Curiosity finds largest-ever organic molecules on Mars
The Mars Curiosity rover's onboard mini-lab has helped confirm the existence of the largest organic molecules ever found on the Red Planet. The trio of long-chain compounds preserved in Martian soil are believed to be the remnants of prebiotic components required for life to develop on Earth. Researchers published evidence on March 24 in the Proceedings of the National Academy of Sciences, which builds on their work that began over a decade ago.
In May 2013, Curiosity started drilling into an area known as 'Yellowknife Bay' in the Gale Crater. Scientists were interested in examining the region not for what it is today, but for what it may have been millions of years ago. Yellowknife Bay wasn't a randomly chosen name—the arid and desolate landscape's features still hint at a large, long-evaporated lakebed.
Curiosity's soil survey, nicknamed 'Cumberland,' has been analyzed multiple times inside its Sample Analysis on Mars (SAM) onboard mini-lab and has yielded a trove of new information about the planet's past. In particular, it is rich in clay minerals that often form in water, and contains sufficient amounts of sulfur to help preserve organic molecules. Cumberland also features nitrates crucial to healthy animal and plant life, as well as methane containing a specific type of carbon associated with biological processes.
Most striking, though, was conclusive confirmation that Yellowknife Bay once hosted an ancient lake, further supporting the theory that Mars was once home to life of some kind.
Experts have since spent years examining data gleaned from SAM mini-lab analyses. In one recent experiment, a team including Glavin and Caroline Freissinet, an astrobiologist at the French National Center for Scientific Research worked to locate evidence of amino acids inside the Cumberland sample. While they didn't find them that time, something else caught their eye: trace amounts of three carbon-chain molecules known as a decane, undecane, and dodecane. With 10, 11, and 12 carbons respectively, researchers believe these organic compounds may be residual fragments of fatty acids needed for cell membrane formation and other biological functions.
These fatty acids aren't always definitive proof of life, however. Geological events like water-mineral interactions in hydrothermal vents can also produce similar molecules. That said, the length of many of the Cumberland soil carbon-chains could suggest otherwise. Depending on the molecule, organic life fatty acids often contain chains of 11-13 carbon atoms, while non-biological fatty acids usually contain 12 or fewer carbons. This means that at least some of the large organic molecules detected by Freissinet's team may have once existed in organic life. What's more, the discovery eases worries that Martian biosignatures couldn't survive tens of millions of years of exposure to destructive oxidation and radiation.
'Our study proves that, even today, by analyzing Mars samples we could detect chemical signatures of past life, if it ever existed on Mars,' Freissinet, who also served as the latest study's lead author, said in a statement.
'There is evidence that liquid water existed in Gale Crater for millions of years and probably much longer, which means there was enough time for life-forming chemistry to happen in these crater-lake environments on Mars,' added Daniel Glavin, study co-author and sample return senior scientist at NASA's Goddard Space Flight Center.
Unfortunately, Freissinet and colleagues can only discover so much using Curiosity's SAM mini-lab. Organic fatty acid chains are often much longer than just 12 carbons, but the rover's equipment isn't designed to detect those. Luckily, NASA is ready and willing to assist in the next chapter of Martian exploration.
'We are ready to take the next big step and bring Mars samples home to our labs to settle the debate about life on Mars,' Glavin said.
Glavin, Freissinet, and colleagues may be waiting a while for that next step, however. While NASA has long planned on a Mars Sample Return mission, a ballooning budget and an uncertain future may push the project as far back as 2040.
Hashtags

Try Our AI Features
Explore what Daily8 AI can do for you:
Comments
No comments yet...
