Early Earth haze likely provided ultraviolet shield for planet

June 3, 2010
A new study by CU-Boulder researchers indicates a thick organic haze shrouding Earth several billion years ago was similar to the one now hovering over Saturn’s largest moon, Titan (above) and may have protected primordial life on the planet from damaging ultraviolet radiation. Credit: Image courtesy NASA/JPL/Space Science Institute.

A new study shows a thick organic haze that enshrouded early Earth several billion years ago may have been similar to the haze now hovering above Saturn's largest moon, Titan, and would have protected primordial life on the planet from the damaging effects of ultraviolet radiation.

The University of Colorado at Boulder scientists believe the haze was made up primarily of methane and nitrogen chemical byproducts created by reactions with light, said CU-Boulder doctoral student Eric Wolf, lead study author. Not only would the haze have shielded early Earth from UV light, it would have allowed gases like ammonia to build up, causing greenhouse warming and perhaps helped to prevent the planet from freezing over.

The researchers determined the haze of hydrocarbon aerosols was probably made up of fluffy, shaped somewhat like cottonwood tree seeds that would have blocked UV but allowed visible light through to Earth's surface, Wolf said.

Prior to the new study, the prevailing scientific view was that the atmosphere of Earth some 3 billion years ago was primarily made up of with lesser amounts of carbon dioxide, methane, hydrogen and water vapor, said Wolf. "Since show early Earth could not have been warmed by alone because of its low levels, other greenhouse gases must have been involved. We think the most logical explanation is methane, which may have been pumped into the atmosphere by early life that was metabolizing it."

A paper on the subject by Wolf and CU-Boulder Professor Brian Toon of the atmospheric and oceanic sciences department is being published in the June 4 issue of Science. NASA's Planetary Atmosphere Program funded the study.

The output of the sun during the Archean period some 3.8 billion to 2.5 billion years ago is thought to have been 20 percent to 30 percent fainter than today, said Wolf. But previous work by other scientists produced geological and biological evidence that indicates Earth's surface temperatures were as warm or warmer than today.

As part of the early Earth study, Wolf and Toon used a climate model from the National Center for Atmospheric Research and concepts from lab studies by another CU group led by chemistry and biochemistry Professor Margaret Tolbert that help explain the odd haze of Titan, the second largest moon in the solar system and the largest moon of Saturn. Titan came under intense study following the arrival of the Cassini spacecraft at Saturn in 2004, allowing scientists to determine it was the only moon in the solar system with both a dense atmosphere and liquid on its surface.

Previous modeling efforts of early Earth haze by other scientists assumed that aerosol particulates making up the haze were spherical, said Wolf. But the spherical shape does not adequately account for the optical properties of the haze that blanketed the planet.

Lab simulations helped researchers conclude that the Earth haze likely was made up of irregular "chains" of aggregate particles with greater geometrical sizes than spheres, similar to the shape of aerosols believed to populate Titan's thick atmosphere. Wolf said the aggregate aerosol particulates are believed to be fragmented geometric shapes known as fractals that can be split into parts.

During the Archean period there was no ozone layer in Earth's atmosphere to protect life on the planet, said Wolf. "The UV shielding methane haze over early Earth we are suggesting not only would have protected Earth's surface, it would have protected the atmospheric gases below it -- including the powerful , ammonia -- that would have played a significant role in keeping the early Earth warm."

CU-Boulder researchers estimated there were roughly 100 million tons of haze produced annually in the atmosphere of early Earth during the Archean. "If this was the case, an early Earth atmosphere literally would have been dripping organic material into the oceans, providing manna from heaven for the earliest life to sustain itself," Toon said.

"Methane is the key to make this climate model run, so one of our goals now is to pin down where and how it originated," said Toon. If Earth's earliest organisms didn't produce the methane, it may have been generated by the release of gasses during volcanic eruptions either before or after life first arose -- a hypothesis that will requires further study, he said.

The new CU-Boulder study will likely re-ignite interest in a controversial experiment by scientists Stanley Miller and Harold Urey in the 1950s in which methane, ammonia, nitrogen and water were combined in a test tube. After Miller and Urey ran an electrical current through the mixture to simulate the effects of lightning or powerful UV radiation, the result was the creation of a small pool of amino acids -- the building blocks of life.

Toon said the theory of early Earth being shrouded by a gaseous blanket containing methane and ammonia first arose in the 1960s and was subsequently discarded by scientists. In the 1970s and 1980s some scientists suggested the early Earth atmosphere was similar to those on Mars and Venus with lots of carbon dioxide, another theory that eventually went by the wayside. Since CO2-rich atmospheres do not produce organic molecules easily, scientists began looking in deep-sea volcanic vents and at wayward asteroids to explain early Earth life.

