Large Zenith Telescope

Large spinning bath of liquid mercury used to probe the early universe

Image of Large Zenith Telescope located in British Columbia, Canada | The 6-m Large Zenith Telescope.

The 6-m Large Zenith Telescope.

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Image of Large Zenith Telescope located in British Columbia, Canada | The 6-m Large Zenith Telescope. Image of Large Zenith Telescope located in British Columbia, Canada | The UBC Liquid Mirror Observatory, at an altitude of 400 meters in the Malcolm Knapp Research Forest. Image of Large Zenith Telescope located in British Columbia, Canada | Image taken with the Large Zenith Telescope. Image of Large Zenith Telescope located in British Columbia, Canada | View of the UBC Liquid-Mirror Observatory and the surrounding forest. Image of Large Zenith Telescope located in British Columbia, Canada | The assembled primary mirror support system. Image of Large Zenith Telescope located in British Columbia, Canada | View from above the telescope showing the main segments that comprise the primary mirror surface. Image of Large Zenith Telescope located in British Columbia, Canada | View of the mirror undergoing testing using water instead of mercury.

Category Inspired Inventions, Instruments of Science, Optical Oddities

With a six-meter diameter and weighing in at three metric tons, the Large Zenith Telescope is the third-largest optical telescope in North America and the largest liquid mirror telescope in the world. Completed in 2003, the telescope is housed in the UBC Liquid-Mirror Observatory at Malcolm Knapp Research Forest, overlooking British Columbia's Fraser Valley.

Isaac Newton first advanced the idea for a liquid telescope. He realized that a liquid made to rotate inside a container would take the form of a paraboloid (shaped like an oval cup ), precisely the shape needed for the primary mirror of a telescope. Unfortunately for Newton, without a stable source of rotation such as an electric motor, building such a telescope was not possible.

Utilizing current technology, however, the scientists and engineers at the Large Zenith Telescope have realized Newton's aspirations. The LZT employs a six-meter dish filled with a thin layer of mercury. A motor rotates this liquid mirror at a constant rate of six revolutions per minute and walls at the edges of the dish prevent the mercury from spilling over the sides. To support the massive mirror, a special air bearing was engineered that could withstand a 10-metric ton load. This bearing differs from conventional ones in that it uses a thin film of pressurized air to reduce the friction at the interface of the two surfaces.

Land-based liquid mirror telescopes have several advantages and disadvantages compared to their solid mirror counterparts. The major advantages of a liquid mirror telescope are that they are relatively inexpensive, costing about one percent of a conventional mirror, and they can be built much larger. The disadvantages are that the mirror can only point straight up towards the zenith, because it would lose its shape if it were to tilt, and the most common metal employed, mercury, is highly toxic to humans and animals. Extraterrestrial liquid mirror telescopes are advantageous as well, and NASA hopes to one day put one on the moon.

The science topics investigated at the LZT include cosmology, the large-scale structure of the universe, and the evolution of galaxies. With a telescope that can only point overhead, the scientists are somewhat limited in what they can study. Nevertheless, the instrument is used for long-term sky surveys in which the light from over 100,000 distant galaxies is analyzed and supernova searches where astronomers aim to capture the explosive energy of a star in its dying moments.

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The UBC Liquid-Mirror Observatory is located within the Malcolm Knapp Research Forest, 70 km east of Vancouver. The observatory is accessible by foot and is a 45 minute walk from the gate. At present, the observatory cannot accommodate public tours except by special request for small groups.

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