Hubble Space Telescope images exceptionally fluffy galaxy

In this week’s image from the Hubble Space Telescope, you can see an unusual type of galaxy called an ultra-diffuse galaxy. The galaxy GAMA 526784 is shown as a smear of light across the center of the image and is around four billion light-years away located in the constellation of Hydra.

“Ultra-diffuse galaxies such as GAMA 526784 have a number of peculiarities,” Hubble scientists write. “For example, they can have either very low or high amounts of dark matter, the invisible substance thought to make up the majority of matter in the universe. Observations of ultra-diffuse galaxies found some with an almost complete lack of dark matter, whereas others consist of almost nothing but dark matter. Another oddity of this class of galaxies is their unusual abundance of bright globular clusters, something not observed in other types of galaxies.”

The ultra-diffuse galaxy GAMA 526784 appears as a tenuous patch of light in this image from the NASA/ESA Hubble Space Telescope. This wispy object resides in the constellation Hydra, roughly four billion light-years from Earth. ESA/Hubble & NASA, R. van der Burg; Acknowledgment: L. Shatz

This image was collected as part of a Hubble project to learn more about ultra-diffuse galaxies by imaging them at ultraviolet wavelengths. These galaxies can be as big as 60,000 light-years across, which is around the same size as our Milky Way galaxy, but contain just 1% of the number of stars as the Milky Way. This has led to them being called the “fluffiest” galaxies.

Recommended Videos

The low star densities of these galaxies mean it is hard to say how they have survived, as it would be expected that they would have been pulled apart. That’s where the dark matter comes in — researchers think that those galaxies with high levels of dark matter might be protected by these dark matter cushions.

But then, how to explain the very diffuse galaxies which contain almost no dark matter? Researchers still don’t have a good answer to this question. The only possibility so far is that two of these ultra-diffuse galaxies which are lacking in dark matter, NGC 1052-DF2 and NGC 1052-DF4, could have formed in the same group at the same time and that there might be something odd about the particular environment they formed in.

Editors' Recommendations

Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Get out the scrapers: Euclid space telescope is getting deiced

If you thought it was annoying to deice your car in the winter, then spare a thought for the engineers whose job it is to deice telescopes in space. The European Space Agency's (ESA) Euclid space telescope is currently undergoing a deicing procedure to remove a few layers of water ice that are less than a nanometer thick but enough to impede the telescope's highly accurate measurements.

Artist's impression of the Euclid mission in space. ESA. Acknowledgement: Work performed by ATG under contract for ESA

Read more
The expansion rate of the universe still has scientists baffled

The question of how fast the universe is expanding continues to confound scientists. Although it might seem like a fairly straightforward issue, the reality is that it has been perplexing the best minds in physics and astronomy for decades -- and new research using the James Webb Space Telescope and the Hubble Space Telescope doesn't make the answer any clearer.

Scientists know that the universe is expanding over time, but what they can't agree on is the rate at which this is happening -- called the Hubble constant. There are two main methods used to estimate this constant: one that looks at how fast distant galaxies are moving away from us, and one that looks at leftover energy from the Big Bang called the cosmic microwave background. The trouble is, these two methods give different results.

Read more
See planets being born in new images from the Very Large Telescope

Astronomers have used the Very Large Telescope to peer into the disks of matter from which exoplanets form, looking at more than 80 young stars to see which may have planets forming around them. This is the largest study to date on these planet-forming disks, which are often found within the same huge clouds of dust and gas that stars form within.

A total of 86 young stars were studied in three regions known to host star formation: Taurus and Chamaeleon I, each located around 600 light-years away, and Orion, a famous stellar nursery located around 1,600 light-years away. The researchers took images of the disks around the stars, looking at their structures for clues about how different types of planets can form.

Read more