Tag Archives: Earth

Life

In an effort to determine if conditions were ever right on Mars to sustain life, a team of scientists, including a Michigan State University professor, has examined a meteorite that formed on the red planet more than a billion years ago.

And although this team’s work is not specifically solving the mystery, it is laying the groundwork for future researchers to answer this age-old question.

The problem, said MSU geological sciences professor Michael Velbel, is that most meteorites that originated on Mars arrived on Earth so long ago that now they have characteristics that tell of their life on Earth, obscuring any clues it might offer about their time on Mars.

“These meteorites contain water-related mineral and chemical signatures that can signify habitable conditions,” he said. “The trouble is by the time most of these meteorites have been lying around on Earth they pick up signatures that look just like habitable environments, because they are. Earth, obviously, is habitable.

“If we could somehow prove the signature on the meteorite was from before it came to Earth, that would be telling us about Mars.”

Specifically, the team found mineral and chemical signatures on the rocks that indicated terrestrial weathering – changes that took place on Earth. The identification of these types of changes will provide valuable clues as scientists continue to examine the meteorites.

“Our contribution is to provide additional depth and a little broader view than some work has done before in sorting out those two kinds of water-related alterations – the ones that happened on Earth and the ones that happened on Mars,” Velbel said.

Image Credit: Michigan State University

Image Credit: Michigan State University

The meteorite that Velbel and his colleagues examined – known as a nakhlite meteorite – was recovered in 2003 in the Miller Range of Antarctica. About the size of a tennis ball and weighing in at one-and-a-half pounds, the meteorite was one of hundreds recovered from that area.

Velbel said past examinations of meteorites that originated on Mars, as well as satellite and Rover data, prove water once existed on Mars, which is the fourth planet from the sun and Earth’s nearest Solar System neighbor.

“However,” he said, “until a Mars mission successfully returns samples from Mars, mineralogical studies of geochemical processes on Mars will continue to depend heavily on data from meteorites.”

Velbel is currently serving as a senior fellow at the Smithsonian Institution’s National Museum of Natural History in Washington D.C.

The research is published in Geochimica et Cosmochimica Acta (citation below), a bi-weekly journal co-sponsored by two professional societies, the Geochemical Society and the Meteoritical Society.

Source: Michigan State University

Reference:

Stopar, J., Taylor, G., Velbel, M., Norman, M., Vicenzi, E., & Hallis, L. (2013). Element abundances, patterns, and mobility in Nakhlite Miller Range 03346 and implications for aqueous alteration Geochimica et Cosmochimica Acta, 112, 208-225 DOI: 10.1016/j.gca.2013.02.024

Image Credit: NASA

Image Credit: NASA

Martian exploration is unquestionably a hot topic right now. Mainstream media outlets have largely focused on the most visible efforts of the Curiosity mission, and that’s a good thing. While people might be thrilled with the photographs that they have an opportunity to view on their screens however, they may be less familiar with the implications of this research for the future.

For instance, previously little was known about how the Martian permafrost segments melted, and some researchers weren’t even convinced that significant melting occurred. Mars has no visible oceans, and that means that there really isn’t anywhere for huge amounts of fluid to flow. Thanks to current research efforts, data collected thus far has put together a more complete image of the melt patterns of sedimentary rocks on the Red Planet.

This data is useful in helpful in determining whether life once existed on Mars. While permafrost melt patterns aren’t really able to confirm or deny astrobiology theories, they’re an awfully good start. Although it’s not possible to determine if there were ever organisms that evolved as a result of these flows simply by looking at them, some researchers may argue that further probes are necessary to delve into this area further.

Outside of the search for life (current or prior) on Mars, the seasonal melting model also suggests that oceans could eventually be constructed on the planet. This is particularly exciting where terraforming projects are concerned. With stores of carbon dioxide readily available in the Martian atmosphere, it may be possible to produce something similar to a greenhouse effect. Once this occurs, plant life would be able to produce readily available supplies of oxygen (that stuff we humans need to live) while cooling off the planet in the process.

