
The oceans span 70 per cent of the planet, their
depths contain virtually all of Earth's life-supporting
area, and all along the ocean floor 90 per cent
of the planet's earthquakes occur. Yet we know
more about the planet Mars than we know about the
hostile environment of the deep sea.
THE NEPTUNE OCEAN OBSERVATORY
will fill part of the oceanographic void. Three
thousand kilometres of anchored fibre-optic
cable, interactive instruments, and a small
band of underwater rovers will bring the Internet
to the sea, and the sea to anywhere there’s
a computer and a Web connection.
The plan is bold: weave power
and data wires across the Juan de Fuca plate—from
Vancouver Island to Oregon, at depths of 3,000
metres below the surface of the Pacific. Network
nodes along the fibre-optic web will support
multiple sensors, video cameras, and underwater
robots. Scientists at computer screens—far
from the bone-crushing pressures, near-freezing
temperatures, and eternal darkness of the deep
ocean—will conduct experiments and collect
data at speeds of 10 gigabytes, every second,
for three decades.
At the centre of this emerging
era of ocean discovery is the University of Victoria.
In October, the governments of Canada and BC
authorized funding of $62.4 million dollars—easily
the largest research grant in the university’s
history—for UVic’s development and
management of NEPTUNE Canada and its consortium
of 12 Canadian universities. The project, a joint
venture with several top US marine research institutions
led by the University of Washington, has a projected
budget of $300 million. Equipment should be in
place by 2007 and operational by 2008.
Now comes the incredible logistical,
technical, and scientific challenge of building
an underwater laboratory.
1. ON CAMPUS, NEPTUNE (it
stands for “North-East Pacific Time-Series
Undersea Networked Experiments”) is setting
up shop in the university’s new Technology
Enterprise Facility. Project leader Chris Barnes
is a geologist who specializes in studying
the earliest remnants of animal life, hundreds
of millions of years old. But lately he’s
been cast in another role: as a leader of this
multi-million dollar ocean exploration.
Barnes—colleagues admire
his “boundless energy”—is highly
regarded for his research and track record in
assembling science infrastructure. He arrived
at UVic in 1989 to create and direct the School
of Earth and Ocean Sciences, stepping down two
years ago to take on NEPTUNE. He’s since
been travelling almost non-stop, building support
for an opportunity he says is too good to pass
up.
“NEPTUNE is going to
revolutionize the way that we do ocean science,” says
Barnes. “We’ve been wanting, forever,
to look at the deep ocean, but we’ve only
been able to look at little bits. Now, all of
a sudden, we’re looking at being able to
see it all.”
The deep sea has largely eluded
standard oceanographic instruments. Satellites
can only penetrate the top micrometres of the
ocean’s surface. Oceanographic research
cruises are intermittent and, in the stormy north
Pacific, generally limited to summer months.
So marine biologists like UVic’s Verena
Tunnicliffe, who researches hydrothermal vent
communities, may venture out to them one summer
only to return the next year to find things completely—and
inexplicably—changed. NEPTUNE’s systems
will help scientists find out how and why these
and other environmental changes occur, as they
occur.
Tunnicliffe leads project VENUS
(Victoria Experimental Network Under the Sea),
a smaller, mid-depth version of NEPTUNE that
will focus on the waters around southern Vancouver
Island and Georgia Strait. VENUS will also be
a test bed for NEPTUNE technology. Tunnicliffe
sees the two projects challenging traditional
research methods, to get into a sort of dialogue
with their subject: “Instead of it being
one-way, we will now be able to interrogate the
ocean.”
2. NEPTUNE'S remotely
operated vehicles—like submersible Mars
rovers—will perform experiments on demand.
After docking at stations along the fibre-optic
array, they’ll deliver and receive data
almost instantly.
“It’s a revolution
in technology. We can bring power and the Internet
into the deep ocean,” says Barnes. NEPTUNE’s
power cables will carry thousands of times the
energy available to standard, battery-powered
oceanographic instruments. “If we can supply
lots of power, then not only can we use existing
instruments, but we can develop new ones.”
NEPTUNE’s feasibility
study described it as a “project with no
blueprint.”
“That’s about right,” says
Peter Phibbs, associate director of engineering
and operations at NEPTUNE Canada. A telecommunications
veteran, Phibbs has placed cable on the ocean
floor from New York to Brazil. But NEPTUNE poses
distinct challenges.
“The way the telecom
companies do it is to survey first, look for
any sort of bump or a crack or anything ugly
on the seabed, and avoid it like the plague,” explains
Phibbs. “NEPTUNE’s kind of interested
in the bumps.” Robots will be designed
to lay cable along rough topography near underwater
volcanoes or the hydrothermal black smokers so
abundant on the Juan de Fuca plate.
At every stage, NEPTUNE technical
staff will have to modify existing technologies
to make them more reliable, or develop new ones.
Phibbs’ US counterpart
is Bruce Howe, with the University of Washington’s
Applied Physics Lab. Howe is working with engineers
at UW to develop electronic components for the
system.
“Oceanographers have
been putting instruments into the water for many
years,” says Howe, “but everything
is sealed up. It’s all fixed. There are
no changes to the underwater system. Here, we’re
doing something radically different. We’re
violating the protective cocoon. Manufacturers
of connectors haven’t done much in this
depth of water.”
NEPTUNE’s gear, down
as far as 3,000 metres from the surface, will
be subjected to crushing water pressures. The
weight of the water can cause instruments to
implode. “We’re proposing,” says
Howe, “to take them to pretty much the
limit of what they’re going to do.”
Recently a glitch was found
in the nodes UW researchers have developed to
route network power and data. Each node dissipates
up to 300 watts of heat. “That may not
sound like much, but underwater it’s a
huge amount,” says Howe. “And it
turns out it’s not easy to get that heat
out of the pressure case and into the water.” The
solution is to coat the instruments in a highly
conductive new fluid called fluorinert.
Talk to the techies and one
word, reliability, comes up again and again.
At each step engineers must balance the expense
of buying highly reliable components against
the projected cost of maintaining them for 30
years.
“Underwater, nothing
is easy,” says Phibbs. “Each piece
is complicated and challenging. But it’s
all doable.”
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