Mars
© ESA
En kunstners illustration af Det Europæiske Rumagenturs ExoMars Trace Gas Orbiter, der registrerer den grønne glød af ilt i Mars' atmosfære. Denne emission, der blev opdaget ved Mars' dagslys, svarer til den natglød, der fra rummet ses omkring Jordens atmosfære.
Det Europæiske Rumfartsagenturs Trace Gas Orbiter (TGO) opdagede en smaragdglød i Mars 'uklare atmosfære, hvilket markerer første gang fænomenet er blevet opdaget i en verden udenfor Jorden, rapporterer en ny undersøgelse.

'En af de lyseste emissioner, der er set på Jorden, stammer fra natglød. Mere specifikt fra iltatomer, der udsender en bestemt bølgelængde af lys, der aldrig er blevet set omkring en anden planet,' sagde undersøgelsens hovedforfatter Jean-Claude Gérard fra Université de Liège i Belgien i en erklæring.

'Imidlertid har denne type emission været forventet at kunne forekomme på Mars i omkring 40 år - og takket være TGO har vi fundet det,' sagde Gérard


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As Gérard noted, the green emission is characteristic of oxygen. Skywatchers at high latitudes here on Earth can see this signature in the ethereal, multicolored displays known as the auroras, which are generated by charged particles from the sun slamming into molecules high up in the atmosphere.

But night glow is different. It's caused by the interaction of sunlight with atoms and molecules in the air, which generates a subtle but continuous light. This emission is hard to see, even here on Earth; observers often need an edge-on perspective to make it out, which is why some of the best images of our planet's green night glow come courtesy of astronauts aboard the International Space Station (ISS).

Day glow, the diurnal component of this constant emission, is even harder to spot. And it's driven by a slightly different mechanism.

"Night glow occurs as broken-apart molecules recombine, whereas day glow arises when the sun's light directly excites atoms and molecules such as nitrogen and oxygen," European Space Agency (ESA) officials wrote in the same statement.

Gérard and his colleagues used TGO's Nadir and Occultation for Mars Discovery (NOMAD) instrument suite, which includes the Ultraviolet and Visible Spectrometer (UVIS), to study the Red Planet's air in a special observing mode from April through December of last year.

"Previous observations hadn't captured any kind of green glow at Mars, so we decided to reorient the UVIS nadir channel to point at the 'edge' of Mars, similar to the perspective you see in images of Earth taken from the ISS," study co-author and NOMAD principal investigator Ann Carine Vandaele, of the Institut Royal d'Aéronomie Spatiale de Belgique in Belgium, said in the same statement.

The team scanned the Martian atmosphere at altitudes between 12 miles and 250 miles (20 to 400 kilometers). They found the green oxygen glow at all heights, though it was strongest around 50 miles (80 km) up and varied with the Red Planet's distance from the sun.

The researchers also performed modeling work to better understand what's driving the glow. Those calculations suggested the light is driven mainly by the breakup of carbon dioxide, which makes up 95% of Mars' thin atmosphere, into carbon monoxide and oxygen.

TGO saw these stripped oxygen atoms glowing in both visible and ultraviolet light, with the visible emission about 16.5 times more intense than the UV.

"The observations at Mars agree with previous theoretical models, but not with the actual glowing we've spotted around Earth, where the visible emission is far weaker," Gérard said. "This suggests we have more to learn about how oxygen atoms behave, which is hugely important for our understanding of atomic and quantum physics."

TGO has been circling Mars since October 2016. The orbiter is part of the two-phase European-Russian ExoMars program, which plans to launch a life-hunting rover called Rosalind Franklin toward the Red Planet in 2022. (The Rosalind Franklin was originally supposed to lift off this summer, but technical issues with the spacecraft's parachute and other systems caused the mission to miss that window.)

The new TGO results, which were published online today (June 15) in the journal Nature Astronomy, will be helpful to the Rosalind Franklin team, ESA officials said.

"This type of remote-sensing observation, coupled with in situ measurements at higher altitudes, helps us to predict how the Martian atmosphere will respond to seasonal changes and variations in solar activity," Håkan Svedhem, ESA's TGO project scientist, said in the same statement.

"Predicting changes in atmospheric density is especially important for forthcoming missions, including the ExoMars 2022 mission that will send a rover and surface science platform to explore the surface of the Red Planet," said Svedhem, who is not a co-author of the new study.