The research efforts currently under way may help scientists to determine more efficient methods of accomplishing this Martian overhaul. For instance, scientists currently know that seasonal melts could provide the necessary ingredients for seasons that are somewhat similar to those on Earth. Winter phases might be useful for helping to reduce the planets’ cooling process as well.

Tracking weather patterns on the Red Planet might also help researchers who would prefer to manipulate the Martian climate with lenses or shields. Once enough is known about weather and geological patterns on Mars, large lenses could be built in geostationary orbit. These would increase the amount of sunlight directed towards the planet. While engineers would have to be extremely careful not to pump dangerous levels of ultraviolet radiation towards colonists, these mirror systems might help to provide necessary light and heat for the planet once we’ve colonized the planet.

Detecting salt solutions have also helped researchers to better understand the chemical composition of the Martian surface. Industrial facilities may some day work mines on the planet to retrieve resources that are necessary to sustain human colonists. This could, in essence, create an economy on the planet. Additionally, as mineral resources continue to become increasingly rare on Earth, these materials could prove invaluable to future Earth-based citizens as well. Rovers actually prove that mining on Mars could probably be done with current technology – yet another benefit derived from current research efforts.

Few will deny that we are witnessing history almost daily as results from the Curiosity mission are released to the world. While this is without question an amazing time, I think it’s important that we recognize the amazing research being conducted in the process – research that could potentially impact the future of humanity in ways we are currently unable to understand.

Mars Earth comparison

Reference:

Peters, G., Smith, J., Mungas, G., Bearman, G., Shiraishi, L., & Beegle, L. (2008). RASP-based sample acquisition of analogue Martian permafrost samples: Implications for NASA’s Phoenix scout mission Planetary and Space Science, 56 (3-4), 303-309 DOI: 10.1016/j.pss.2007.10.001

Amato P, Doyle SM, Battista JR, & Christner BC (2010). Implications of subzero metabolic activity on long-term microbial survival in terrestrial and extraterrestrial permafrost. Astrobiology, 10 (8), 789-98 PMID: 21087159

Image Credit: University of Washington

Image Credit: University of Washington

Researchers still have much to learn about the volcanism that shaped our planet’s early history. New evidence from a team led by Carnegie’s Frances Jenner demonstrates that some of the tectonic processes driving volcanic activity, such as those taking place today, were occurring as early as 3.8 billion years ago. Their work is published in Geology [citation below].

Upwelling and melting of the Earth’s mantle at mid-ocean ridges, as well as the eruption of new magmas on the seafloor, drive the continual production of the oceanic crust. As the oceanic crust moves away from the mid-ocean ridges and cools it becomes denser than the underlying mantle. Over time the majority of this oceanic crust sinks back into the mantle, which can trigger further volcanic eruptions. This process is known as subduction and it takes place at plate boundaries.

Credit: Image of southwest Greenland by Jacques Descloitres, MODIS Land Rapid Response Team, courtesy of NASA Visible Earth.

Credit: Image of southwest Greenland by Jacques Descloitres, MODIS Land Rapid Response Team, courtesy of NASA Visible Earth.

Volcanic eruptions that are triggered by subduction of oceanic crust are chemically distinct from those erupting at mid-ocean ridges and oceanic island chains, such as Hawaii. The differences between the chemistry of magmas produced at each of these tectonic settings provide ‘geochemical fingerprints’ that can be used to try to identify the types of tectonic activity taking place early in the Earth’s history.

Previous geochemical studies have used similarities between modern subduction zone magmas and those erupted about 3.8 billion years ago, during the Eoarchean era, to argue that subduction-style tectonic activity was taking place early in the Earth’s history. But no one was able to locate any suites of volcanic rocks with compositions comparable to modern mid-ocean ridge or oceanic island magmas that were older than 3 billion years and were also free from contamination by continental crust.

Because of this missing piece of the puzzle, it has been ambiguous whether the subduction-like compositions of volcanic rocks erupted 3.8 billion years ago really were generated at subduction zones, or whether this magmatism should be attributed to other processes taking place early in the Earth’s history. Consequently, evidence for subduction-related tectonics earlier than 3 billion years ago has been highly debated in scientific literature.

