Most martian news reaches you at the end of a very long relay, and almost none of it begins with a scientist announcing something. It begins with a compressed image file landing at a ground station outside Madrid, or Canberra, or Goldstone in the Mojave, tagged with a sol number and a camera name. Weeks or years later, some fraction of that file turns into a headline. What happens in between is the whole story, and knowing its shape changes how you read every Mars article.
This is a field guide to that pipeline: how a raw frame becomes a paper, why a preprint is not a result, and why “signs of life” in a headline nearly always translates to “chemistry we cannot yet explain.”
The First Thing You See Is a Half-Baked Thumbnail
Curiosity and Perseverance both carry radios capable of talking straight to Earth, and both use them as little as possible. Direct-to-Earth transmission is slow and eats power. The bulk of the data goes upward instead, in short bursts, to whichever orbiter happens to be passing overhead — Mars Odyssey, which has been in orbit since 2001, or Mars Reconnaissance Orbiter, or MAVEN, or ESA’s Trace Gas Orbiter, all of which double as relay stations. The orbiter stores the packets and dumps them to the Deep Space Network on its own schedule. Add a one-way light delay that swings between roughly four and twenty-four minutes, and you get the most misunderstood fact about Mars coverage: nothing is live. Ever.
What arrives first is usually ugly. Hazard camera frames come through a fisheye lens that bows the horizon. Compression leaves blocky artifacts, dust sits on the optics, pixels die, and dropped data lines leave black gashes across the scene. NASA posts these raw frames publicly, more or less unfiltered, within hours of downlink — which is genuinely remarkable and also the single richest source of nonsense on the internet. Every “alien skull spotted on Mars” video is someone zooming five hundred percent into a forty-pixel compression artifact on a rock.
There is a second trap in the same place. Many published Mars images are white balanced, stretched to show how the scene would look under Earth’s daylight so geologists can compare rocks against terrestrial samples. Other versions keep the actual butterscotch cast of light filtered through suspended dust. Both are honest. If you have seen someone point at two versions of the same rock and claim NASA is hiding a blue sky, this is what they found.
Preprint, Paper, Press Release
Between the raw frame and the announcement sits an unglamorous middle. Engineers calibrate the data and deposit the finished products in NASA’s Planetary Data System, typically after a proprietary period of several months during which the instrument team gets first look. That archive is public and permanent, and almost nobody outside the field opens it.
Meanwhile the science team argues. The first public trace of a new result is often a two-page abstract at the Lunar and Planetary Science Conference, held every March in The Woodlands, Texas. Those abstracts are not peer reviewed. They are closer to a scientist saying “here is what we think we are seeing, come argue with us in the poster hall.” A surprising number of Mars stories are born there.
Then the manuscript, and here the three categories worth separating properly.
A preprint — posted to arXiv or the Earth and Space Science Open Archive — is a real paper by real researchers that has not been through review. Read them. Just know the version you are reading may not survive contact with three referees. A peer-reviewed paper in Science, Nature Astronomy, Icarus or Astrobiology has survived that contact, which filters out a lot of bad work and by no means all of it. Review is a floor, not a verdict.
A press release is a third thing entirely, and it is the one you almost always encounter. It is written by a communications office at NASA, JPL or a university whose measurable job is attention. Good releases are accurate — the caveats are simply parked in paragraph six, where nobody reads them. The damage happens downstream, when aggregators rewrite the release rather than the paper, then rewrite each other. Four hops later the hedge is gone and the qualifier has become a claim.
Why “Signs of Life” Almost Always Means “Interesting Chemistry”
Organic molecules are not life. Carbon chemistry is spectacularly common without any biology involved. The Murchison meteorite carries amino acids. The Bennu sample that OSIRIS-REx dropped into the Utah desert in September 2023 holds amino acids and nucleobases, from an asteroid that was never alive. Water reacting with olivine in hot rock — serpentinization — produces organics and methane on its own. When Curiosity’s onboard chemistry lab reports chlorobenzene, thiophenes or long-chain alkanes in a mudstone, the finding is that Mars preserved complex carbon for three billion years. That is a real result about preservation, not about biology.
