Curiosity rover detects never-before-seen organic compounds on Mars in new experiment

NASA’s Curiosity Mars rover uncovered a diverse mix of organic molecules on Mars, including chemicals widely considered building blocks for the origin of life on Earth.

The findings, which come from a chemical experiment performed for the first time on another world, reveal that the Martian surface can preserve the kinds of molecules that could serve as signs of ancient life. However, this experiment cannot distinguish between organic compounds from potential past life on Mars and those formed through geologic processes or delivered by meteorites.

Definitively identifying signs of past life would require returning rock samples to Earth.

The study was led by Amy Williams, Ph.D., a professor of geological sciences at the University of Florida and a scientist on the Curiosity and Perseverance Mars rover missions. Curiosity landed on Mars in 2012 to find evidence that ancient Mars had conditions that could support microbial life billions of years ago; the Perseverance rover, which landed in 2021, was sent to look for signs of any ancient life that might have formed.

“We think we’re looking at organic matter that’s been preserved on Mars for 3.5 billion years,” said Williams, who helped develop this chemical experiment. “It’s really useful to have evidence that ancient organic matter is preserved, because that is a way to assess the habitability of an environment. And if we want to search for evidence of life in the form of preserved organic carbon, this demonstrates it’s possible.”

Williams and an international collaboration of researchers published their findings April 21 in the journal Nature Communications.

Among the 20-plus chemicals identified by the experiment, Curiosity spotted a nitrogen-bearing molecule with a structure similar to DNA precursors — a chemical never before spotted on Mars. The rover also identified benzothiophene, a large, double-ringed, sulfurous chemical often delivered to planets by meteorites.

“The same stuff that rained down on Mars from meteorites is what rained down on Earth, and it probably provided the building blocks for life as we know it on our planet,” Williams said.

NASA’s Curiosity Mars rover took this selfie at a location nicknamed “Mary Anning” after a 19th century English paleontologist. This was the site of the chemical experiment uncovering diverse organic molecules on Mars, in the Glen Torridon region, which scientists believe was a site where ancient conditions would have been favorable to supporting life, if it ever was present.Credit:NASA/JPL-Caltech/MSSS

Led by NASA’s Jet Propulsion Laboratory, Curiosity Mars landed in Gale crater, in a former lake bed, in August 2012. The rover conducted the experiment in 2020 in the Glen Torridon region of the crater, an area rich in the clay minerals that indicate the area once contained water. Those clays can hold on to and preserve organic chemicals better than other minerals, making them a prime target for uncovering these compounds.

The experiment was conducted by the instrument suite known as the Sample Analysis at Mars, or SAM. Led in part by Jennifer Eigenbrode, Ph.D., an astrobiologist at NASA’s Goddard Space Flight Center and co-author of the new study, SAM has been responsible for many of the mission’s most important discoveries about organic chemistry, atmosphere and habitability on Mars.

Using a chemical known as TMAH, the experiment broke apart larger organic molecules so they could be analyzed by onboard instruments within SAM. With only two cups of the TMAH chemical onboard Curiosity, success required careful planning and choosing the most favorable location to sample.

The promising results come as future missions — including the Rosalind Franklin mission to Mars and the Dragonfly expedition to Saturn’s moon Titan — plan to bring the TMAH test onboard to search for organic compounds.

“We now know that there are big complex organics preserved in the shallow subsurface of Mars, and that holds a lot of promise for preserving large complex organics that might be diagnostic of life,” Williams said.

 

Also Read:

NASA’s Perseverance Rover Gets the Dirt on Mars

What’s Mars made of ? Japanese study throws light and opens up new study

 

How future volcanic eruptions will impact Earth’s ozone layer

The next major volcanic eruption could kick-start chemical reactions that would seriously damage the planet’s already besieged ozone layer.

The extent of damage to the ozone layer that results from a large, explosive eruption depends on complex atmospheric chemistry, including the levels of human-made emissions in the atmosphere. Using sophisticated chemical modeling, researchers from Harvard University and the University of Maryland explored what would happen to the ozone layer in response to large-scale volcanic eruptions over the remainder of this century and in several different greenhouse gas emission scenarios. The research was published recently in Geophysical Research Letters.

