Skeptophilia (skep-to-fil-i-a) (n.) - the love of logical thought, skepticism, and thinking critically. Being an exploration of the applications of skeptical thinking to the world at large, with periodic excursions into linguistics, music, politics, cryptozoology, and why people keep seeing the face of Jesus on grilled cheese sandwiches.
Showing posts with label End Devonian Extinction. Show all posts
Showing posts with label End Devonian Extinction. Show all posts

Tuesday, November 15, 2022

Roots of the problem

It's natural enough to think that humans are the only organisms that damage their own habitat.  We certainly seem to be doing a damn good job of it.  But there have been other times living things have sown the seeds of their own destruction.

One good example is the Great Oxidation Event -- sometimes, justifiably, nicknamed the "Oxygen Holocaust."  It occurred just over two billion years ago, and hinges on one rather surprising fact; oxygen is a highly reactive, toxic gas.

There's good evidence that aerobic respiration -- the set of biochemical reactions that allows us to burn the glucose in our food, and which provides us with the vast majority of the energy we use -- evolved first as a mechanism for detoxifying oxygen, and only afterward got co-opted into being an energy pathway.  The problem was that prior to the Great Oxidation Event, all of the organisms had been anaerobes, which are capable of releasing energy without oxygen.  To the vast majority of anaerobes, oxygen is a deadly poison.  That's why when there was a sudden, massive injection of oxygen into the Earth's atmosphere a couple of billions of years ago, the result was that just about every living thing on Earth died.

The tipping point came with the evolution of yet another energetic pathway: photosynthesis.  Photosynthesis was a tremendous innovation, as it allowed organisms to harness light energy instead of chemical energy, but it had one significant downside.  The first part of the reaction chain of photosynthesis breaks up water molecules and releases oxygen.  So when the first photosynthesizers evolved -- probably something like modern cyanobacteria -- oxygen gas began to pour into the oceans and atmosphere.

Something like 99% of life on Earth died.

The survivors fell into three groups: (1) the handful of organisms that had some early form of aerobic respiration as a detoxification pathway; (2) anaerobes that had a way of hiding from the oxygen, like today's methanogens that live in anaerobic mud; and (3) the photosynthesizers themselves.

From the organisms that survived that catastrophic bottleneck came every living thing we currently see around us.

So we're far from being the only organisms that cause ecological problems.  The reason the topic comes up, in fact, is because of another example I'd never heard of until I bumped into a paper in the Geological Society of North America Bulletin last week; the Devonian mass extinctions, which are one of the "Big Five" extinction events that have struck the Earth.  This particular series of cataclysms wiped out an estimated seventy percent of marine species, but it may have been triggered by the evolution of something that seems innocuous, even benevolent.

Tree roots.

Plants had only colonized the land during the previous period, the Silurian, enabled to do so by yet another innovation; the evolution of vascular tissue.  The internal plumbing vascular plants have (the xylem and phloem you probably remember from your biology classes) allow plants to move water farther and faster, so they were no longer so tied to living in ponds and lakes.  Plus, vascular tissue in many plants doubles as support tissue, so this facilitated growing taller (a significant advantage when you're competing with your near neighbors for light).

But if you're taller, you're also more likely to topple when it's windy.  So then there's selection for who's got the best support system.  The winners: plants with roots.

Devonian Forest by Eduard Riou (ca. 1872) [Image is in the Public Domain]

Like vascular tissue, roots are multi-purpose.  They not only provide support and anchoring, they're good at creating lots of absorptive surface area for water and nutrients.  (Some roots are also evolved to store starch -- carrots come to mind -- but that's an innovation that seems to have come much later.)  So now we have a competition between plants for who's got the best supports, and who can access nutrients from the soils the fastest.

Roots very quickly became good at twisting their way into rocks.  You've undoubtedly seen it; tree roots clinging to, and breaking up, rocks, asphalt, cement, pretty much any barrier they can get a foothold into.  When that happened, suddenly there's an erosive force breaking up bedrock and transporting nutrients (especially phosphorus) into plant tissue.  Phosphorus began to leach out of the rock into the soil, and when the plants died all the phosphorus in the tissue was released into rivers, streams, and lakes.

The result was a massive influx of nutrients into bodies of water.

