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London Times Article on the Venus Transit of 1874
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DEC. 12, 1874



On Wednesday last, at different times for the different observing stations on the globe, but in each case within about four hours, took place the expected astronomical phenomenon, which had not been seen since 1769. The planet Venus, being located from the sun 66,000,000 miles-above two thirds of the earth's probable distance from the sun - passes around the sun by an interior orbit within the orbit described around the sun by our own planet. It happens, twice in a hundred years, but at an interval of eight years only, that Venus comes directly between us and the sun. The visible effect to spectators in the daytime who can see the sun is that a small black spot, which is actually the body of that planet, seems to travel slowly across the sun's apparent disc. It's size relatively to that of the sun's apparent disc is that of a pea on a cheese plate. In those parts of the globe where it happened to be day at the time of the transit precise observations were made by scientific parties sent out here and there from Europe. The result is of some importance, because from comparison of the exact times at which successive phenomena occurred at different stations the astronomers will be able to compute the sun's real distance from us, which is not yet certainly known.

The observations made at the cost of the British Government, under the direction of Sir G. B. Airy, Astronomer Royal, are at nine different stations. Captain G. L. Tupman of the Royal Marine Artillery, is at the head of this service.
The persons sent out to the various stations and, sub-stations- and now, as far as is known, at their respective posts-are as follow: Sandwich Islands-At Honolulu, Captain Tupman, assisted. by Lieutenant F. E. Ramsden, RN., and Mr. J. W. Nichol; at Hawaii,Professor G. Forbes, assisted by Mr. H. G Barnacle; at Atooi, Mr. H. Johnson and Lieutenant E. J. W. Noble, R.M.A. On KerguelenIsland, in the South Indian Ocean, the Rev. Father Perry, Astronomer of Stonyhurst College, who observes at Christmas Harbour, assisted by the Rev. W. Sidgreaves, also of Stonyhurst, Lieutenant S. Goodridge, RN., and Mr. J. B. Smith; while at Port Palliser, on the same island, Lieutenant C. Corbet, R.N., takes command, his assistant being Lieutenant U. E. Coke, R.N. On Rodriguez Island, east of Mauritius, in the Indian Ocean, Lieutenant C. B. Neate, R. N., has charge, and his aids are Mr. C. E. Burton and Lieutenant R. Hogan, R. N. Lord Lindsay has also set up a station, at his own private cost, in Mauritius. The New Zealand chief is Major H. Palmer, R.E., and his assistants are Lieutenants L. Darwin, R.E., and. H. Crawford, R. N. Lastly, in Egypt, at Cairo, Captain C. Orde Brown, R.A., has charge. With him are Mr. S. Hunter and Captain Abney, whose dry-plate photographic process is employed throughout the British stations. Captain Abney has taken his standpoint at Thebes. Each party is supplemented by three non-commissioned officers or privates of time Royal Engineers. Advantage has been taken of the sojourns on Kerguelen Island and Rodriguwz to prosecute some natural-history researches. The Royal Society appointed a geologist (Mr. H. Slater, B.A.), a botanist (Mr. Balfour), and a zoologist; (Mr. G. Gulliver, B.A.) to accompany the party to latter island.

     The various expeditions, with instruments, houses, and stores, sailed for their respective posts during the past summer and autumn, and are believed to have arrived without mishap. The German, French, American, Russian, Dutch, and Italian Governments have occupied different stations in Eastern Asia, the Pacific Ocean, and elsewhere.

     We learnt by telegraph, from several distant places, that the observations had been successfully made. At Calcutta, Roorkee, and Kurrachee, in India, but not at Madras, the weather allowed the sun to be seen, and the moments of contact to he noted. At Nagasaki, in Japan, and at a station in Silmeria, favourable results were gained. The British observers in Egypt, at Thebes and Cairo, obtained a most complete success. It is of these stations in Egypt we have now to speak more particularly in connection with our two illustrations.

     Captain Ordo Brown, R.A., the chief of thin expedition in Egypt, was introduced to the Khedive by General Stanton, her Majesty's Consul-General. His Highness at once furnished the principal station on the Mokatteni Heights, 600 ft. above Cairo, with tents, a guard, and a mounted escort. A telegraph line was laid front the Mokattem Heights to the office of the Eastern Telegraph Company at Cairo, to connect that station with Greenwich, through the Submarine, Gibraltar, and Malta cable.

     The telegraph office at Cairo was also put in communication with the observing station at Thebes, under Captain Abney, R.E.His Highness sent a steamer to tow the Thebes branch of the expedition to its destination, and caused all the huts and instrument to be brought up by special train from Suez.

     We give two illustrations of the Mokattem Heights station. Our Correspondent at Cairo was favoured by Captain Orde Brown with the following memorandum :-"The Mokattem heights, above the citadel of Cairo, have been chosen for the primary astronomical station for observing the transit of Venus. This situation possesses several recommendations. The geographical position of Cairo is the best one for establishing electrical communication between Greenwich and the astronomical stations not only in Egypt, but also those in India and Australia. The Mokattem hills are east of all the cultivated country; and, having only desert between them and the horizon, there is little liability to mists. Moreover, the heights have a command of about 600 ft. above Cairo, which places the station above the morning mists which cling to the ground."

     One of our Illustrations represents Captain Brown superintending the conveyance of his material up the heights, a service entailing considerable risk of damage to the valuable Instruments he had in his charge. Everything, however, reached it destination safely. Our smaller Engraving is a view of the camp and observatories, with the mosque at Cairo in the plain below.

     At the Mokattem Heights and at Suez the egress of Venus from the sun's disc was observed in all its phases. At Thebes, in addition to these observations, a series of fifty photographs were taken with the Janssen's slide by Captain Abney, including the critical instant of contact. From the Mokattem Heights telegraph time-signals were exchanged with Suez and Thebes, and with Greenwich, through the submarine line of the Eastern Telegraph Company, which is some hundred miles longer than the Atlantic cable, and much smaller.

     The Astronomer Royal, at Greenwich, has received communications from Colonel Tennant at Roorkee, where one hundred photographs were taken ; and detailed telegrams of telescopic and micrometer observations near Cairo and Suez, and of photographic observations at Thebes, of the transit of Venus, have been received. All are perfectly successful.