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Leslie Stephen (1832–1904) was an English biographer, and a writer on philosophy, ethics and literature. He was educated at Eton, King's College, London, and then Trinity College in Cambridge, where he remained as a fellow and a tutor for his entire career. He was also a keen mountaineer, taking part in first ascents of nine peaks in the Alps. He served as the first editor (1885–91) of the Dictionary of National Biography and in 1871 he became editor of the Cornhill Magazine. During his eleven-year tenure he wrote two successful books on ethics, of which this work, published in 1882, was one. It was widely adopted as a standard textbook on moral philosophy, and became one of the most influential publications on the ideas of evolutionary ethics that had been inspired by Darwin's theory of evolution by natural selection.
Though Kant is best known for his strictly philosophical works in the 1780s, many of his early publications in particular were devoted to what we would call 'natural science'. Kant's Universal Natural History and Theory of the Heavens (1755) made a significant advance in cosmology, and he was also instrumental in establishing the newly emerging discipline of physical geography, lecturing on it for almost his entire career. In this volume Eric Watkins brings together new English translations of Kant's first publication, Thoughts on the True Estimation of Living Forces (1746–9), the entirety of Physical Geography (1802), a series of shorter essays, along with many of Kant's most important publications in natural science. The volume is rich in material for the student and the scholar, with extensive linguistic and explanatory notes, editorial introductions and a glossary of key terms.
This two-volume work, first published in 1843, was John Stuart Mill's first major book. It reinvented the modern study of logic and laid the foundations for his later work in the areas of political economy, women's rights and representative government. In clear, systematic prose, Mill (1806–73) disentangles syllogistic logic from its origins in Aristotle and scholasticism and grounds it instead in processes of inductive reasoning. An important attempt at integrating empiricism within a more general theory of human knowledge, the work constitutes essential reading for anyone seeking a full understanding of Mill's thought. Volume 1 contains Mill's introduction, which elaborates upon his definition of logic as 'not the science of Belief, but the science of Proof, or Evidence'. It also features discussions of the central components of logical reasoning - propositions and syllogisms - in relation to Mill's theories of inductive reasoning and experimental method.
Within a few years of the publication of his Critique of Pure Reason in 1781, Immanuel Kant (1724–1804) was recognized by his contemporaries as one of the seminal philosophers of modern times – indeed as one of the great philosophers of all time. This renown soon spread beyond German-speaking lands, and translations of Kant's work into English were published even before 1800. Since then, interpretations of Kant's views have come and gone and loyalty to his positions has waxed and waned, but his importance has not diminished. Generations of scholars have devoted their efforts to producing reliable translations of Kant into English as well as into other languages.
There are four main reasons for the present edition of Kant's writings:
Completeness. Although most of the works published in Kant's lifetime have been translated before, the most important ones more than once, only fragments of Kant's many important unpublished works have ever been translated. These include the Opus postumum, Kant's unfinished magnum opus on the transition from philosophy to physics; transcriptions of his classroom lectures; his correspondence; and his marginalia and other notes. One aim of this edition is to make a comprehensive sampling of these materials available in English for the first time.
Availability. Many English translations of Kant's works, especially those that have not individually played a large role in the subsequent development of philosophy, have long been inaccessible or out of print. Many of them, however, are crucial for the understanding of Kant's philosophical development, and the absence of some from English-language bibliographies may be responsible for erroneous or blinkered traditional interpretations of his doctrines by English-speaking philosophers.
Organization. Another aim of the present edition is to make all Kant's published work, both major and minor, available in comprehensive volumes organized both chronologically and topically, so as to facilitate the serious study of his philosophy by English-speaking readers.
Consistency of translation. Although many of Kant's major works have been translated by the most distinguished scholars of their day, some of these translations are now dated, and there is considerable terminological disparity among them. Our aim has been to enlist some of the most accomplished Kant scholars and translators to produce new translations, freeing readers from both the philosophical and literary preconceptions of previous generations and allowing them to approach texts, as far as possible, with the same directness as present-day readers of the German or Latin originals.