Jenner and her team collected 3.8 billion-year-old volcanic rocks from Innersuartuut, an island in southwest Greenland, and found the samples have compositions comparable to modern oceanic islands, such as Hawaii.

“The Innersuartuut samples may represent the world’s oldest recognized suite of oceanic island basalts, free from contamination by continental crust”, Jenner said. “This evidence strengthens previous arguments that subduction of oceanic crust into the mantle has been taking place since at least 3.8 billion years ago.”

Source: Carnegie Institution

Reference:

Jenner, F., Bennett, V., Yaxley, G., Friend, C., & Nebel, O. (2013). Eoarchean within-plate basalts from southwest Greenland Geology DOI: 10.1130/G33787.1

Svensen H (2012). Geochemistry: Bubbles from the deep. Nature, 483 (7390) PMID: 22437609

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Universe

Understanding Space – Celestial Objects

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Space is a big, fascinating, and stunningly beautiful place. The universe is full of stars, galaxies, nebulae, planets, moons and much more. Ranging from lifeless rocky worlds such as Mercury to vast galaxies tens of thousands of light-years across, space is home to truly awesome displays of nature. Celestial objects, also known as astronomical objects, comprise the physical entities that make up the universe.

The universe has a hierarchal structure. On the smallest scales of astronomical objects, there is the Earth and our moon. The Earth is part of our solar system of eight planets while, in turn, our solar system is one of billions in the Milky Way galaxy. The Milky Way is one of 54 galaxies in the Local Group, a part of one of many superclusters that make up the universe – everything that exists.

The following guide, roughly in order from the smallest to the largest celestial objects, will help you to understand the scale of the universe, its hierarchal structure and some of the many fascinating things that lie beyond the borders of our world.

1 – Meteors

MeteoriteMeteors are small, rocky debris floating around in the vacuum of space ranging in size from grains of sand to massive boulders. When these enter the atmosphere of Earth or any other celestial body, they are called meteoroids. These bombard us constantly, but the vast majority of them burn up as they descend into the Earth’s atmosphere. This is precisely what shooting stars are – small, burning debris making brief streaks of light in the night sky as they are vaporized. If a meteoroid is either large enough or travelling fast enough to make it through the atmosphere without being annihilated, it will make it to the ground, becoming a meteorite.

Fun Facts about Meteors

  • The largest known meteorite is the Hoba meteorite in Namibia weighing about sixty tons. It is the worlds heaviest naturally occurring chunk of iron and it is believed to have hit Earth’s surface about 80,000 years ago.
  • The best-known meteor showers are the Perseids and Leonids that fall every year in August and November respectively.
  • Some meteorites on Earth originated from Mars, such as the famous Allan Hills 84001 meteorite. This one attracted a great deal of attention due to the presence of possible fossilized remains of Martian bacteria.

2 – Comets

CometComets are small, icy celestial bodies composed of a nucleus, coma and tail. The nucleus comprises the solid bulk of the comet and ranges in size from a hundred meters to a few dozen kilometers. Comets are characterized by spectacular comas and tails, leaving a long trail of bright matter behind them. There are over 4,000 known comets in the solar system and some have been known since ancient times. Many comets have enormous, elliptical orbits around the sun, many reaching maximum distances far beyond the orbit of Pluto.

Fun Facts about Comets

  • Extremely bright comets typically appear no more than once every decade. These are known as the Great Comets and are visible to the naked eye.
  • One of the most famous comets, Halley’s Comet (shown above) may have been the Star of Bethlehem referred to in the Bible. Halley’s Comet makes an appearance every 75 years.
  • The Great Comet of 1811 was clearly visible for almost nine months. It had a coma fifty percent longer than the diameter of the sun – up to 1,000,000 miles long!

3 – Asteroids

Asteroid MissionAsteroids are small celestial bodies of which there are many millions around the Solar System. Asteroids orbit the Sun just like planets do, but they are far smaller. Because of this, they also have negligible gravitational pulls and no atmospheres to speak of. Also, because of their lack of size and gravity, smaller asteroids are irregularly-shaped rather than near-perfect spheres like planets and dwarf planets. The majority of known asteroids are located in the Asteroid Belt between the orbits of Mars and Jupiter. Asteroids are also found in the Kuiper Belt beyond the orbit of Pluto.

