scholarly journals Crystalline stenonian time features from earth and beyond

Substantia ◽  
2021 ◽  
pp. 99-114
Author(s):  
Desmond E. Moser

The writings of Niels Stensen (Steno) on mineral growth and modification in his Prodromus, together with his work on time and process in other solids, are here synthesized as five classes of time features defined by changes in the visible continuity of either or both chemistry and orientation. This organization highlights Steno’s implicit recognition of the fractal, scale-invariant nature of natural time features with regard to space, time, and material. The effectiveness and validity of this Stenonian geochronology framework is demonstrated down to atom scale with modern case studies of the U-Pb geochronology mineral zircon from samples originating from the Earth, Moon, and Mars and spanning most of solar system history. Recently discovered nano-scale features, here termed chronostructures, were intimated by Steno in his corpuscular view of mineral behaviour. The remarkable advances in the Prodromus are seen here as a resulting from the intersection of Steno’s highly attuned approach to visual perception, his adoption of Stoic (Senecan) ethics early in his career to guide his natural philosophy, and the influence of the Galilean scientific environment of Florence. It is shown that, by virtue of its scale-invariant and intensive properties, Stenonian geochronology continues to serve as an independent and critical check on the accuracy of absolute geochronology measurements of geologic time given the latter’s inherent dependence on sample volume and the assumption of the chemically closed system.  In this way Steno’s scientific legacy continues to help propel human understanding of how we see our place in time. 

2009 ◽  
Vol 14 (1-3) ◽  
pp. 290-315 ◽  
Author(s):  
Michael Shank
Keyword(s):  

AbstractIn 1499, while Copernicus studies in Bologna, the commentary on Sacrobosco's Sphere by the Padua master Francesco Capuano da Manfredonia first appears in print. It will be revised and reprinted several times thereafter. Like Copernicus, Capuano has a high view of astronomy and mingles astronomical and physical considerations (flies moving on wheels, men on ships, impetus, comets, raptus). Also, Capuano offers a flawed argument against a two-fold (diurnal and zodiacal) motion of the Earth. Multiple thematic resonances between Capuano's commentary and De revolutionibus, I, 5-11, suggest the hypothesis that Copernicus is answering Capuano, whose work was owned by Joachim Rheticus, if not Copernicus himself.


Author(s):  
Elisabeth Ervin-Blankenheim

This book is a scientific, historical, and philosophical narrative for general readers that explores the relationship between humans and the Earth and the geologic principles of time, plate tectonics, and change in life forms. Illustrated with striking historical maps, figures, and pictures, this comprehensive work can be read as a thrilling biography of the Earth itself, including narrative sections on the lives of pioneering geologists; the reality and sublimity of geologic time; the birth, destruction, and rebirth of the planet and its atmosphere over repeated cycles spanning some 4-plus billion years; the science underlying both mountain building and oceanic evolution; the influence of climate change and species extinction on the development of the Earth; and the interplay between not only how Earth has influenced life but how life, in turn, has distinctly shaped our planet.


2021 ◽  
Vol 40 (2) ◽  
pp. 293-331
Author(s):  
GIAN BATTISTA VAI

Anniversaries for the two founding fathers of geology occurring in the same year prompted a comparative evaluation of how the two contributed to establishing the basic principles of the discipline. To do so, passages from their publications, codices and manuscripts have been quoted directly. The Stenonian principles (‘original horizontality’, ‘original continuity’, and ‘superposition of individual strata’) are present in Leonardo’s notebooks amazingly formulated, using similar wording when studying the same area more than 150 years earlier. Also, Stenonian priority in naming and explaining geological concepts and processes (e.g., faulting, folding, angular unconformity, relative chronology) are mirrored in Leonardo’s writings and pictorial works. While Steno enjoys priority in stepwise restoration of the geological history of a given region, Leonardo was the first to construct a 3D geological profile representation and geomorphologic maps. Lastly, the paper focuses on diverging stances of the two savants about the Noachian Deluge and the age of the Earth. Already 500 years ago, Leonardo had solved the question of marine fossil remains of organic origin found in the mountains implying the possibility of deep geologic time in a statement of ‘eternalism’. 350 years ago, Steno solved the same question in a different way in which he retained a basic role for the Deluge and assumed a short age for the Earth by focusing mainly on short-lived sedimentary and geomorphologic processes.


