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                <text>... de rest zijn details : Einstein 1905-2005</text>
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                <text>&lt;p&gt;
	 &lt;/p&gt;
&lt;p&gt;
	&lt;span class="goog_qs-tidbit goog_qs-tidbit-0"&gt; Tentoonstellinggids&lt;/span&gt;&lt;/p&gt;
&lt;p&gt;
	&lt;span class="goog_qs-tidbit goog_qs-tidbit-0"&gt;De tentoonstelling ,,... de rest zijn details" zal van 15 juli tot&lt;/span&gt; 18 september te zien zijn. Ze wordt georganiseerd door de Katholieke Universiteit Leuven, en is eerder te zien in Leuven en Kortrijk," vertelt cultuurschepen Christine Beirens. ,,Onze cultuurdienst en bibliotheek zullen daarnaast een aanvullende tentoonstelling over Einstein in De Haan samenstellen. Als afsluiting van de tentoonstelling is &lt;span class="goog_qs-tidbit goog_qs-tidbit-1"&gt;er een vormingsweekend met professor Christian Maes als gastdocent.&lt;/span&gt; Daarnaast organiseert Markant een Einstein-fotozoektocht."&lt;/p&gt;
&lt;!--para7--&gt;</text>
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	&lt;span class="f"&gt;Miklós&lt;/span&gt; &lt;span class="e"&gt;Konkoly&lt;/span&gt; &lt;span class="a"&gt;Thege&lt;/span&gt; (1842-1916) was a wealthy Hungarian nobleman who established a private observatory at Ógyalla, nowadays a state institution known as the &lt;span class="e"&gt;Konkoly&lt;/span&gt; Observatory. This interesting book is the proceedings of a workshop held in 1999 to celebrate the 100th anniversary of the founding of the Astronomical Research Institute of the Hungarian Academy of Sciences, based on the &lt;span class="e"&gt;Konkoly&lt;/span&gt; Observatory. There are five parts to the book. The first is about the history of the &lt;span class="e"&gt;Konkoly&lt;/span&gt; Observatory and its activities. &lt;span class="e"&gt;Konkoly&lt;/span&gt; &lt;span class="a"&gt;Thege&lt;/span&gt; was very active in instrumental matters - his book Praktische Anleitung ... (1883) was influential during the period when &lt;span class="d"&gt;astrophysics&lt;/span&gt; was undergoing its first period of rapid development, and a copy of it exists in the SAAO collection. &lt;span class="e"&gt;Konkoly&lt;/span&gt; was a pioneer in astronomical photometry and spectroscopy and made use of the Zöllner visual photometer as well as the schraffierkassette method for photographic photometry. The second part of the book is concerned with early &lt;span class="d"&gt;astrophysics&lt;/span&gt; in various countries. The article on Japanese astronomy around 1899 (by M Takeuti) deals with a period not covered by articles in English. At this time, Japan was still recovering from the two centuries of isolation imposed by the Edo Shogunate, and research astronomy was just beginning. CD Laney's Astronomy in the Dismal Swamp, a quirky collection of stories about the Royal Observatory, Cape, follows. Other chapters deal with the Marseille Observatory and the French astronomer Jules Janssen (1824-1907). Two articles by J Hearnshaw and K Staubermann deal with the history of astronomical photometry in the third part. The fourth part is about early female astronomers and the difficulties they faced, including paragraphs on Dorothea Klumpke (who married Isaac Roberts), Agnes Clerke, Maria Mitchell and the famous ladies of the Harvard Observatory who worked on spectral classification and the Cepheid period-luminosity relation. Most of the last part is a fascinating account of the cosmological development of General Relativity by Einstein, de Sitter, Lanczos, Lemaître Friedmann and Robertson, and how they influenced and were influenced by the observers. Nowadays one tends to think of Edwin Hubble in connection with the expansion of the Universe, but he was only one of several to whom the credit for this work is due. The article on this subject by H Duerbeck and W Seitter attemps to give an unbiassed history of early developments.&lt;/blockquote&gt;
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                <text>1543-1642, een eeuw Copernicanisme : ook voor de Zuid-Nederlander?</text>
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                <text>1642, een eeuw Copernicanisme: ook voor de Zuid Nederlander? (Steve Philips) home lijst scripties inhoud vorige ... volgende 4.1 Van Aristoteles tot Galileï. Het Copernicanisme is een onderdeel van de grote Wetenschappelijke Revolutie, die in de tweede helft van de zestiende eeuw begon. Deze verandering in de gedachten schudde in de loop der tijden definitief het oude aristotelische-ptolemeïsch of geocentrisch wereldbeeld door elkaar. Aristoteles (384 – 322 v. Chr.) ging ervan uit dat de aarde het centrum van het heelal vormde. Volgens hem waren er ook vier oerelementen: aarde, water, lucht en vuur. In hun zuiverste toestand werden ze de vier aardse sferen genoemd. Deze bevonden zich in het ondermaanse. Buiten het ondermaanse trof men een ring van zeven bolvormige lagen uit ether (de vijfde materie) aan. Elk van deze lagen of sferen bevatte een planeet. De toen gekende planeten waren: Zon, Maan, Mercurius, Venus, Mars, Jupiter, Saturnus. Daaromheen was het firmament, een achtste sfeer met de vaste sterren erop gemonteerd. De buitenste bewegende sfeer, die alle andere sferen in beweging zette, werd aangeduid als het Primum Mobile. Daarachter bevond zich het verblijf van God, in aristotelische termen als de Onbewogen Beweger aangeduid. . Alles wat zich buiten het ondermaanse bevond, was ook niet aan verandering onderhevig en volmaakter dan de aardse ‘zaken’. Daarom werd een komeet in het aristotelisch denken als iets ondermaans beschouwd.</text>
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	&lt;span class="reviewText"&gt;Well-balanced, carefully reasoned study relates astronomy to political, social conditions of the day. Part I covers ancient astronomy, including Ptolemaic theory; Part II discusses Copernicus, Kepler, Newton, laws of celestial mechanics. Part III covers modern developments up to work of Eddington. Author saw astronomy as an adventure of the mind. Illustrated.&lt;/span&gt;&lt;/div&gt;