Fun Facts about Asteroids

  • An asteroid impact may have been what wiped out the dinosaurs in the Cretaceous-Palaeogene extinction event 65.5 million years ago.
  • Some asteroids have moons (satellites), such as 243 Ida and its tiny moon, Dactyl. Until its discovery, it was thought that only planets had moons.
  • Asteroids may one day be used for mining thanks to their abundance of valuable metals and materials.

4 – Dwarf Planets

Dwarf PlanetDwarf planets are characterized as small planets that are massive enough to have gravitational forces great enough make them spherical in shape. They also orbit the sun directly. Most notably, Pluto is a dwarf planet that was reclassified as such in 2006, until which point it had, since its discovery in 1930, been described as the Solar System’s ninth planet. All of the five known dwarf planets are considerably smaller than the Earth’s Moon. Dwarf planets may also have their own moons. Pluto, for example, has at least five. Dwarf planets are too small and do not have a high enough gravitational pull to be able to retain any more than a trace atmosphere.

Fun Facts about Dwarf Planets

  • Ceres, in spite of being the smallest known dwarf planet, was the first one discovered due to the fact that it is the largest non-planetary body in the inner solar system. It was discovered in 1801.
  • All other dwarf planets are found in the Kuiper Belt extending beyond the orbit of Pluto.
  • In 2015, NASA’s New Horizons space probe will visit the dwarf planet Pluto and take the first ever photos of its surface.

5 – Moons

Europa - MoonMoons, known as natural satellites in the scientific community, are objects ranging in size from tiny asteroids to bodies larger than the planet Mercury. They are gravitationally bound to their host planets, just as the Moon is to Earth. Earth, of course, has only one moon, but some of the other planets in the Solar System have dozens. In total, there are at least 176 moons in the Solar System. Mercury and Venus have none as far as we know, while Mars has two and the gas giant planets have dozens. The first moons discovered around other planets were the four Galilean moons of Jupiter in 1610 by Galileo.

Fun Facts about Moons

  • Many smaller moons are captured asteroids, pulled into the orbit of planets by powerful gravitational pulls. The two Martian moons, Phobos and Deimos are two such moons.
  • One of Saturn’s moons, Titan, is the only moon in the Solar System known to have a thick atmosphere. Because of this and other factors, it remains one of the first places in the Solar System to search for extraterrestrial life.
  • Jupiter has more moons than any other planet in the Solar System with a total of 67! The four largest of these are Io, Europa (shown on right above), Ganymede, and Callisto. Ganymede is actually larger than the planet Mercury. These four moons are known as the Galilean moons.

6 – Planets

PlanetsThere are a total of eight planets in our solar system. Our solar system is comprised of the inner planets and the outer planets. The inner planets, in order of distance from the Sun, are Mercury, Venus, Earth, and Mars. Far beyond the orbit of Mars lie the outer planets, Jupiter, Saturn, Neptune and Uranus. These four planets are gas giants and, thanks to their size and gravitational influence, they each have numerous moons. Gas giants have no known solid surface. The planets of the Solar System vary dramatically. Mercury is a lifeless rock, Venus is a hellish inferno, Earth is home to the only forms of life that we know of and Mars still remains our first candidate in the search for extraterrestrial life either long dead or still present. Since 1995, many hundreds of planets have been discovered orbiting other stars as well. These are known as extrasolar planets.

Fun Facts about Planets

  • There are more than 850 planets orbiting stars other than our own (the Sun), and more are being discovered every week in large part due to the work of the Kepler Space Telescope.
  • Venus is the hottest planet in the Solar System with surface temperatures high enough to melt lead and air pressures as high as those one kilometer under the sea.
  • Water, a key ingredient for life as we know it, is common throughout the Solar System. Water ice is widely distributed on Mars and exists on the Moon, many comets and asteroids, and on various other astronomical bodies.

