As far back as he can remember, Craig Nance has loved two
things: astronomy and electronics. So as the facility
engineer for the world's largest optical/infrared
telescopes, he is a happy man indeed. The fact that the
telescopes, known as the W.M. Keck Observatory, happen
to be in one of the loveliest places on the planet,
namely on the Big Island of Hawaii, just seems like
overkill.
This engineer does work hard. At the office by 7 a.m.
most days, Nance is never quite sure what the day will
throw his way. Install a dye-laser system to help
correct for atmospheric distortion to incoming
starlight? Figure out how to run a ground wire into arid
rocky terrain at 4200 meters above sea level? Damp
vibrations from dozens of machines and industrial motors
along an 85-meter path? Nance has worked on all that and
more.
Though Nance points out that every project at the
observatory is a team effort, that he's just "doing what
needs to get done," a quick glance at the dozen or so
to-do lists scribbled on his office whiteboard says
otherwise. As he talks about the variety of problems
he's been called in to fix, you quickly get the sense
that Nance is the go-to guy at Keck.
As a boy in Jacksonville, Fla., he built his own
telescopes from scratch and was an avid backyard sky
watcher. When he couldn't decide between the
college-preparatory track in high school or electronics
repair in vocational school, he took both, even though
it meant giving up his summers.
At Florida State University, in Tallahassee,
electrical engineering was a natural fit. After getting
his BSEE in 1991 and an MSEE in 1994, Nance's next stop
was the U.S. Air Force. From 1994 to 1997, he served as
a commissioned officer at the Arnold Engineering
Development Center, a huge testing facility near
Tullahoma, Tenn. The experience "taught me to be an
engineer and to work on large machinery," Nance recalls.
What he didn't like was being "one little cog in a big
machine. If I stayed, I could see myself becoming the
world's leading expert in one very tiny area. That
seemed terribly boring."
With the end of the Cold War and the downsizing of
the military, Nance got the nudge he needed. One day, an
older engineer took him aside and told him to "figure
out what you really want to do." Nance replied that he'd
always liked astronomy but didn't have the right degree.
"Don't worry about that," his friend said. Everyone
needs engineers.
Though Nance wasn't completely convinced, he thought
he'd take a shot at "the brass ring." While scanning an
online job listing hosted by the IEEE, he spotted an
opening that seemed tailor-made. A new advanced optical
telescope in Texas needed an electrical engineer. Nance
applied for and got the job, and soon found himself in
the Davis Mountains of West Texas, at the McDonald
Observatory. By 1999, he was the observatory's
facilities manager.
In 2000, he made the move to Keck, which was like
landing on cloud nine—literally. Keck sits atop Mauna
Kea, a dormant volcano that shoots up more than 4
kilometers above sea level. Trade winds sweep the summit
free of clouds, making it an ideal spot for stargazing.
Reachable only by a 2-hour, bone-jarring drive along
loose gravel switchbacks, it's a precarious place to
work—it towers above 40 percent of the Earth's
atmosphere, and unaccustomed visitors can grow
lightheaded. For those reasons, the observatory's
administrative office is in Waimea, a small town at the
volcano's base. "I do my thinking back at headquarters
before heading up to the summit to work," Nance says.
Every Monday starts with a staff meeting to run down
upcoming observations, repairs, maintenance, and the
like. Astronomers vie for observing time on Keck, so
they fully expect everything to work properly when they
show up. "Some nights the weather doesn't allow us [to
work], sometimes the moon is a factor, but we never want
to lose a pristine night because something breaks,"
Nance says. That's a tall order, given that Keck is a
unique machine—its instruments are mostly custom built
and require constant care.
Keck, operated by the California Institute of
Technology, the University of California, and NASA,
shares Mauna Kea with 12 other observatories, but it's
by far the largest and most complex. The sensitivity of
any telescope depends in great part on the size of its
primary mirror. But there are physical limits to how big
you can make a single mirror. Keck gets around that by
using segmented mirrors. Computer-controlled sensors and
actuators on each of the 36 hexagonal segments
continually make fine adjustments, down to 4 nanometers,
so that the segments work as if they were one giant
mirror 10 meters across.
A constant thrill for Nance is rubbing elbows with
the biggest names in astronomy and getting an insider's
preview of their news-making discoveries—planets beyond
our solar system, stars being consumed by the black hole
at the galaxy's center, storms raging on Uranus.
He doesn't even mind that the scientists get all the
glory. He sees himself as part of a long tradition of
engineers in astronomy. On his desk sits a photo of
Russell Porter, the legendary telescope designer who
played a pivotal role in the birth of California's
Palomar Observatory—an engineer, like Nance.
"If I won the lottery tomorrow," he says, "I'd still
do pretty much what I'm doing now."
More about the Keck telescope and the electronics
discussed by Craig Nance, is available at
http://www2.keck.Hawaii.edu/. The
site also has the latest news about the telescopes'
astronomical discoveries. “Optical Interferometry Comes
of Age," Peter R. Lawson, Sky & Telescope, May 2003,
p. 30–39, offers a detailed yet readable explanation of
how advanced observatories like Keck are taking
advantage of a 19th-century technique known as
interferometry to obtain extremely high-solution images.