Many of my posts have focused on the search for life on
Mars. And like detectives sorting
through clues, astrobiologists are meticulously closing in on what I predict
will be the first confirmation of life off the planet Earth.
But Mars isn’t the only game in town. The Jovian moon
Europa -- four times farther away than Mars -- beckons astrobiologists. Since the
Voyager flybys of the late 1970s, scientists have hypothesized that a global
ocean with more fresh water that on all on Earth exists miles beneath the rock-hard icy crust. Why? Observational evidence for that ocean has been
mounting.
Life might be able to subsist by extracting energy from possible hydrothermal
vents at the seafloor, as some species do on Earth. Brown material filling a cobweb of cracks on the moon's surface might contain organic compounds, too -- Europa could be the solar
system’s biggest cesspool.
Its greater distance from Earth than Mars aside, exploring Europa will be technologically more daunting, more expensive, and more scientifically challenging.
Europa is embedded in a radiation field maintained by
Jupiter’s powerful magnetic field that bakes unshielded spacecraft electronics. Temperatures
on the moon’s surface are a frigid -250 degrees Fahrenheit -- challenging
mechanical operation and power generation. The feeble sun, 500 million miles
away, is just 4 percent as bright as seen from Earth.
This week, planetary scientists meeting at a conference in
Moscow are discussing the science goals and experiments to be performed by a
Europa lander.
Funding for such a mission, however, is problematic.
NASA scheduled the Jupiter Icy Moons Orbiter (JIMO) for a 2017 launch but was canceled in 2005. (NASA recently did approve a
Jupiter orbiter Discovery-class mission for arrival at Jupiter in 2016). Now under
consideration is the Europa Joint Systems Mission (EJSM) an ESA/NASA
program. But given NASA’s flat space science budget, it’s going to be a stiff competition with other planetary programs standing in the food line.
Nevertheless, we will eventually explore Europa because it is just too enticing to pass up.
Based on various concept studies this is how a mission might
unfold:
Completing a decade-long voyage, a Europa orbiter spirals
into the Jovian system (the vehicle has low thrust ion engines, so it
simply can’t “hit the brakes” when it reaches Jupiter). During the 65-day
spiral-in the orbiter’s cameras scrutinize Europa to search for a safe but scientifically
interesting looking landing site. By then astrogeologists may be confident that
Europa’s large cracks and smooth “ponds” are sites of recent chaotic activity where
water has reached the surface.
After entering orbit about Europa, the mothership releases a
small lander probe that has traveled piggyback along the journey. The probe deploys
airbags and free-falls under Europa’s gravitational pull, which about 1/6th
Earth gravity. The saucer-shaped lander touches down and the airbags are jettisoned.
The lander performs the functions of any robotic space
tourist: monitoring surface temperature, seismic activity, and radiation flux
from Jupiter. A pair of spectrometers use laser light to illuminate, and sometimes
vaporize, surface ices to study Europa’s chemistry and look for organic compounds.
The camera sends back images of an exotic, tortured looking terrain.
During the mission Jupiter eclipses the sun once every 3.5
days. An on-board nuclear generator not only provides power to keep the lander operating, but warm too, especially during the blackout. But nothing can protect the craft
from the blistering radiation that would kill any human in 10 minutes. The radiation-hardened probe is doomed to a life
expectancy of only 30 days on Europa.
With luck, the Europa landing site has relatively recent breaks in the surface due to a melting of the crust by a subsurface "lava-lamp" water plume, tectonics, or a meteorite impact.
The Europa lander has a baggage weight limit of 40 pounds of
science experiments. Unlike the Mars Viking Landers from the 1970s, the lander
can accommodate just a single astrobiology lab. It is dedicated to studying any
organic chemistry present and identifying any sources of chemical disequilibrium
on the surface – the driving energy flow for life.
Before the lander fizzles out, a tiny pocket-sized probe melts its way down to a depth of just a few inches and then is retracted into the lander with a water sample.
The water is filtered, and chemically analyzed for organic matter.
The first results are likely be ambiguous when it comes to finding
life on Europa, unless the probe’s camera photographs Europa whales beached and
frozen stiff on the surface.
The water sample may not be large enough to capture a
single microbe if they are thinly dispersed in the Europa ocean. But if we get lucky, there could be
nutrient-rich regions near the boundary between ice and water near Europa’s
surface.
Whatever the astrobiology data – or lack thereof -- comes from the
lander, it serves to guides the follow-on mission: An autonomous, robotic, ocean-exploring spacecraft.
This next and far pluckier lander will carry a
torpedo-shaped cryobot that will melt its way through the ice and come
face-to-face with anything that might be within the subterranean ocean.
Photos: NASA
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