7 – Stars

StarStars form the center of solar systems, just like our own star, the Sun, is the center of our own Solar System. When you look up at the sky on a clear night, you can start to grasp the vastness of space and the countless trillions of stars in the universe. The vast majority of stars are far more massive than even the largest planets, with the smallest ones being considerably larger the Jupiter and the largest ones being hundreds times bigger than the Sun. The Sun is nothing special as far as stars go and, in fact, there are billions of other stars just like it in our galaxy alone. Just like the Sun, many other stars host planetary systems, some of which may be very much like our own (and possibly home to extraterrestrial life). Stars are classified by spectrum types and are designated by letters. Our sun is a class G star.

Fun Facts about Stars

  • The largest known star is the red hypergiant called VY Canis Majoris. 3 billion kilometers (about 1.86 billion miles) in diameter, the star would extend further than Saturn’s orbit if placed in our Solar System.
  • Our own star, the Sun, is approximately 1.4 million kilometers (nearly 870,000 miles) in diameter.
  • The nearest star to Earth other than the Sun is the triple-star system, Alpha Centauri, 4.3 light-years away. 4.3 light-years equates to approximately 40,000,000,000,000 kilometers. Travelling at 252,800 km/h, the speed of the fastest man-made object, the Helios 2 space probe, would take around 18,000 years to reach it.

8 – Galaxies

GalaxyStars make up galaxies such as our own galaxy, the Milky Way. The Milky Way is one of many billions of galaxies in the known universe. The Milky Way alone contains between 100 and 400 billion stars. Galaxies are vast, gravitationally bound systems containing not only stars, but also nebulae, rogue planets (planets without a host star) and various other celestial bodies. They fall into three broad classes described as elliptical, spiral and lenticular galaxies. Our own galaxy is a barred spiral galaxy characterized by an extremely bright and dense center of stars surrounded by swirling arms. Our own star system lies in one of the arms of the Milky Way orbiting the galactic center at a distance of 26,000 light-years (each light-year is roughly 6 trillion miles). The nearest proper galaxy beyond the Milky Way is Andromeda, about 2.5 million light-years away across a virtually empty void.

Fun Facts about Galaxies

  • The most distant galaxies tell us about the history of the universe. This is because we see them as they were when the light left them – effectively, we are looking back in time.
  • There are only three galaxies visible to the naked eye from Earth. These are the dwarf galaxies known as the Small and Large Magellanic Clouds and the Andromeda Galaxy.
  • There are at least 100 billion galaxies in the known universe, but there may be dozens times more than that.

9 – The Universe

Universe2The observable universe comprises absolutely everything that we can see from Earth. Anything that is further away than the edge of the observable universe is invisible to us due to the fact that the light has not yet completed the long journey to Earth. The furthest we can see is approximately 13.75 billion light-years. The universe is made up of superclusters containing clusters of galaxies such as the Local Cluster where our own Milky Way galaxy is located. What lies beyond the observable universe is not known, although the universe is still generally thought to be finite. The universe is believed to have been created by the Big Bang and has been rapidly expanding ever since.

Fun Facts about the Universe

  • The universe is approximately 93 billion light-years in diameter, but due to the fact that the universe is expanding, we can still see things that are too far away, because we are seeing them as they were when they were closer to us.
  • The largest known object in the universe is the Sloan Great Wall, an enormous wall of galaxies about 1.38 billion light-years in length.
  • The size of the universe and the number of galaxies and stars in them suggest that life-supporting worlds, although clearly rare, could easily number in the billions.

Honorable Mention – Black Holes

Black HoleBlack holes are perhaps the most fascinating and bizarre of all the objects in space. Sometimes, when a star dies, it starts to collapse, the matter of which it is composed becoming more and more densely packed. Eventually, the star is so massive that its gravitational pull becomes so great that the escape velocity reaches the speed of light. When not even light is able to escape the surface, the star becomes invisible and only detectable by its influence on the surrounding area. The black hole is composed of an event horizon that marks the point of no return. Additionally, black holes have a gravitational singularity in the center that is infinitely dense, yet has no volume. At this point, the laws of physics simply break down, making black holes the most enigmatic objects in existence. Black holes are thought to exist in the center of many galaxies, including the Milky Way.