Related Articles
Yahoo
8 hours ago
- Yahoo
European Mars orbiter spies crumbling crater 'soaked in layers of Martian history' (photo)
When you buy through links on our articles, Future and its syndication partners may earn a commission. A European Mars probe captured a stunning view of a Martian crater that's rich in many of the features that help scientists reconstruct the planet's dynamic history over billions of years. The image, taken in October 2024 using the High Resolution Stereo Camera (HRSC) on the European Space Agency's (ESA) Mars Express orbiter, shows a crumbling crater called Deuteronilus Cavus. It is "soaked in layers of Martian history," having been exposed to volcanic lava flows, erosion from liquid water, repeated freeze-thaw cycles that expanded its edges, and layers of wind-blown volcanic dust settling over time, according to a statement from the space agency. Located in a transitional zone between the planet's rugged southern highlands and smoother northern lowlands, Deuteronilus Cavus is believed to originally have formed following an impact roughly 4.1 to 3.7 billion years ago, when Mars and other planets were being bombarded by huge numbers of asteroids and comets. Over time, the nearly circular 75-mile-wide (120 kilometers) depression has been eroded by water and ice, enlarging it to nearly twice its initial size. ESA shared a fun "recipe" outlining the series of events that shaped the crater, offering valuable insights into the planet's climatic and geological evolution. For example, the presence of clay minerals indicates past interactions between volcanic materials and water, hinting at the possibility of ancient habitable environments, according to the statement. This is further supported by channels cut through the crater's rim, likely formed by surface water flow or the collapse of weakened ground above draining subsurface water. Meanwhile, grooves in the crater rim suggest that ice once formed when Mars' axis tilted more sharply away from the sun than it does now. Related Stories: — Mars: Everything you need to know about the Red Planet — Facts about ESA's Mars Express orbiter — What happened to all the water on Mars? Here's why the debate continues "The linear grooves indicate where boulders frozen into the base of a glacier were dragged along, gouging out the troughs visible today," ESA officials said in the statement. "Around the base of the crater's inner walls, we can see the smooth, tongue-shaped ends of rock-covered glaciers. These 'debris aprons' formed when ice mixed together with rocky debris along the crater walls during a period of glaciation, and slowly crept downslope." The crater's interior also exhibits a mix of rock knobs, mesas, channels and plains, believed to be remnants of a collapsed central peak. Dark volcanic ash covers much of the crater floor, while surrounding wrinkle ridges mark ancient lava flows. "This feature-rich crater has all the ingredients for exploring Mars' varied geological processes, giving us a tantalizing taste of its complex history," ESA officials said in the statement.
Yahoo
14 hours ago
- Yahoo
These mysterious dark ‘streaks' on Mars aren't what scientists initially believed
Mysterious dark streaks first observed on Mars in the 1970s are not what many believed they were. Scientists now say the curious features that stretch for hundreds of meters down Martian slopes were likely signs of wind and dust activity — not water. 'A big focus of Mars research is understanding modern-day processes on Mars — including the possibility of liquid water on the surface,' Adomas Valantinas, a postdoctoral researcher at Brown University, said in a statement. 'Our study reviewed these features but found no evidence of water. Our model favors dry formation processes.' Valantinas and the University of Bern's Valentin Bickel coauthored the research which was recently published in the journal Nature Communications. To reach these conclusions, the researchers used a machine learning algorithm to catalog as many of the odd streaks as they could, creating a first-of-its-kind- global Martian map containing some 500,000 from more than 86,000 high-resolution images from NASA's Mars Reconnaissance Orbiter. Then, they compared their map to databases and catalogs of other factors, including temperature, wind speed, hydration, and rock slide activity. They looked for any correlations over hundreds of thousands of cases. The authors found that the ominous streaks that don't last for decades, known as recurring slope lineae or RSLs, are not generally associated with factors that suggest a liquid or frost origin. Those factors might include a specific slope orientation, high surface temperature fluctuations, and high humidity. The features were more likely to form in places with above-average wind speed and dust deposition. That points to a dry origin of formation, and they seem to show up in the same locations during the warmest periods of the Martian year before mysteriously vanishing. They concluded that the older slope streaks, which run down cliff faces and crater walls, most likely form when dust suddenly slides off slopes following seismic activity, winds, or even the shockwaves from meteoroid impacts. The streaks appear most often near recent impact craters, where shockwaves may shake the surface dust loose. The shorter-lived ones are typically found in places where dust devils or rockfalls are frequent. 'There were statistically significant correlations between new impact sites and the appearance of nearby slope streaks in certain regions, supporting this view,' NASA said. Previously, some had interpreted those streaks as liquid flows. It's possible that small amounts of water could mix with enough salt to create a flow on the frozen Martian surface, Brown University noted. The red planet was once more temperate, and there is water under the surface of Mars. Others believed they were triggered by dry process. These results cast new doubt on slope streaks and RSLs as habitable environments. 'That's the advantage of this big data approach,' Valantinas said. 'It helps us to rule out some hypotheses from orbit before we send spacecraft to explore.'
