Monday, 7 July 2014

NASA Press Release: Ocean on Saturn Moon Could be as Salty as the Dead Sea


Glimpsing Saturn through Titan's haze. Source: NASA




RELEASE 14-185


Scientists analyzing data from NASA’s Cassini mission have firm evidence the ocean inside Saturn's largest moon, Titan, might be as salty as the Earth's Dead Sea.

The new results come from a study of gravity and topography data collected during Cassini's repeated flybys of Titan during the past 10 years. Using the Cassini data, researchers presented a model structure for Titan, resulting in an improved understanding of the structure of the moon's outer ice shell. The findings are published in this week’s edition of the journal Icarus.

"Titan continues to prove itself as an endlessly fascinating world, and with our long-lived Cassini spacecraft, we’re unlocking new mysteries as fast as we solve old ones," said Linda Spilker, Cassini project scientist at NASA's Jet Propulsion Laboratory (JPL) in Pasadena, California, who was not involved in the study.

Additional findings support previous indications the moon's icy shell is rigid and in the process of freezing solid. Researchers found that a relatively high density was required for Titan's ocean in order to explain the gravity data. This indicates the ocean is probably an extremely salty brine of water mixed with dissolved salts likely composed of sulfur, sodium and potassium. The density indicated for this brine would give the ocean a salt content roughly equal to the saltiest bodies of water on Earth.

"This is an extremely salty ocean by Earth standards," said the paper's lead author, Giuseppe Mitri of the University of Nantes in France. "Knowing this may change the way we view this ocean as a possible abode for present-day life, but conditions might have been very different there in the past."

Cassini data also indicate the thickness of Titan's ice crust varies slightly from place to place. The researchers said this can best be explained if the moon's outer shell is stiff, as would be the case if the ocean were slowly crystalizing, and turning to ice. Otherwise, the moon's shape would tend to even itself out over time, like warm candle wax. This freezing process would have important implications for the habitability of Titan's ocean, as it would limit the ability of materials to exchange between the surface and the ocean.

A further consequence of a rigid ice shell, according to the study, is any outgassing of methane into Titan's atmosphere must happen at scattered "hot spots" -- like the hot spot on Earth that gave rise to the Hawaiian Island chain. Titan's methane does not appear to result from convection or plate tectonics recycling its ice shell.

How methane gets into the moon's atmosphere has long been of great interest to researchers, as molecules of this gas are broken apart by sunlight on short geological timescales. Titan's present atmosphere contains about five percent methane. This means some process, thought to be geological in nature, must be replenishing the gas. The study indicates that whatever process is responsible, the restoration of Titan's methane is localized and intermittent.

"Our work suggests looking for signs of methane outgassing will be difficult with Cassini, and may require a future mission that can find localized methane sources," said Jonathan Lunine, a scientist on the Cassini mission at Cornell University, Ithaca, New York, and one of the paper's co-authors. "As on Mars, this is a challenging task."

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. JPL manages the mission for NASA's Science Mission Directorate in Washington.

For more information about Cassini, visit

http://www.nasa.gov/cassini
and
http://saturn.jpl.nasa.gov

-end-





Dwayne Brown
Headquarters, Washington
202-354-1726
dwayne.c.brown@nasa.gov

Preston Dyches
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-7013
preston.dyches@jpl.nasa.gov


All text copyright NASA 2014

Saturday, 5 July 2014

SETI Press Release: Field Tests in Mojave Desert Get Us One Step Closer Towards Manned Asteroid Missions



 Pascal Lee (SETI Institute and Mars Institute) (right) and Sgt Andre Pearson (U.S. Army, NTC) conduct “small body” geological sampling in simulated spacesuits while anchored and tethered on a steep boulder slope at Asteroid Hill, National Training Center, Fort Irwin, California. 15 April 2013. Source: NASA



Press Release, Mountain View, California, 14 May 2013. A team of researchers from the SETI Institute, the Mars Institute, NASA Ames Research Center, and the space robotics company Honeybee Robotics, has successfully completed a first series of field tests aimed at investigating how humans will explore and work on Near-Earth Asteroids (NEAs) and eventually the two moons of Mars, Phobos and Deimos.

