2019-07-01_Discover

(Rick Simeone) #1

Methane


Hydrogen

Hydrogen

Carbon

Hydrogen

Hydrogen

82 DISCOVERMAGAZINE.COM


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the chemical reactions that allow plant


and animal cells to produce energy. And


those chemical reactions depend on the


basic fact that the membrane is an oily


structure interacting with a watery cell


inside of it.


But the team won’t be using methane


or ethane, the liquid hydrocarbons that


fill Titan’s lakes, for its experiments.


Those substances are liquids only when


exposed to incredibly cold temperatures


like those found on Titan’s surface, not


those usually found in chemistry labs


on Earth. Instead, the researchers are


sticking with hydrocarbons like hexane,


which is a good analogue for methane


but stays in liquid form at room tem-


perature, as well as chloroform and


others. The boundaries of these droplets


— where oil meets water — serve as a


simple analogue for the early develop-


ment of cell membranes.


Maurer’s experiments won’t produce


anything you could reasonably call a


cell membrane, but they just might shed


some light on the basic chemistry that can


occur at the boundary of oil and water.


“We kind of need this


oil phase in our cells to


drive energy generation,”


says Maurer, “and so it makes


sense that you could, in some way,


make an oil droplet have functionality


that’s similar to an aqueous cell by using


the surface of the oil droplet to drive


reactions.”


This team isn’t the first to think about


the idea of alien cell membranes. In a


2015 Science Advances paper, planetary


scientist Jonathan Lunine of Cornell


University, working with two chemical


engineers (none of the three is involved


in Bracher’s project), used digital model-


ing to determine that vinyl cyanide — a


compound made of nitrogen, carbon,


and hydrogen, also called acrylonitrile


— could theoretically form rudimentary


barriers in methane.


“To call it a membrane would be to give


it too much credit, but it’s at least some-


thing [that] kind of encloses and could


create a kind of container,” Lunine says. In


2016, he and chemist Martin Rahm (then


at Cornell, and currently at Chalmers


University of Technology) digitally mod-


eled compounds of hydrogen cyanide,


showing they could bind together


to form sheets and rolls in a


simulated hydrocarbon sea.


And then in 2017, another


paper published in Science


Advances announced the


discovery of evidence for


vinyl cyanide on Titan,


marking a step forward


in the search for molecules


capable of supporting life on the


distant moon.


Back on Earth, Maurer’s experiment


is simple. She and her colleagues want to


see if they can get compounds to cross


that oil-water boundary at all. They’ll start


with the familiar genetic molecules DNA


and RNA, but these will need some help


crossing over. The backbone of nucleic


acids like DNA and RNA is a chain of


smaller molecules called phosphates,


which have a slight negative charge. But


WATER AND LIFE


Water is a polar molecule consisting of two hydrogen atoms and one oxygen atom.


The oxygen atom in one water molecule tends to be attracted to a hydrogen atom in a


neighboring water molecule, and vice versa, giving water its unique properties. These


properties are essential for the chemistry of life on Earth.


For the chemical processes of life to happen, molecules must be able to connect,


separate, and reconnect in specific ways. Think about DNA replication, for instance.


The base pairs that make up the genetic code bond when their negatively charged


hydrogen atoms are attracted to positively charged atoms in another nucleotide. Those


bonds hold the two strands of the double helix together, but because the hydrogen


in water molecules also bonds this way, it’s relatively easy for enzymes to “unzip” the


double helix for replication, then bind the two new strands together again.


However, the molecules of life won’t work in hydrocarbons the way they do in water.


That’s because most hydrocarbons don’t tend to form hydrogen bonds. But it’s possible


that other molecules floating around in a lake of methane could bond and react in ways


that let them carry out the basic chemical functions of life. — K.N.S.


Hydrothermal vents form when seawater enters
fissures in the ocean floor, is heated by the hot
magma beneath, and boils back up through the
cracks. The vents are often teeming with life,
including microorganisms that convert minerals
and other chemicals into energy. Such vents
could provide a hospitable environment for life
elsewhere in the universe as well.

OUT THERE

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