NASA's SPHEREx telescope has mapped water ice scattered across stretches of interstellar space spanning more than 600 light-years, and the finding reframes a basic assumption about planetary habitability: having water nearby may not be an accident.
The observations, published in the Astrophysical Journal on April 15, show that ice — the raw stuff of oceans and atmospheres — is not a scarce resource delivered by rare early impacts. It is a routine, distributed supply line. SPHEREx found water ice in the giant molecular clouds that seed new solar systems, including regions more than 600 light-years across in the Milky Way's Cygnus X complex. The data came from the mission's spectroscopic survey, which detects ices by the specific wavelengths of infrared light they absorb.
"Water is being incorporated into planetary systems as they form — not just as a one-time delivery, but as an ongoing supply chain," said Phil Korngut, an instrument scientist for SPHEREx at Caltech and JPL. He described vast frozen complexes as "interstellar glaciers" that could deliver a massive water supply to new solar systems being born in the region.
The implications flip the usual wonder-story framing. The question is not where Earth's water came from — it has been known for years that icy asteroids and comets delivered it. The question is how often that delivery happens, and whether conditions for habitability are common or rare. SPHEREx's all-sky survey, the first of four planned, provides the statistical baseline to answer that. By late 2025, the spacecraft had completed its first full-sky spectroscopic map, giving researchers a galaxy-wide view of ice distribution for the first time.
Traditional telescopic observations of interstellar ice required pointing at individual star-forming regions one at a time. SPHEREx, launched March 11, 2025, maps entire sky regions simultaneously using a design that splits incoming light into 102 distinct infrared colors, letting it identify specific molecules by their absorption signatures. The instrument is the first infrared mission specifically designed to find ice molecules over the entire sky via large-scale spectral survey. Ground-based telescopes cannot do this because water ice absorbs and blocks the wavelengths needed for detection from the ground.
The ice mapped by SPHEREx is not floating freely. It forms on the surface of dust particles no larger than the particles found in candle smoke, in regions dense enough that thick dust shields the ice from destructive ultraviolet radiation. The absorption maps broadly trace dense, cold, well-shielded regions consistent with active ice formation happening now — not just preserved ancient ice. "We can investigate the environmental factors that contribute to different ice formation rates across large areas of interstellar space," said Gary Melnick, an astronomer at the CfA and lead of the Interstellar Ices project.
The 13-institution science team behind the result spans the US, South Korea, and Taiwan. The telescope and spacecraft bus were built by BAE Systems in Boulder, Colorado. Jamie Bock of Caltech and JPL leads the mission; Olivier Doré of JPL and Caltech is project scientist. Joseph Hora of the Harvard-Smithsonian Center for Astrophysics is lead author on the ApJ paper.
SPHEREx is designed to trace the evolution of water and molecular ices from the interstellar medium into star systems — not just map where ice exists now, but follow the material through time. Three more all-sky surveys remain planned. The next full dataset will improve resolution on the ice maps and expand coverage to the galactic center and southern sky. Whether that data confirms ice distribution is uniform across galaxy types or varies with star formation density is the open question the mission is built to answer.