NASA Hubble Study Finds Dwarf Galaxies Eject Most of Their Oxygen
Researchers using NASA's Hubble Space Telescope published a study on November 2, 2026, showing that dwarf galaxies lose most of the oxygen produced by their stars. The team analyzed 37 nearby dwarf galaxies under the Galaxies Losing Oxygen via Winds project. They discovered that energy from massive stars and supernova explosions drives oxygen out of these small stellar systems into surrounding space far more effectively than existing computer models predict. Oxygen is the third most abundant element in the universe after hydrogen and helium, making it a key indicator of how galaxies evolve and share chemical elements with intergalactic space. Understanding how dwarf galaxies lose oxygen helps scientists trace how fundamental chemical building blocks spread throughout the cosmos. The research shows that low-mass galaxies retain only a small fraction of the oxygen created within them, leaving open questions about where these heavy elements ultimately settle.
What was announced
Astronomers using NASA’s Hubble Space Telescope published research in The Astrophysical Journal examining 37 nearby dwarf galaxies. These small galaxies contain between a few thousand and hundreds of millions of stars. The team measured oxygen levels across stars, gas, and dust as part of the Galaxies Losing Oxygen via Winds (GLOW) project, which received funding from NASA and the National Science Foundation.
The observations revealed that dwarf galaxies retain only a small fraction of the oxygen generated by their stars. Energy from massive stars and supernova explosions creates powerful galactic winds. These winds blow oxygen out of the galaxies and into intergalactic space much more efficiently than theoretical models had anticipated. The researchers combined archival optical data from Hubble with observations from the Spitzer Space Telescope, the Very Large Array, and the Australia Telescope Compact Array to make their calculations.
What it means
Oxygen is the most common element in the universe after hydrogen and helium. Because its production in stars is well understood and easy to measure, astronomers use oxygen to track how galaxies build up heavy elements over time.
The GLOW project demonstrates that low-mass galaxies act as major suppliers of chemical elements to the intergalactic medium, which is the space between galaxies. Previous research from 2014 established that larger galaxies like the Milky Way lose oxygen into surrounding gas haloes called the circumgalactic medium. This new study shows that even small galaxies drive heavy elements out into surrounding space, changing how astronomers model galaxy growth and chemical enrichment across cosmic time.
What the announcement does not tell us
The announcement does not confirm where the missing oxygen ultimately resides. It remains unclear whether the oxygen stays in the gas halo surrounding each dwarf galaxy or if the galactic winds launch it completely out of the galaxy's local environment.
The release also does not provide exact percentages for how much oxygen was expected versus how much was detected in the 37 galaxies. Additionally, the announcement mentions future observation programs using NASA's Nancy Grace Roman Space Telescope and James Webb Space Telescope, but it does not specify dates for when those projects will begin or release data.
How this was written
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NASA’s Hubble studied 37 nearby dwarf galaxies and found that much of the oxygen they expected to see is missing.
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