Hostname: page-component-848d4c4894-p2v8j Total loading time: 0.001 Render date: 2024-05-31T11:26:29.883Z Has data issue: false hasContentIssue false

The Kottamia Observatory and Other Aspects of Astronomy in Egypt

Published online by Cambridge University Press:  30 March 2016

A.M.I. Osman*
Affiliation:
National Research Institute of Astronomy and Geophysics Helwan-Cairo, Egypt

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The 74-inch (1.8m) telescope of Kottamia Observatory is the largest telescope in North Africa and the Middle East. It stands on a plateau 485m above sea-level and 70km to the east of Cairo. The latitude is 25° 55’.9 N and the longitude 31° 49’.5E. The telescope is of conventional type, having Newtonian (f/4.9), Cassegrain (f/18) and coudí (f/28.9) foci; it was built by Grubb-Parsons (U.K.). The main mirror is of Duran 50 glass, and has a clear aperture of 74 inches (1.8m) and a focal length, for its paraboloidal surface, of 360 inches (9.2m). The secondary mirrors are of fused quartz. The telescope is provided with a Newtonian camera, a single-channel photoelectric photometer, a Cassegrain spectrograph comprising two cameras with dispersions of 100 Amm−1 and 48 Amm−1 at 4800A and a coude spectrograph with two cameras allowing dispersions of 20Amm−1 and 6Amm−1. A four-component correcting lens has been supplied to be mounted at the Newtonian focus, in order to reduce the effect of coma on photographic observations.

Type
IV. Working Group Meetings
Copyright
Copyright © Kluwer 1995