![Gamma-ray burst [GRB]. Credit: Cruz Dewilde/ NASA SWIFT.](https://nasaspacenews.com/wp-content/uploads/2025/05/gamma-ray-burst-credit-nasa-swift-cruz-dewilde-1-75x75.jpg)
NASA’s Perseverance rover has just made history—again. On March 15, 2024, during a violent solar outburst, the rover captured something never before seen from the surface of another world: a visible green aurora shimmering in the Martian night sky. This is no ordinary milestone. It marks the first time an aurora has been photographed on Mars in visible light, and it’s as groundbreaking as it sounds.
Auroras Beyond Earth: What Makes This Discovery Unique
Auroras form when energetic particles from the Sun slam into a planet’s atmosphere and interact with gas molecules, producing light. On Earth, these stunning visuals are guided by our planet’s global magnetic field, funneling charged particles to the poles. Mars, however, lacks such a global shield.
Instead, Mars has localized magnetic fields—fossil remnants of what was once a planetary dynamo. These crustal magnetic regions can still deflect and trap solar particles, but the resulting auroras are scattered, faint, and difficult to capture—especially with a visible light camera.
But thanks to careful planning and one perfectly timed solar storm, that’s exactly what happened. Perseverance’s Mastcam-Z snapped a historic image of green auroral emissions—a feat never before achieved on another planet’s surface.
The Solar Superstorm That Made It Happen
The aurora event was triggered by a massive solar flare on March 15, 2024, which launched a coronal mass ejection (CME)—a blast of solar energetic particles (SEPs)—toward Mars. SEPs are high-energy particles that can energize atoms in the upper atmosphere, leading them to emit light.
What made this event ideal wasn’t just its intensity but its timing within the Sun’s 11-year cycle. Scientists had predicted that the solar maximum would occur during this period—a peak in solar activity that increases the frequency of such powerful flares.
This allowed researchers, led by Elise Knutsen from the University of Oslo, to coordinate rover instruments with space weather predictions, anticipating the optimal moment to observe the phenomenon.
How NASA Pulled It Off: Planning Meets Precision
Capturing something this rare takes more than luck. It took a collaboration across multiple NASA teams and scientific institutions, including:
- NASA’s Moon to Mars (M2M) Space Weather Office
- The Community Coordinated Modeling Center (CCMC)
- NASA Goddard Space Flight Center
- Jet Propulsion Laboratory (JPL)
- University of Oslo and UC Berkeley
Using solar event simulations and real-time space weather data, these teams coordinated precisely when Perseverance should look to the sky. Its Mastcam-Z imager and SuperCam spectrometer were aligned to detect the faint green glow—thought to result from excited oxygen atoms, similar to auroras on Earth.
As Knutsen stated, “The trick was to pick a good CME, one that would inject enough charged particles into Mars’ atmosphere to create an aurora bright enough for Mastcam-Z to detect.”
Why Green? The Science Behind Martian Auroras
On Earth, green auroras are typically produced when oxygen atoms are excited by solar particles at altitudes around 100 km. The emission line—at 557.7 nanometers—produces the characteristic green glow.
On Mars, the same process was hypothesized to occur, but confirming it in visible light was a challenge due to the planet’s thin atmosphere—less than 1% of Earth’s surface pressure—and patchy magnetic shielding.
Now, with visible confirmation from Perseverance, these long-standing theories are finally validated. The green glow wasn’t just recorded by camera—it matched emission lines recorded by MAVEN’s SEP instrument, confirming that what Perseverance saw was indeed a green aurora.
A New Way to Study Space Weather on Mars
This discovery opens a new frontier in space weather science. Until now, Martian auroras were detectable only in ultraviolet, requiring orbiting spacecraft like NASA’s MAVEN to study them from above.
With this new method, we can now study auroras from the surface, providing an entirely different vantage point for understanding how solar storms interact with planetary atmospheres.
Katie Stack Morgan, acting project scientist at NASA’s JPL, emphasized this milestone, saying: “Perseverance’s observations confirm a new way to study these phenomena that’s complementary to what we can observe with orbiters.”
Why This Matters for Future Human Missions
Here’s where things get even more exciting. Astronauts on future Mars missions may be able to see these auroras with their own eyes.
Just imagine standing on the Martian surface, looking up at a sky glowing faint green from energized particles. It’s more than just a breathtaking sight—it’s also a crucial signal.
These auroras can indicate the intensity of solar activity and the amount of radiation bombarding the atmosphere—an essential factor for astronaut safety. By understanding auroral conditions, NASA can better prepare for radiation shielding, habitat design, and even mission timing to avoid solar storms.
What We Learn About Mars from This
The fact that visible auroras are even possible on Mars tells us a lot. It means that atmospheric density, magnetic regions, and solar particle interactions combine in just the right way to produce an optical effect, even without a global magnetic field.
This challenges previous assumptions that visible auroras couldn’t occur on thin-atmosphere planets. It also raises new questions: could similar auroras exist on Venus, Titan, or exoplanets with localized magnetism?
With this finding, Mars continues to surprise us—and it invites us to rethink planetary weather systems far beyond Earth.
What’s Next: A Future of Sky Watching on Mars
With the confirmation of visible-light auroras, future missions will almost certainly integrate aurora monitoring systems as part of their standard toolkit. These observations can help:
- Monitor space weather conditions in real time.
- Study variability in the Martian atmosphere.
- Provide alerts for incoming CMEs during crewed missions.
- Inspire future astronauts with unforgettable visual phenomena.
More importantly, NASA now knows that its rover-based imaging systems are capable of this kind of detection—paving the way for more advanced, multi-spectral observations in future surface missions.
Conclusion: A New Glow in the Martian Story
NASA’s Perseverance rover has once again redefined what’s possible in planetary exploration. By capturing the first visible-light aurora on Mars, it has not only given scientists a new tool for atmospheric study but also offered a poetic glimpse into what humans on Mars might one day see with their own eyes.