From 13 to 15 April 2013, field experiments were conducted at the U.S. Army’s National Training Center (NTC) at Fort Irwin, California, to evaluate geotechnical methods and systems that will enable humans to be productive explorers in the low gravity environment of small rocky bodies. Sub-kilometer sized NEAs, Phobos, and Deimos are among destinations currently considered by NASA for future human missions into Deep Space.

“Human missions to Near-Earth Asteroids and to the moons of Mars present us with the exciting challenge of exploring planetary bodies with extremely low gravity” says Pascal Lee, planetary scientist at the SETI Institute and leader of the field test. “The goal of our field test was to learn how to characterize the physical properties of small body surfaces, and to test ideas that might enable humans to more productively explore these low-gravity worlds.”


The Mojave field test included three investigations: 1) a study of whether conventional field tools commonly used to characterize the mechanical properties of soils on Earth are suitable for small bodies; 2) an evaluation of how different anchoring systems might allow robotic spacecraft and astronauts to remain bound to a low gravity body; 3) a study of how astronauts might conduct geological sampling on a small body while using anchors and tethers.“It’s important to analyze and understand how conventional civil engineering methods and systems perform in natural settings on Earth before adapting them to the exploration of small bodies” explains Kris Zacny, Director of planetary exploration robotics at Honeybee Robotics in Pasadena, California. Honeybee Robotics is the company that developed the Rock Abrasion Tool (RAT) on NASA’s Mars Exploration Rovers, Spirit and Opportunity, and the Sample Manipulation System (SMS) and Dust Removal Tool (DRT) on NASA’s Mars Science Laboratory (MSL) rover, Curiosity.

The Mojave field test was carried out on a small rocky hill at the NTC with many exposed blocks of weathered granite called tors. The site, now named “Asteroid Hill”, is reminiscent of the blocky surface of Near-Earth Asteroid (25143) Itokawa, which was explored in 2005 by Japan’s Hayabusa robotic spacecraft. “While neither the composition of the rocks nor the gravity at Asteroid Hill are similar to what they are on NEAs, the relevance of the site resides in the similarity in terrain texture (gravel and block abundance and sizes), topography, and scale between Asteroid Hill and Itokawa” notes Lee.

“This is an interesting analog site for planning future NASA robotic and human asteroid exploration, as it not only resembles the surface of the only sub-kilometer NEA explored by spacecraft to date, Itokawa, but it is well supported logistically by the U.S. Army’s National Training Center” said Terry Fong, Director of the Intelligent Robotics Group at NASA Ames Research Center.

The Mojave field test builds on an existing partnership between NASA and the U.S. Army’s National Training Center at Fort Irwin. The latter is home to NASA’s Goldstone Deep Space Network (DSN) tracking station. “The National Training Center’s participation in this field test with NASA represents another positive development in our Joint Interagency Intergovernmental and Multinational (JIIM) partnership. It allows NTC to showcase it’s soldiers, the NTC community, and NTC’s vast training resources” said Cyle Fena, Deputy G3 at the NTC.

The Mojave Field Test will be featured as part of an upcoming television documentary filmed by First Canyon Media, Inc, titled Mission Asteroid. Produced by the Canadian Broadcasting Corporation (CBC), Mission Asteroid is expected to air in North America in Fall 2013.

For more information, please visit www.seti.org and www.marsinstitute.info or contact:

Ms. Karen Randall
SETI Institute, Public Affairs Office Email: krandall@seti.org
Tel: +1 650 960 4537

Mr. Pascal Lee
Mars Institute
E-mail: pascal.lee@marsinstitute.net




All text copyright SETI and Mars Institute 2014

Friday, 4 July 2014

Knowing The Age of a Star Will Help Determine its Planets' Habitability

X-Class Solar Flare. Source: NASA

In about 4 or 5 billion years, the Sun will become a red giant, its atmosphere bloated, Earth's surface rendered uninhabitable. But life will have ceased to exist on Earth a lot sooner than this. Runaway heating will cause massive climate change effects. It is possible that with this increased influx of energy, the resulting storms may make it very difficult for life to survive, with ferocious winds sandblasting the Earth, while other regions bake in unbearable heat. If human civilizations still exist on Earth, they may have migrated towards the polar regions to survive the increased temperatures.

