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                <text>De wetenschap van de kosmos</text>
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                <text>&lt;p&gt;
	Wat zou iedereen moeten weten van de sterrenkunde? Hoeveel sterren er zijn en welke namen ze in verschillende culturen hebben gekregen, is wellicht niet zo relevant. Belangrijker is het inzicht dat de scheikundige elementen in sterren zijn ontstaan, dat wij sterrenstof zijn, en dat de hele kosmos in evolutie is en een begin heeft gehad dat we de oerknal noemen. Verder willen wij graag weten hoe uniek onze planeet en haar biosfeer zijn in dit grote heelal. Deze topics komen in dit boek dan ook uitgebreid aan bod. Daarnaast is er veel aandacht voor misschien wel het meest fundamentele inzicht uit de studie van het heelal: de wetten van de natuurwetenschappen zijn,in tegenstelling tot bijvoorbeeld onze taalwetten, overal geldig. De herkenning van de universaliteit van de natuurwetten betekent niet dat we alles weten, maar het maakt het laboratorium om ze te bestuderen een stuk groter! De universaliteit van de natuurwetten is vooral een goede leidraad gebleken bij het ontrafelen van onze geschiedenis in kosmisch perspectief. Want ten gronde stelt de sterrenkunde dezelfde vraag als elke andere wetenschap: wie zijn wij?&lt;/p&gt;
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                <text>This book describes what will ultimately happen to the contents of the universe. To understand the universe in the far future, we must first describe its present state and structure on the grand scale, and how its present properties arose. Dr Islam explains these topics in an accessible way in the first part of the book. From this background he speculates about the future evolution of the universe and predicts the major changes that will occur. The author has largely avoided mathematical formalism and therefore the book is well suited to general readers with a modest background knowledge of physics and astronomy.</text>
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                <text>&lt;p&gt;
	Most astronomers and physicists now believe that the matter content of the Universe is dominated by dark matter: hypothetical particles which interact with normal matter primarily through the force of gravity. Though invisible to current direct detection methods, dark matter can explain a variety of astronomical observations. This book describes how this theory has developed over the past 75 years, and why it is now a central feature of extragalactic astronomy and cosmology. Current attempts to directly detect dark matter locally are discussed, together with the implications for particle physics. The author comments on the sociology of these developments, demonstrating how and why scientists work and interact. Modified Newtonian Dynamics (MOND), the leading alternative to this theory, is also presented. This fascinating overview will interest cosmologists, astronomers and particle physicists. Mathematics is kept to a minimum, so the book can be understood by non-specialists.&lt;/p&gt;
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	 &lt;/p&gt;
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	&lt;p&gt;
		How did the Solar System's chemical composition evolve? This textbook provides the answers in the first interdisciplinary introduction to cosmochemistry. It makes this exciting and evolving field accessible to undergraduate and graduate students from a range of backgrounds, including geology, chemistry, astronomy and physics. The authors - two established leaders who have pioneered developments in the field - provide a complete background to cosmochemical processes and discoveries, enabling students outside geochemistry to understand and explore the Solar System's composition. Topics covered include: - synthesis of nuclides in stars - partitioning of elements between solids, liquids and gas in the solar nebula - overviews of the chemistry of extraterrestrial materials - isotopic tools used to investigate processes such as planet accretion and element fractionation - chronology of the early Solar System - geochemical exploration of planets Boxes provide basic definitions and mini-courses in mineralogy, organic chemistry, and other essential background information for students. Review questions and additional reading for each chapter encourage students to explore cosmochemistry further.&lt;/p&gt;
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                <text>An introduction to Distance Measurement in Astronomy</text>
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                <text>&lt;div&gt;
	Distance determination is an essential technique in astronomy, and is briefly covered in most textbooks on astrophysics and cosmology. It is rarely covered as a coherent topic in its own right. When it is discussed the approach is frequently very dry, splitting the teaching into, for example, stars, galaxies and cosmologies, and as a consequence, books lack depth and are rarely comprehensive.
