XCVIII. Observations on the tides in the Island of St. Helena: in a letter from the Rev. Nevil Maskelyne, A. M. F. R. S. to Thomas Birch, D. D. Secretary to the Royal Society

1761 ◽  
Vol 52 ◽  
pp. 586-606 ◽  

Reverend Sir, Not having met with any observations of the tides made in a place so near the line as this, or at an island situated in the middle of so large an ocean, I was desirous of making some experiments on this subject.

1761 ◽  
Vol 52 ◽  
pp. 558-577 ◽  

Sir, During the course of my voyage from England to this place, I made frequent observations of the distance of the Moon from the Sun and fixed star. in order to determine our longitude: and, as from their agree­ment with each other, I humbly conceive it will be allowed, that the longitude may in general be ascer­tained by this method to sufficient exactness for nau­tical purposes, I flatter myself it may not be disagreeable to the Royal Society, if I communicate to them, through your hands, the results of my observations.


1761 ◽  
Vol 52 ◽  
pp. 21-25 ◽  

Dr. Watson lately received a letter from the Abbé De la Caille at Paris, in which he takes notice, "That although the pa- "rallax of the moon seems sufficiently well deter"mined, by the observations made in 1751, in "Europe and at the Cape of Good Hope; never- "theless, an element of this importance cannot be “too well ascertained.


2019 ◽  
Vol 52 (1) ◽  
pp. 65-83 ◽  
Author(s):  
JIM BENNETT

AbstractNevil Maskelyne, the Cambridge-trained mathematician and later Astronomer Royal, was appointed by the Royal Society to observe the 1761 transit of Venus from the Atlantic island of St Helena, assisted by the mathematical practitioner Robert Waddington. Both had experience of measurement and computation within astronomy and they decided to put their outward and return voyages to a further use by trying out the method of finding longitude at sea by lunar distances. The manuscript and printed records they generated in this activity are complemented by the traditional logs and journals kept by the ships’ officers. Together these records show how the mathematicians came to engage with the navigational practices that were already part of shipboard routine and how their experience affected the development of the methods that Maskelyne and Waddington would separately promote on their return. The expedition to St Helena, in particular the part played by Maskelyne, has long been regarded as pivotal to the introduction of the lunar method to British seamen and to the establishment of the Nautical Almanac. This study enriches our understanding of the episode by pointing to the significant role played by the established navigational competence among officers of the East India Company.


1761 ◽  
Vol 52 ◽  
pp. 196-201 ◽  

My Lord, I am sorry I cannot have the honour of gratifying your Lordship, and the Royal Society, with an account of a more complete observation of the transit of Venus, than what I here­-with transmit to you.


1761 ◽  
Vol 52 ◽  
pp. 434-443 ◽  

My Lord, When we reflect upon the great degree of perfection, to which the sciences are at present brought, and, at the same time, consider from what low beginnings in former times they have arisen to this hight, we are apt to please ourselves with the idea of a certain kind of superiority, which we imagine we enjoy above the learned, who have gone before us.


1761 ◽  
Vol 52 ◽  
pp. 26-28

Sir, In a letter which I wrote to you from this place, the beginning of this week, I desired you would, in your answer to Abbé De la Caille, acquaint him, that I had proposed to the Royal Society the observations of the moon's parallax, before his letter came; and that Dr. Bradley was to make observations at Greenwich, correspondent to mine at St. Helena; and that I was drawing up a list of the proper observations to be made, and the proper stars with which the moon was to be com­pared, which I proposed to transmit to the Abbé De la Caille, in order that he might attend to the same observations, if he thought proper.


2011 ◽  
Vol 38 (2) ◽  
pp. 220-228 ◽  
Author(s):  
Spencer G. Sealy ◽  
Mélanie F. Guigueno

For centuries, naturalists were aware that soon after hatching the common cuckoo (Cuculus canorus) chick became the sole occupant of the fosterer's nest. Most naturalists thought the adult cuckoo returned to the nest and removed or ate the fosterer's eggs and young, or the cuckoo chick crowded its nest mates out of the nest. Edward Jenner published the first description of cuckoo chicks evicting eggs and young over the side of the nest. Jenner's observations, made in England in 1786 and 1787, were published by the Royal Society of London in 1788. Four years before Jenner's observations, in 1782, Antoine Joseph Lottinger recorded eviction behaviour in France and published his observations in Histoire du coucou d'Europe, in 1795. The importance of Lottinger's and Jenner's observations is considered together.


In previous communications to the Royal Society, I have shown that if we consider the sun’s declination at the quarter-days of the May year and at the solstices, and also the changes due to precession in the places of five or six of the more conspicuous stars visible, at any epoch, in these latitudes we are able to account for the alignments investigated in the stone monuments in Cornwall and Devon. The present paper deals with a special class of circles in Aberdeenshire in which the method of indicating alignments shows a striking difference. The Cornish method was that still set out in the instructions for the erection of the Gorsedd circle of the Welsh Eisteddfod, the sighting, or directing, stones were placed some distance outside the circle. In Aberdeenshire the method employed was to place a long, recumbent stone generally between two of the upright stones of the circle itself and to obtain the direction of the rising sun or star by sighting across the circle at right angles to the length of the recumbent stone.


1832 ◽  
Vol 122 ◽  
pp. 539-574 ◽  

I have for some time entertained an opinion, in common with some others who have turned their attention tot he subject, that a good series of observations with a Water-Barometer, accurately constructed, might throw some light upon several important points of physical science: amongst others, upon the tides of the atmosphere; the horary oscillations of the counterpoising column; the ascending and descending rate of its greater oscillations; and the tension of vapour at different atmospheric temperatures. I have sought in vain in various scientific works, and in the Transactions of Philosophical Societies, for the record of any such observations, or for a description of an instrument calculated to afford the required information with anything approaching to precision. In the first volume of the History of the French Academy of Sciences, a cursory reference is made, in the following words, to some experiments of M. Mariotte upon the subject, of which no particulars appear to have been preserved. “Le même M. Mariotte fit aussi à l’observatoire des experiences sur le baromètre ordinaire à mercure comparé au baromètre à eau. Dans l’un le mercure s’eléva à 28 polices, et dans Fautre l’eau fut a 31 pieds Cequi donne le rapport du mercure à l’eau de 13½ à 1.” Histoire de I'Acadérmie, tom. i. p. 234. It also appears that Otto Guricke constructed a philosophical toy for the amusement of himself and friends, upon the principle of the water-barometer; but the column of water probably in this, as in all the other instances which I have met with, was raised by the imperfect rarefaction of the air in the tube above it, or by filling with water a metallic tube, of sufficient length, cemented to a glass one at its upper extremity, and fitted with a stop-cock at each end; so that when full the upper one might be closed and the lower opened, when the water would fall till it afforded an equipoise to the pressure of the atmo­sphere. The imperfections of such an instrument, it is quite clear, would render it totally unfit for the delicate investigations required in the present state of science; as, to render the observations of any value, it is absolutely necessary that the water should be thoroughly purged of air, by boiling, and its insinuation or reabsorption effectually guarded against. I was convinced that the only chance of securing these two necessary ends, was to form the whole length of tube of one piece of glass, and to boil the water in it, as is done with mercury in the common barometer. The practical difficulties which opposed themselves to such a construction long appeared to me insurmount­able; but I at length contrived a plan for the purpose, which, having been honoured with the approval of the late Meteorological Committee of this Society, was ordered to be carried into execution by the President and Council.


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