Charles Darwin and Sir John FW Herschel
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Mister Mary Somerville: Husband and Secretary
Open Research Online The Open University’s repository of research publications and other research outputs Mister Mary Somerville: Husband and Secretary Journal Item How to cite: Stenhouse, Brigitte (2020). Mister Mary Somerville: Husband and Secretary. The Mathematical Intelligencer (Early Access). For guidance on citations see FAQs. c 2020 The Author https://creativecommons.org/licenses/by/4.0/ Version: Version of Record Link(s) to article on publisher’s website: http://dx.doi.org/doi:10.1007/s00283-020-09998-6 Copyright and Moral Rights for the articles on this site are retained by the individual authors and/or other copyright owners. For more information on Open Research Online’s data policy on reuse of materials please consult the policies page. oro.open.ac.uk Mister Mary Somerville: Husband and Secretary BRIGITTE STENHOUSE ary Somerville’s life as a mathematician and mathematician). Although no scientific learned society had a savant in nineteenth-century Great Britain was formal statute barring women during Somerville’s lifetime, MM heavily influenced by her gender; as a woman, there was nonetheless a great reluctance even toallow women her access to the ideas and resources developed and into the buildings, never mind to endow them with the rights circulated in universities and scientific societies was highly of members. Except for the visit of the prolific author Margaret restricted. However, her engagement with learned institu- Cavendish in 1667, the Royal Society of London did not invite tions was by no means nonexistent, and although she was women into their hallowed halls until 1876, with the com- 90 before being elected a full member of any society mencement of their second conversazione [15, 163], which (Societa` Geografica Italiana, 1870), Somerville (Figure 1) women were permitted to attend.1 As late as 1886, on the nevertheless benefited from the resources and social nomination of Isis Pogson as a fellow, the Council of the Royal networks cultivated by such institutions from as early as Astronomical Society chose to interpret their constitution as 1812. -
Autobiography of Sir George Biddell Airy by George Biddell Airy 1
Autobiography of Sir George Biddell Airy by George Biddell Airy 1 CHAPTER I. CHAPTER II. CHAPTER III. CHAPTER IV. CHAPTER V. CHAPTER VI. CHAPTER VII. CHAPTER VIII. CHAPTER IX. CHAPTER X. CHAPTER I. CHAPTER II. CHAPTER III. CHAPTER IV. CHAPTER V. CHAPTER VI. CHAPTER VII. CHAPTER VIII. CHAPTER IX. CHAPTER X. Autobiography of Sir George Biddell Airy by George Biddell Airy The Project Gutenberg EBook of Autobiography of Sir George Biddell Airy by George Biddell Airy This eBook is for the use of anyone anywhere at no cost and with almost no restrictions whatsoever. You may copy it, give it away or re-use it under the terms of the Project Gutenberg Autobiography of Sir George Biddell Airy by George Biddell Airy 2 License included with this eBook or online at www.gutenberg.net Title: Autobiography of Sir George Biddell Airy Author: George Biddell Airy Release Date: January 9, 2004 [EBook #10655] Language: English Character set encoding: ISO-8859-1 *** START OF THIS PROJECT GUTENBERG EBOOK SIR GEORGE AIRY *** Produced by Joseph Myers and PG Distributed Proofreaders AUTOBIOGRAPHY OF SIR GEORGE BIDDELL AIRY, K.C.B., M.A., LL.D., D.C.L., F.R.S., F.R.A.S., HONORARY FELLOW OF TRINITY COLLEGE, CAMBRIDGE, ASTRONOMER ROYAL FROM 1836 TO 1881. EDITED BY WILFRID AIRY, B.A., M.Inst.C.E. 1896 PREFACE. The life of Airy was essentially that of a hard-working, business man, and differed from that of other hard-working people only in the quality and variety of his work. It was not an exciting life, but it was full of interest, and his work brought him into close relations with many scientific men, and with many men high in the State. -
Further Reading: Michael Faraday
