Royal fossils: The Royal Society and progress in palaeontology

Author(s):  
G. E. Budd

The study of the remains of past life is a relatively young discipline, and one that has been defined partly by conflicting demands placed on it by both the life and Earth sciences. Fellows of The Royal Society have made critical contributions both to the growth of material knowledge of the subject and to the expansion of its theoretical basis, especially in the formative decades at the beginning of the 19th century. In particular, British palaeontologists and stratigraphers were pre-eminent in the shift away from viewing the Earth as a young creation conforming to the account in Genesis and towards the modern view of it as an ancient and dynamic system with a distinct history. Despite these early Earth science interests, palaeobiological subjects were also soon a topic of research, ranging from the reconstruction of ancient ecologies to the description of extinct organisms such as the dinosaurs. Nevertheless, palaeontology has notoriously failed to make signal contributions to evolutionary theory and the recent development of areas where palaeontology does have a unique imput to make, such as the global patterns of biodiversity through time and the controversy over mass extinction, has largely been a North American concern. British palaeontologists have, however, made fundamental contributions to the study of major evolutionary radiations, and this tradition is well represented in the current research interests of extant Fellows. Palaeontology remains a poorly defined discipline with little sense of an overarching paradigm, but one important future prospect probably lies with the revival of evolutionary morphology and development as neontological subjects.

1798 ◽  
Vol 88 ◽  
pp. 527-566

Reverend Sir, Such is the subject of the inclosed paper, and such the repu­tation for skill and industry, which the many valuable papers you have communicated to the Royal Society, and your other learned works, have justly procured to you, that it could not with more propriety be submitted to the judgment of any other person than yourself, even if the writer of it were a stranger to you. But there are circumstances which render my presenting it to you, in some measure, a duty. I had the advantage of being, for some years, your Assistant in the Royal Observatory at Greenwich; during which time, you made the important observations on the mountain Schehallien , in Scotland, which afford an ocular demonstration of the attraction of that mountain, and a strong argument for the general attraction of matter, a subject nearly connected with that of the following pages; and it was from you that I received the problem of which you will here find an improved solution.


1863 ◽  
Vol 12 ◽  
pp. 306-312 ◽  

In one of the four communications which the authors have already had the honour of presenting to the Royal Society on the subject of the measurement of the chemical action of light, the attempt was made to determine experimentally the laws regulating the distribution of the chemical action of the sunlight and diffuse daylight on the surface of the earth when the sky is perfectly unclouded and the atmosphere clear. The methods of measurement there employed do not, unfortunately, apply to the much more usually occurring case of cloudy skies and hazy atmosphere.


1873 ◽  
Vol 163 ◽  
pp. 587-627 ◽  

In the years 1869 and 1870 I communicated to the Royal Society the results of a series of experiments made with the view of determining, if possible, the amount of radiant heat coming to the earth from the moon in various conditions of phase, and the nature of that heat as regards the average refrangibility of the rays. Though more successful than I had at first been led to expect, the imperfect accordance between many of the observations still left much to be desired, and the novelty and importance of the subject appeared sufficient to render it advisable to pursue the investigation with greater care and closer attention to details than had hitherto been deemed necessary. Since the conclusion of the series of observations which form the subject of the second paper above referred to, nothing (with the exception of a short series of observations in August and October 1870, of which mention is made towards the end of this paper) was done towards pursuing the subject till the spring of the following year (1871), when the series of observations which form the subject of the present paper were commenced, the same apparatus (only slightly modified) being used and the same method of observation adopted; but, with the view of obtaining an approximate value of the absorption of the moon’s heat in its passage through our atmosphere, and of rendering possible the satisfactory comparison of observations made at different zenith-distances of the moon, the observations were in many cases carried on at intervals at all possible zenith- distances on the same night, and the most favourable opportunities for observing the moon at very different zenith-distances in various conditions of the atmosphere were not lost.


2009 ◽  
Vol 45 ◽  
pp. 268-279
Author(s):  
Andrew Cambers

Life, the afterlife, and life beyond the Earth are matters of scientific inquiry as well as religious belief. As we might expect, in the wake of the scientific revolution of the seventeenth century, the afterlife was subjected to new scrutiny. Such scrutiny, notably the demonology of Joseph Glanvill and Henry More, both fellows of the Royal Society, was undoubtedly scientific and serious, even if it has rarely been treated as such by scholars preferring to treat belief in witchcraft as a hangover from an earlier age. Far from being opposed, or necessarily pulling in opposite directions, the conjunction of science and religion in this era breathed new life into old problems and opened up new questions for debate. One such area, with a long history as a philosophical conundrum, was the possibility of life beyond Earth. It is this question, its place within religious cultures, and its relation to traditional ideas about the afterlife, that is the subject of this essay.