	&lt;p&gt;
		 &lt;/p&gt;
	&lt;p&gt;
		Adopting a unique and engaging approach to the subject &lt;strong&gt;An Introduction to distance Measurement in Astronomy&lt;/strong&gt; will take the reader on a journey from the solar neighbourhood to the edge of the Universe, discussing the range of distance measurements methods on the way. The book will focus on the &lt;em&gt;physical&lt;/em&gt; processes discussing properties that underlie each method, rather than just presenting a collection of techniques.&lt;/p&gt;
	&lt;p&gt;
		 &lt;/p&gt;
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		As well as providing the most compressive account of distance measurements to date, the book will use the common theme of distance measurement to impart basic concepts relevant to a wide variety of areas in astronomy/astrophysics.&lt;/p&gt;
	&lt;p&gt;
		 &lt;/p&gt;
	&lt;p&gt;
		The book will provide an updated account of the progress made in a large number of subfields in astrophysics, leading to improved distance estimates particularly focusing on the underlying physics. Additionally it will illustrate the pitfalls in these areas and discuss the impact of the remaining uncertainties in the complete understanding of the Universes at large. As a result the book will not only provide a comprehensive study of distance measurement, but also include many recent advances in astrophysics.&lt;/p&gt;
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	&lt;div style="height:auto;"&gt;
		&lt;div&gt;
			&lt;div&gt;
				This comprehensive volume reviews the current theory and measurement of various parameters related to the evolution of the universe. Topics include inflation, string theory and the history of cosmology in the context of current measurements being made of the Hubble constant, matter density, and dark energy. Observational results are included from the Sloan, Digital Sky Survey, Keck, Magellan, cosmic microwave background experiments, Hubble space telescope and Chandra. Featuring chapters by leading authorities in the field, this book is a valuable resource for graduate students and professional research astronomers.&lt;/div&gt;
		&lt;/div&gt;
	&lt;/div&gt;
	&lt;div style="height:20px;"&gt;
		&lt;div&gt;
			&lt;a href="http://www.amazon.com/Measuring-Modeling-Universe-Observatories-Astrophysics/dp/052175576X#"&gt;Show More&lt;/a&gt;&lt;/div&gt;
	&lt;/div&gt;
	&lt;div style="padding-top:3px;"&gt;
		&lt;a href="http://www.amazon.com/Measuring-Modeling-Universe-Observatories-Astrophysics/dp/052175576X#"&gt;Show Less&lt;/a&gt;&lt;/div&gt;
&lt;/div&gt;
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	Clusters of galaxies are the largest and most massive collapsed systems in the Universe, and as such they are valuable probes of cosmological structure and galaxy evolution. The advent of extensive galaxy surveys, large ground-based facilities, space-based missions such as HST, Chandra and XMM-Newton and detailed numerical simulations makes a particularly exciting time to be involved in this field. The review papers in this volume span a comprehensive range of research in this area, including theoretical expectations for the growth of structure, survey techniques to identify clusters, metal production and the intracluster medium, galaxy evolution in the cluster environment and group-cluster connections. With contributions from leading authorities in the field, this volume is appropriate both as an introduction to this topic for physics and astronomy graduate students, and as a reference source for professional research astronomers.&lt;/div&gt;
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                <text>Het geheim van de kosmologie ontrafeld</text>
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                <text>In het jaar 1610 brengt Galileo Galileï zijn boodschap van de sterren. Met zijn publicatie Sidereus Nuncius (Sterrenbericht) markeert hij het begin van de moderne astronomie.&lt;br /&gt;&lt;br /&gt;
Zowat 400 jaar later geeft Gustaaf C. Cornelis de moderne lezer een stand van zaken. Deze historische ontdekkingsreis naar verleden en heden van de kosmologie is geen traditioneel handboek of encyclopedisch naslagwerk. Het is een associatief gegroeid relaas waarin de auteur met uiterste precisie scherpstelt op sleutelpassages van het kosmologische verhaal, waarin hij populaire misvattingen rechtzet en de rol van de wiskunde aantoont zonder te vervallen in een specialistisch formularium.&lt;br /&gt;&lt;br /&gt;
Heel wat (vaak gestelde) vragen passeren de revue: Hoe komen sterren tot ontwikkeling?&lt;br /&gt;&lt;br /&gt;
Waar komen de elementen vandaan? Waarom is de Aarde rond? Waarom werd Galileï door het Vaticaan veroordeeld? Was Einstein nu echt religieus of niet? Waarom weten we zoveel en toch zo weinig? Wat is wetenschap? Wat is filosofie?&lt;br /&gt;&lt;br /&gt;
Het resultaat is een wetenschapshistorische pageturner, waarin gaandeweg de rode draad zichtbaar wordt: de beslissende rol die de sterrenkunde gespeeld heeft in de totstandkoming van het huidige kosmologische wereldbeeld.&lt;br /&gt;&lt;br /&gt;
Het geheim van de kosmologie ontrafeld is een wetenschappelijk onderbouwd verhaal over sterren kunde en sterrenkundigen. Een eigenzinnig verhaal, verrassend, intens en wijd. Een cyclisch, associatief en idiosyncratisch verhaal van een gepassioneerd wetenschapsfilosoof. Een levensverhaal, ten dienste van een waarheid, zijn waarheid.&lt;br /&gt;&lt;br /&gt;</text>
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                <text>Stephen Hawking is de meest briljante theoretisch natuurkundige sinds Einstein. Hij is waarschijnlijk het grootste wetenschappelijke genie van deze tijd. Hij is tevens een succesvol schrijver die de ingewikkeldste onderwerpen voor gewone geesten toegankelijk maakt. Stephen Hawking in 3 minuten is een beknopte kennismaking met dit uitzonderlijke genie. Elk onderwerp is verdeeld in stukjes die de lezer in 3 minuten makkelijk tot zich kan nemen. De 3 delen Leven, Theorieën en Invloed beslaan elk een uur vol fascinerende feiten.</text>
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