# Dwarf Galaxies Expel Majority of Stellar Oxygen into Intergalactic Space

New research reveals small galaxies struggle to retain oxygen produced by massive star explosions.

- **Source:** [Universe Today](https://www.universetoday.com)
- **Published:** 2026-11-09
- **Topic:** [science](https://brifing.si/c/science)
- **Original article:** <https://www.universetoday.com/articles/nearby-dwarf-galaxies-show-surprising-lack-of-oxygen-says-paper>
- **On Brifing:** https://brifing.si/s/dcf1c795-3758-481b-9e9e-ff18edfb1224

## Oxygen as Cosmic Tracer

Oxygen is the universe's third most abundant element, making it a critical tracer for chemical evolution. Because its production in stars is well understood, astronomers use it to map how heavy elements like iron and nickel distribute across galaxies. This study focuses on how galaxies recycle matter throughout their lifetimes.

## Study of Dwarf Galaxies

Researchers analyzed 37 nearby dwarf galaxies, ranging from thousands to hundreds of millions of stars, using the Hubble Space Telescope. By examining individual star histories, the team calculated expected oxygen production versus actual retention. The findings, published in The Astrophysical Journal, highlight a significant discrepancy in chemical composition across these systems.

## Low Retention Rates

On average, these dwarf galaxies retain only 11 percent of the oxygen their stars produce. Retention varies significantly, with the most efficient galaxies holding about 25 percent, while the least efficient retain as little as 4 percent. Larger galaxies typically maintain three to four times more oxygen than these smaller counterparts.

## Supernovae Driven Winds

Massive stars end their lives in core-collapse supernovae, creating energetic winds that push oxygen-rich gas outward. Because dwarf galaxies possess weak gravitational fields, they struggle to contain this material. Consequently, most oxygen is expelled from the galaxy, leaving only a small fraction within the stars, gas, and interstellar dust.

## The GLOW Project

The Galaxies Losing Oxygen via Winds (GLOW) project investigates how heavy elements move between galaxies, their surrounding Circumgalactic Medium (CGM), and intergalactic space. By combining Hubble, Spitzer, and ground-based radio telescope data, researchers aim to track the lifecycle of oxygen and understand why current formation simulations often underestimate these losses.

## Impact of Galactic Location

Proximity to larger neighbors influences oxygen retention. Galaxies located within 3 million light-years of a massive neighbor tend to keep more oxygen, possibly due to surrounding gas pressure or re-accretion of expelled material. Conversely, isolated galaxies consistently retain less than 15 percent of their total produced oxygen, suggesting environmental factors matter.

## Missing Oxygen Mystery

The final destination of the expelled oxygen remains largely unknown. Previous studies found only 1 to 7 percent in the hot gas halos, with even cooler gas accounting for at most one-third of the total. Much of the missing material likely resides in the intergalactic medium, far beyond the host galaxy's reach.

## Future Observational Goals

Researchers plan to utilize the Nancy Grace Roman Space Telescope and James Webb Space Telescope to study even smaller, fainter galaxies. By zooming in on massive stars, astronomers hope to confirm if these dwarf systems act as the universe's primary oxygen spreaders, effectively seeding space with the building blocks of life.

## Sources covering this story

- [Universe Today — Nearby Dwarf Galaxies Exhibit Unexpected Oxygen Deficiency](https://www.universetoday.com/articles/nearby-dwarf-galaxies-show-surprising-lack-of-oxygen-says-paper)
- [Mashable — Dwarf Galaxies Expel Majority of Their Stellar Oxygen](https://mashable.com/science/hubble-telescope-dwarf-galaxies-missing-oxygen)
- [Mashable — Small Galaxies Expel Most Oxygen Produced by Their Stars](https://mashable.com/science/hubble-telescope-dwarf-galaxies-missing-oxygen)

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_Summary written by Brifing from the original reporting. Copyright in the original article belongs to its publisher; read the full piece at the link above._