Image Credits: NASA/JPL

Image Credit: NASA Ames

Image Credit: NASA Ames

I often ask others if they would live in space or on another planet if given the opportunity. More often than not, the answer is in the affirmative. But what if you were given the chance and actually wanted to go, but were declined because you weren’t selected by a computer algorithm as one of the lucky space travelers? Or worse, what if you were declined because of your cultural background or because your genetic profile was deemed inappropriate?  What about those that do venture off to live in space or on other worlds…will they suffer the types of loneliness that individuals experience in major cities here on Earth today? These are the questions that I thought I’d delve into today.

Loneliness in Space

Overcrowding is a major concern in many parts of the world today. People often feel like they’re being shoved into boxes that they don’t really fit into. Since the early days of the Industrial Revolution, a great number of individuals have felt as if they are all alone in the world. Large cities don’t make for the best of neighbors. Even though other members of the human race surround people, they’re seldom able to make any genuine connections with those who live close by. This sort of a problem is only worsened by the prospect of space colonization.

The feeling of loneliness is usually portrayed as being experienced by those who are truly without anyone near them. However, individuals can actually become lonelier when other people that they don’t connect with show up within their circle of friends. Of course, in many cases, these people don’t even really have a circle of friends in the first place.

While one person adrift in space might be able to comfort him or herself with the idea that others are back home on planet Earth, ironically the same cannot always be said of someone who were to live in a colony habitat. If other people surrounded that same individual, he/she would probably end up experiencing increased feelings of loneliness — just as so many do in cities around the world today.

This is something that’s been observed by Earthbound psychologists for decades, but it would possibly worsen in orbital complexes and on colonized worlds. Sci-fi writers have long stressed the importance of choosing the right colonists for space missions based on genetic profiles. But it seems that culture and the ability to work together are actually more important indicators of who should go off together into the great unknown.

Un-natural Selection

Using some sort of computer algorithm to select candidates for space travel is probably the worst idea I can imagine. This is a common trope in many pieces of fiction, but engineers working on global cities might have actually found a better way to psychologically equip generations of space pioneers. They have suggested that those who are culturally similar to people they live with might very well make the best partners. Seems like common sense, right?

Source: NASA

Source: NASA

While this sounds reasonable, it opens up an entirely new thought process for those who are planning generational space missions. If colony ships are set out on extremely long voyages, people will want to be with those that they have bonded with or care about. Letting a community choose who they want to be with the same way that they always have on Earth might be the best idea.

Genetic selection might sound logical and some people have suggested that it could produce the best stock for other worlds. However, this is a throwback to the sort of eugenic thinking that predominated the early 20th century. It was a mistake here on Earth and the same holds true of space. If space colonies are ever actually going to solve population problems, they need to be able to function much like regular cities do today. By letting people live in space the same way that they always have on Earth, the average citizen is far more likely to adapt to others in an acceptable manner.

There are those who would say that this limits diversity, but in reality it doesn’t. Genetic selection programs and the like would actually seek to create a race of space colonists who are in some way similar to one another. This would limit diversity, and would also have the side-effect of making a civilization less resistant to disease or similar catastrophes. For instance, one colony of microbes could wipe out an entire colony if it were built in such a way. The same could be said of a generational space mission attempting to reach another star system.

Humanity has never been perfect. It is these imperfections that very well may help our species to survive in space in the future.

Reference:

Yusof, N., & van Loon, J. (2012). Engineering a Global City: The Case of Cyberjaya Space and Culture, 15 (4), 298-316 DOI: 10.1177/1206331212453676

Saaty, T., & Sagir, M. (2012). Global awareness, future city design and decision making Journal of Systems Science and Systems Engineering, 21 (3), 337-355 DOI: 10.1007/s11518-012-5196-z

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While scientists like to bandy origin of life theories around, they seldom make the connection to astrobiological research. These theories, however, have a lot to suggest about how life may have developed on other worlds. According to recent studies, low-density vesicular volcanic rock material like pumice might have acted as something like a natural laboratory for chemical reactants that produced the so-called primordial soup. Early geological records show that pumice clasts were abundant in the approximate 3,460 Ma era period.

