Aspheric polishing with a stressed lap
The 1990s will see the construction of six to eight optical telescopes with effective diameters in the range 6.5 m
to 16m, all larger than any existing telescope. The huge increases in light-gathering power have come about only
through innovative mirror and telescope designs, for gravity
does not allow a simple scaling up of existing 4-m-class
telescopes. Thus, three new primary mirror concepts are
being pursued vigorously: the segmented mirror of the
10m Keck Telescope,1 which consists of 36 thin 1.8-m
segments of solid low-expansion glass ceramic; monolithic thin meniscus mirrors of the same material for the European Southern Observatory's 4
x 8.2-m Very Large Telescope2 and
the 7.5 m Japanese National Large
Telescope; and spin-cast borosilicate honeycomb mirrors up to 8 m in diameter for three projects involving the University of Arizona and two U.S. national telescope projects.
Log in or Become a member to view the full text of this article.
This article may be available for purchase via the search at www.osapublishing.org.
OSA Members get the full text of Optics & Photonics News, plus a variety of other member benefits.