1826 ◽  
Vol 116 ◽  
pp. 548-578 ◽  

The ellipticity of the earth, deduced by Captain Sabine from a series of pendulum experiments the most extensive, and apparently the most deserving of confidence, that has ever been made, differs considerably from that which, as is generally believed, is indicated by geodetic measures. The difference can only be explained by errors of observation, by peculiarities of local circumstances, or by some defect in the theory which connects the figure of the earth with the variation of gravity on its surface: under the last head may be placed defects in the mathematical part of the theory, and errors in the assumptions of the original constitution and present state of the earth. It was with a view to ascertain the sufficiency of the mathematical theory, that I undertook the investigations contained in this paper. The celebrated proposition called Clairaut's theorem, by which the earth's ellipticity is inferred from the variation of gravity on its surface, is obtained only by the rejection of the squares and higher powers of the ellipticity. It is by the same rejection that the figure of the earth, supposed a heterogeneous fluid, is proved to be an elliptic spheroid. It appeared therefore probable, that a more accurate theory might introduce some modification into Clairaut's theorem, and might also show he figure of the earth to differ from an ellipsoid ; and there was no reason to think that the first approximation to that figure was more accurate, than the first approximation to the motion of the moon’s perigee. The result of my investigation does not at all serve to reconcile the pendulum observations made by Captain Sabine with the measures of degrees : and with respect to one object, which I hoped to obtain, I am therefore completely unsuccessful. The theory shows, however, that the earth’s figure, on the usual suppositions as to its constitution, is not an elliptic spheroid; and the formulæ which I have obtained will give the means of determining very exactly the figure of the earth, when the experiments on the variation of gravity, or the measures of arcs on the earth’s surface, shall be thought sufficiently accurate. As the subject is one whose interest is not confined to the present time, I have ventured to offer my investigations to the Royal Society. The first part of the following sheets contains the theory of the heterogeneous earth, pushed so far as to include all the terms of the second order: it is succeeded by a comparison of this theory with Captain Sabine’s results, and with the best arcs of the meridian that have been measured and in the conclusion, I have offered some suggestions on the propriety of repeating some of these measures.


1857 ◽  
Vol 8 ◽  
pp. 60-61 ◽  

In the preparation of my course of lectures, I have found it necessary to re-investigate much of the above-named branch of mechanics, and I have now a paper in preparation on the subject, which I propose to offer to the Royal Society when it is ready. In the meanwhile, it appears to me that the two fundamental principles on which my researches are based are of such a nature, that they may very properly be communicated to the Royal Society at once. They are as follows:― I. Principle o f the Stability of Earth . At each point in a mass of earth the directions of greatest and least compressive stress are at right angles to each other; and the condition of stability is, that at each point the ratio of the difference of those stresses to their sum shall not exceed the sine of the angle of natural slope of the earth.


1873 ◽  
Vol 10 (108) ◽  
pp. 248-261
Author(s):  
O. Fisher

The subject of Captain Hutton's lecture, on the Formation of Mountains, delivered at Wellington, New Zealand, is one which has engaged a good deal of my attention, and was discussed by me in a paper read before the Cambridge Philosophical Society, and printed in their Transactions. In that paper I attributed the elevating force, which has raised mountain ranges, to the contraction of the heated interior of the earth, and subsequent wrinkling of the crust so as to accommodate itself to the diminished nucleus. This was an old hypothesis, but I believe the amount of horizontal pressure produced in that manner had not been estimated before. Mr. Mallet, the eminent seismologist, read a paper on the same subject before the Royal Society in May, 1872, in ignorance of what I had written, and came to the same conclusion as myself as to the amount of the horizontal pressure.


1829 ◽  
Vol 119 ◽  
pp. 103-120

May I take the liberty of addressing to you, as President of the Royal Society, a request that you will communicate to the Society, if you shall deem them worthy of its notice, the observations on the aurora borealis which I am about to detail in this letter, and which have been made by me at various times under very favourable circumstances, arising out of the very frequent occurrence of the meteor in the latitude of my residence, about 57° 15' N. The immediate occasion of this communication is the interest you have manifested in the subject, in your observations on a luminous belt seen at Rose-morran in Cornwall, 29th September last, published in the Phil. Mag. vol. iv. page 453; and likewise a paper by John Dalton, F. R. S., published in the Phil. Trans. 1828, “On the Height of the Aurora Borealis above the Surface of the Earth; particularly of one seen on the 29th of March, 1826.” Mr. Dalton in that paper, supposing the same luminous belt was seen on the 29th of March at places distant from each other at the same time, infers its height to have been 100 miles and upwards.


1970 ◽  
pp. 47-55
Author(s):  
Sarah Limorté

Levantine immigration to Chile started during the last quarter of the 19th century. This immigration, almost exclusively male at the outset, changed at the beginning of the 20th century when women started following their fathers, brothers, and husbands to the New World. Defining the role and status of the Arab woman within her community in Chile has never before been tackled in a detailed study. This article attempts to broach the subject by looking at Arabic newspapers published in Chile between 1912 and the end of the 1920s. A thematic analysis of articles dealing with the question of women or written by women, appearing in publications such as Al-Murshid, Asch-Schabibat, Al-Watan, and Oriente, will be discussed.


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