Many critics consider The Initials of the Earth to be the quintessential novel of the Cuban Revolution and the finest work by the Cuban writer and filmmaker Jesús Díaz. Born in Havana in 1941, Díaz was a witness to the Revolution and ardent supporter of it until the last decade of his life. In 1992 he took up residence as an exile in Berlin and later in Madrid, where he died in 2002. This is the first of his books to be translated into English. Originally written in the 1970s, then rewritten and published simultaneously in Havana and Madrid in 1987, The Initials of the Earth spans the tumultuous years from the 1950s until the 1970s, encompassing the Revolution and its immediate aftermath. The novel opens as the protagonist, Carlos Pérez Cifredo, sits down to fill out a questionnaire for readmission to the Cuban Communist Party. It closes with Carlos standing before a panel of Party members charged with assessing his merit as an “exemplary worker.” The chapters between relate Carlos’s experiences of the pre- and postrevolutionary era. His family is torn apart as some members reject the Revolution and flee the country while others, including Carlos, choose to stay. He witnesses key events including the Bay of Pigs invasion, the Cuban missile crisis, and the economically disastrous sugar harvest of 1970. Throughout the novel, Díaz vividly renders Cuban culture through humor, slogans, and slang; Afro-Cuban religion; and references to popular music, movies, and comics. This edition of The Initials of the Earth includes a bibliography and filmography of Diaz’s works and a timeline of the major events of the Cuban revolutionary period. In his epilogue, the Cuban writer Ambrosio Fornet reflects on Díaz’s surprising 1992 renunciation of the Revolution, their decades-long friendship, and the novel’s reception, structure, and place within Cuban literary history.

The Creator sat upon the throne, thinking. Behind him stretched the illimitable continent of heaven, steeped in a glory of light and color; before him rose the black night of Space, like a wall. His mighty bulk towered rugged and mountain-like into the zenith, and His divine head blazed there like a distant sun. At His feet stood three colossal figures, diminished to extinction, almost, by contrast -- archangels -- their heads level with His ankle-bone. When the Creator had finished thinking, He said, "I have thought. Behold!" He lifted His hand, and from it burst a fountain-spray of fire, a million stupendous suns, which clove the blackness and soared, away and away and away, diminishing in magnitude and intensity as they pierced the far frontiers of Space, until at last they were but as diamond nailheads sparkling under the domed vast roof of the universe. At the end of an hour the Grand Council was dismissed. They left the Presence impressed and thoughtful, and retired to a private place, where they might talk with freedom. None of the three seemed to want to begin, though all wanted somebody to do it.

The Early Earth: Accretion and Differentiation provides a multidisciplinary overview of the state of the art in understanding the formation and primordial evolution of the Earth. The fundamental structure of the Earth as we know it today was inherited from the initial conditions 4.56 billion years ago as a consequence of planetesimal accretion, large impacts among planetary objects, and planetary-scale differentiation. The evolution of the Earth from a molten ball of metal and magma to the tectonically active, dynamic, habitable planet that we know today is unique among the terrestrial planets, and understanding the earliest processes that led to Earth’s current state is the essence of this volume. Important results have emerged from a wide range of disciplines including cosmochemistry, geochemistry, experimental petrology, experimental and theoretical mineral physics and geodynamics. The topics in this volume include: Condensation of primitive objects in the solar nebula, planetary building blocks Early and late accretion and planetary dynamic modeling Primordial differentiation, core formation, Magma Ocean evolution and crystallization This volume will be a valuable resource for graduate students, academics, and researchers in the fields of geophysics, geochemistry, cosmochemistry, and planetary science.

'Earth's Climate' summarises the major lessons to be learned from 550 million years of climate changes, as a way of evaluating the climatological impact on and by humans in this century. The book also looks ahead to possible effects during the next several centuries of fossil fuel use.

Our planet faces many challenges. In 2013, an international partnership of more than 140 scientific societies, research institutes, and organizations focused its attention on these challenges. This project was called Mathematics of Planet Earth and featured English- and French-language blogs, accessible to nonmathematicians, as part of its outreach activities. This book is based on more than 100 of the 270 English-language blog posts and focuses on four major themes: A Planet to Discover; A Planet Supporting Life; A Planet Organized by Humans; and A Planet at Risk. Readers will learn about the challenges that confront the Earth today, and how mathematics and mathematicians contribute to a better understanding of some of these challenges. ?

To understand climate change today, we first need to know how Earth’s climate changed over the past 450 million years. Finding answers depends upon contributions from a wide range of sciences, not just the rock record uncovered by geologists. In Earth’s Climate Evolution, Colin Summerhayes analyzes reports and records of past climate change dating back to the late 18th century to uncover key patterns in the climate system. The book will transform debate and set the agenda for the next generation of thought about future climate change. The book takes a unique approach to the subject providing a description of the greenhouse and icehouse worlds of the past 450 million years since land plants emerged, ignoring major earlier glaciations like that of Snowball Earth, which occurred around 600 million years ago in a world free of land plants. It describes the evolution of thinking in palaeoclimatology and introduces the main players in the field and how their ideas were received and, in many cases, subsequently modified. It records the arguments and discussions about the merits of different ideas along the way. It also includes several notes made from the author’s own personal involvement in palaeoclimatological and palaeoceanographic studies, and from his experience of working alongside several of the major players in these fields in recent years. This book will be an invaluable reference for both undergraduate and postgraduate students taking courses in related fields and will also be of interest to historians of science and/or geology, climatology and oceanography. It should also be of interest to the wider scientific and engineering community, high school science students, policy makers, and environmental NGOs. Reviews: "Outstanding in its presentation of the facts and a good read in the way that it intersperses the climate story with the author's own experiences. [This book] puts the climate story into a compelling geological history." -Dr. James Baker "The book is written in very clear and concise prose, [and takes] original, enlightening, and engaging approach to talking about 'ideas' from the perspective of the scientists who promoted them." -Professor Christopher R. Scotese "A thrilling ride through continental drift and its consequences." - Professor Gerald R. North "Written in a style and language which can be easily understood by laymen as well as scientists." - Professor Dr Jörn Thiede "What makes this book particularly distinctive is how well it builds in the narrative of change in ideas over time." - Holocene book reviews, May 2016 "This is a fascinating book and the author’s biographical approach gives it great human appeal." - E Adlard