From Cornell: “Life ‘not as we know it’ possible on Saturn’s moon Titan”

Cornell Bloc

Cornell University

September 24, 2016
Feb. 27, 2015
Anne Ju
amj8@cornell.edu

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Graduate student James Stevenson, astronomer Jonathan Lunine and chemical engineer Paulette Clancy, with a Cassini image of Titan in the foreground of Saturn, and an azotosome, the theorized cell membrane on Titan. Jason Koski/University Photography

Liquid water is a requirement for life on Earth. But in other, much colder worlds, life might exist beyond the bounds of water-based chemistry.

Taking a simultaneously imaginative and rigidly scientific view, Cornell chemical engineers and astronomers offer a template for life that could thrive in a harsh, cold world – specifically Titan, the giant moon of Saturn. A planetary body awash with seas not of water, but of liquid methane, Titan could harbor methane-based, oxygen-free cells that metabolize, reproduce and do everything life on Earth does.

Their theorized cell membrane, composed of small organic nitrogen compounds and capable of functioning in liquid methane temperatures of 292 degrees below zero, is published in Science Advances, Feb. 27. The work is led by chemical molecular dynamics expert Paulette Clancy, the Samuel W. and Diane M. Bodman Professor of Chemical and Biomolecular Engineering, with first author James Stevenson, a graduate student in chemical engineering. The paper’s co-author is Jonathan Lunine, the David C. Duncan Professor in the Physical Sciences in the College of Arts and Sciences’ Department of Astronomy.

Lunine is an expert on Saturn’s moons and an interdisciplinary scientist on the Cassini-Huygens mission that discovered methane-ethane seas on Titan. Intrigued by the possibilities of methane-based life on Titan, and armed with a grant from the Templeton Foundation to study non-aqueous life, Lunine sought assistance about a year ago from Cornell faculty with expertise in chemical modeling. Clancy, who had never met Lunine, offered to help.

“We’re not biologists, and we’re not astronomers, but we had the right tools,” Clancy said. “Perhaps it helped, because we didn’t come in with any preconceptions about what should be in a membrane and what shouldn’t. We just worked with the compounds that we knew were there and asked, ‘If this was your palette, what can you make out of that?’”

On Earth, life is based on the phospholipid bilayer membrane, the strong, permeable, water-based vesicle that houses the organic matter of every cell. A vesicle made from such a membrane is called a liposome. Thus, many astronomers seek extraterrestrial life in what’s called the circumstellar habitable zone, the narrow band around the sun in which liquid water can exist. But what if cells weren’t based on water, but on methane, which has a much lower freezing point?

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A representation of a 9-nanometer azotosome, about the size of a virus, with a piece of the membrane cut away to show the hollow interior. James Stevenson

The engineers named their theorized cell membrane an “azotosome,” “azote” being the French word for nitrogen. “Liposome” comes from the Greek “lipos” and “soma” to mean “lipid body;” by analogy, “azotosome” means “nitrogen body.”

The azotosome is made from nitrogen, carbon and hydrogen molecules known to exist in the cryogenic seas of Titan, but shows the same stability and flexibility that Earth’s analogous liposome does. This came as a surprise to chemists like Clancy and Stevenson, who had never thought about the mechanics of cell stability before; they usually study semiconductors, not cells.

The engineers employed a molecular dynamics method that screened for candidate compounds from methane for self-assembly into membrane-like structures. The most promising compound they found is an acrylonitrile azotosome, which showed good stability, a strong barrier to decomposition, and a flexibility similar to that of phospholipid membranes on Earth. Acrylonitrile – a colorless, poisonous, liquid organic compound used in the manufacture of acrylic fibers, resins and thermoplastics – is present in Titan’s atmosphere.

Excited by the initial proof of concept, Clancy said the next step is to try and demonstrate how these cells would behave in the methane environment – what might be the analogue to reproduction and metabolism in oxygen-free, methane-based cells.

Lunine looks forward to the long-term prospect of testing these ideas on Titan itself, as he put it, by “someday sending a probe to float on the seas of this amazing moon and directly sampling the organics.”

