By Alderson T.L.
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As we saw in Chapter 3, larger diameter telescopes are needed in order to see fine details in the sky, but bigger means more money and work. `Scruff' 41 Figure 4a The Interplanetary Scintillation (IPS) Array used by Hewish and Bell-Burnell to discover pulsars. The array consists of 1,000 posts hammered into the ground, and strung with almost 200 km of wire, making a total of 2,048 aerials. ) Hewish got around the problem by designing a phased-array antenna that not only simulated the resolution of a radio telescope 1,000 kilometers across using a much smaller area, but one that would daily survey the entire visible sky.
Answers to these and a hundred other questions kept astronomy buzzing, but the next logical step was to see just how many quasars were out there and what they were like. Fortunately, the star-like appearance of quasars led to an ingenious method of finding more of them. If you've ever looked at the night sky and known which bright points were stars and which very few were planets, you may have noticed that the planets don't twinkle. The simple reason is that, seen from Earth, the planets have a small but definite diameter.
Using the 48 inch Schmidt telescope on Mount Palomar Observatory he discovered many galaxy clusters. Between 1937 and 1941 Zwicky discovered 18 supernovae in other galaxies at a time when the sum total of supernova discoveries by all other astronomers was 12. In 1934 Zwicky and Baade collaborated on one of the most important predictions in the history of astronomy. They had witnessed a number of major events in physics: the development of quantum theory, the discovery of the neutron, and the growing knowledge of stellar evolution.
(6,3)-MDS Codes over an Alphabet of Size 4 by Alderson T.L.