NASA Selects 19 New Citizen Science Proposals in 2026

So far, 2026 has seen a flood of successes for volunteers who do NASA science, exemplifying NASA’s commitment to gold-standard science, transparent, reproducible and intrinsically collaborative. The institutional report frames the development in practical terms and ties it to the broader mission or observing effort.

It is relevant because astronomy does not advance on single detections. The field builds confidence by accumulating independent observations across different wavelengths, instruments and epochs until isolated signals become defensible conclusions. What looks convincing in one dataset can dissolve when a second instrument looks at the same target, and what looks marginal can solidify when follow-up campaigns confirm the original reading. The current standard requires that a result survive this triangulation before the community treats it as settled. Explore This Section Science Citizen Science NASA Selects 19 New Citizen. Overview Resources Opportunities Citizen Science Highlights About Science Activation So far, 2026 has. The Citizen Science Seed Funding Program The Citizen Science Seed Funding Program (CSSFP-25) of NASA’s Science Mission Directorate aims to support scientists and other experts to.

This project will invite you to search data from NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) mission to find. The Science Activation Program The Science Activation Program (SciAct) from NASA’s Science Mission Directorate supports a portfolio of competitively selected, collaborative.

The Citizen Science Seed Funding Program (CSSFP-25) of NASA’s Science Mission Directorate aims to support scientists and other experts to develop citizen Science Citizen Science. The Zooniverse platform, with grant from NASA, reached a milestone of 1 billion classifications.

Even with all of those achievements, our science community is already working on the next round of new volunteer projects and innovations. NASA’s Science Mission Directorate has selected nineteen proposals from research teams in 2026 that will result in new opportunities for you to do NASA science.

What gives the story weight is not just the object itself, but the way the measurement trims the range of plausible physical explanations. Astronomy has accumulated enough cases to know that the most interesting results are rarely the ones that confirm expectations cleanly; they are the ones that confirm some expectations while complicating others, or that open a parameter space that previous instruments could not reach. The scientific community evaluates these contributions by asking whether the new data constrain a model in a way that older data could not, and whether those constraints survive systematic review.

The Citizen Science Seed Funding Program (CSSFP-25) of NASA’s Science Mission Directorate aims to support scientists and other experts to develop citizen science projects and. This project will invite you to search data from NASA's SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) mission to find.

Because the account originates with NASA News Releases, it functions best as a primary institutional report that is close to the data and operations, not as independent scientific validation. Institutional communications are produced by organizations with legitimate interests in presenting their work in a favorable light, which does not make them unreliable but does make them partial. Details that complicate the narrative, including instrument limitations, unexpected failures and results below projections, tend to be minimized relative to progress messages. Technical documentation and peer-reviewed publications, where they exist, provide the complementary layer that institutional releases cannot substitute.

The next step is to see whether other instruments and other wavelengths tell the same story. Campaigns with JWST, the VLT, the forthcoming Extremely Large Telescopes and radio arrays will provide the spectral coverage and spatial resolution needed to move from detection to physical characterization. The timeline for that kind of confirmation is typically measured in years, not months, which is worth keeping in mind when reading the current result.

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