.
A new ophiuroid species from the Hauptrogenstein Formation (Middle Jurassic, Bajocian) of the Rehhag ridge near Schöntal, northwestern Switzerland, is described based on 34 specimens. The impression of an indeterminate astropectinid sea star has also been found. The fully articulated specimens have been smothered by mobile oolitic dunes or sandwaves. The site can be genetically classified as an obrution deposit and belongs to the widely recognized “Hauptrogenstein type”. The remains are assigned to the genus Geocoma d’Orbigny 1850, best known from the type species, G. carinata (Münster), from the Tithonian Plattenkalk of Zandt. As suggested by Kutscher (1997) this species also includes Ophiocten kelheimense Boehm 1889, now documented by numerous well-preserved specimens from the Plattenkalk of Hienheim. Kutscher assigned the Hienheim specimens to the genus Sinosura Hess 1964 and used both names though G. carinata has priority. Despite rather small differences Sinosura is retained as a valid genus besides Geocoma, and both are placed in the family Aplocomidae Hess 1965. Geocoma and Sinosura share small adpressed arm spines with Aplocoma d’Orbigny 1852. Aplocoma is represented by a number of Triassic and Jurassic species, and the subfamily Aplocominae is proposed herein for the three genera. A second subfamily, Ophiopetrinae, is proposed for the genera Ophiopetra Enay &; Hess 1962 and Ophiohybris Hess 1964, and is characterized by larger, erect arm spines.  相似文献   
6.
This paper is concerned with the famous fossil-bearing carbonate concretions of the Romualdo Member of the Santana Formation Konservat Lagerstätten of north-east Brazil. This palaeontologically important horizon was first dated as Cretaceous by the French palaeoichthyologist Louis Agassiz on the basis of fish fossils obtained by Bavarian explorers Spix and Martius between 1817 and 1820 and Scottish botanist and explorer George Gardner between 1836 and 1841. Gardner equated the concretion level with the English Albian ‘Upper Greensands’ on the basis of an imagined similarity of stratigraphic sequence with that of the Isle of Wight, southern England. Since then high precision dating of this remarkable deposit has proved elusive and the concretion-bearing part of the Santana Formation has been variously dated as early Late Cretaceous or late Early Cretaceous. Attempts at greater precision over the last 30 years have cited its age variously as Aptian, Albian or possibly Cenomanian, but few reliable data have been presented to support these dates.  相似文献   
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