Further Reading: Michael Faraday General reading Geoffrey Cantor, Michael Faraday: Sandemanian and Scientist. A Study of Science and Religion in the Nineteenth Century, (London, 1991). David Gooding, Experiment and the Making of Meaning: Human Agency in Scientific Observation and Experiment, (Dordrecht, 1991). David Gooding and Frank A.J.L. James (eds.), Faraday Rediscovered: Essays on the Life and Work of Michael Faraday, 1791‐1867, (London, 1985). Frank A.J.L. James (ed.), ‘The Common Purposes of Life’: Science and society at the Royal Institution of Great Britain, (Aldershot, 2002). Frank A.J.L. James, Michael Faraday: A very short Introduction. (Oxford, 2010) Alan E. Jeffreys, Michael Faraday: A List of His Lectures and Published Writings, (London, 1960). Published books by Faraday, mainly collections of papers and lecture notes, some published after his death: Chemical Manipulation, Being Instructions to Students in Chemistry. (1827). Experimental Researches in Electricity, Vol I, II& III (1837, 1844, 1855) Experimental Researches in Chemistry and Physics (1859). W. Crookes. ed. A Course of six lectures on the Various Forces of Matter (1860) W. Crookes. ed. A Course of six lectures on the Chemical History of a Candle, (1861) W. Crookes. ed. On the Various Forces in Nature. (1873) The liquefaction of gases (1896.) Published texts by Faraday The vast majority of Faraday’s manuscripts, apart from letters, have been published on microfilm and cd. Frank A.J.L. James, Guide to the Microfilm edition of the Manuscripts of Michael Faraday (1791‐1867) from the Collections of the Royal Institution, The Institution of Electrical Engineers, The Guildhall Library [and] The Royal Society, (2nd ed., Wakefield, 2001). -
Herschel, Humboldt and Imperial Science
CHAPTER 41 Herschel, Humboldt and Imperial Science Christopher Carter In science, the nineteenth century is known as the beginning of a systematic approach to geophysics, an age when terrestrial magnetism, meteorology and other worldwide phenomena were studied for the first time on a large scale. International efforts to study the earth’s climate, tides and magnetic field became common in the first half of this century, in large part because of the impetus given to the field by the work of Alexander von Humboldt. Due to Humboldt’s influence, a system of geomagnetic observatories soon covered most of the European continent.1 But one prominent nation remained outside of this system of observations. Despite Britain’s inherent interest in geomag- netic studies (due to its maritime concerns) the laissez-faire attitudes of the British political system weakened efforts to subsidize state funded scientific projects. Not until the 1830s did Britain join with other European nations in the geophysical arena. This cooperation was beneficial to the science, as it brought not only Britain’s considerable scientific resources to bear on the problem, but it also opened up Britain’s imperial holdings as new stations to expand the observational system. Humboldt’s 1836 letter to the Duke of Sussex (President of the Royal Society), suggesting the establishment of geomagnetic observatories in Brit- ish colonies, provides an initial point of reference for our investigations.2 However, while welcomed by the scientific community, Humboldt’s appeal 1. By 1835, continental geomagnetic stations were operating at Altona, Augsburg, Berlin, Breda, Breslau, Copenhagen, Freiburg, Goettingen, Hanover, Leipzig, Marburg, Milan, Munich, St. -
The Astronomy of Sir John Herschel
Introduction m m m m m m m m m m m Herschel’s Stars The Stars flourish, and in spite of all my attempts to thin them and . stuff them in my pockets, continue to afford a rich harvest. John Herschel to James Calder Stewart, July 17, 1834 n 2017, TRAPPIST-1, a red dwarf star forty light years from Earth, made headlines as the center of a system with not one or two but Iseven potentially habitable exoplanets.1 This dim, nearby star offers only the most recent example of verification of the sort of planetary system common in science fiction: multiple temperate, terrestrial worlds within a single star’s family of planets. Indeed, this discovery followed the an- nouncement only a few years earlier of the very first Earth-sized world orbiting within the habitable zone of its star, Kepler-186, five hundred light years from Earth.2 Along with other ongoing surveys and advanced instruments, the Kepler mission, which recently added an additional 715 worlds to a total of over five thousand exoplanet candidates, is re- vealing a universe in which exoplanets proliferate, Earth-like worlds are common, and planets within the habitable zone of their host star are far from rare.3 Exoplanetary astronomy has developed to the point that as- tronomers can not only detect these objects but also describe the phys- ical characteristics of many with a high degree of confidence and pre- cision, gaining information on their composition, atmospheric makeup, temperature, and even weather patterns. 3 © 2018 University of Pittsburgh Press. All rights reserved. -
