Icy Islands at the Edge: How Webb Found Tiny Worlds ✛ ✎

Original: "The Luminosity Function of Ultra-Faint Trans-Neptunian Objects Detected by JWST"
arXiv:2609.09044v1 · 2026-09-08 · arXiv non-exclusive · independent analysis · 2 min
The James Webb Space Telescope spotted city-sized icy chunks beyond Neptune, and their size distribution turns out to be the same across the board.

Beyond the planet Neptune, in the dark and cold distance, drifts a multitude of icy chunks, like islands in an ocean. These chunks have remained nearly unchanged for four billion years and hold memories of how planets were born. But spotting the small ones has been extremely difficult: they shine fainter than a candle seen from the Moon. Now the James Webb Space Telescope has managed to see even those the size of a city, about ten kilometers across.

The telescope imaged the same patch of sky three times, with five-day gaps. During that time, a distant chunk shifts against the background stars, like a slow raft among stationary buoys. To catch such faint light, scientists aligned the images according to each candidate's motion, then used a computer program trained on artificial examples to discard false signals. In this way, they found 27 genuine icy islands.

It turned out that the brightness distribution of these chunks, meaning how many large ones and how many small ones, is the same for two different groups: those on calm, circular orbits and those on tilted, elongated paths. This implies that both kinds were born in the same way.

This discovery helps us understand how planets come into being. Previously, it was thought that the number of icy chunks should drop off at small sizes, but Webb has shown that they continue to exist even down to ten kilometers. Now scientists know that the bulk of the Kuiper Belt's mass is concentrated in bodies around 200 kilometers across, not in small debris. The census of icy islands is just beginning, and many more discoveries lie ahead.

The faintest reliably detected object, JPB24, is 100 times fainter than the brightest in the survey, 2015 GK56, and its brightness is comparable to a candle flame at the distance of the Moon.

\Sigma(m) = 10^{\alpha(m-m_0)}
The surface density of objects per square degree grows as a power of brightness with slope α.
\Sigma_{\text{tapered}} = \ln(10) \cdot \exp(-10^{\beta(m_B-m)}) \cdot 10^{(\alpha-\beta)m - \alpha m_0} \cdot (\alpha \cdot 10^{\beta m} + \beta \cdot 10^{\beta m_B})
A model with a smooth cutoff at the bright end, predicted by streaming instability simulations.
Concepts
JWST nirspec jwst red sources james webb space telescope miri neutrino detection scintillator juno neutrino detection neutron star light emission subaru telescope neutron star composition zwicky transient facility lithium niobate nustar superdense matter Niño 4