Yahoo
21 hours ago
- Yahoo
Why does NASA's Perseverance rover keep taking pictures of this maze on Mars?
When you buy through links on our articles, Future and its syndication partners may earn a commission. If you've spent any time perusing the carousel of raw images from NASA's Perseverance Mars rover, you might have stumbled across an odd subject: a tiny, intricate maze etched into a small plate, photographed over and over again. Why is the Perseverance rover so obsessed with this little labyrinth? It turns out the maze is a calibration target — one of 10 for Perseverance's Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals instrument, otherwise known for its fun acronym, SHERLOC. This Sherlock Holmes–inspired tool is designed to detect organic compounds and other minerals on Mars that could indicate signs of ancient microbial life. To do that accurately, the system must be carefully calibrated, and that's where the maze comes in. Located on the rover's seven-foot (2.1-meter) robotic arm, SHERLOC uses spectroscopic techniques — specifically Raman and fluorescence spectroscopy — to analyze Martian rocks. In order to ensure accurate measurements, it must routinely calibrate its tools using a set of reference materials with specific properties. These are mounted on a plate attached to the front of the rover's body: the SHERLOC Calibration Target. "The calibration targets serve multiple purposes, which primarily include refining the SHERLOC wavelength calibration, calibrating the SHERLOC laser scanner mirror, and monitoring the focus and state of health of the laser," Kyle Uckert, deputy principal investigator for SHERLOC at NASA's Jet Propulsion Laboratory, tells The target is arranged in two rows, each populated with small patches of carefully selected materials. The top row includes three critical calibration materials: aluminum gallium nitride (AlGaN) on sapphire discs; the UV-scattering material Diffusil; and Martian meteorite SaU008, whose mineral makeup is already known and helps align wavelength calibration with real Martian geology. This is also where you'll find the maze. Why a maze? "SHERLOC is all about solving puzzles, and what better puzzle than a maze!" says Uckert. The purpose of the maze target is to calibrate the positioning of the laser scanner mirror and characterize the laser's focus, which requires a target with sharply contrasting spectral responses. The maze serves this purpose well." The maze is made of chrome-plated lines just 200 microns thick (about twice the width of a human hair) printed onto silica glass. "There are no repeating patterns and the spectrum of the chrome plating is distinct from the underlying silica glass," says Uckert. That makes it possible to measure the laser's focus and accuracy with extreme precision. If you look closely at the maze, you'll also notice a Sherlock Holmes portrait right at the center. While it's a cheeky nod to the instrument's name, it serves a practical function. "SHERLOC spectral maps can resolve the 200 micron thick chrome plated lines and the 50 micron thick silhouette of Sherlock Holmes at the center of the maze," Uckert notes. Like the portrait, the bottom half of the SHERLOC Calibration Target also serves a dual purpose: spectral instrument calibration and spacesuit material testing. It contains five samples of materials used in modern spacesuits, including some materials you might be familiar with, like Teflon, Gore-Tex, and Kevlar. And don't miss the "fun" target in this row — there's a geocache marker backing a polycarbonate target, and it does indeed have a tie-in to Sherlock Holmes. RELATED STORIES: — Perseverance rover's Mars samples show traces of ancient water, but NASA needs them on Earth to seek signs of life — Perseverance Mars rover finds 'one-of-a-kind treasure' on Red Planet's Silver Mountain — Perseverance Mars rover becomes 1st spacecraft to spot auroras from the surface of another world These materials are actively being tested under Mars conditions to determine how they hold up over time in situ, which is crucial for planning human exploration of the Red Planet. "Note that we use all of these materials to fine-tune SHERLOC," adds Uckert. "As a bonus, the spacesuit materials support unique science that will help keep future astronauts safe." Now, if all these Sherlock Holmes–related Easter eggs on the SHERLOC Calibration Target aren't enough for you, there's one final link. SHERLOC has a color camera as part of its instrumentation suite that sometimes images the target, and it's called the Wide Angle Topographic Sensor for Operations and eNgineering. Yes, SHERLOC's sidekick is called WATSON.