Stevenson said he was in part inspired by science fiction writer Isaac Asimov, who wrote about the concept of non-water-based life in a 1962 essay, “Not as We Know It.”

Said Stevenson: “Ours is the first concrete blueprint of life not as we know it.”

See the full article here .

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Once called “the first American university” by educational historian Frederick Rudolph, Cornell University represents a distinctive mix of eminent scholarship and democratic ideals. Adding practical subjects to the classics and admitting qualified students regardless of nationality, race, social circumstance, gender, or religion was quite a departure when Cornell was founded in 1865.

Today’s Cornell reflects this heritage of egalitarian excellence. It is home to the nation’s first colleges devoted to hotel administration, industrial and labor relations, and veterinary medicine. Both a private university and the land-grant institution of New York State, Cornell University is the most educationally diverse member of the Ivy League.

On the Ithaca campus alone nearly 20,000 students representing every state and 120 countries choose from among 4,000 courses in 11 undergraduate, graduate, and professional schools. Many undergraduates participate in a wide range of interdisciplinary programs, play meaningful roles in original research, and study in Cornell programs in Washington, New York City, and the world over.

From Science Alert: “Saturn’s biggest moon could support a new kind of alien life”

ScienceAlert

Science Alert

6 JUL 2016
DAVID NIELD

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Titan. NASA

When it comes to looking for life on other planets, scientists tend to focus their search on planets that have the right conditions for liquid water to form, but Saturn’s moon Titan might just point the way to the existence of life without water.

Researchers in the US have been analysing the chemical composition of Saturn’s largest satellite, and think the presence of hydrogen cyanide (HCN) molecules in the atmosphere could pave the way for different forms of life to evolve.

That’s because HCN reacts to form polymers including polyimine, and polyimine is able to absorb a wide spectrum of light – so wide that it’s enough to capture light penetrating Titan’s dense and hazy atmosphere.

With that light, the scientists think polyimine could be a possible catalyst for life.

“Polyimine can exist as different structures, and they may be able to accomplish remarkable things at low temperatures, especially under Titan’s conditions,” said chemist Martin Rahm from Cornell University.

“We are used to our own conditions here on Earth,” he adds. “Our scientific experience is at room temperature and ambient conditions. Titan is a completely different beast.”

Titan is Earth-like in that its surface is covered with lakes, rivers, and seas, but these are made up of liquid methane and ethane rather than water. The nitrogen and methane in the air make the planet’s surface too toxic for humans to survive, but the researchers suggest other types of life could prosper.

The study builds on the Cassini-Huygens missions that have been ongoing for nearly 20 years.

NASA/ESA/ASI Cassini Spacecraft
NASA/ESA/ASI Cassini Spacecraft

ESA Huygens Probe on Cassini
ESA Huygens Probe on Cassini

The data collected by the Cassini orbiter and Huygens probe – which landed on Titan back in 2005 – have been invaluable in allowing the Cornell team to simulate a prebiotic chemical trail that could lead to life… but not quite life as we know it.

The data from the NASA probes was plugged into a computer simulation run by Rahm and his team, which revealed that polyimine could spark life in the ultra-cold temperatures on the surface of Titan. Polyimine’s precursor, hydrogen cyanide, has previously been linked to the start of life on Earth.

“If future observations could show there is prebiotic chemistry in a place like Titan, it would be a major breakthrough,” said Rahm. “This paper is indicating that prerequisites for processes leading to a different kind of life could exist on Titan, but this [is] only the first step.”

The research could mean Titan offers two chances of hosting alien life. Scientists think that there is liquid water under the frozen surface of Titan, but locked away in a massive underground ocean – and there’s a lot of speculation that these kinds of underground oceans located throughout the Solar System could hypothetically give rise to life.

In any case, if the researchers turn out to be right about the polyimine, we can broaden our search for extraterrestrial life beyond planets that very closely match Earth’s environments – and that could be pretty huge.

Watch this space.

The findings have been published in Proceedings of the National Academy of Sciences.

See the full article here .

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