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Although the surface of the mirror is
smooth, the underside features a
honeycomb pattern of 1,681 hexag-
onal spaces, seen here (opposite)
through the top of the reflector. This
results in a stiffer piece of glass that
is 80 percent lighter than a compa-
rable solid chunk. More important,
Once the glass cools, the team
lifts the slab from the furnace
using a temporary fixture they
secure to the surface with super-
sticky adhesive. The disc, which is
27.5 inches thick, gets a good
scrubbing top and bottom. Then
technicians flip the unwieldy mass
FRAMING SWEAT-PROOF
the design sheds heat much faster
come nightfall, minimizing thermal
distortion. Imagine hot air shim-
mering above a road, except it’s
coming off your billion-dollar tele-
scope, obscuring your view. The
resulting images will be sharper and
clearer come showtime.
upside down to install 157 brack-
ets called load spreaders that
distribute the mirror’s weight as
evenly as possible. That hardware,
which the crew is preparing to
install here (above), affixes the
finished product to its designated
spot within the telescope.