Showing posts with label Chicxulub meteorite. Show all posts
Showing posts with label Chicxulub meteorite. Show all posts

Wednesday 15 September 2021

Life in a rut: if microbes are commonplace, where does that leave intelligent aliens?

A few years ago I wrote about how Mars' seasonal methane fluctuations suggested - although far from confirmed - that microbial life might be present just under the Martin surface. Now another world in our solar system, the Saturnian moon Enceladus, has ignited discussion along similar lines.

The Cassini probe conducted flybys of Enceladus over a decade, revealing that Saturn's sixth largest moon was venting geyser-like jets of material, including water vapour, from its southern polar region. The material being emitted from these vents also included organic compounds and methane, hinting that this distant moon's watery oceans may also contain alien methane-producing microbes. Whereas Titan and Europa were originally deemed the moons most suitable for life, Enceladus's status has now been boosted to second only to Mars, with conditions not dissimilar to those in the oceans of the early Earth.

Of course, unknown geochemical processes cannot be ruled out, but nonetheless the quality of the evidence is such as to invite further exploration of Enceladus. There have been at least seven potential mission designs proposed by various bodies, including NASA and ESA, to gain more information about the moon and its geysers. Several of these include landers, while others would fly through a plume in order to examine the vented material for biosignatures. However, to date none have received official funding confirmation. As it stands the first probe to arrive might be billionaire Yuri Milner's privately-funded Breakthrough Enceladus, rather than one from a major organisation. However, don't hold your breath: the earliest any of these missions is likely to reach Enceladus is at some point in the 2030s.

What happens if future probes find evidence of microbial life on both Mars and Enceladus? Or even, whenever a method is found to reach it, in the ice-covered oceans of Jupiter's moon Europa? The first key fact will be whether they are genetically independent of Earth biota or if the panspermia hypothesis - the delivery of microbes via cometary and meteorite impact - has been proven. If that turns out not to be the case and multiple instances of life arose separately within a single solar system, this has some profoundly mixed implications for the search for extraterrestrial intelligence (SETI). After all, if simple life can arise and be sustained on three or even four very different worlds - including bodies far outside their solar system's 'Goldilocks zone' - then shouldn't this also imply a much higher chance of complex alien life evolving on exoplanets? 

Yet despite various SETI programmes over the past few decades, we have failed to pick up any signs of extraterrestrial intelligence - or at least from other technological civilisations prepared to communicate with radio waves, either in our galactic neighbourhood or with super high-powered transmitters further away. This doesn't mean they don't exist: advanced civilisations might use laser pulses at frequencies our SETI projects currently don't have the ability to detect. But nonetheless, it is a little disheartening that we've so far drawn a blank. If there is microbial life on either Mars or Enceladus - or even more so, on both worlds, never mind Europa - then a continued lack of success for SETI suggests the chances of intelligent life evolving are far lower than the probability of life itself arising.

In effect, this means that life we can only view via a microscope - and therefore somewhat lacking in cognitive ability - may turn out to be common, but intelligence a much rarer commodity. While it might be easy to say that life on both Enceladus and Mars wouldn't stand much of a chance of gaining complexity thanks to the unpleasant environmental conditions that have no doubt existed for much of their history, it's clear that Earth's biota has evolved via a complex series of unique events. In other words, the tortuous pathways of history have influenced the evolution of life on Earth.

Whereas the discovery of so many exoplanets in the past decade might imply an optimistic result for the Drake equation, the following factors, being largely unpredictable, infrequent or unique occurrences, might suggest that the evolution of complex (and especially sapiens-level intelligent) life is highly improbable:

  • The Earth orbits inside the solar system's Goldilocks zone (bear in mind that some of the planets have moved from the region of space they were created in) and so water was able to exist in liquid form after the atmospheric pressure became high enough.
  • The size and composition of the planet is such that radioactivity keeps the core molten and so generates a magnetic field to block most solar and cosmic radiation.
  • It is hypothesised that the Earth was hit by another body, nicknamed Theia, that both tilted the planet's axis and caused the formation of the Moon rather than having a catastrophic effect such as tearing our world apart, knocking it on its side (like Uranus) or removing its outer crust (like Mercury).
  • The Moon is comparatively large and close to the Earth and as such their combined gravitational fields help to keep Earth in a very stable, only slightly eccentric orbit. This is turn has helped to maintain a relatively life-friendly environment over the aeons. 
  • The Earth's axial tilt causes seasons and as such generates a simultaneous variety of climates at different latitudes, providing impetus for natural selection.
  • The Great Unconformity and hypothesised near-global glaciation (AKA Snowball Earth) that might have caused it suggests this dramatic period of climate change led to the development of the earliest multi-cellular life around 580 million years ago.
  • Mass extinctions caused rapid changes in global biota without destroying all life. Without the Chicxulub impactor for example, it is unlikely mammals would have radiated due to the dominance of reptiles on the land.
  • Ice ages over the past few million years have caused rapid climate fluctuations that may have contributed to hominin evolution as East African forests gave way to grasslands.

