Self Organizing Space Dust Could Be a Precursor to Life

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As if searching for life wasn’t already difficult enough, physicists now think that clouds of particles in space could mimic the behaviour of life: dividing, replicating and even evolving. This discovery could help scientists understand how life got started here on Earth, and offers intriguing possibilities for life that could evolve in the interstellar clouds of outer space.

This discovery comes from European and Australian researchers, and their work is published in today’s issue of the New Journal of Physics. They developed computer simulations that showed how clouds of molecules naturally organize themselves into complex helix-like structures that resemble DNA.

Over time, an electrical process called polarization organizes the molecules into more and more complex structures. According to the researchers, this suggests a mechanism where organic molecules could assemble faster than in previous models. This shorter time frame means that complex life could be prevalent across the Universe – they get part of the way in space, and then finish off when they reach a planet. Astronomers have already observed vast clouds of these particles out in space with radio telescopes.

Life on Earth requires water, and these molecules wouldn’t have access to the liquid in the near absolute zero temperatures of interstellar space; however, they are able to interact through this polarization process. So there might be a limit, where the structures can’t become complex enough to seed life on young planets. But this process could begin the formation of life, from a random collection of atoms to more complex molecules, and eventually the precursors of life. Evolution could then take over.

Original Source: Science Now

Enceladus is an Unlikely Home for Life

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When Cassini discovered geysers of water ice fountaining off of Saturn’s moon Enceladus, it was easy to think: life! Wherever we have liquid water here on Earth, scientists have found microbial life thriving; even in the strangest environments. A new model of just how Enceladus generates those geysers has made the possibility of microbial life being able to survive on Enceladus very unlikely.

When the geysers were first discovered, scientists dubbed the process “Cold Faithful”. In this model, tidal interactions between Enceladus and Saturn heat the moon, creating shallow pockets of liquid water under an ice shell. Pressure builds up under the ice, causing it to burst open, and water ice to spray out into space.

But a new model, developed by researchers at the University of Illinois, explains how Enceladus could be producing geyser-like plumes of water ice without an environment hospitable to life. Instead, the process would be called “Frigid Faithful”, and wouldn’t require liquid water at all.

Enceladus is covered in a layer of stiff ice compounds called clathrates, which could go down to a depth of tens of kilometres. Even with a moderately warm heat source underneath the moon’s south pole, these clathrates could deform and create the tiger stripe cracks and fractures which have been observed.

Instead of having pools of water near the surface, these cracks extend down up to 35 kilometres, and maintain almost the exact same temperature all the way down – as cold as 150 degrees below zero. And that wouldn’t be hospitable to life.

So where are the geysers coming from? As the clathrates dissociate, they produce gases that travel up the tiger stripes. This gas then leaks into space, and seen as the plumes that Cassini observed. Here’s what one of the researchers, Gustavo Gioia, had to say:

“This is indeed a frigid Enceladus. It appears that high heat fluxes, geyser-like activity and complex tectonic features can occur even if moons do not have hot, liquid or shifting interiors.”

Original Source: UIUC News Release

An Experiment to Test Panspermia

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One of most intriguing, and controversial, theories astrobiology is the concept of Panspermia. This idea proposes that life on Earth might have began on another planet, or maybe even out in interstellar space. Scientists have discovered just how hardy microbial life can be, surviving long journeys in the vacuum, cold, and radiation of space. Now an experiment has been devised to see how well microbes can withstand reentry through the Earth’s atmosphere.

The experiment, designed by Professor John Parnell from the University of Aberdeen, involves bolting a Scottish rock to the outside of an ESA research spacecraft. When the Foton M3 mission launches on Friday, September 14th, microbes in the rock will enjoy the acceleration of liftoff, 12 days of microgravity and vacuum, and then re-entry through the Earth’s atmosphere.

“The objective behind this is to look at the rock’s behaviour when it is exposed during re-entry through the Earth’s atmosphere – when temperatures are extreme. This will tell us something about the likelihood of life being transferred between planets on meteorites.

