A Lunar Liquid Mirror Telescope (LLMT) is under study thanks to a grant from NASA. J. Roger Angel, a regents professor at the University of Arizona, is leading a project to study the feasibility of a 100 meter LLMT at the moon's south pole.
Why liquid mirrors? Ever since 1668, when Isaac Newton built the first reflector telescope with a one-inch diameter mirror made of metal, astronomers have longed for bigger parabolic mirrors. Opticians expend a great deal of effort to grind larger and larger pieces of glass to just this shape.
Liquid Mirror Telescopes were first talked about several hundred years ago. Imagine a bowl of mercury at the center of a lazy susan. When you give it a spin, the surface of the liquid forms that highly prized shape - a parabola. The bigger the bowl, the bigger the resulting mirror.
The first serious attempts to actually build a LMT took place in the early twentieth century. Robert W. Wood, a physicist at Johns Hopkins University, built a working telescope, but could not accurately control the speed of the turntable, resulting in a mirror with a variable focal length. (The rotation must be controlled to less than one part in 100,000 during exposure.) Pictures of star trails were focused in some places, but blurry in others.
The LMT concept has been made to work. The Large Zenith Telescope at the University of British Columbia uses a 6-meter mirror, making it the third largest optical telescope in North America. It was built at a cost of approximately $1 million. A telescope with a conventional glass mirror of the same size would cost $100 million.
It is hoped that similar savings might apply when constructing telescopes on the moon. In addition, the moon is completely free from atmospheric absorptions and distortion.
The only disadvantage of the LMT is that you cannot tilt it; it must remain perpendicular to the local gravitational field. You can only use it to look at what is directly above the telescope; however, a mirror of this size could take a very penetrating look at its patch of sky.
"You would be seeing things farther back in time than
anyone has ever seen any galaxy or star or quasar," [Angel] explained.
"It could give you a chance to see what was happening at a very early
(From J. Roger Angel and the LLMT)
Obviously, for such a project to be attempted, there would need to be substantial infrastructure already im place on the moon. As Dr. Angel remarked, "You could not justify that kind of infrastructure (just) to build this kind of telescope, but if the infrastructure already were there, this is something that looks feasible to do."
There is a very early reference to a large liquid mirror telescope in science fiction; but this LMT is on Mars, not the moon. In his excellent 1934 novella Old Faithful, author Raymond Z. Gallun writes about a Martian named 774, who has a desperate need to contact Earth:
Piercing the dome, opposite the upper end of the cylinder,
was a circular opening through which a portion of the starlit sky was visible;
and at the base of the cylinder a great bowl rotated rapidly, like a huge
wheel... The bowl contained mercury. As the container spun on its perfectly
balanced axis, centrifugal force caused the mercury to spread in a thin,
precisely distributed layer over the inside of the bowl, forming a concave
surface that acted admirably as a mirror for Number 774's gigantic reflecting
telescope. It's area, and its consequent light-gathering capacity, was many
times greater than any rigid mirror that could have been constructed without
(Gallun appears to err in his use of the LMT; read more about the Martian LMT)
(This Science Fiction in the News story used with permission from Technovelgy.com - where science meets fiction.)