2019-07-01_Discover

(Rick Simeone) #1

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called enzymes help reactions happen


fast enough to be useful. The team doesn’t


have alternative enzymes to go with its


membranes and genetic material, though.


“We have backbones we’re making,


and we’re going to have base pairs, but


the problem is we don’t have an enzyme


that will replicate it because the backbone


chemistry is not the same,” says Williams.


“We really have to start at a more basic


chemical level and try to work forward


as far as we can.”


LOOKING FOR ALIEN LIFE


“A lot of this is going to be exploratory


science,” says Butch. “I think it’s a really


cool idea for just pushing the boundaries


of what our assumptions about the transi-


tion from chemistry to biology actually


looks like.” In other words, no synthetic


alien organism is going to crawl out of the


test tube.


“I don’t think that we’re going to dis-


cover the origin of life in the next three


years or that we’re going to figure out


exactly how life could develop [on other


worlds] in nonpolar solvents in the next


three years,” says Bracher. “What this proj-


ect is really about is starting to figure out


how the rules of the game might change


from life as we know it in water to some


new form of life that works in oil and non-


polar solvents, whether here on Earth or


on distant planets.”


What that will tell us, Bracher and his


colleagues hope, is whether the precursors


of biochemistry might be able to take shape


in an ocean made of something other than


water. If the answer is yes, then that means


our current search for life has a huge


blind spot.


“Our problem with looking for life is


that we are looking for our life, largely.


‘Follow the water’ might find some life,


but it might not find other kinds of life,”


says Williams. By demonstrating that at


least basic biochemistry can arise in other


liquids, the team may help open new habit-


able zones, or at least keep some interesting


places from being ruled out.


The results could provide useful ideas


about not only where, but how to look


for life as we don’t know it. For instance,


Earth’s atmosphere


is rich in oxygen


because plants


and cyanobacte-


ria release it as a


product of pho-


tosynthesis. If


Bracher and his


team can identify


potential molecular


building blocks for alien


cells, they might also be able to predict


which chemicals those cells breathe out


into the atmosphere of their home world.


In 2005, astrobiologist Chris McKay


worked out how organisms on Titan might


metabolize acetylene or ethane, and real-


ized that they’d leave a noticeable signature


in Titan’s atmosphere — which, it turns


out, may actually be present, though the


evidence isn’t yet clear. The Cassini and


Huygens probes observed both the lack


of an ethane layer around the moon and


a lack of acetylene on its surface, though


both were expected. The depletion of these


substances could be due to a “biological


sink” — life consuming them and leading


to their absence.


This kind of research can guide how we


comb through the reams of data already


in hand from missions like Cassini, says


Lunine. “No one’s really looked through


the data very carefully for them, so one can


go back now, seeing that they have these


interesting properties, and really try to dig


through the data to see if it’s actually there,”


he says.


Ultimately, tinkering with alien bio-


chemistry is a step into the unknown, and


although the team has some ideas about


what to expect, they’re also prepared for


surprises along the way.


“My expectation is that a lot of things


that we think are challenges to life will turn


out to not be, and things we don’t realize


are difficulties will all of a sudden [turn out


to] be incredibly hard,” says Travisano. “It


will be interesting what doesn’t work and


what does. Expect surprises.”^ D


Kiona N. Smith is a science and technology


journalist, science history blogger, and science


correspondent for Ars Technica.


While Titan is a major focus of the search


for life in the solar system, there are other


icy worlds where life might thrive: Europa,


Iapetus, Enceladus, and Triton are among


the candidates that could host life.


TRITON


EUROPA


IAPETUS


ENCELADUS


OUT THERE

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