Liquid water may be a necessity for life in purely astrobiological terms, but a storm-lashed, sunbaked world would be hellish. The presence of water is a good starting point, but the age of a planet's parent star must also be factored in when ascertaining the habitability of newly discovered worlds.

Ancient Proteins Show That Evolution Can Take Hairpin Turns

Cortisol molecule. Source: Wikimedia Commons

By resurrecting ancient protein molecules, geneticist Joe Thornton at the University of Chicago has concluded from studies of an early precursor to the protein responsible for the stress response, the Glucocorticoid Receptor (GR), that modern GR could only have developed in one way.

This essentially means that mammalian biology could have turned out very differently. In terms of evolution, such an improbable developmental quirk would suggest that life arising elsewhere might be very different from that on Earth.

many of our body’s systems work as they do because of very unlikely chance events that happened in our deep evolutionary past - See more at: http://www.astrobio.net/news-brief/resurrected-proteins-alternate-histories-sure-path-modernity-physiology/#sthash.DnUSrw3b.dpuf
many of our body’s systems work as they do because of very unlikely chance events that happened in our deep evolutionary past - See more at: http://www.astrobio.net/news-brief/resurrected-proteins-alternate-histories-sure-path-modernity-physiology/#sthash.DnUSrw3b.dpuf
many of our body’s systems work as they do because of very unlikely chance events that happened in our deep evolutionary past - See more at: http://www.astrobio.net/news-brief/resurrected-proteins-alternate-histories-sure-path-modernity-physiology/#sthash.DnUSrw3b.dpuf
"Many of our body's systems work as they do because of very unlikely chance events that happened in our deep evolutionary past," Joe Thornton told Astrobiology Magazine.

You can read the full article here.

many of our body’s systems work as they do because of very unlikely chance events that happened in our deep evolutionary past - See more at: http://www.astrobio.net/news-brief/resurrected-proteins-alternate-histories-sure-path-modernity-physiology/#sthash.DnUSrw3b.dpuf


Thursday, 3 July 2014

Life Among the Stars: Why We Can Be 100% Sure That Intelligent Life Exists in Space

 Galaxy-IC-3418. Source: NASA

This was my first astrobiology article, originally published on Yahoo; it gives a very basic overview of the subject of astrobiology, the possibility of extraterrestrial contact, and the idea that human life may not be entirely of this planet.

Can intelligent life arise in the cosmos? The existence of human beings is living proof that it can. So that’s the title of this article covered. But does life exist elsewhere in space? The scientific community has come round to the idea that it almost certainly does. Astronomers from SETI (Search for Extraterrestrial Intelligence) recently told the United States Congress that we would be able to prove within the next 20 years that alien life exists.

The scientific pursuit for knowledge of life in the universe is called astrobiology. Still think alien life equals flying saucers and little green men? Well, astrobiology is a very real, and very active, branch of scientific enquiry. Institutes of research such as NASA Ames and SETI have focused on some key aspects of astrobiology, including the search for extrasolar planets, the study of extremophiles (organisms that thrive in extreme conditions), and the conditions required for life to appear in the first place.

You may think that Earth is unique in having life, but there may be other places even within our own solar system where life may exist, such as Enceladus, one of Saturn’s moons, with is thought to have an ocean of water under its frozen surface. There is clear evidence that Mars once had water flowing on its surface, so even our closest neighbor may have harbored at least primitive life in its past – and perhaps it still does.

Beyond our solar system, other planets similar to Earth may also have been the birthplace of living organisms. Planets such as the newly discovered Kapteyn b are likely to have at least some of the conditions necessary for life. Interestingly, Kapteyn b is also relatively close to us – only 13 light years away – meaning that we may have a chance of visiting it... once we make the breakthroughs in physics required to master interstellar travel, that is.