“The Orkney rock is a very robust material but it will be interesting to see if organic matter in the rock is robust enough to survive the harsh conditions endured during re-entering the Earth’s atmosphere.”

In theory, asteroid strikes in the past excavated material on other planets, hurling microbe-laden rocks into interplanetary space. The rocks would then act as lifeboats, carrying the microbes to other planets. More importantly, they should protect the bacteria as the rock plunges into the atmosphere.

This experiment will help discover if there’s anything to this idea. Bacteria might just be hardy enough to survive the complete journey from planet to planet.

Original Source:Univ. Of Aberdeen

If There’s Oxygen, There’s Life

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If aliens visited our Solar System, it would only take them a moment to figure out which planet is the one with all the life on it. That’s because our atmosphere has a high percentage of oxygen in its atmosphere. The presence of oxygen in our atmosphere has given scientists the key to searching for life on other worlds. But what if there are purely natural processes, that could confuse the search for life, fooling powerful new space observatories like the Terrestrial Planet Finder and Darwin.

Don’t worry. A new simulation by a team of US researchers shows that no natural process on a habitable world with liquid water could keep high levels of oxygen and ozone present in an alien atmosphere. If there’s oxygen, there’s life.

Most of the oxygen (O2) in the Earth’s atmosphere was thought to have been generated though photosynthesis. Plants use energy from the Sun, taking in carbon dioxide and releasing O2 as a byproduct. Over time, this oxygen has built up in our atmosphere to its current ratio of 21%, with the rest nitrogen and other trace gases.

This ratio is very important to the search for life in the Universe. Over the next few decades, a fleet of spacecraft and experiments are being built that will be so sensitive, they’ll be able to analyze the atmosphere of a distant Earth-sized world. Find oxygen or ozone in that planet’s atmosphere – so goes the thinking – and you’ve found a world with life. Like our own planet, some organic process is refreshing the oxygen in the atmosphere, stopping it from reacting away.

One recently canceled spacecraft is the Terrestrial Planet Finder, which would be sensitive enough to analyze the chemical constituents of a distant atmosphere. Sadly, this mission was scrapped after budgets were transfered to support the Vision for Space Exploration, which will send humans back to the Moon, and on to Mars. Don’t worry, though, the Europeans are working on the problem too with their Darwin mission. And it hasn’t been canceled… yet.

These missions (if they do get launched) will be able to spot oxygen and ozone in a distant world’s atmosphere. But could they be fooled? Are there natural processes that could generate similar levels of oxygen and ozone? If so, then it would make the search for life extremely difficult, generating false positives that would confuse scientists.

There have been a few scenarios that scientists think might create false positives for life. For example, in a runaway greenhouse planet like Venus, large amounts of hydrogen could be escaping from a hot, moist atmosphere. Since this hydrogen is originating from water (H2O), this would leave oxygen behind. If an extrasolar planet was losing its ocean to space, it might fool the detectors.

In another situation, a frozen, Mars-like planet could be large enough to retain heavy gases, but too small to maintain volcanic outgassing. The frozen surface would then inhibit the loss of oxygen, but also not consume it.

The trick to both of these scenarios, though, is that they would exist on planets outside a star’s habitable zone. Careful observers would be able to rule them out ahead of time.

A team of US researchers has developed a simulation to see if there are scenarios that could generate false positives, and they weren’t able to find anything that would fool future telescopes. The research paper is titled Abiotic Formation of O2 and O3 in High-CO2 Terrestrial Atmospheres, and it was recently accepted into the journal Astronomy & Astrophysics.

They ran many simulations, factoring in all the potential variables that would simulate an Earthlike world, including different rates of volcanic outgassing and ultraviolet radiation.

They weren’t able to come up with any scenarios in which a habitable planet with liquid water could generate a false positive result for O2 or O3 that would fool a telescope like the Terrestrial Planet Finder or Darwin.

Original Source: Arxiv research paper

How Different Could Life Be?