Camera Obscura Vs
MAX-PLANCK-INSTITUT FÜR WISSENSCHAFTSGESCHICHTE Max Planck Institute for the History of Science 2006 PREPRINT 307 Erna Fiorentini Camera Obscura vs. Camera Lucida – Distinguishing Early Nineteenth Century Modes of Seeing TABLE OF CONTENTS 1. Distinguishing Technologies: a Box and a Prism 5 2. Untangling Stories: an Old and a New Device 6 3. Parting Fortunes: the New Eclipses the Old 10 4. Diverging Necessities: Old and New Demands 12 5. Discerning Visual Modalities: Projective vs. Prismatic Seeing 20 5.1. Accuracy and Perceptual Experience: Criteria in Comparison 21 5.1.1. Degrees of ‘Truth to Nature’ 21 5.1.2. Degrees of Perceptual Experience 27 5.2. Projective vs. Prismatic: Optical Principles in Comparison 29 6. An Epilogue: the ‘Prismatic’ as the Camera-Lucida-Mode of Seeing 37 CAMERA OBSCURA VS. CAMERA LUCIDA 1 DISTINGUISHING EARLY NINETEENTH CENTURY MODES OF SEEING Erna Fiorentini If we look at Fig. 1, we see a painter holding an inspired pose while beholding and recording the landscape. Although he appears to beindulging in purely aesthetic rapture, he is equipped with optical drawing devices and with many other instruments for observation, tracing and measuring. A Camera Lucida is arrayed on a tripod on the right, surrounded by a telescope, a setsquare, a ruler, a pair of compasses and other devices, while in the background a tent-type Camera Obscura is in use. This motif belonged to Carl Jacob Lindström’s well-known satiric, illustrated book I Stranieri in Italia, printed and distributed in Naples in 1830.2 Moreover, Lindström produced countless further exemplars of this scene in watercolour, engraving and lithography. -
Two Letters from John Herschel to Charles Lyell, 1836-1837 Author(S): Walter F
The Impact of Uniformitarianism: Two Letters from John Herschel to Charles Lyell, 1836-1837 Author(s): Walter F. Cannon Source: Proceedings of the American Philosophical Society, Vol. 105, No. 3 (Jun. 27, 1961), pp. 301-314 Published by: American Philosophical Society Stable URL: http://www.jstor.org/stable/985457 Accessed: 28-06-2018 03:03 UTC REFERENCES Linked references are available on JSTOR for this article: http://www.jstor.org/stable/985457?seq=1&cid=pdf-reference#references_tab_contents You may need to log in to JSTOR to access the linked references. JSTOR is a not-for-profit service that helps scholars, researchers, and students discover, use, and build upon a wide range of content in a trusted digital archive. We use information technology and tools to increase productivity and facilitate new forms of scholarship. For more information about JSTOR, please contact [email protected]. Your use of the JSTOR archive indicates your acceptance of the Terms & Conditions of Use, available at http://about.jstor.org/terms American Philosophical Society is collaborating with JSTOR to digitize, preserve and extend access to Proceedings of the American Philosophical Society This content downloaded from 150.135.165.81 on Thu, 28 Jun 2018 03:03:33 UTC All use subject to http://about.jstor.org/terms THE IMPACT OF UNIFORMITARIANISM Two Letters from John Herschel to Charles Lyell, 1836-1837 WALTER F. CANNON Assistant Professor of History, University of California, Berkeley I. INTRODUCTION how new species are generated. Lyell himself CHARLES DARWIN began the Introduction to was too fearful of orthodox Christian opinion to On the Origin of Species by saying that his ob- assert a naturalistic origin of species in the Prin- servations in South America "seemed to throw ciples, especially as he could specify no mechanism whereby such generation could take place. -
