While a zenith telescope has the disadvantage of not being able to look anywhere but at a small spot straight up, its simplified setup permits the use of a mirror consisting of a smoothly spinning pan filled with liquid mercury. Such a mirror can be made much larger than a conventional mirror, greatly increasing light collecting ability. The LZT is used for transit imaging, meaning that Earth's rotation moves stars along the sensor, and the latent image in the sensor is moved electronically in step with this movement, so that it is read out at the trailing edge.
The telescope made use of parts from the 3-meter diameter NASA Orbital Debris Observatory telescope, which had been using a liquid-mercury mirror for several years.
This mirror was a test, built for $1 million, but it was not suitable for astronomy because of the test site's weather. In 2016 it was noted as the third largest telescope in North America, and for its spinning mercury mirror that cost just 1% of normal mirrors, although it must view upward.[1]
Decommissioning
According to Atlas Obscura the Large Zenith Telescope was decommissioned in the summer of 2016.[2] All of its liquid mercury was stored for other projects.[citation needed]
The website Physics Footnotes also mentioned that the LMT had been decommissioned, but gave no time frame in the undated article.[3]
Science magazine reported in 2019 that the LMT was decommissioned, but was also silent on the date.[4]
Similar projects
The university plans a larger 8-meter liquid-mirror telescope named the Advanced Liquid-Mirror Probe (ALPACA) for astronomical use at an estimated first-light cost of $5 million, $3 million contingency, $10 million for the camera, $5 million for a spectrograph, and $0.3 million operating costs per year.[5]
A larger project is planned, called LAMA, with 66 individual 6.15-meter telescopes with a total collecting power equal to a 55-meter telescope, resolving power of a 70-meter scope.[6][7]
^Hickson, P. and Lanzetta, K. M., 2004, July. Large aperture mirror array (LAMA): project overview. In Second Backaskog Workshop on Extremely Large Telescopes (Vol. 5382, pp. 115–126). International Society for Optics and Photonics.