Skip to main content

Exoplanets with high-oxygen atmospheres are more likely than we thought

This is an artist’s impression of habitable Mars
This is an artist’s impression of habitable Mars Daein Ballard / CC BY-SA 3.0

We know that at different points in Earth’s history, it had very different oxygen levels. There seem to have been times at which oxygen levels increased dramatically, but scientists have long debated what caused these increases. Some researchers believe the increases must have been due to dramatic events like volcanic eruptions or the evolution of new forms of life like land plants.

But that would mean that the odds of a planet developing an oxygen-rich atmosphere are low, and we just so happened to get lucky that these events happened on Earth. It means we’d be pretty unlikely to find exoplanets that also have high levels of oxygen.

Recommended Videos

New research challenges that concept though, by showing that high levels of oxygen aren’t that unlikely. The key ingredient that has been missing from these prior models is phosphorus, according to the authors.

Please enable Javascript to view this content

“We created a computer model of the Earth’s carbon, oxygen, and phosphorus cycles and found that the oxygen transitions can be explained by the inherent dynamics of our planet and likely didn’t require any miraculous events,” the authors explained in a statement.

Phosphorus in the ocean plays a key role in the amount of oxygen on our planet. It enables photosynthesis among tiny marine plants called phytoplankton, which produces oxygen, but high levels of phosphorus can also increase the amount of oxygen consumed in the deep ocean as dead microorganisms are decomposed. This means that oxygen levels could rise or fall rapidly throughout Earth’s history because of the interaction with marine phosphorus.

This tells us not only more about the formation of oxygen on our planet, but also gives us clues to how oxygen could form on other planets. It isn’t necessary, as some had thought, for a dramatic or unusual planetary event to occur to create a change in oxygen levels. Instead, high levels of oxygen like those found on Earth could occur on exoplanets too. This makes the odds of us locating an exoplanet with a high-oxygen atmosphere much higher.

“What is really exciting about all of this is that the oxygenation pattern can be created without the need for difficult and complex evolutionary leaps forward, or circumstantial catastrophic volcanic or tectonic events,” the authors concluded. “So it appears that Earth’s oxygenation may have been inescapable once photosynthesis had evolved — and the chances of high oxygen worlds existing elsewhere could be much higher.”

The research is published in the journal Science.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
Changes in Mars’ atmosphere are driven by enormous CO2 ice cap at its pole
The Martian pole

We're just starting to learn about how complex the atmosphere of Mars is. We know that it is primarily composed of carbon dioxide, but there are also smaller amounts of oxygen and methane there whose levels fluctuate over time. And all the way back in 1966, scientists theorized that the planet's stable cap of carbon dioxide at its pole could have planet-wide effects on the atmosphere.

Now, a new study has looked at the carbon dioxide ice deposit on Mars' south pole and found that it does indeed appear to affect global atmospheric pressure. This is due to several factors: The fact that Mars' atmosphere is very thin, with a surface pressure of 0.6% that of Earth, and the fact Mars wobbles on its axis by up to 10 degrees as it orbits the sun, so at some times its poles are exposed to more sunlight than at other times.

Read more
NASA’S NESSI instrument can pick out the atmospheres of distant exoplanets
The Palomar Hale Telescope Dome With Star Trails

NASA has a new tool to help in the hunt for exoplanets. The New Mexico Exoplanet Spectroscopic Survey Instrument, or NESSI, is an instrument on the Hale Telescope in San Diego which has been in testing since February 2018. Now, it's ready to start investigating the atmospheres of planets outside our solar system.

"NESSI is a powerful tool to help us meet the family," Mark Swain, an astrophysicist and the JPL lead for NESSI, said in a statement. "Twenty-five years ago, to our best knowledge, we thought we were alone. Now we know that -- at least in terms of planets -- we're not, and that this family is extensive and very diverse."

Read more
Mars’ water is evaporating away even faster than we expected
mars proton auroras water loss landscape dry wet 0 1

This artist’s concept depicts the early Martian environment (right) – believed to contain liquid water and a thicker atmosphere – versus the cold, dry environment seen at Mars today (left). NASA’s Goddard Space Flight Center

Billions of years ago, Mars could have been a planet very like Earth with copious liquid water on its surface. But over time, that water rose into Mars's thin atmosphere and evaporated off into space. There are only very small amounts of water vapor left in the atmosphere today, and a new study shows that vapor is being lost even faster than previously believed.

Read more