A 1997 paper by the late Carl Sagan of Cornell University and Christopher Chyba, then at the University of Arizona, proposed that an organic aerosol shield in early Earth's atmosphere would have protected the ammonia wafting beneath it, allowing heating to occur at Earth's surface. But the authors proposed the haze particles were spherical rather than irregular aggregate particles Wolf and Toon suggest and did not consider methane to be the driver of the system, eventually sinking that theory.

"We still have a lot of research to do in order to refine our new view of early Earth," said Wolf. "But we think this paper solves a number of problems associated with the haze that existed over early Earth and likely played a role in triggering or at least supporting the earliest life on the planet."

From space, probably looked much like Titan looks today, said Toon. "It would have been shrouded by a reddish haze that would have been difficult to see through, and the ocean probably was a greenish color caused by dissolved iron in the oceans. It wasn't a blue planet by any means."

Explore further: A Hazy View of Early Earth

Related Stories

A Hazy View of Early Earth

October 12, 2009

Haze in the early Earth atmosphere could have played a crucial role in the origin of life. By forming a protective shield, the haze would have safeguarded organic substances from harmful ultraviolet (UV) radiation.

Titan gives clues to Earth's early history

December 1, 2005

Readings from the Huygens probe of the surface and atmosphere around Saturn's largest moon, Titan, give researchers a peek back through time to when and how Earth's atmosphere formed, and how our primitive planet looked before ...

Titan's Purple Haze Points to a Fuzzy Past

August 2, 2004

Encircled in purple stratospheric haze, Saturn's largest moon, Titan, appears as a softly glowing sphere in this colorized image taken on July 3, 2004, one day after Cassini's first flyby of that moon. Titan has a dense atmosphere ...

Studying Titan's Lakes on Earth

January 28, 2010

A new project aims to replicate the surface on the moon Titan in order to learn more about its hydrocarbon lakes. This study could also tell us about the chemistry that led to the origin of life on early Earth.

Invisible gases form most organic haze in urban, rural areas

July 9, 2007

A new study involving the University of Colorado at Boulder shows that invisible, reactive gases hovering over Earth's surface, not direct emissions of particulates, form the bulk of organic haze in both urban and rural areas ...

Recommended for you

Mysterious deep-Earth seismic signature explained

November 22, 2017

New research on oxygen and iron chemistry under the extreme conditions found deep inside the Earth could explain a longstanding seismic mystery called ultralow velocity zones. Published in Nature, the findings could have ...

Scientists dispute missing dryland forests

November 21, 2017

Scientists are disputing the possibility that a significant portion of the world's forests have been missed in an earlier accounting of ecological diversity.


Adjust slider to filter visible comments by rank

Display comments: newest first

5 / 5 (1) Jun 03, 2010
This theory may better fit Miller & Urey's experiments, but it still leaves questions unanswered.

How did the earth's atmosphere transition from a heavy concentration of ammonia, nitrogen, methane and water vapor to primarily nitrogen, oxygen, and water vapor?

Also, what prevented the water vapor from undergoing oxygenic photosynthesis and therefore generating free oxygen.
2 / 5 (1) Jun 03, 2010
This theory may better fit Miller & Urey's experiments, but it still leaves questions unanswered.

How did the earth's atmosphere transition from a heavy concentration of ammonia, nitrogen, methane and water vapor to primarily nitrogen, oxygen, and water vapor?

Also, what prevented the water vapor from undergoing oxygenic photosynthesis and therefore generating free oxygen.

Just speculation on my part, but the increase in solar activity amy have played a part, along with ongoing geochemical changes and variable vulcanism.

As for the generation of free oxygen- most likely would have immediately been consumed by iron reduction in exposed formations and dissolved in seawater. Think banded iron- albeit smaller-scale.
3 / 5 (2) Jun 04, 2010
Primordial life most likely formed beneath the ocean, at hydrothermal vents. Also, oceans formed very early in earth formation. The atmospheric composition is almost irrelevant to the earliest bacteria.
5 / 5 (1) Jun 04, 2010
How did the earth's atmosphere transition from a heavy concentration of ammonia, nitrogen, methane and water vapor to primarily nitrogen, oxygen, and water vapor?
Oxygen is entirely produced by photosynthetic life. If it weren't for life, there'd be no oxygen in the atmosphere. If all life died out tomorrow, all oxygen will have vanished from the atmosphere a couple of centuries later. Free oxygen is so unnatural, that finding it in the atmosphere of any other planet would be a surefire detection of life.

Once oxygen shows up in the atmosphere, it's the end of methane. That would mean the end of haze (which is purportedly methane-derived.) Which would mean the end of ammonia, due to ultraviolet irradiation. Eventually, enough oxygen builds up to supply the ozone layer and block UV; I guess by that time all the ammonia will have vanished from the atmosphere.

Please sign in to add a comment. Registration is free, and takes less than a minute. Read more

Click here to reset your password.
Sign in to get notified via email when new comments are made.