Given the plethora of units in the German-speaking part of Europe in Kant's day, it is difficult to ascertain exactly which reference standard he was using on any given occasion. We may assume, however, that for the most part he used Prussian measures.
As Kant explains in § 8 of the Physical Geography, one ‘geographical mile’ was taken as 1/15 of a degree, measured along the Earth's circumference. Therefore there are 15 × 360 = 5,400 ‘geographical miles’ in the circumference of the Earth. Taking the modern value of 7,927 English miles for the equatorial diameter of the Earth, a geographical mile is thus 4.612 English miles. This figure may be used for the purposes of comparing Kant's astronomical data with modern measurements, as is done in Appendix ii. (It will be noted that good agreement is found for the diameter of the earth, which shows that the conversion factor of 4.612 is appropriate.) Also, since 7,927 is a known modern value, we may use it to gauge the value of the eighteenth-century units of length employed by Kant, even though we may not know exactly which standard he was referring to at any particular point in his text.It may be noted, however, that according to Ronald Zupko one Rhineland foot (as used in Prussia) was equal to 12.36 English inches (or 1.030 English feet). We have, therefore, a small discrepancy, but the information is adequate to gain a reasonably accurate estimate of which standard of length Kant was using.
The topic of this Kant's essay is whether the Moon has any influence on the Earth's weather. The attraction of the Moon, i.e., the only motive force by which it can have an influence on the atmosphere and possibly also on weather conditions, has a direct effect on the air in accordance with laws of statics, that is, insofar as it is a ponderable fluid. It is a question of deciding a priori whether or not the Moon has any influence on the weather, then the light that it casts on the Earth can be ignored, and so there remains only its attractive force. But the Moon['s attraction] is far too weak to effect any discernible change in the level of the barometer by this means, and, insofar as weather conditions are directly dependent on the cause of change. Therefore, it ought not to have any influence on the weather.
Kant, over the course of five notes, attempts to explain a series of specific meteorological phenomena, sometimes in novel ways. In the first and second notes, he claims that the direction of coastal winds depends on the expansion and contraction of air that is caused by differences in the rate of heating and cooling of the land and the water at sea during the day and at night. In the third, he explains the difference in (east-west) direction arising for winds moving from the Equator. In the fourth note, he talks about the Coriolis effect, and the easterly direction of the trade winds. Finally, Kant provides an account of monsoon winds. The atmosphere should be thought of as a sea of fluid, elastic material constituted, as it were, of layers of different density, which decreases as the height increases.
Kant's "Review of Silberschlag's Work: Theory of the Fireball that appeared on 23 July 1762" was published anonymously on 23 March 1764. While it is uncertain exactly what motivated Kant to respond in this way, the review is clearly positive. This work consists of two main parts, the first of which treats of the atmosphere, and the second of the fireball, to which further addenda are attached with reports and observations that had come in. The first part discusses air and its changes and views the sea of air as an atmosphere and a new division of regions of air is presented in addition to the various considerable remarks about mists, fog, clouds, and rain. The second part treats of the orbit the creation and the use of this meteor in three sections. The three copper plates illustrate the theory, the shape and the path that this fire-mass took.
Kant's aim in the essay Universal Natural History and Theory of the Heavens shows that the main elements of the entire observable universe, laying bare the basic structure that governs the universe. Kant does this in a preparatory section and three parts. In the preface, he is primarily interested in explaining why the view he wants to defend not only represents no threat to religious orthodoxy. In the first part, Kant draws an analogy between the structure of our solar system and that of the Milky Way and then between the Milky Way and the fixed stars. The second part explains the formation of the various significant bodies in our solar system their most distinctive features. In the third part, Kant concludes his treatment by engaging in fanciful speculation about the inhabitants of the other planets of our solar system, and returns to the theological context.
