Previous Article Next Article Table of Contents
The New and Improved 4-m Telescope (1Mar93) (from KPNO, NOAO Newsletter No. 33, 1 March 1993) The first concepts of the KPNO 4-m telescope can be traced to 1961. Most of the systems, both mechanical and electrical, were designed soon thereafter, in the mid to late 1960s. Now, almost thirty years later, component age is starting to take its toll on reliability. Over the summer of 1993, we plan to make a first pass at updating the electronics, computer control systems, and a number of other efficiency related items. The primary effort is going toward replacing the Telescope Control System (TCS), which will be comprised of modern computers and a window-based software system. Considerable hardware upgrades are required to take advantage of the new software, which is based on our experience at the 2.1-m and Coude Feed. The most noticeable improvements for the visiting astronomer will be much improved pointing and tracking, and shorter times in moving from object to object. Also, both the LTO and the observer will have control over the instrument to enhance the efficiency of setup operations by providing a second option for setting configuration parameters. This is the first real software upgrade at the telescope in twenty years, and it requires programs to control all nine supported instruments! In addition, we continue to work toward improving the thermal environment of the telescope and dome. The oil, which is pumped to the telescope bearings, will be cooled, thereby eliminating the single greatest heat polluter in the dome (see article below on our acquisition of a thermal camera). Note that many heat sources have already been removed from the 4-m, and thus the building has only two havens from the cold: the control room, which was heavily insulated last summer, and the computer room, which is seriously air conditioned. In 1994 we plan to improve the ventilation of the dome (following CTIO's lead) to minimize the effects of uncontrollable heat sources and to rebuild the telescope control console, which currently is dominated by outdated and unused buttons and switches. In order to accomplish the scheduled work, the summer shutdown will be extended into late September, which unfortunately means 2-3 weeks less observing time for the fall semester. George Jacoby, Bruce Bohannan, David De Young
Previous Article Next Article Table of Contents