Patience Reveals Potential Chemical Signatures of Ancient Martian Microbes

NASA’s diligent rover has been investigating and sampling igneous fields and sedimentary rocks within the Ezero Crater, providing insights into the geological processes and intriguing characteristics of early Mars, while also searching for potential biological signatures. Upon entering Neretvavalis, on the western edge of Jezero Crater, the rover examined the distinct mudstone and con rock outcrops of the Bright Angel formation. A new paper published in the journal Nature details extensive geological, petrological, and geochemical studies of these rocks.



The impression of this artist shows how Mars looked about 4 billion years ago. Image credit: M. Kornmesser/ESO.

“Upon the rover’s arrival at the Bright Angel formation and while analyzing the local rocks’ composition, our team was notably surprised by their distinctiveness compared to previous findings,” stated Dr. Michael Tice, a geoscientist and astrobiologist at Texas A&M University.

“These findings offer evidence of chemical cycling that organisms on Earth can utilize to harness energy.”

“As we delved deeper, we observed phenomena that could easily be attributed to early Martian life, yet remain challenging to rationalize purely through geological processes.”

“Living organisms conduct chemistry that is naturally prevalent, provided there’s sufficient time and suitable conditions.”

“To optimize our understanding, the chemistry leading to these rocks necessitates either elevated temperatures or biological involvement, and we find no signs of high temperatures here.”

“Nonetheless, these results warrant experimentation and eventually lab studies of the samples collected to completely rule out non-biological explanations.”

The Bright Angel layer comprises mudstone (fine-grained sedimentary rocks composed of silt and clay) and water-laid sedimentary rocks featuring layered beds indicative of a lively environment with flowing rivers and stagnant water.

Employing various instruments from Perseverance, such as Sherloc and PIXL spectrometers, scientists identified organic molecules and small mineral arrangements likely formed through chemical processes related to redox reactions and electron transfers. On Earth, these processes are frequently driven by biological activities.

The most notable characteristics include small nodules and “reaction fronts” – referred to as “poppy seeds” and “leopard spots” by the rover team – consisting of iron phosphate (likely vivianite) and iron sulfide (probably greygeite).

These minerals typically arise in cold, water-laden settings and are frequently associated with microbial metabolism.

“The structural arrangement suggests that they formed through the redox cycling of iron and sulfur along with associated minerals,” Dr. Tice commented.

“On Earth, such formations often occur in sediments where microorganisms consume organic material and ‘breathe’ rust and sulfate. “

“Their existence on Mars provokes an intriguing question: Could a similar process have occurred there?”



The artist’s concept depicts the perseverance of NASA’s Mars Rover on the surface of the red planet. Image credit: NASA/JPL-Caltech.

The Sherloc instrument identified a Raman spectral feature known as the G-band, indicating the presence of organic carbon, in certain Bright Angel rocks.

The most substantial signal originated from a location called Apollo Temple, which exhibited high concentrations of both Vivianite and Greygeite.

“The concurrent presence of this organic matter and redox-sensitive minerals is quite compelling,” Dr. Tice noted.

“This implies that organic molecules might have facilitated the chemical reactions responsible for forming these minerals.”

“It’s crucial to recognize that ‘organic’ doesn’t invariably imply life creation.”

“This suggests the presence of numerous carbon-carbon bonds.”

“Alternative processes can yield organic compounds without biological involvement. The organic compounds identified here could have been synthesized either by or as a result of biological activity.”

“If they originated from an organism, decomposition through chemical reactions, radiation, or heat would have been required to yield the G-band we observe today.”

This research outlines two potential scenarios: Firstly, these reactions might be abiotic (driven by geochemical mechanisms) while microorganisms, similar to those on Earth, could have influenced these reactions.

Interestingly, although some features of the nodules and reaction fronts can be produced by non-biological reactions between organic matter and iron, established geochemical processes that can generate sulfur-related features tend to require relatively high temperatures.