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Over the last few years, biologists have been continuously surprised at life’s ability to survive in extreme environments: in freezing and boiling temperatures, deep underground, and at the bottom of the ocean around geothermal vents. The common ingredients are liquid water, carbon, and an energy source. But in a new research report developed by the National Research Council, entitled The Limits of Organic Life in Planetary Systems, a multidisciplinary team of scientists investigated alternative ways that life could exist and even thrive.

Life that would be completely alien to the processes we have here on Earth.

The assumption about the search for life in the Solar System is that it would share certain traits in common with life “as we know it”. That means liquid water as a solvent, so that organic molecules can interact in solution. Animal metabolism would require carbon to provide energy storage, chemical reactions and the creation of structures.

But according to this paper, water isn’t the only biosolvent that life could use. In fact, it’s not even the best one. For example, on Saturn’s frigid moon Titan, liquid ammonia could act as a solvent. Non-carbon-based molecules could serve the functions of storage, structure and chemical reactions.

This paper suggests that researchers should expand their understanding of what forms life could take here on Earth, as well as the environments that it could exist in. It also encourages space mission designers to make their experiments more flexible, able to detect unusual life processes, instead of the plain old water/carbon life we’ve got here on Earth.

You can read the press release here, or download the entire report as a PDF file or read it online. Don’t worry, it’s really well written and very accessible to most readers, just scan past the pages of organic molecules and enjoy the writing.

Imagining Plants on another Planet

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If and when astronomers finally start discovering life on other worlds, they’ll be wondering what kinds of lifeforms are there. They probably won’t have plants as we know them, but there’ll be some kind of life that converts light from the Sun into energy. What would this life look like?

It turns out, the look of the plant life on another planet will depend on the light from the Sun. This is according to new research from Robert Blankenship at Washington University in St. Louis. Plants here on Earth are green because of chlorophyll, which converts solar power into sugars for metabolism. But this isn’t the best molecule. Ideally, you want something black, which absorbs all of the light.

Blankenship is part of a NASA working group at the Jet Propulsion Laboratory. They’re studying the light that comes from stars and extrasolar planets, looking for clues that would hint at extrasolar life. Specifically, they’re looking for elements which are out of balance from what a world should be if it was completely lifeless. For example, here on Earth, the free oxygen in our atmosphere wouldn’t be around if there wasn’t a natural process replenishing it. There’s also a very specific wavelength of light, 700 nanometres out, where there are signs of very intense chlorophyll absorption.

Original Source: Washington University in St. Louis News Release

Microbes Travel With Our Spacecraft

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Wherever humans go, our microbes go too. Astronauts on board Mir experienced this first hand. Even thought the spaceship was cleaned as thoroughly as possible before launch, years of human habitation made it a breeding ground for molds and microbes. Over time, these wee beasties can build up, and cause a genuine health concern for spacefaring humans.

A recent article on NASA’s Science website traces the history of microscopic astronauts. In one encounter, visiting US astronauts on board Mir removed an instrument panel and discovered a grapefruit-sized ball of cloudy water, which had condensed from humidity. The water couldn’t escape, so it just built up over time. Samples brought back to Earth showed it contained several dozen species of bacteria and fungi.

On board Mir, organisms were found growing on rubber gaskets around windows, on spacesuit components, copper wire insulation. Pretty much everywhere. And the International Space Station has the problem too. Astronauts have discovered patches of mold growing on a panel where they hang their exercise clothes.

NASA is working on new tools that will help astronauts be able to detect different kinds of microbes and fungi, and then choose the right cleaning compound for the job.

Original Source: Science@NASA

NASA’s Next Probe Should Visit Europa

Europa. Image credit: NASA/JPLArizona State University professor Ronald Greeley thinks that NASA’s next flagship mission to the outer planets should be sent to Europa, to help determine if the Jovian moon is a good place to search for life. Greeley presented his rationale at the annual meeting of the American Association for the Advancement of Science in San Francisco.
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