The evolutionary biologist Stephen Jay Gould often discussed 'contingency', claiming that innumerable historical events had led to the evolution of Homo sapiens and therefore that if history could be re-run, most possible paths would not lead to a self-aware ape. Therefore, despite the 4,800 or so exoplanets discovered so far, some within their system's Goldilocks zone, what is the likelihood such a similar concatenation of improbable events would occur of any of them? 

Most people are understandably not interested in talking to microbes. For a start, they are unlikely to gain a meaningful reply. Yet paradoxically, the more worlds that microbial life is confirmed on, when combined with the distinct failure of our SETI research to date, the easier it is to be pessimistic; while life might be widespread in the universe, organisms large enough to view without a microscope, let alone communicate with across the vast reaches of interstellar space, may be exceedingly rare indeed. The origins of life might be a far easier occurrence than we used to think, but the evolution of technological species far less so. Having said that, we are lucky to live in this time: perhaps research projects in both fields will resolve this fundamental issue within the next half century. Now wouldn't that be amazing?

Sunday 23 June 2019

Spray and walk away? Why stratospheric aerosols could be saviours or destroyers

My first scientific encounters with aerosols weren't particularly good ones. In my early teens, I read that the CFC propellants used as aerosols were depleting the ozone layer. Therefore, tiny atmospheric particles had negative connotations for me from my formative years. This was further enforced by Carl Sagan and Richard Turco's 1990 book A Path Where No Man Thought: Nuclear Winter and the End of the Arms Race, which discussed the potentially devastating effects of high-altitude aerosol's around the world following a nuclear attack. Strike two against these pesky particles!

Of course aerosols aren't just man-made. The stratospheric dust particles generated following the Chicxulub impact event 66 million years ago are known to have been instrumental in the global climate disruption that wiped out the dinosaurs and many other life forms. This would have been in addition to the thousands of years of environmental changes caused by sulfur aerosols from the Deccan Traps supervolcano. Rather more recently, the Mount Tambora volcanic eruption in 1815 led to starvation and epidemics around the world for up to three years.

Now that our civilisation is generating a rapid increase in global temperatures, numerous solutions are being researched. One of the most recent areas involves reducing the amount of solar radiation reaching the Earth's surface. Several methods have been suggested for this, but this year sees a small-scale experiment to actually test a solution, namely seeding the atmosphere with highly reflective particles in an artificial recreation of a volcanic event. The Stratospheric Controlled Perturbation Experiment (SCoPEx) is a solar geoengineering project involving Harvard University that will use a balloon to release calcium carbonate in aerosol form at about twenty kilometres above the Earth's surface, analysing the local airspace the following day to assess the effects.

This experiment is controversial for several reasons. Firstly, it doesn't lead to any reduction in greenhouse gases and particulate pollutants; if anything, by sweeping the issue under a stratospheric rug, it could allow fossil fuel corporations to maintain production levels and reduce investment in alternatives. If the recent reports by meteorologists that natural and non-intentional man-made aerosols are already mitigating global warming, then the gross effects of heat pollution must be higher than realised!

Next, this sort of minute level of testing is unlikely to pinpoint issues that operational use might generate, given the chaotic nature of atmospheric weather patterns. To date, numerous computer simulations have been run, but bearing in mind how inaccurate weather forecasting is beyond ten days, nothing can be as accurate as the real thing. Therefore at what point could a test prove that the process is effective and safe enough to be carried out on a global scale? Possibly it might require such a large scale experiment that it is both research and the actual process itself!

The duration that the aerosols remain aloft is still not completely understood, hinting that regular replenishment would be essential. In addition, could the intentionally-polluted clouds capture greater amounts of water vapour, at first holding onto and then dropping their moisture so as to cause drought followed by deluge? Clouds cannot be contained within the boundaries of the testing nation, meaning other countries could suffer these unintended side-effects.

It may be that as a back-up plan, launching reflective aerosols into the stratosphere makes sense, but surely it makes much more sense to reduce greenhouse gas emissions and increase funding of non-polluting alternatives? The main emphasis from ecologists to date has been to remove human-generated substances from the environment, not add new ones in abundance. I'm all for thinking outside the box, but I worry that the only way to test this technique at a fully effective level involves such a large scale experiment as to be beyond the point of no return. Such chemical-based debacles as ozone depletion via chlorofluorocarbons (CFCs) prove that in just a matter of decades we can make profound changes to the atmosphere - and badly effect regions furthest removed from the source itself.  So why not encourage more reducing, reusing and recycling instead?

Sunday 24 February 2019

Core solidification and the Cambrian explosion: did one begat the other?

Let's face it, we all find it easier to live our lives with the help of patterns. Whether it's a daily routine or consultation of an astrology column (insert expletive of choice here) - or even us amateur astronomers guiding our telescopes via the constellations - our continued existence relies on patterns. After all, if we didn't innately recognise our mother's face or differentiate harmless creatures from the shape of a predator, we wouldn't last long. So it shouldn't be any surprise that scientists also rely on patterns to investigate the complexities of creation.

Richard Feynman once said that a scientific hypothesis starts with a guess, which should perhaps be taken with a pinch of salt. But nonetheless scientists like to use patterns when considering explanations for phenomena; at a first glance, this technique matches the principle of parsimony, or Occam's Razor, i.e. the simplest explanation is usually the correct one - excluding quantum mechanics, of course!