Charles Darwin and John Herschel*
432 South African Journal of Science 105, November/December 2009 Research Articles Charles Darwin and John Herschel* B. Warner The influence of John Herschel on the philosophical thoughts of Charles Darwin, both through the former’s book, Natural Philosophy, and through their meeting in 1836 at the Cape of Good Hope, is discussed. With Herschel having himself speculated on evolution just a few months before he met Darwin, it is probable that he stimulated at least the beginnings of the latter’s lifelong work on the subject. : evolution, Cape of Good Hope, Charles Darwin, John Herschel He never talked much, but every word which he uttered was worth listening to. Charles Darwin, about Sir John Herschel His Majesty’s Ship Beagle, commanded by Captain Robert Fitz- Roy and carrying Charles Robert Darwin as the naturalist on board, arrived in Simon’s Bay on 31 May 1836 on the final stage of a voyage around the world that had taken four and a half years and had still another six months to go. One of FitzRoy’s duties was to check the accuracy of 22 marine chronometers, destined for use by the Royal Navy; the presence of the Royal Observatory in Cape Town gave him the finest opportunity to carry this out, with the result that the Beagle stayed in port for Charles Darwin as a young man.Watercolour by George Richmond, after the return 18 days—longer than at any other port during the circumnaviga- of the Beagle. tion (they stayed for five weeks in the Galapagos, but island- hopped). -
From William Hyde Wollaston to Alexander Von Humboldt
This article was downloaded by: [Deutsches Museum] On: 15 February 2013, At: 08:42 Publisher: Taylor & Francis Informa Ltd Registered in England and Wales Registered Number: 1072954 Registered office: Mortimer House, 37-41 Mortimer Street, London W1T 3JH, UK Annals of Science Publication details, including instructions for authors and subscription information: http://www.tandfonline.com/loi/tasc20 From William Hyde Wollaston to Alexander von Humboldt - Star Spectra and Celestial Landscape Jürgen Teichmann a & Arthur Stinner b a Deutsches Museum and Ludwig-Maximilians-University, München, Germany b University of Manitoba, Winnipeg, Canada Version of record first published: 13 Feb 2013. To cite this article: Jürgen Teichmann & Arthur Stinner (2013): From William Hyde Wollaston to Alexander von Humboldt - Star Spectra and Celestial Landscape, Annals of Science, DOI:10.1080/00033790.2012.739709 To link to this article: http://dx.doi.org/10.1080/00033790.2012.739709 PLEASE SCROLL DOWN FOR ARTICLE Full terms and conditions of use: http://www.tandfonline.com/page/terms-and- conditions This article may be used for research, teaching, and private study purposes. Any substantial or systematic reproduction, redistribution, reselling, loan, sub-licensing, systematic supply, or distribution in any form to anyone is expressly forbidden. The publisher does not give any warranty express or implied or make any representation that the contents will be complete or accurate or up to date. The accuracy of any instructions, formulae, and drug doses should be independently verified with primary sources. The publisher shall not be liable for any loss, actions, claims, proceedings, demand, or costs or damages whatsoever or howsoever caused arising directly or indirectly in connection with or arising out of the use of this material. -
Appendix Visitors' Accounts of the Herschels at Work
Appendix Visitors’ Accounts of the Herschels at Work We are fortunate that a number of visitors to the Herschel homes in the 1780s have left us detailed accounts of William and Caroline at work in this, their most productive period. These accounts enrich the picture we derive from the siblings’ own written records. The earliest is by the French geologist BARTHÉLEMY FAUJAS DE SAINT-FOND (1741–1819), and describes the night he spent at Datchet, 15/16 August 1784, when the sweeps for nebulae had been under way for nearly eight months. From it we learn that already at this date the 20-ft was capable of being moved out of the meridian, and indeed that it could be used to track the rotation of the heavens: I arrived at Mr. Herschell’s about ten