Tuesday, 2 September 2025

A little ramble through 19th century astronomy - Plans to observe the Transit of Venus from Russia

 Nature June 6th 1872

Transit of Venus

In a letter from General Otto Struve, director of the Palkowa Observatory and Astronomer Royal of Russia, to Prof. Newcomb, of the Washington Observatory, detailing the Russian preparations  for observing the forthcoming Transit of Venus, and printed in HARPERS’S WEEKLY, he remarks that the inquiries into the meteorological conditions of the stations selected have given on the whole, very satisfactory results, particularly for the station on the coast of the Pacific  Ocean and in Eastern Siberia (84 pr cent of clear sky for December).

In two only of the stations chosen, Tashkent and Astrabad, these conditions are not sufficiently satisfactory. For this reason the observers designed for Tashkent will probably go to a place about 100  miles west of that town; and instead of Astrbad it is proposed to take either the island of Aschuradeh , in the Caspian Sea, or, of possible to cross the Elburz Mountains and establish observers at Schahrech, In Persia 9with nearly absolute certainty of clear sky).

The total number of Russian stations will be twenty-four each of them provided with only one instrument for the transit observation. These instruments are – three 4 inch heliometers, three photo heliographs, four 6inch equatorial and four 4 inch equatorials, provided with filar micrometres and spectroscopic apparatus and ten 4 inch telescopes, designed merely for contact observations.  Each station will also be furnished with clocks, chronometers, and the instruments necessary for exact determination of time. The principal instruments have already been ordered.

Most of them will be ready for use in the curse of the present or beginning of next year. For these instruments the observers are also in a great part selected. They will all visit Palkowa for a certain time in 1873 to exercise themselves in the observations.

The geographic positions of the stations will be determined by the transit observers; but all stations on which the transit has been successfully observed will be carefully determined afterwards by special expeditions of the general staff or the navy. For this purpose, a principal line of telegraphic longitudes, will probably be laid next year through all Siberia to Nicolajevsk, with which line the other stations of that part of Russia can easily be joined, either by telegraphic or chronometric operations.

With regards to photographic observations, Prof Struve states that the two observers, one at Vilna and Dr Vogel at Bothkamp, in Holstein, have been perfectly successful in taking instantaneous observations with dry plates.


                                                      www.theramblingastronomer.co.uk

No comments:

Post a Comment