The field has an actual scale for this, which more martian news coverage should use: the Confidence of Life Detection scale, proposed in 2021 to keep everyone honest. It runs seven levels, from “we detected a signal consistent with biology” to “independent teams reproduced it and ruled out every non-biological explanation.” Essentially every Mars claim ever made lives at level one or two.
The best current example sits in a sealed tube. In July 2024 Perseverance drilled a mudstone in the Bright Angel formation, in a valley on the rim of Jezero Crater, and found leopard-spot textures — millimetre-scale reaction fronts containing vivianite, an iron phosphate, and greigite, an iron sulfide. On Earth those minerals commonly form where microbes are metabolizing organic matter in wet sediment. They also form abiotically at higher temperatures. The team published in Nature in September 2025 and called it a potential biosignature — exactly the right phrase, and exactly the phrase that got shortened everywhere else. Perseverance cannot settle it. The instruments that could are in laboratories on Earth, and the sample sits in a tube waiting for a return mission whose cost runs into the billions and whose design keeps being rethought.
Four Times the Story Outran the Data
On 25 July 1976, Viking 1 photographed a mesa in the Cydonia region at about 43 metres per pixel. A dropped data bit put a black speckle roughly where a nostril belongs, NASA released the frame with a jokey caption about a rock formation resembling a head, and the Face on Mars was born. Mars Global Surveyor re-photographed it in 1998 and again in 2001 at better than two metres per pixel. It is a hill. That took twenty-five years.
ALH 84001, a meteorite picked up in the Allan Hills of Antarctica in 1984, went further. A team led by David McKay reported in Science in 1996 that it contained carbonate globules, polycyclic aromatic hydrocarbons, magnetite grains and tube-shaped features tens of nanometres long, and read the combination as fossil martian microbes. There was a statement from the White House lawn. Then every strand came apart: the magnetite could form without biology, the organics could be contamination or abiotic, and the tubes were smaller than any confirmed cell. The rock did not prove life. It did more or less create modern astrobiology as a funded discipline, which is a strange kind of legacy.
Methane is the argument that never ended. Curiosity’s tunable laser spectrometer measures a faint background inside Gale Crater, under a part per billion, punctuated by spikes an order of magnitude higher. ESA’s Trace Gas Orbiter arrived with far better sensitivity, looked at the whole atmospheric column, and reported essentially nothing. Both can be true if gas seeps from the ground at night and is destroyed or dispersed before it mixes upward. Or one instrument is fooling itself. Nobody has closed it, and even a confirmed detection would settle little, because serpentinization makes methane without a single living cell.
Recurring slope lineae are the cleanest cautionary tale in modern martian news. Dark streaks on warm slopes, first described from orbital imagery in 2011, growing in summer and fading in winter. In 2015 a spectral study reported hydrated salts within them, a NASA press conference followed, and the world learned that liquid water flows on Mars today. Follow-up work in 2017 showed the streaks stop at slopes right around the angle of repose for dry sand, behaving like granular flows, and that the spectrometer’s footprint was far wider than the streaks themselves. The reading now leans dry, with brine a minority possibility.
Where the Originals Live
All of this is checkable, and faster than it sounds. The raw image galleries for both rovers are open to anyone. The Planetary Data System holds calibrated archives. HiRISE publishes its orbital images with captions written by the people who targeted them, and ESA’s Planetary Science Archive covers the European missions. Best of the lot are the mission update blogs, where working scientists write a few hundred words about what their rover did that sol and sign their names to it.
Three questions handle most cases. Is this a peer-reviewed paper, a conference abstract, or a press release? Does the claim rest on a detection or on an upper limit? Has anyone independently measured the same thing? If a story survives all three, it is probably worth your attention.
If you would rather follow Mars this way — sources first, hedges intact, headlines last — that is more or less the house style at SETIworld. Come read with us, argue in the threads, and bring the papers.