Have you ever seen what happens when chemical fertilizers get into a pond?  It fosters algal blooms, and when the algae dies and decomposes, the oxygen levels plummet and the entire pond dies.

That's what happened during the late Devonian Period -- but planet-wide.

The huge reef-building rugose and tabulate corals and stromatoporid sponges were wiped out en masse.  Other groups, such as trilobites and brachiopods, which depended on the reefs for habitat and food, got knocked back hard as well.

All, the authors claim, because of a nifty innovation in the structure of land plants.

It's tempting to think that the environment is stable; we look around us and think things have always been this way, and will always be this way.  What more of us need to understand is that while the global ecosystem is resilient up to a point, there is always a tipping point.  The scary part is we can pass that point suddenly, without even realizing it.  Then before we're even aware of what's happened, the last chance to turn things around is gone.

The difference between what happened during the Great Oxidation Event and the Devonian Mass Extinctions, and what's happening now, is that back then there was no conscious awareness on the part of the organisms who created the problem and those that were affected.  Now, we have (or should have) the awareness to see what is happening, and enough knowledge to make some smart decisions and halt the self-destructive path we're on.

Let's hope that it's not too late.

****************************************


Friday, August 21, 2020

Deadly fireworks

I've always thought it would be amazingly cool to witness a supernova.

Imagine it.  Within a few hours, a dim, ordinary-looking star increases in luminosity until it outshines every other astronomical object in the sky except the Sun and Moon.  It's visible during the day and you can read by its light at night.  It's not a blink-and-you'll-miss-it phenomenon, either; the light from the massive explosion peaks rapidly but declines slowly.  Most supernovae will be visible for months, before dimming to near-invisibility, ending as neutron stars or black holes.

There are lots of candidates for what could be the next supernova, although don't get your hopes up; most of these fall into the "some time in the next million years" category.  Yeah, it could happen tomorrow, but I wouldn't put money on it.  Still, the list is sizable, and here are five of the best possibilities:
  • Betelgeuse (720 light years away, in the constellation Orion).  This one got some serious press a few months ago because it suddenly started to decrease in brightness, and astronomers wondered if this was a prelude to an explosion.  What appears to have happened is that there was turbulence in the star's core that blew a cloud of dust from its surface, obscuring the star and making it appear to dim.  So we're still waiting for this red supergiant to explode, and probably will be for a while.
  • IK Pegasi (154 light years away, in the constellation Pegasus).  IK Pegasi isn't well known because at an apparent magnitude of 6, it's not visible to the naked eye, but it bears mention as the nearest serious supernova candidate.  It's a double star -- a main-sequence star and a massive white dwarf orbiting a common center of mass.  As the main-sequence star evolves, it will become a red giant, with a radius large enough that its white dwarf companion will start suctioning matter from its surface.  When the white dwarf reaches what's called the Chandrasekhar Limit -- 1.4 solar masses -- it will explode cataclysmically as a Type 1a supernova.  This will not only be spectacular but potentially dangerous -- a topic we will revisit shortly.
  • VY Canis Majoris (3,820 light years away, in the constellation Canis Major).  Another star not visible to the naked eye, VY Canis Majoris is a lot more spectacular than you'd think to look at it.  It's the largest star known, with a mass fifteen times that of the Sun, and a radius so large that if you put it where the Sun is, its surface would be about at the orbit of Jupiter (so we'd be inside the star).  This "hypergiant" is one of the most luminous stars in the Milky Way, and is only dim because it's so far away.  This one is certain to go supernova, probably some time in the next 100,000 years, and the remnants will collapse into a black hole.
  • Eta Carinae (7,500 light years away, in the constellation Carina).  Eta Carinae is another huge star, with a radius twenty times that of the Sun, but what makes this one stand out is its bizarre behavior.  In 1837 it suddenly brightened to being one of the five brightest stars in the night sky, then over the next sixty years faded to the point that it was only visible in binoculars.  Detailed observations have shown that it blew out a huge cloud of material in "The Great Eruption," which is now the Homunculus Nebula.  It's a unique object, which makes it hard to predict its future behavior.  What seems certain is that it'll eventually explode, but there's no telling when that might occur.
The consensus amongst astronomers, however, is that the next likely supernova probably isn't on the list -- that it will be a previously-unknown white dwarf or an unremarkable-looking red giant.  We know so little about supernovas that it's impossible to predict them with any kind of accuracy.  And while this is an exciting prospect, we'd better hope that the next supernova isn't too close.