Samples collected from the Pilbara region in Western Australia exhibit signs of carbon. Traces of titanium oxide and iron sulfide were also found in the samples. Both of these are catalysts for certain reactions that suggest basic life processes. Other researchers have pointed to aluminosilicate minerals in the geological samples, which might be some sort of remains left by prokaryote life forms. Early prokaryotes might have colonized the clasts before they were buried, and therefore what scientists are currently examining are modified forms of what would have otherwise been regular rocks.

In any case, these are some of the earliest examples of life forms currently known to researchers. By examining these samples, it’s somewhat same to assume that a profile can be put together of what substances to look for when searching for remnants of life in astronomical materials. Asteroids are probably what have been covered the most in these studies, but they aren’t the only places to search. If a meteorite were to strike Earth that resembles these clasts, it would pretty exciting nevertheless.

When taking soil samples from other planets, researchers haven’t always been sure what they’re looking for. The Viking probes on Mars attempted to incubate microbes, and this proved relatively fruitless. However, future missions could instead try to locate geological samples that resemble those collected from the Pilbara region. There are plenty of samples in laboratory storage facilities anyway, and these could be examined without any real problems if permission could be granted to scientists.

That’s assuming that evolution takes an identical path on every planet. While some people might suggest this is a shortsighted way to look at the problem, it does have the benefit of making the fewest assumptions. Either way, there’s no reason not to take a look at existing rock samples to see if they match any of these chemical configurations. There’s little risk, and the benefit for a pretty impressive reward if successful.

Reference:

Martin D. Brasiera, Richard Matthewmana, Sean McMahonb, Matt R. Kilburnc, & David Wacey (2013). Pumice from the ∼3460 Ma Apex Basalt, Western Australia: A natural laboratory for the early biosphere Precambrian Research, 224, 1-10 : 10.1016/j.precamres.2012.09.008

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Some people have proposed that planets composed mostly of water could serve as cradles for advanced cetacean civilizations. There may be some truth to this. Research proves that cetacean brains have changed considerably throughout the 55 million years that they’ve inhabited the Earth. That’s one of the reasons that they’re so often cited in academic research involving astrobiology. Cetacean species represent the only real alternative evolution to intelligence that’s currently recognized by a majority of scientists.

While it might seem arrogant to say, cetaceans are not currently thought to be as intelligent as humans. Aquatic mammals are brilliant, and they sometimes seem to have psychological processes that resemble those of humans. In fact, they have many of the same psychological issues that humans do. However, they aren’t quite the same here on Earth.

Still, it seems that aquatic mammals could reach an even higher level of development if given enough time and/or the right environment. Proposing worlds where this is true is an interesting thought experiment. Tools and technology have evolved on Earth to be useful to those with hands and feet. This makes it hard to believe that aquatic mammals could construct civilizations resembling those on Earth.

Nevertheless, it’s possible for dolphins and whales to use many tools adapted for them by human handlers. They might very well have developed similar adaptations in their own cultures. No colony of such animals on Earth has ever created such things by themselves, so for now it’s merely an interesting concept. However, that doesn’t mean it’s impossible for this to occur on a planet where there was little or no threat to survival.

Some research has provided fantastical solutions for problems involving the use of tools by aquatic mammals. For instance, writers have sometimes suggested that machines could be manipulated by some form of telepathy. For now, that sort of thing is completely beyond our comprehension or understanding. Regardless though, the idea that aquatic beings could have developed superior intelligence and capabilities on other planets is a pretty cool one in my opinion. What do you think?

Nikolai Kardashev once speculated that advanced extraterrestrial civilizations could be classified by their energy usage. While energy conservation is stressed on Earth, energy is vast in space. Therefore, societies that have already journeyed to the stars can [theoretically] experience growth in ways that humanity can only dream of. He proposed that the first step in extraterrestrial development was the planetary level.