“Every observation we’ve made regarding these rocks indicates that they haven’t been subjected to heat capable of producing leopard spots and poppy seeds,” Dr. Tice remarked.

“If that’s accurate, we must genuinely contemplate the possibility that such formations were created by bacteria-like life forms existing in the Martian lake sediments over 300 million years ago.”



Views of Perseverance path through Neretva Vallis and the formation of Bright Angels. Image credit: Hurowitz et al., doi: 10.1038/s41586-025-09413-0.

The research team underscores that while the evidence is not definitive proof of past life, the findings align with NASA’s criteria for potential biosignatures. This characteristic paves the way for further inquiries to ascertain the biological or non-biological origins.

Perseverance has collected core samples from a Bright Angel layer named Sapphire Canyon, which are currently housed in sealed tubes onboard the rover.

This sample is prioritized for future return to Earth in a prospective mission.

“Once we return this sample to Earth, we can investigate it using far more sensitive instruments than those we can deploy on Mars,” Dr. Tice explained.

“We could analyze the isotopic composition of organic materials, fine mineralogy, and conduct searches for microfossils if they exist.”

“More tests can also help determine the maximum temperatures these rocks were subjected to, and whether high-temperature geochemical processes are the most plausible explanations for any potential biological signatures.”

“The similarities between processes on Mars and Earth are indeed remarkable. However, there’s one crucial distinction.”

“It’s fascinating to note that life employs some of the same processes on both planets around the same epochs.”

“We observe signs of microorganisms in Earth’s rocks of similar ages where iron and sulfur interact with organic matter in comparable ways, but we don’t encounter the exact features seen in Mars’ ancient stones.”

Due to tectonic activities, the majority of Earth’s rocks have been altered significantly, making it unique and spectacular to witness this phenomenon on another planet.”

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Ja Hurowitz et al. 2025. Redox-driven minerals and organic associations at Jezero Crater, Mars. Nature 645, 332-340; doi:10.1038/s41586-025-09413-0

This article is based on a press release provided by Texas A&M University.

Source: www.sci.news

Patience Unveils the Aurora at Visible Wavelengths on Mars

Mars exhibits various aurora processes despite its thin atmosphere and absence of global magnetic fields. Previously, all aurora observations have been conducted in ultraviolet wavelengths from orbit. In a recent study, planetary scientists reported the observation of a green visible wavelength aurora, generated from the atomic oxygen line at 557.7 nanometers (nm), detected by NASA’s Perseverance rover using the Supercam and Mastcam-Z instruments.



The first visible image of the green aurora on Mars (left) taken by the NASA Perseverance rover’s Mastcam-Z instrument. On the right is a comparison image of the night sky on Mars without aurora, featuring the Moon Deimos on Mars. The moonlit Mars night sky, primarily illuminated by the larger moon Phobos (outside the frame), has a reddish-brown tint due to atmospheric dust. Consequently, the addition of green aurora light results in a green-yellow tone in the left image. Image credits: NASA/JPL-CALTECH/ASU/MSSS/SSI.

On Earth, auroras occur when solar particles interact with the magnetic field, colliding with atmospheric gases at the poles and emitting light.

Green, the most frequently observed color, results from excited oxygen atoms emitting light at a wavelength of 557.7 nm.

Researchers have theorized for years that green auroras could also manifest on Mars, but noted they would likely be more diffuse and harder to capture than those on Earth.

Due to the absence of a global magnetic field, Mars experiences a distinct type of aurora compared to Earth.

One such type is the Solar Energy Particle (SEP) Aurorae, identified by NASA’s Maven mission in 2014.

These auroras occur when high-energy particles from the sun impact the Martian atmosphere, leading to a luminous display in the night sky.

“Our findings open up new avenues for aurora research and affirm that future astronauts on Mars could witness these phenomena,” stated Dr. Ellis Knutsen, a postdoctoral researcher at the University of Oslo.