The Homunculus Nebula with Eta Carinae at the center [Image licensed under the Creative Commons ESA/Hubble, Cosmic Fireworks in Ultraviolet Eta Carinae Nebula, CC BY 4.0]

Not only do supernovas produce a lot of light, they generate a tremendous amount of radiation of other kinds, including cosmic rays.  A close supernova could produce enough cosmic rays to wipe out the ozone layer -- leading to a huge influx of ultraviolet light from the Sun, with devastating effects.

Scarily, this may have already happened in Earth's history.  One of the lesser-known mass extinctions occurred at the end of the Devonian Period, 359 million years ago.  Because it is poorly understood, and was dwarfed by the cataclysmic Permian-Triassic Extinction a little over a hundred million years later, it's not one you tend to read about in the paleontology-for-the-layperson books.  Even so, it was pretty significant, wiping out 19% of known families and 50% of known genera, including placoderms (armored fish), cystoids (a relative of the starfish), and graptolites (colonial animals not closely related to any living species).  Most striking were the collapse of reef-forming corals -- reefs didn't begin to form again on any significant scale until the Mesozoic Era, almost two hundred million years later -- and the near-complete wipeout of vertebrates.  The latter left no vertebrate species over a meter long (most of them were under ten centimeters), and again, it was millions of years before any kind of recovery took place.

Fortunately for us, it eventually did, because we're talking about our ancestors, here.

The cause of this catastrophe has been a matter of speculation, but a team led by Brian Fields, astrophysicist at the University of Illinois, may have found a smoking gun.  In a paper this week in Proceedings of the National Academy of Sciences, we find out that the most likely cause for the End-Devonian Extinction is a nearby supernova that caused the collapse of the ozone layer, leading to the Earth's surface being scorched by ultraviolet light.  This triggered a massive die-off of plants -- which had only recently colonized the land -- and worldwide anoxia.  

The result?  A mass extinction that hit just about every taxon known.

The idea that a supernova might have been to blame for the End-Devonian Extinction came from the presence of hundreds of thousands of plant spores in sedimentary rock layers that showed evidence of what appeared to be radiation damage.  This isn't conclusive, of course; the Fields et al. team is up front that this is only a working hypothesis.  What they'll be looking for next is isotopes of elements in those same rock layers that are only produced by bombardment with radiation, such as plutonium-244 and samarium-146.  "When you see green bananas in Illinois, you know they are fresh, and you know they did not grow here," Fields said, in an interview in Science Daily.  "Like bananas, Pu-244 and Sm-146 decay over time.  So if we find these radioisotopes on Earth today, we know they are fresh and not from here -- the green bananas of the isotope world -- and thus the smoking guns of a nearby supernova."

So as much as I'd love to witness a supernova in my lifetime, it'd be nice if it was one well outside of the terrifyingly-named "kill zone" (thought to be about 25 light years or so).  And chances are, there's nothing inside that radius we need to worry about.  If any of the known supernova candidates explode, we'll almost certainly be able to enjoy the fireworks from a safe distance.

***************************

Fan of true crime stories?  This week's Skeptophilia book recommendation of the week is for you.

In The Poisoner's Handbook:Murder and the Birth of Forensic Medicine in Jazz Age New York, by Deborah Blum, you'll find out about how forensic science got off the ground -- through the efforts of two scientists, Charles Norris and Alexander Gettler, who took on the corruption-ridden law enforcement offices of Tammany Hall in order to stop people from literally getting away with murder.

In a book that reads more like a crime thriller than it does history, Blum takes us along with Norris and Gettler as they turned crime detection into a true science, resulting in hundreds of people being brought to justice for what would otherwise have been unsolved murders.  In Blum's hands, it's a fast, brilliant read -- if you're a fan of CSI, Forensics Files, and Bones, get a copy of The Poisoner's Handbook, you won't be able to put it down.

[Note: if you purchase this book using the image/link below, part of the proceeds goes to support Skeptophilia!]