Oxygen & Wildfires: Clues to Early Life

How big can an insect get? One night a few years back, I opened the door onto our patio to let the dogs out and an enormous flying, buzzing thing came through the door. When I say ‘enormous,’ I simply mean it was big enough to startle both dogs enough that they ran upstairs, causing me to grab for a flyswatter as it flitted and hummed around the room. I lost sight of it and suddenly all was silent. Our cat had sprung, and the bug was quickly dispatched. We dubbed it ‘Mothra’ and added it to our dog lore. After all, where were our Border Collie and Sheltie when we needed them? Peering down at us from the upstairs landing, while the cat did the dirty work.

‘Mothra’ was probably no more than an inch long — he was noisier than he was big. But there was a time when ‘enormous’ really meant something. Meganeura is a genus of insects dating to the Carboniferous period when creatures related to our own familiar dragonfly boasted wingspans of two feet or more. Meganeura monyi is considered one of the largest flying insects ever, a creature that fed not only on other insects but also on small amphibians, and could probably have made off with a present-era cat. Sufficient reason to keep the screen door closed.

Image: An artist’s conception of Meganeura monyi. Good luck if one of these gets into your living room. Credit: Surface Vision.

Some people believe that gigantism in some animal groups was the result of higher levels of oxygen in the atmosphere, the consequence of the colonization of land by plants. And some would argue that higher amounts of oxygen allowed vertebrates to colonize land surfaces. Today we’ve got an oxygen level of 21 percent, but we know the levels have varied greatly in the past 400 million years and have declined steadily since the middle of the Cretaceous.

Studying this has been tricky because we use geochemical models to estimate the level of atmospheric oxygen, and various models produce differing results. But new work just published in Nature Geoscience now shows that the amount of charcoal preserved in ancient peat bogs provides a measure of how much oxygen was available in the past and may be the best way to measure the phenomenon. The variation is striking. Charcoal found in coal has remained at concentrations between 4-8 percent over the past 50 million years, indicating oxygen levels similar to today. But some earlier periods show a charcoal percentage as high as 70 percent.

That latter figure implies, according to Andrew Scott (Royal Holloway University of London) that high levels of atmospheric oxygen would have been available to spread frequent, large fires in both the Carboniferous and Permian periods, from 320-250 million years ago, and the Middle Cretaceous, approximately 100 million years ago. Says Scott: “It is interesting that these were times of major change in the evolution of vegetation on land with the evolution and spread of new plant groups, the conifers in the late Carboniferous and flowering plants in the Cretaceous.”

We may be dealing with a self-perpetuating mechanism: Frequent, hot fires resulting from high levels of atmospheric oxygen could have caused more erosion and thus greater burial of organic carbon, which creates a cycle keeping oxygen levels high. The burial of carbon was particularly high during the late Paleozoic, which is marked by the accumulation of huge coal deposits. Ian Glasspool (Field Museum, Chicago) notes the relationship between oxygen and flammability:

“Atmospheric oxygen concentration is strongly related to flammability. At levels below 15% wildfires could not have spread. However, at levels significantly above 25% even wet plants could have burned, while at levels around 30 to 35%, as have been proposed for the Late Paleozoic, wildfires would have been frequent and catastrophic”.

The mystery then becomes why oxygen levels stabilized in the last 50 million years. We have much to learn about the mechanisms promoting and regulating life on our own planet. How useful it will ultimately be to be able to compare what we find on other planets with our own history. The discovery of biomarkers in the atmosphere of an extraterrestrial world would be met with celebration, but it will also remind us how little we know about how those biomarkers change over time and the effect those changes have on indigenous life.

The paper is Glasspool & Scott, “Phanerozoic concentrations of atmospheric oxygen reconstructed from sedimentary charcoal,” Nature Geoscience, published online 1 August, 2010 (abstract).

tzf_img_post

Imaging Giants and Dwarfs

Was it really three years ago that New Horizons moved past Jupiter, returning images of its stunning systems of storms and cloud? The mission continues to go well, and the photo below, taken by the spacecraft’s Long Range Reconnaissance Imager (LORRI) paints an unusual portrait of Jupiter and two of its largest moons from a distance of more than 16 AU, looking back toward the inner system. Note how faint the moons are, the consequence of the fast shutter speed used, with an exposure time of 0.009 seconds. I like what mission principal investigator Alan Stern says:

“This haunting image of Jupiter – far in the distance back in the Sun’s warmer clines from whence New Horizons came – reminds us of Voyager’s family postcard of the planets taken from beyond Neptune’s orbit about 20 years ago. Perhaps after we flyby Pluto in 2015, we’ll try something similar from our perch aboard New Horizons.”

Image: The New Horizons team looked back at Jupiter during Annual Checkout (ACO) 4 to test the Long Range Reconnaissance Imager (LORRI)’s ability to image targets close, in angle, to the Sun. This image was taken on June 24, when New Horizons was 16.3 astronomical units (about 1.5 billion miles) from Jupiter, at a spacecraft-Sun-planet angle of only 17 degrees. Looking like Earth’s moon at a quarter phase, Jupiter is clearly resolved, with an apparent diameter of nearly 12 LORRI pixels. LORRI also picks up the moons Ganymede and Europa, even though the exposure time was only nine milliseconds and these Galilean satellites are extremely faint in comparison to Jupiter. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute.

Meanwhile, looking at gas giants from any angle reminds me of the progressive escalation from planet to brown dwarf to star, especially in light of the new find — a 36 Jupiter-mass companion — around the star PZ Tel A. The object is a brown dwarf separated by about 18 AU from the star, a distance similar to that between the Sun and Uranus. That’s a tight separation given that the brown dwarf was discovered through direct imaging, where orbital separations greater than 50 AU are the more likely outcome.

PZ Tel B is evidently on a highly eccentric orbit — Beth Biller (University of Hawaii), lead author on the paper on this work, says ‘in the last ten years, we have literally watched it careen through its inner solar system’ — and images as recent as seven years ago show it obscured by the glare of its primary, an indication it is moving outward quickly from the star. Its orbital motion has implications for the kinds of planets that can form in such a system.

Image: PZ Tel A and B. The vast majority of light from PZ Tel A has been removed from this image using specialized image analysis techniques. The size of the orbit of Neptune is shown for comparison; PZ Tel B would lie within Neptune’s orbital dimensions and is one of the few brown dwarfs or exoplanets imaged at a distance of < 30 AU from its parent star. Credit: Beth Biller and the Gemini NICI Planet-Finding Campaign, Gemini Observatory/AURA. PZ Tel A is a young, Sun-like star about twelve million years old, still surrounded by significant amounts of circumstellar dust. Sifting a brown dwarf out of its glare is remarkable work, using adaptive optics coupled to the Near-Infrared Coronagraphic Imager (NICI), which can detect companions a million times fainter than the host star at 1 arcsecond separations. The science fiction writers among us can now go to work imagining what a similar brown dwarf would be like in our own system, and how it might affect a nearby civilization's thoughts on expanding into space. More can be found in the paper, which is Biller et al., "The Gemini NICI Planet-Finding Campaign: Discovery of a Close Substellar Companion to the Young Debris Disk Star PZ Tel," slated for publication in Astrophysical Journal Letters and available as a preprint.

tzf_img_post