On March 15, 2024, the Sun’s solar flare production and the accompanying coronal mass ejection prompted auroras across the solar system, including Mars, with Perseverance capturing them for the first time from another planet’s surface.

Dr. Knutsen and his team utilized data from SEP instruments on NASA’s Maven spacecraft and ESA’s Mars Express spacecraft to verify the detection.

“They’re actively tracking this,” remarked Dr. Shannon Curry, a researcher at Maven and at the Institute of Atmospheric Astronomy at the University of Colorado, Boulder.

“We are thrilled to rapidly advance this observation and look forward to revealing what astronauts might see there.”

By correlating Perseverance’s observations with data from Maven’s SEP instrument, researchers can better analyze the detected 557.7 nm radiation from solar energy particles.

This emission line is identical to the green aurora on Earth, implying that future Mars astronauts may witness this type of aurora.

“The visibility of auroras from Perseverance enables new methods to study these phenomena, complementing orbital observations of Mars,” noted Dr. Katie Stack Morgan, the project scientist for Perseverance at NASA’s Jet Propulsion Laboratory.

“A deeper understanding of auroras and the conditions on Mars that facilitate their formation is crucial for preparing to send human explorers there safely.”

The team’s study was published in the journal Advances in Science.

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Elise W. Knutsen et al. 2025. Detection of the visible wavelength aurora on Mars. Advances in Science 11 (20); doi:10.1126/sciadv.ads1563

Source: www.sci.news

Mastering the Art of Patience: A Game Where Waiting is Key

aPatience may not always be easy to practice, especially during mundane and tedious moments. However, there can still be joy and peace found in the simplicity of everyday life. Optiillusion introduces a tongue-in-cheek patience simulator called While Waiting to capture this unique experience. Producer Dong Zhou explains, “While we’re waiting for things like buses, stuck in traffic, or standing in line, we often seek entertainment. Most people just resort to using their phones, but is that truly engaging? It’s time to turn waiting into a playful experience by turning mundane moments into a fun game where players can find ways to pass the time.”

While waiting. Photo: Optillusion Games

While Playing, players join Adam on his journey through mundane tasks like waiting for a bus, standing in line for a ride, or watching the rain from a window. Zhou states, “Waiting isn’t just a negative experience; it’s a part of life that comes with its own set of expectations and anxieties.” As Adam’s experiences evolve from simple pleasures to deep aspirations, the game becomes a story of personal growth. “In different waiting scenarios, Adam feels a range of emotions like happiness, relief, or sadness. However, he understands that waiting is the only option,” Zhou adds.

Through whimsical depictions of scenarios like elevator lobbies, doctor’s offices, and airport baggage claims, While Waiting presents a series of patience-testing challenges that resonate with common frustrations. While a sense of fatalism looms, the game incorporates profound reflections on life alongside playful anime humor. Zhou hopes players will not only find amusement but also ponder the deeper meanings interwoven within the game.

To ease the restlessness that waiting brings, While Waiting offers various mini-games to help pass the time, such as luggage stacking or filling out paperwork. Zhou explains, “These mini-games can range from arcade games to puzzles or action games, each level offering a unique experience. While players won’t win cash prizes, the games are designed to keep them entertained while waiting for time to pass. Whether you choose to act or not, the game’s theme revolves around the inevitability of waiting.”

Drawing inspiration from classic animated comedies like “Tom and Jerry,” While Waiting incorporates orchestral music that emphasizes the contemplative and whimsical aspects of this patient journey. The brass and string instrumentation offers a musical reprieve from the discomfort of inaction in daily life.

Despite its quirky and light-hearted nature, While Waiting delves into profound themes. As players approach the conclusion, they revisit earlier scenes and contemplate the cyclical nature of life with fresh insights and emotions. Zhou concludes, “Life is a mix of joy and sorrow, and I hope players will appreciate the value of each waiting moment they encounter.”

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While Waiting is set to launch on PC later this year

Source: www.theguardian.com