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                <text>Complete, thorough history: Near Eastern, early Greeks, homocentric theories, Ptolemaic system, medieval cosmology, Copernicus, Kepler, etc. This volume is a Dover republication of Dreyer's "History of the Planetary Systems from Thales to Kepler" originally published in 1906. &lt;span class="goog_qs-tidbit goog_qs-tidbit-0"&gt;The first Dover reprint, revised and with a foreword by W.H. Stahl, was published in&lt;/span&gt; 1953.</text>
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                <text>The Celestial Sphere: its Poles true even if he moves to another place. A sphere has, however, only one centre, and therefore if the sphere remains fixed the observer cannot move about and yet always remain at the centre. The old astronomers met this difficulty by supposing that the celestial sphere was so large that any possible motion of the observer would be insignificant in comparison with the radius of the sphere and could be neglected. It is often more convenient—when we are using the sphere as a mere geometrical device for representing the position of the stars—to regard the sphere as moving with the observer, so that he always remains at the centre. 8. Although the stars all appear to move across the sky (§ 5), and their rates of motion differ, yet the distance between any two stars remains unchanged, and they were / consequently regarded as being attached to the celestial ' sphere. Moreover a little careful observation would have shown that the motions of the stars in different parts of the sky, though at first sight very different, were just such as would have been produced by the celestial sphere—with the stars attached to it—turning about an axis passing through the centre and through a point in the northern sky close to the familiar pole-star. This point is called the pole. As, however, a straight line drawn through the centre of a sphere meets it in two points, the axis of the celestial sphere meets it again in a second point, opposite the first, lying in a part of the celestial sphere which is permanently below the horizon. This second point is also called a pole; and if the two poles have to be distinguished, the one mentioned first is called the north pole, and the other the south pole. The direction of the rotation of the celestial sphere about its axi... </text>
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                <text>One of America's best-known essayists on science, physicist Jeremy Bernstein, here presents his latest collection of work. Drawn from over ten years of writing for magazines such as The Atlantic, The New York Review of Books, The New Yorker, and Scientific American, these essays provide illuminating accounts of the lives of some of this century's most important scientists and the value of their work. Bernstein's fans who remember these pieces from their original publication will be pleased to see that many that had to be cut - sometimes drastically - to fit magazine space requirements are here restored to their original length. Bernstein has added introductions and postscripts to many essays as well. In all, this collection contains a great deal of new and unpublished material. An added bonus is Bernstein's four pieces of published fiction - three of which are hilarious send-ups of academic and sexual politics at a small and (we hope) imaginary college.</text>
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	What star is that? Where is the Southern Cross? Who was Orion? This book answers these questions and many more. Its unique simplified maps make it easy to find the constellations in the southern hemisphere skies, and the stars within them. Clear instructions guide the user on how to gauge sizes and distances, and move easily between constellations. This new edition has been updated with additional mythology information, and a list of the planet positions up to 2016. The ancient myths and legends of the sky are retold to add to the mystery of the stars. Of value to all ages, this book introduces the patterns of the starry skies in a memorable way. No equipment is needed to use this practical guide: apart from normal sight and clear skies. Magically illustrated, this is an ideal introduction to launch the young astronomer on a journey across the starlit skies.&lt;/p&gt;
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	'You don't need a telescope to learn where the constellations are - this book tells you exactly how to find them simply by looking at the sky. It's a useful skill to acquire: you can impress your friends when you stumble out of the pub by pointing out what's where in the night sky. The legends are fascinating too. This is a good book for someone who hasn't made their mind up about investing in a telescope.' The Times 'Its unique, simplified maps not only make constellations easy to find but also help locate the stars within them. Without having to use a telescope or other astronomical equipment, readers can gauge the sizes and separations between constellations, and easily move from one to the other, by simply following the book's clear instructions. In addition, the ancient myths and legends surrounding the constellations, are retold, providing a rich historical perspective.' Astronomical Society of the Pacific 'This accessible book provides you with simple, straightforward maps of the southern sky constellations and the mythology of some of the more notable ones. It's a must if you're planning a trip to go observing Down Under.' BBC Sky at Night 'Ideal for the back-garden star-gazer ... this handbook helps one navigate through the visible stars and constellations without needing a telescope, and provides sufficient background information and historical anecdotes to whet the appetite of all but the most persistent armchair astronomer. ... The descriptive charts are plentiful, uncomplicated and clearly labelled, and anticipate most queries that could arise during casual viewing. ... a good incentive to get out of that armchair and have a good try. For those who normally see the southern skies, this volume is an excellent way to get started.' The Observatory&lt;/p&gt;
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