2021 ◽  
pp. 163-180
Author(s):  
Elisabeth Ervin-Blankenheim

The way the planet has changed through geologic time, and life on it, the account of the Earth, is the topic of this and the next three chapters, starting in this chapter with the Precambrian Supereon. The overarching principles of geologic time, plate tectonics, and evolution worked dynamically to create the biography of the planet. This chapter traces back to the recesses of the geologic record and early Earth, from its birth and the formation of the Moon through seven-eighths of its existence, a huge span of time. Early life forms emerged during this supereon in the Archean Eon and had a profound influence on other Earth systems. Life interacted and changed the chemistry of the atmosphere through photosynthesis, so much so that the changes are thought to have sent planetary systems over an edge into multiple “Snowball Earth” episodes when most of the planet froze over. In addition to the beginning of organic life and climate, the emergence and configuration of the continents during the Precambrian are covered. Events of this supereon set the stage for the burgeoning of life forms in the next eon, the Phanerozoic.


Author(s):  
Peter Anstey

John Locke was the leading English philosopher of the late seventeenth century. His two major works, An Essay concerning Human Understanding and Two Treatises of Government, both published in 1690, have exerted enormous influence on subsequent thought, particularly in metaphysics, theory of knowledge and political philosophy. Locke’s writings were central to the philosophy of the Enlightenment in the eighteenth century and set the terms of reference for modern liberalism. Educated in the arts at Oxford, a friend of Robert Boyle and Isaac Newton, and a close associate of the leading politician the first Earl of Shaftesbury, Locke’s intellectual range was broad. He trained as a physician, dabbled in chemistry and botany and throughout his life kept abreast of developments in natural philosophy. At the same time, he developed theories of natural law and religious toleration, contributed to debates on contemporary economic issues, wrote a primer on the philosophy of education, defended the reasonableness of Christianity and maintained an extensive correspondence and intellectual network. It was not until the publication of the Essay when Locke was in his late 50s, however, that he became a public intellectual. The Essay provides an analysis of the scope and limits of the faculty of human understanding, using a sophisticated theory of ideas. It contains four books, the first of which seeks to refute the view that the mind contains innate metaphysical and moral principles. The second book sets out Locke’s theory of ideas and contains original and penetrating treatments of the nature of the will and motivation and the nature of personal identity. It also contains Locke’s theory of material qualities with his famous distinction between primary and secondary qualities, and discussions of the nature of substance, duration, infinity and the association of ideas. Book Three deals with the nature of language, the theory of essences, and provides an account of the way in which humans divide substances into species. Book Four uses the resources set out in the preceding books to develop a theory of knowledge and belief and to explore the differences between faith and reason. Central to Locke’s project is the view that all knowledge is constructed out of ideas. Knowledge in its most basic form is nothing but the perception of the agreement or disagreement of ideas and ideas can only be acquired through the senses or through introspection on the operations of our minds. Once the understanding is furnished with enough simple ideas from these two sources of experience, it sets about constructing complex ideas, forming propositions out of its various ideas and giving the ideas names. Locke is fundamentally opposed to the view that knowledge and reason begin with a set of basic principles or maxims, such as that the whole is the sum of its parts. This is the motivation for his arguments against the claim that principles are innate. Instead we must construct the principles of all the different sciences from scratch out of our stock of ideas. In the cases of mathematics and morality this can be achieved. In the case of our knowledge of the sorts or species of substances we encounter in the external world, however, we are significantly constrained. This is because our senses are limited and we do not have epistemic access to the inner natures of things. We can see many effects but the underlying causes of those effects, such as magnetism or cohesion, are out of reach. As a result, Locke is pessimistic about the prospects of natural science, though he does believe that the method of experimental philosophy, particularly natural history, gives us the best chance to extend our knowledge of the natural world. Moreover, he believes that of all the speculative systems of natural philosophy, the corpuscular view of matter is the most intelligible. Locke’s political philosophy gives us some insight into his conception of the form that a demonstrative moral philosophy might take. However, the precise relation between the Two Treatises and the Essay remains a controversial issue. The starting point for Locke’s view of the formation of civil society is the natural equality of every human being. We are equal in freedom and equal in both power and obligation with respect to the law of nature. However, in the absence of civil society – that is, in the state of nature – we suffer many inconveniences, particularly with regard to protecting property and applying the law of nature. It is only by consenting to give up our basic power to enforce the law of nature, a power that is common to all, to an authority, that we are able to overcome the inconveniences of the state of nature. In so doing, we secure the integrity of our property, that is, our life, liberty and possessions. The handing over of our basic power does not render us politically impotent however. For, should the government, whether a democracy, oligarchy or monarchy, break the people’s trust, the citizens have a right of resistance and can dissolve the government. Locke’s Two Treatises was published anonymously and did not embroil him in ongoing debate in his own day, though its subsequent influence was profound. The same cannot be said of another anonymous work, his A Letter Concerning Toleration, which argued that religious toleration should be extended to all but atheists and those who submit to foreign authority. The most vigorous reaction to Locke’s writings, however, was to the Essay, particularly to Locke’s account of personal identity as continuity of consciousness and his suggestion that matter fitly disposed might have the power of thought. These two issues are indicative of the rich philosophical resources within the Essay, both in its positive theses and its illustrative material, which have ensured that this work continues to be read and studied with profit today.