The Earth’s stratosphere is still recovering from the historic release of chlorofluorocarbons (CFCs) and other ozone-depleting chemicals. Even though CFCs were phased out by the Montreal Protocol 30 years ago, levels of chlorine-containing molecules in the atmosphere are still elevated. Explosive volcanic eruptions that inject large quantities of sulfur dioxide into the stratosphere facilitate the chemical conversion of chlorine into more reactive forms that destroy ozone.

Researchers have long known that when concentrations of chlorine from human-produced CFCs are high, ozone depletion will result following a volcanic eruption. When levels of chlorine from CFCs are low, volcanic eruptions can actually increase the thickness of the ozone layer. But exactly when this transition happens — from eruptions that deplete ozone to eruptions that increase ozone layer thickness — has long been uncertain. Previous research has put the window of the transition anywhere between 2015 to 2040.

The Harvard researchers found that volcanic eruptions could result in ozone depletion until 2070 or beyond, despite declining concentrations of human-made CFCs.

“Our model results show that the vulnerability of the ozone column to large volcanic eruptions will likely continue late in to the 21st century, significantly later than previous estimates,” said David Wilmouth, who directed the research and is a project scientist at the Harvard John A. Paulson School of Engineering and Applied Sciences and the Department of Chemistry and Chemical Biology.

So, why is this shift happening so much later than previously thought?

“Previous estimates did not take into account certain natural sources of halogen gases, such as very-short lived bromocarbons originating from marine plankton and microalgae,” said Eric Klobas, lead author and Harvard chemical physics PhD candidate.

Accounting for these emissions fine-tunes the timing of the shift from eruptions that cause ozone depletion to eruptions that increase the thickness of the ozone layer. These natural sources of bromine become especially important in the lower stratosphere after concentrations of human-emitted CFCs have declined.

“We found that the concentration of bromine from natural, very short-lived organic compounds is critically important,” said Klobas. “Even small, part-per-trillion changes in the amount of bromine from these sources can mean the difference between a late 21st century volcanic eruption resulting in ozone column depletion or ozone column enhancement.”

The researchers then explored how a volcanic event the size of the Mount Pinatubo eruption, which shot about 20 million metric tons of sulfur dioxide into the stratosphere in 1991, would impact the ozone layer in 2100. The team modeled four different greenhouse gas emission scenarios, ranging from very optimistic to what is commonly considered the worst-case scenario.

The team found that the most optimistic projection of future greenhouse gas concentrations resulted in the most ozone depletion from a volcanic eruption. Conversely, in the pessimistic scenario in which greenhouse gas emissions continue to increase rapidly throughout the 21st century, a Mount Pinatubo-size eruption would actually lead to a slight increase in ozone. The researchers found that the colder stratospheric temperatures and higher methane levels in this scenario would curb important ozone-depleting chemical reactions.

But, here’s the kicker: all of the above scenarios assumed that the volcanic eruption would only inject sulfur into the stratosphere, like the 1991 eruption of Mount Pinatubo in the Philippines. If the eruption were to also inject halogen-containing chemicals such as hydrogen chloride (HCl) into the stratosphere, the results could be dire.

“If volcanic halogens, which are commonly present in large quantities in volcanic eruptions, were to partition substantially into the stratosphere — in any greenhouse gas emission scenario, at any point in the future — it would potentially cause severe losses of stratospheric ozone,” said Klobas.

In such a case, the United States could see a prolonged and significant decrease in ozone layer thickness – upwards of 15 to 25 percent in the highest halogen scenario modeled. Even small reductions in the thickness of the ozone layer, which shields the surface of the Earth from DNA-destroying ultraviolet radiation, can adversely impact human health and other life on this planet.

“These eruptions are highly unusual events but the possibility does exist, as evidenced in the historical record,” said Wilmouth.