o’clock. I entered by a staircase, into a room which was decorated with maps, instruments of astronomy, and natural philosophy, spheres, celestial globes, and a large harpsichord. Instead of the master of the house, I observed, in a window at the farther end of the room, a young lady seated at a table, which was surrounded with several lights; she had a large book open before her, a pen in her hand, and directed her attention alternately to the hands of a pendulum-clock, and the index of another instrument placed beside her, the use of which I did not know: she afterwards noted down her observations. I approached softly on tiptoe, that I might not disturb a labour, which seemed to engage all the attention of her who was engaged in it; and, having got close behind her without being observed, I found that the book she consulted was the Astronomical Atlas of Flamstead, and that, after looking at the indexes of both the instruments, she marked, upon a large manuscript chart, points which appeared to me to indicate stars. -
John Couch Adams: Mathematical Astronomer, College Friend Of
John Couch Adams: mathematical astronomer, rsta.royalsocietypublishing.org college friend of George Gabriel Stokes and promotor Research of women in astronomy Davor Krajnovic´1 Article submitted to journal 1Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, D-14482 Potsdam, Germany Subject Areas: xxxxx, xxxxx, xxxx John Couch Adams predicted the location of Neptune in the sky, calculated the expectation of the change in Keywords: the mean motion of the Moon due to the Earth’s pull, xxxx, xxxx, xxxx and determined the origin and the orbit of the Leonids meteor shower which had puzzled astronomers for almost a thousand years. With his achievements Author for correspondence: Adams can be compared with his good friend George Davor Krajnovic´ Stokes. Not only were they born in the same year, e-mail: [email protected] but were also both senior wranglers, received the Smith’s Prizes and Copley medals, lived, thought and researched at Pembroke College, and shared an appreciation of Newton. On the other hand, Adams’ prediction of Neptune’s location had absolutely no influence on its discovery in Berlin. His lunar theory did not offer a physical explanation for the Moon’s motion. The origin of the Leonids was explained by others before him. Adams refused a knighthood and an appointment as Astronomer Royal. He was reluctant and slow to publish, but loved to derive the values of logarithms to 263 decimal places. The maths and calculations at which he so excelled mark one of the high points of celestial mechanics, but are rarely taught nowadays in undergraduate courses. -
The Search for Planet X Transcript
The Search for Planet X Transcript Date: Thursday, 22 October 2009 - 12:00AM Location: Museum of London The Search for Planet X Professor Ian Morison The Hunt for Planet X This is a story that spanned over 200 years: from the discovery that Uranus was not following its predicted orbit and was thus presumably being perturbed by another, as yet undiscovered planet, Neptune, followed by the search for what Percival Lowell called "Planet X" that would lie beyond Neptune (where X means unknown), and finally the search for a tenth planet beyond Pluto (where X means ten as well). As we shall see, the search for a tenth planet effectively ended in August 2006 when Pluto was demoted from its status as a planet and the number of planets in the solar system was reduced to eight. Uranus Uranus was the first planet to have been discovered in modern times and though, at magnitude ~5.5, it is just visible to the unaided eye without a telescope it would have been impossible to show that it was a planet rather than a star, save for its slow motion across the heavens. Even when telescopes had come into use, their relatively poor optics meant that it was charted as a star many times before it was recognised as a planet by William Herschel in 1781. William Herschel had come to England from Hanover in Germany where his father, Isaac, was an oboist in the band of the Hanoverian Foot Guards. As well as giving his third child, Freidrich Wilhelm Herschel, a thorough grounding in music he gave him an interest in the heavens.