Skip to main content

Hubble spots a ‘superbubble’ in a beautiful emission nebula

The Hubble Space Telescope may be experiencing problems this week, but it continues to offer a massive trove of data for astronomers to explore — including this week’s image of the beautiful and mysterious nebula N44.

This nebula has a highly unusual feature: A hole in its center, hundreds of light-years across, which forms a gap called a “superbubble.” N44 is a type of nebula called an emission nebula, which means it is a cloud of dust and gas which has been ionized by radiation from nearby stars and so which emits light in the visible wavelength. However, emission nebulae don’t typically have big holes in their centers, and scientists are still figuring out why N44 has this odd feature.

A dark, starry gap called a “superbubble,” visible in this Hubble Space Telescope image of Nebular N44 in the upper central region.
N44 is a complex nebula filled with glowing hydrogen gas, dark lanes of dust, massive stars, and many populations of stars of different ages. One of its most distinctive features, however, is the dark, starry gap called a “superbubble,” visible in this Hubble Space Telescope image in the upper central region. NASA, ESA, V. Ksoll and D. Gouliermis (Universität Heidelberg), et al.; Processing: Gladys Kober (NASA/Catholic University of America)

“The hole is about 250 light-years wide and its presence is still something of a mystery,” the Hubble scientists write. “Stellar winds expelled by massive stars in the bubble’s interior may have driven away the gas, but this is inconsistent with measured wind velocities in the bubble. Another possibility, since the nebula is filled with massive stars that would expire in titanic explosions, is that the expanding shells of old supernovae sculpted the cosmic cavern.”

N44 is huge, spanning 1,000 light-years across, and is located 170,000 light-years away in a satellite galaxy of the Milky Way called the Large Magellanic Cloud. Researchers have identified the bright blue area shown at the bottom right of the bubble as being the hottest region where stars are being formed at the fastest rate. The creation of hot stars gives rise to stellar winds which are unusually powerful in this nebula, reaching incredible speeds of over 4 million miles per hour.

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Asteroid impacted by spacecraft is reshaped like an M&M ‘with a bite taken out’
An illustration shows a spacecraft from NASA's DART mission approaching the asteroid it was intended to redirect.

In 2022, the world watched with fascination as NASA deliberately crashed a spacecraft into an asteroid in a test of what kind of defense options might be available to humanity if an incoming asteroid ever threatened Earth. Observers could tell very quickly that the test, called the Double Asteroid Redirection Test or DART, was successful in changing the asteroid's orbit. But now astronomers have learned more, finding that the impact may have reshaped the asteroid significantly.

The asteroid impacted, called Dimorphos, is very small at around 500 feet across, and the DART spacecraft crashed into it at a tremendous speed of nearly 4 miles per second. Researchers have now used computer modeling to see the effects of this impact, given the limited amount of information we have on the composition and uneven surface of Dimorphos.

Read more
Hubble spots a massive star forming amid clouds of dust and gas
This image from the NASA/ESA Hubble Space Telescope is a relatively close star-forming region known as IRAS 16562-3959.

A stunning new image from the Hubble Space Telescope shows the birth of a new, massive star at around 30 times the mass of our sun. Nestled with a nearby star-forming region called IRAS 16562-3959, the baby star is located within our galaxy and around 5,900 light-years from Earth.

You can see the sparkle of bright stars throughout the image, with the star-forming region visible as the orange-colored clouds of dust and gas stretching diagonally across the frame. These clouds are where dust and gas clump together to form knots, gradually attracting more dust and gas, growing over time to become protostars.

Read more
Hubble spies baby stars being born amid chaos of interacting galaxies
Galaxy AM 1054-325 has been distorted into an S-shape from a normal pancake-like spiral shape by the gravitational pull of a neighboring galaxy, seen in this Hubble Space Telescope image. A consequence of this is that newborn clusters of stars form along a stretched-out tidal tail for thousands of light-years, resembling a string of pearls. They form when knots of gas gravitationally collapse to create about 1 million newborn stars per cluster.

When two galaxies collide, the results can be destructive, with one of the galaxies ending up ripped apart, but it can also be constructive too. In the swirling masses of gas and dust pulled around by the gravitational forces of interacting galaxies, there can be bursts of star formation, creating new generations of stars. The Hubble Space Telescope recently captured one such hotbed of star formation in galaxy AM 1054-325, which has been distorted into an unusual shape due to the gravitational tugging of a nearby galaxy.

Galaxy AM 1054-325 has been distorted into an S-shape from a normal pancake-like spiral shape by the gravitational pull of a neighboring galaxy, as seen in this Hubble Space Telescope image. A consequence of this is that newborn clusters of stars form along a stretched-out tidal tail for thousands of light-years, resembling a string of pearls. NASA, ESA, STScI, Jayanne English (University of Manitoba)

Read more