An example in which a potential pattern was widely publicised prior to confirmation via hard data was that of periodic mass extinction, the idea being that a single cause might be behind the five greatest extinction events. Four years after Luis Alvarez's team's suggestion that the 66 million year-old Chicxulub impactor could have caused the Cretaceous-Paleogene extinction, paleontologists David Raup and Jack Sepkoski published a 1984 paper hypothesising extinctions at regular intervals due to extraterrestrial impacts.

This necessitated the existance of an object that could cause a periodic gravitational perturbation, in order for asteroids and comets to be diverted into the inner solar system. The new hypothesis was that we live in binary star system, with a dwarf companion star in an highly elliptical, 26 million-year orbit. This would be responsible for the perturbation when it was at perihelion (i.e. closest approach to the sun).

What's interesting is that despite the lack of evidence, the hypothesis was widely publicised in popular science media, with the death-dealing star being appropriately named Nemesis after the Greek goddess of retribution. After all, the diversification of mammals was a direct result of the K-T extinction and so of no small importance to our species.

Unfortunately, further research has shown that mass extinctions don't fall into a neat 26 million-year cycle. In addition, orbiting and ground-based telescopes now have the ability to detect Nemesis and yet have failed to do so. It appears that the hypothesis has reached a dead end; our local corner of the universe probably just isn't as tidy as we would like it to be.

Now another hypothesis has appeared that might appear to belong in a similar category of neat pattern matching taking precedence over solid evidence. Bearing in mind the importance of the subject under scrutiny - the origin of complex life - are researchers jumping the gun in order to gain kudos if proven correct? A report on 565 million year-old minerals from Quebec, Canada, suggests that at that time the Earth's magnetic field was less than ten percent of what it is today. This is considerably lower than earlier estimate of forty percent. Also, the magnetic poles appear to have reversed far more frequently during this period than they have since.

As this is directly related to the composition of the Earth's core, it has led to speculation that the inner core was then in the final stage of solidification. This would have caused increased movement in the outer liquid, iron-rich core, and thus to the rapid generation of a much higher magnetic field. In turn, the larger the magnetic field dipole intensity, the lower the amount of high energy particles that reach the Earth's surface, both cosmic rays and from our own sun. What is particularly interesting about this time is that it is just (i.e. about twenty million years) prior to the so-called Cambrian explosion, following three billion years or so of only microbial life. So were these geophysical changes responsible for a paradigm shift in evolution? To confirm, we would need to confirm the accuracy of this apparently neat match.

It's well known that some forms of bacteria can survive in much higher radiation environments than us larger scale life forms; extremophiles such as Deinococcus radiodurans have even been found thriving inside nuclear reactors. Therefore it would seem obvious that more complex organisms couldn't evolve until the magnetic field was fairly high. But until circa 430 million years ago there was no life on land (there is now evidence that fungi may have been the first organisms to survive in this harsh environment). If all life was therefore in the sea, wouldn't the deep ocean have provided the necessary radiation protection for early plants and animals?

By 600 million years ago the atmospheric oxygen content was only about ten percent of today's value; clearly, those conditions would not have been much use to pretty much any air-breathing animals we know to have ever existed. In addition, the Ediacaran assemblage, albeit somewhat different from most subsequent higher animals, arose no later than this time - with chemical evidence suggesting their development stretched back a further 100 million years. Therefore the Canadian magnetic mineral evidence seems to be too late for the core solidification/higher magnetic field generation to have given the kick start to a more sophisticated biota.

In addition, we shouldn't forget that it is the ozone layer that acts as an ultraviolet shield; UVB is just as dangerous to many organisms, including near-surface marine life, as cosmic rays and high-energy solar particles. High-altitude ozone is thought to have reached current density by 600 million years ago, with blue-green algae as its primary source. O2 levels also increased at this time, perhaps driven by climate change at the end of a global glaciation.

Although the "Snowball Earth" hypothesis - that at least half of all ocean water was frozen solid during three or four periods of glaciation - is still controversial, there is something of a correlation in time between the geophysical evidence and the emergence of the Ediacaran fauna. As to the cause of this glacial period, it is thought to have been a concatenation of circumstances, with emergent plate tectonics as a primary factor.

How to conclude? Well, we would all like to find neat, obvious solutions, especially to key questions about our own origin. Unfortunately, the hypothesis based on the magnetic mineral evidence appears to selectively ignore the evolution of the Ediacaran life forms and the development of the ozone layer. The correlation between the end of "Snowball Earth" and the Ediacaran biota evolution is on slightly firmer ground, but the period is so long ago that even dating deposits cannot be accurate except to the nearest million years or so.

It's certainly a fascinating topic, so let's hope that one day the evidence will be solid enough for us to finally understand how and when life took on the complexity we take for granted. Meanwhile, I would take any speculation based on new evidence with a Feynman-esque pinch of salt; the universe frequently fails to match the nice, neat, parcels of explanations we would like it to. Isn't that one of the factors that makes science so interesting in the first place?