Hubble and Webb find that far-out solar system objects 'remember' the past
For the first time, scientists used the combined power of NASA's Hubble and James Webb Space Telescopes to study some of the most far-flung bodies in our solar system.
Key points
- Focus: For the first time, scientists used the combined power of NASA's Hubble and James Webb Space Telescopes to study some of the most far-flung bodies in
- Detail: Science reporting: verify primary technical documentation
- Editorial reading: science reporting; whenever possible, verify the cited primary source.
For the first time, scientists used the combined power of NASA's Hubble and James Webb Space Telescopes to study some of the most far-flung bodies in our solar system, trans-Neptunian objects. The science-journalism coverage adds useful context, while the strongest evidential footing still comes from the underlying data, papers or institutional documentation.
That matters 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. These objects are so small that even with NASA's Hubble and Webb space telescopes, they appear only as tiny points of light. NASA, ESA, Leah Hustak (STScI) For the first time, scientists used the combined power of NASA's Hubble and James Webb Space Telescopes to study some of the most far-flung bodies.
In two complementary papers published Tuesday in The Astronomical Journal, teams analyzed the color, composition and size distribution of 27 newly discovered tiny, dim TNOs. Candidates from the University of Victoria in Canada and Northern Arizona University in Flagstaff, under the guidance of the National Research Council of Canada, examined a patch.
Discover the latest in science, tech, and space with over 100, 000 subscribers who rely on Phys. org for daily insights. Webb discovered 27 new, remarkably dim TNOs, including one so faint it is equivalent to standing on Earth and seeing a small swarm of fireflies on the moon.
The smallest one they observed has a diameter of about 3 miles (5 kilometers), which is about five times smaller than what is possible to detect with the most sensitive. This project would not have been possible without Hubble and Webb working together to detect and characterize these TNOs.
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.
With Hubble's sensitivity in visible light and Webb's in infrared, the space telescopes provide more insights than either can on its own. Eduardo et al, The Luminosity Function of Ultrafaint Trans-Neptunian Objects Detected by JWST, The Astronomical Journal (2026).
Because this item comes through Phys. org Space as science journalism, it should be treated as contextual reporting rather than primary evidence. Good science reporting can identify why a result matters, connect it to the wider literature and make technical work readable, but the decisive evidence remains in the original paper, dataset, mission release or technical record. That distinction is especially important when a story is later repeated by aggregators, because repetition increases visibility, not evidential strength.
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.

Original source: Phys. org Space