In this essay, Kant presents a description of the Lisbon earthquake and the events surrounding it. The earthquake was preceded by a vapour rising into the air that turned red in the atmosphere and made the torrential rains that ensued blood-red as well. Kant describes the tsunami caused by the earthquake, its effects in distant places, its speed of transmission and extent as well as its influence on springs. He theorizes about what geographical features are most conducive to earthquakes and the directions of motion of an earthquake, speculating the connection between earthquakes and the seasons and the influence of earthquakes on atmospheric conditions as well as their potential uses. Kant concludes with a sketch of a theodicy, according to which man often inappropriately views himself rather than nature as a whole as the object of God's actions, and in addition, man is in no position to know God's intentions.
In this essay, Kant defines what it would mean for the earth to be ageing, warning in particular against anthropocentric conceptions. He also provides detailed evaluations of four different accounts of how the earth might be ageing and by what causal mechanisms. The first is by the rivers stripping fertile salts from the land and delivering them into the ocean, thereby robbing the land of its ability to grow and sustain life. The second is by the rivers depositing sediment into the sea, which raises the sea until it inundates the land. The third is by the decrease of water (from the oceans) and the resultant increase of land. The fourth is by the decrease and gradual exhaustion of a hypothetical general 'world spirit' that sustains all living beings on earth. He concludes by criticizing those who would appeal to comets to explain "all manner of extraordinary" events.
Leibniz claimed to demonstrate that one of Descartes's fundamental laws of motion was false. Considerable controversy ensued, as two comprehensive natural philosophies were at stake. The central point of Kant's Thoughts on the True Estimation of Living Forces is seen as a sustained attempt at resolving this vis viva debate. This chapter presents the preface and three chapters of this book. In the preface, Kant makes the case that his thoughts should be taken seriously. In chapter one, Kant considers the proper notion of force and distinguishes two different kinds of motions that are fundamental resolving the debate. In chapter two, he presents a critique of Leibniz's position and of the various arguments he and his followers had advanced in its favor. In the third chapter, Kant presents his own resolution of the conflict between the Cartesian and the Leibnizian measures of force.
Kant published the first essay, "On the causes of earthquakes on the occasion of the calamity that befell the western countries of Europe towards the end of last year", in two instalments. His main contention is that earthquakes are caused by the conflagration of a mixture of iron filings, sulphur, or vitriolic acid, and water that has been compressed in extensive caverns lying below the Earth's surface. He argues that earthquakes are connected with volcanic activity, which have the same cause; and denies that they are caused by electricity, but allows for a connection with magnetic materials and atmospheric changes. According to Kant, the main line of earthquakes follows the direction of the highest mountains, and thus the countries that are chiefly affected are close to these, especially if they are enclosed by two mountain ranges, in which case the tremors combine from both sides.
On 1 April 1758, Kant published a short essay on motion and rest that contained a clear illustration of how he approaches the fundamental principles of mechanics. Kant presents an attack first on the concept of absolute motion and then on a conception of inertia that rests on absolute motion. Kant then turns to criticize what he takes to be the standard conception of inertia, namely the force a body at rest has to resist another body changing its state. Kant proceeds to adduce two further arguments against the traditional notion of inertia based on difficulties that arise in explaining how a body at rest could nonetheless suddenly set itself in motion prior to impact; and how motion could still occur if action and reaction were equal and thus cancelled each other out. He explains the law of continuity, and derives rules of impact from his corrected concept of motion.
Among Kant's publications, Physical Geography has a complex origin. It is a compilation of a variety of sources such as notes that Kant made for himself and updated only sporadically, student transcripts from different classes over several decades, and Rink's independent additions. Two further features of Kant's Physical Geography that need mention. First, Kant's contributions to physical geography can be assessed only against the background of the current state of knowledge of geography in general and of physical geography in particular. Second, Kant's knowledge of different geographical facts derives not from first-hand experience, given that he never travelled far from Konigsberg and thus never ventured outside the boundaries of East Prussia, but exclusively from the reports of others. Particularly the parts of the present work describing nature or dealing with natural history would require an almost complete revision.