Given the age of the universe and the likelihood that there are countless places suitable for life to arise, it is possible that some of these have developed intelligence. Of these, some may have organized themselves into civilizations, developed technology, and even mastered space flight. Other worlds, much older than our own, would have had more time to develop, and may possess knowledge and technology far in advance of our own.

What would happen if we actually made contact with an extraterrestrial civilization? Given the likelihood of their existence, and the possibility that some of them may be capable of advanced space travel, a visit from another race is plausible, if unlikely. What implications for civilization would a meeting of our cultures hold? Even knowing that they exist, via direct obervation, or through radio or other communications, would have a profound effect on our society. Religious beliefs, political ideology, scientific knowledge, even the way in which people go about their daily lives – everything would be affected in ways that are difficult to predict. In short, it would be the single most important shift in human perspective ever.

That’s assuming ETs don’t just destroy us outright: a visiting envoy may unwittingly carry diseases to which we would have no immunity; or worse: they may actively seek to eradicate us. A highly advanced race may view us as dangerous, backwards and barbaric, and they’d have a point. Or they may be after our resources, what’s left of them. At the very least, the Earth would certainly be of scientific interest to a visiting race. Physicist Stephen Hawkins has warned against making our position known, since extraterrestrial races may not have our best interests at heart.

But what are our best interests, anyway? After all, it could be advantageous for Earth to be part of a consortium of civilizations, provided they let us in. To be able to share scientific knowledge, to learn and make use of new discoveries, and to understand incredible new cultures, would broaden humanity’s horizons in ways our ancestors could never have imagined.

Never before have we been so close to finding extraterrestrial life. But what if the distinction between terrestrial and extraterrestrial life isn't quite that straightforward? The theory of panspermia describes the ability of microorganisms to propagate suitable habitats in space, surviving the harsh vacuum between worlds, by travelling on meteorites and other space debris. Is it possible that some of the bacteria and viruses on Earth were actually brought here by meteorites? Considering that part of human DNA actually comes from viruses  it may be possible that human beings are at least partially extraterrestrial in origin. But even without extraterrestrial virus DNA, the idea that we are not entirely of this Earth is a practical certainty: NASA scientists have found some of the amino acidsnecessary for life on comets, confirming that some of the components of life came to Earth from space. The line between terrestrial and extraterrestrial is being continually blurred; Earth biology is truly a blend of astronomical sources.

We are close to discovering that life exists elsewhere. As soon as scientists find even the first bacterium in space, we will have to accept that we may not be alone, and that one day we may take our place in a far wider community than we had previously imagined.

Sunday, 2 March 2014

Earth Dodged a Bullet: The Solar Superstorm Nobody Told You About

The July 2012 solar superstorm almost struck Earth. Source: NASA

A recent communication from NASA describes how close the Earth came to getting a debilitating blast from the Sun two years ago. A double coronal mass ejection (CME) narrowly missed the Earth, shooting out radiation that would have knocked out all telecommunications devices on the planet, along with all electrically powered equipment.

Described as a solar superstorm, the July 2012 CMEs would have caused lasting damage: "If it had hit, we would still be picking up the pieces," says Daniel Baker of the University of Colorado. Although it somehow failed to make the news in 2012, the event was described in a paper produced by NASA scientists at the time entitled "A major solar eruptive event in July 2012: Defining extreme space weather scenarios".

"I have come away from our recent studies more convinced than ever that Earth and its inhabitants were incredibly fortunate that the 2012 eruption happened when it did," Baker said in the recent press release from NASA. "If the eruption had occurred only one week earlier, Earth would have been in the line of fire."

A report by the National Research Council into the socio-economic impact of such an event warned of "extensive social and economic disruptions."

It went on to add, "Power outages would be accompanied by radio blackouts and satellite malfunctions; telecommunications, GPS navigation, banking and finance, and transportation would all be affected.

"Some problems would correct themselves with the fading of the storm: radio and GPS transmissions could come back online fairly quickly.