Background Reading [PDF]: Discipline of Choice for Public Policy Issues Concerning Extraterrestrial Life

Beings that had developed societies at the planetary level could be classified as Type I cultures. Humanity could be called a Type I culture. Type II civilizations used all of the power present in a star system. Species living in a Type III society would use power at the galactic level.

Public policy decisions surrounding extraterrestrial life have to be tempered around the possibility of coming into contract with members of different levels of technology. Scientific speculation illustrates the possibility of far more Type I societies than either of the other two classifications. Likewise, one might assume that most extraterrestrial life is microbial. Nevertheless, one could just as easily argue that visitors from another world would need to be at the galactic stage of development in order to survive the incredible voyage between two star systems. Trips could take immeasurable amounts of time at faster than light speeds. Sub-light vessels might take centuries to travel from one star to another.

Information on research surrounding the subject of extraterrestrial life has made policy decisions rather difficult. Governmental organizations are already pressured to make logical decisions regarding the possibility of contact with alien races. However, to what degree the public should know about these things is a major ethical question.

Freedom of Information Act mandates caused numerous US federal documents to be placed online. French documents were posted in 2007. The United Kingdom followed suit in 2008. Only time will tell what changes in public policy these documents will force.

It’s highly unlikely anyone will come across some sort of alien cover-up, but these do provide a framework for exo-political decision-making. Governments could then feel that passing laws dealing with extraterrestrial civilizations are normal. There would be plenty of consequences from that happening.

Additional Learning Resources:

Photo of the martian meteorite ALH84001. Dull, dark fusion crust covers about 80% of the sample. Image Credit: NASA/JSC

While most people associate the term microfossil with the strange ALH 84001 object, there are plenty of other more concrete examples of tiny fossilized organisms. Research conducted with scanning electron microscope equipment has created a wide array of scientific literature regarding these small remains of living organisms. While marine objects don’t necessary have anything to directly do with the biogenic hypothesis of structures in meteorites, they do suggest that it’s possible for some meteorites to have remnants of antediluvian organisms.

This includes shergottite, nakhlite and chassignite meteorites that have come from Mars. It might be ironic that less attention is paid to Venus, when that planet is perhaps more like the Earth than Mars is. In fact, Venus is sometimes called Earth’s twin.

Structures resembling fossils make up the most solid body of proof for extraterrestrials. While research carried out by organizations like SETI isn’t usually accepted by mainstream academia, ALH 84001 showed up on the nightly news. These stories also illustrate the value of finding meteorite material on the Earth’s surface. Space exploration is a noble goal, but the process of recovering meteorites is far easier. It’s something that can be done immediately without any additional technology. That makes it a low hanging fruit for the hands of hungry scientific investigators.

Reference:

Emmanuelle J. Javaux, Craig P. Marshall, & Andrey Bekker (2010). Organic-walled microfossils in 3.2-billion-year-old shallow-marine siliciclastic deposits Nature, 463, 934-938 DOI: 10.1038/nature08793

Additional Learning Resources:

ResearchBlogging.org

Christiaan Huygens (1629-1695) was a Dutch polymath who is well known in some circles to this day. While he spent some time in France and England, Huygens lived the latter portion of his life in his native Holland. Having commented on religion while living in many different countries, Huygens espoused a personal philosophy similar to many aspects of modern science.

The modern pendulum clock was among his more illustrious inventions. Horology is the study of measuring time, and it became something of an obsession for him. Nevertheless, he’s also well remembered among astronomers for discovering the moon Titan. His contributions to the field of optics made modern telescope construction possible as well.

While his calculations regarding stellar distances weren’t always accurate, they were always interesting. Huygens made a screen facing the sun and from measurements taken with this device, he figured out that the sun was approximately the same intensity as that of Sirius. By taking the angle and diameter of the hole, Huygens surmised that Sirius was 30,000 times further away from the Earth than the sun is. However, Sirius is actually around 500,000 times further away. Huygens didn’t realize that Sirius was several times brighter than the sun. Strangely enough, his calculations were accurate for the data he was working with.