Skip to main content

There’s an asteroid surprise in this week’s Hubble image

This week’s image from the Hubble Space Telescope shows a small but intriguing galaxy called UGC 7983, which is thought to be similar to some of the earliest galaxies that existed in the universe. Located 30 million light-years away in the constellation of Virgo, it looks like a hazy fuzz and is small enough to be considered a dwarf galaxy. Its unusual shape also make it a specific type called a dwarf irregular galaxy.

As well as the galactic star of the show, the frame of the image is littered with galaxies of all types that are visible in the background, as well as many nearby stars dotting the image that are located much closer than the background galaxies.

A host of astronomical objects throng this image from the NASA/ESA Hubble Space Telescope. Background galaxies ranging from stately spirals to fuzzy ellipticals are strewn across the image, and bright foreground stars much closer to home are also present, surrounded by diffraction spikes. In the centre of the image, the vague shape of the small galaxy UGC 7983 appears as a hazy cloud of light. UGC 7983 is around 30 million light-years from Earth in the constellation Virgo, and is a dwarf irregular galaxy — a type thought to be similar to the very earliest galaxies in the Universe.
A host of astronomical objects throng this image from the NASA/European Space Agency Hubble Space Telescope. Background galaxies ranging from stately spirals to fuzzy ellipticals are strewn across the image, and bright foreground stars much closer to home are also present, surrounded by diffraction spikes. In the center of the image, the vague shape of the small galaxy UGC 7983 appears as a hazy cloud of light. ESA/Hubble & NASA, R. Tully; CC BY 4.0

Astronomers are interested in studying dwarf galaxies like this one to learn about the formation of galaxies in the early universe. Researchers know that galaxies that formed when the universe was young, in the first few billion years after the Big Bang, were quite different from most of the galaxies we see today. And we know that dwarf irregular galaxies tend to have large amounts of dust and gas in them, making them hotbeds of star formation.

Dwarf galaxies were important during a period of the universe called the Epoch of Reionization, when early stars began to spread the first light throughout the universe. That’s why the James Webb Space Telescope is studying dwarf galaxies like the nearby Small Magellanic Cloud to learn more about how early stars and galaxies may have formed.

As well as being important for learning about the early universe, there’s another interesting feature to this image too. In the top left you can see a streak of light that was created by a small asteroid which happened to be passing by when the image was taken. If you look very closely, you can see the streak is broken up into four lines, which represent the four exposures that were combined to create the final image.

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Hubble spots a bright galaxy peering out from behind a dark nebula
The subject of this image taken with the NASA/ESA Hubble Space Telescope is the spiral galaxy IC 4633, located 100 million light-years away from us in the constellation Apus. IC 4633 is a galaxy rich in star-forming activity and also hosts an active galactic nucleus at its core. From our point of view, the galaxy is tilted mostly towards us, giving astronomers a fairly good view of its billions of stars.

A new image from the Hubble Space Telescope shows a galaxy partly hidden by a huge cloud of dust known as a dark nebula. The galaxy IC 4633 still shines brightly and beautifully in the main part of the image, but to the bottom right, you can see dark smudges of dust that are blocking the light from this part of the galaxy.

Taken using Hubble's Advanced Camera for Surveys (ACS) instrument, the image also incorporates data from the DECam instrument on the Víctor M. Blanco 4-meter Telescope, which is located in Chile. By bringing together data from the space-based Hubble and the ground-based DECam, astronomers can get a better look at this galaxy, located 100 million light-years away, and the dark dust partially obscuring it.

Read more
James Webb images capture the galactic winds of newborn stars
A team of astronomers used the NASA/ESA/CSA James Webb Space Telescope to survey the starburst galaxy Messier 82 (M82), which is located 12 million light-years away in the constellation Ursa Major. M82 hosts a frenzy of star formation, sprouting new stars 10 times faster than the Milky Way galaxy. Webb’s infrared capabilities enabled scientists to peer through curtains of dust and gas that have historically obscured the star formation process. This image from Webb’s NIRCam (Near-Infrared Camera) instrument shows the centre of M82 with an unprecedented level of detail. With Webb’s resolution, astronomers can distinguish small, bright compact sources that are either individual stars or star clusters. Obtaining an accurate count of the stars and clusters that compose M82’s centre can help astronomers understand the different phases of star formation and the timelines for each stage.

A stunning new pair of images from the James Webb Space Telescope show a new view of a familiar galaxy. Messier 82 is a famous starburst galaxy, full of bright and active star formation, and scientists are using Webb to study how stars are being born in the busy conditions at the center of the galaxy.

Astronomers used Webb's NIRCam instrument to observe the galaxy, and by splitting the resulting data into shorter and longer wavelengths, you can see different features which are picked out in the bustling, active region where stars are forming.

Read more
Stunning image shows the magnetic fields of our galaxy’s supermassive black hole
The Event Horizon Telescope (EHT) collaboration, who produced the first ever image of our Milky Way black hole released in 2022, has captured a new view of the massive object at the center of our Galaxy: how it looks in polarized light. This is the first time astronomers have been able to measure polarization, a signature of magnetic fields, this close to the edge of Sagittarius A*. This image shows the polarized view of the Milky Way black hole. The lines mark the orientation of polarization, which is related to the magnetic field around the shadow of the black hole.

The Event Horizon Telescope collaboration, the group that took the historic first-ever image of a black hole, is back with a new stunning black hole image. This one shows the magnetic fields twirling around the supermassive black hole at the heart of our galaxy, Sagittarius A*.

Black holes are hard to image because they swallow anything that comes close to them, even light, due to their immensely powerful gravity. However, that doesn't mean they are invisible. The black hole itself can't be seen, but the swirling matter around the event horizon's edges glows brightly enough to be imaged. This new image takes advantage of a feature of light called polarization, revealing the powerful magnetic fields that twirl around the enormous black hole.

Read more