"Other problems would be lasting: a burnt-out multi-ton transformer, for instance, can take weeks or months to repair. The total economic impact in the first year alone could reach $2 trillion, some 20 times greater than the costs of a Hurricane Katrina."

So what is the probability that a flare this big could actually hit Earth? Physicist Pete Riley published a recent paper in Space Weather called "On the probability of occurrence of extreme space weather events" in which he explained that there is a 12% chance that a flare of this magnitude will strike Earth in the next ten years.

And according to Ashley Dale, writing in Physics World, violent superstorms occur every 150 years - and we're five years overdue.

With odds like these, it may be a good idea to be prepared. According to advice available from the US Government, families should have a communications plan, and households should have emergency kits on hand. Check out the ready.gov website for more ways in which you can be prepared for an extreme space weather event. You can also keep an eye on solar storm warnings with NOAA's Space Weather Prediction Center.

Monday, 28 October 2013

The Ecology and Conservation of Puma concolor in North America

Puma concolor. Source: U.S. National Park Service

The Ecology and Conservation of Puma concolor in North America


The cougar, Puma concolor, is a large American cat, up to 2.6 m in length, with a comparatively small, rounded head with muscular jaws and characteristically rounded ears. It has a uniformly beige coat; the uniformity of colour is expressed in the cougar’s Latin name, concolor, and differentiates it from any other American cat species, all of which, for example the lynx, are patterned to some degree (Miller, 2007).

Taverna et al. (1990) describe the habitat of the cougar as being the most wide-ranging of any large American carnivore, inhabiting rocky outcrops, low to dense shrub, chaparral, and densely wooded areas. Maehr et al. (2004) even identifies shopping centres in Florida as viable habitat for the cougar, where the animals exhibit similar traits to populations living in naturally sparse landscapes.

The cougar was once widespread throughout the whole of the United States (Sweanor, et al.,1999). Human persecution forced the cougar into remote western regions, effectively removing it from the eastern states. P. concolor has a range encompassing 13 western states, while subspecies P. concolor coryi and P. concolor stanleyana exist in Florida (Maehr et al., 2002).

Habitat fragmentation, mainly by the building of roads is leading to cougar ranges being limited (Beier, 1993), and a need for a minimum habitat area study for cougars has been identified in order to properly maintain cougar numbers in the face of social, industrial and economic progress.

Husseman et al. (2003) found that wolves and cougars share a prey base. Elk form the main prey item for wolves and cougars. Mule deer, bighorn sheep and mountain goats make up the rest of the prey base. However, wolves were found to be more likely to take juveniles of all prey species, while cougars were able to take adults, reducing direct competition.

Beier (1993) reported that the independent nature of adult female cougars acted to regulate density, and that male density was separately defined by the territorial nature of adult males. Female density is primarily regulated by vegetative land cover, geological factors, and prey accessibility, since it is her responsibility to raise young and provide suitable cover and sustenance for them. Male numbers are affected by competition for females, and so their range is partially delimited by the same abiotic factors that influence distribution of females. However, since ground cover is less of an issue for the adaptable cougar, it is behaviours, particularly sexual and parental, that govern range, with ranges being relative to those of other adults, and density regulation may therefore been seen as an extension of behavioural factors.

Population dynamics are further affected by competition from bears and wolves, where those species’ ranges overlap with cougar territories (Riley et al., 2004). Wolves are being actively reintroduced throughout the western United States, and there is a projected conflict of interests between both conserved species (Sweanor et al., 2000). White-tailed deer are colonising many valley locations in the western states(Ripple, 2006), and these are being followed by cougars not normally associated with valley environments. In fact, wolf habitation of valleys may have affected cougar range at the time when these two species were first learning to live together, and may have been the deciding factor in limiting cougars to higher altitudes in those areas.

The recent cougar colonisation of valleys, such as those in Yellowstone National Park, has led to confrontations between wolves and cougars, in some cases leading to mortality in both species (Knopf, 2009). Wolf conservation is therefore impacting on cougar regeneration, forcing the cats to live in less desirable habitats, such as rocky areas to which the cougars are better adapted than the wolves.