2020 ◽  
Author(s):  
Paloma Ramírez Vongrejova ◽  
María José Massé Rodríguez

<p><span>There is widespread agreement among my fellow colleagues who teach Geology that the History of our planet is a tough topic for teenagers. Unfortunately, not only is the subject considered boring but also useless by the majority of our school students.</span></p><p><span>Our experience teaching these contents in a traditional way has shown us that pupils vaguely remember anything. In order to give a different approach to this issue and, therefore, to promote meaningful learning, we have designed a project where students must be fully engaged.</span></p><p><span>First, the class was organized in cooperative learning groups, so they had to collaborate to complete the task. Then, they started the research period using laptop computers available in the school. Students now dealt with specific vocabulary such as the geologic time scale terms but also a variety of events that occurred from the very first moments, from the formation of the Earth itself to the development of the big reptiles that have always fascinated children and adults, especially their dramatic extinction.</span></p><p> <span><span>Once the topic was developed in detail, they were required to make a poster on scale with the information collected. It was undeniable that pictures or photographs must cover most of the poster as long as short sentences describing both biological and geological phenomena. What we were also concerned about their learning was to improve their creativity. Because of this, they were encouraged to make their own drawings.</span></span></p><p><span>Students really liked the activity, built stronger relationships between them and the final products were so amazing that were exhibited in the walls of the hallways outside their classroom.</span></p><p><span>All these events have been recorded in the rocks so geologists could unfold part of the mysteries of our History. Our teenagers discovered them an represented them for us to enjoy.</span></p>


2020 ◽  
Author(s):  
Claire Marie Guimond ◽  
Oliver Shorttle ◽  
John F. Rudge

<p>Topography is a crucial component of the Earth system: having rock exposed to the atmosphere lets surface temperatures self-regulate via silicate weathering, for example. However, there are limits to a lithosphere’s capacity to support mountains or valleys over geologic time. We see in our solar system that the range in a body’s elevations tends to decrease with increasing planet mass. These trends, inherent to planetary building materials, are modelled using well-studied concepts from geodynamics. As a first step, we predict feasible thermal evolutions and dynamic topography scaling relationships for rocky planets, eventually gearing to ask how massive a planet can be and still likely maintain subaerial land.</p>


1989 ◽  
Vol 8 (2) ◽  
pp. 103-105
Author(s):  
Cecil Schneer

There is evidence of consciousness of natural time as far back as the Early Ice Age in recorded observations of the recurrent and successive appearances of the moon. The idea of geologic time was broached as part of the 17th century scientific revolution in the same milieu as the ideal time of rational mechanics, but the sense of time drawn from observations of the earth transcended the limitations of ideal physical law. Inapplicable to "…an unlimited assemblage of local instabilities…" (Maxwell, 1877 p. 14), the laws of physics by definition are independent of the very particulars of time and place that are the essence of historical science. In the 18th century, Hutton formulated a physically dynamic theory of earth history as an indefinitely repeating series of cycles, while continental geologists such as Arduino and Werner constructed an ordinal classification of the major rock formations from primary crystalline basement to the alluvium of the present surface. The detailed scale of geological time as expressed in the geologic column was made possible by the discovery (principally by G. Cuvier and A.Brongniart and independently W. Smith) of the principle of faunal succession. By 1836, a consensus on the main outlines of the structure and biologic, as well as lithologic, succession was reached that held almost up to the present day. With temporal succession, the static scala naturae of Aristotle became first the progressionism of the great chain of being and finally, Darwinian evolution. The idea of geologic time encompasses all that we have learned of the history of our earth and its life.


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