The sampling and monitoring techniques currently employed by scientists looking at the regeneration of P. concolor in North America are various and range from active trapping (Sweanor et al., 2000) to passive tracking (Miller, 2007).

Spring activated animal snares were set up around Wyoming by Sweanor et al. (2000) to capture independent adults and mature cubs. These animals were ear-tagged, radio-collared and marked with coded ear tattoos. In a separate study in Florida, radio-tagged cougars were monitored by aircraft (Maehr et al., 2002)

Bounties were regularly paid to cougar hunters (Knopf et al., 2009; Riley et al., 2004), and although this practice has ceased, the term bounty is still used to refer to hunted animals. However, cougars have been reclassified as game animals and are still hunted in all states except California and Oregon. Bag counts are currently limited to one kill per day per season, and kills are recorded, leading to a reliable system of cougar population assessment. Changes in hunting style have led to conflict with new legislation, however: the practice of treeing has been banned in all states except Texas (Sweanor, et al., 2000). This entails hunting a cat with dogs until it runs up a tree. The cat is then surrounded and shot at close range. Although curtailing overt cruelty towards cougars, the ban on treeing has had the knock-on effect of reducing the amount of time a hunter has to look at the animal before killing it. Legislation limits the killing of females; when treeing an animal, hunters could differentiate between males and females and spare the latter. Now, however, both sexes are shot indiscriminately.

A roadkill survey in Florida by Lotz and Land (2007) estimated the Florida cougar population and set out to discover the relationship between road deaths and recorded births. The lowest annual estimate of cougar births was determined by analysing birth and death rates of known cougar populations as well as numbers of cougar bodies found on local roads. It was found that the amount of Florida cougar roadkills formed a set percentage of the total numbers of the cougar population, suggesting that the roads were disturbing established cougar ranges.

Cougars have dog-like tracks (Miller, 2007), but a number of features easily distinguish the two species. Kill sites can also identify predators: kill efficiency, wound depth and length, subcutaneous haemorrhaging, carcass entrance and covering of prey are all indicative of predator identity.

Ever since Europeans colonised the land mass now known as the United States, any dangerous animal was considered fair game (Knopf et al., 2009), and could be destroyed to protect livestock as well as the settlers. All wild animals were considered a food source in the early days of the formation of the United States, so cougars may well have been hunted for sustenance as well as for homeland security reasons.

Three waves of cougar management have occurred in modern times: firstly, an attempt at total annihilation, succeeded by managed sport hunting to ameliorate livestock depredation, and finally an ostensibly concerted effort to protect the cougar’s place in natural American ecosystems (Riley, 2004).

It has been demonstrated (Ripple et al., 2006) that the removal of cougars has allowed populations of their prey species, particularly ungulates, to multiply exponentially. These large numbers of unpredated ungulates in turn over-graze the native herbaceous biomass, leading to the collapse of trophic cascades and causing localised secondary extinctions.

However, P. concolor is now regaining some of its former North American territories (Gloyne et al., 2001; Maehr et al., 2002; Sweanor et al., 2000). This is due in large part to a relaxation of human persecution and a coordinated effort on behalf of the majority of states (Knopf et al., 2009), with the notable exception of Texas, where cougars are regarded as a pest species and hunting remains unregulated. Wildlife underpasses are also being used in Florida to counter habitat fragmentation (Lotz, M., Land, D., 2007) and are shown to be positively affecting local cougar populations.

In terms of habitat, the eastern regions of the United States present large, viable ecosystems into which the cougar can be reinserted. The cougar should be able to pick up its role as a top predator relatively easily in those areas where habitat allows, and suitable prey species still exist (Taverna, 1999). However, the cougar’s main obstacle to reintroduction in Northern America is the public. Beier (1991) suggests that the cougar’s negative image, caused mainly by an increase in attacks on humans as the cougar’s range extends towards concentrations of human habitation, could be positively altered through information campaigns, and by providing visitors to areas of known habitation with advice regarding possible encounters.


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