Skip to main content

Hubble images the spooky Spider Galaxy

This week’s image from the Hubble Space Telescope shows an irregular galaxy, the spindly arms and clawed shape of which has led to it being named the Spider Galaxy. Located 30 million light-years away, the galaxy also known as UGC 5829 is an irregular galaxy that lacks the clear, orderly arms seen in spiral galaxies like the Milky Way.

This image from the NASA/ESA Hubble Space Telescope shows the irregular galaxy UGC 5829.
This image from the NASA/ESA Hubble Space Telescope shows the irregular galaxy UGC 5829. ESA/Hubble & NASA, R. Tully, M. Messa

As it is diffuse and faint, this galaxy has not often been studied. It does have a similarly named partner galaxy, the Spiderweb Galaxy, or MRC 1138-262, which has been more extensively studied — including by Hubble. The Spiderweb Galaxy is located 300 times further from Earth than the Spider Galaxy, but has been a target for research looking into how smaller galaxies merge to create one larger galaxy.

As for the Spider Galaxy, this image is made up of data from two different research programs. “The data in this image come from two Hubble observing programs. The first used Hubble’s Advanced Camera for Surveys to look at relatively nearby galaxies in an effort to build color versus brightness diagrams of the stars in these galaxies. Each observation only took one Hubble orbit (about 95 minutes) but provided a valuable archival record of the types of stars in different galaxies and therefore different environments,” Hubble scientists explain in a statement.

“The second program used Hubble’s Wide Field Camera 3 to look at star clusters in dwarf galaxies. Their observations leveraged Hubble’s ultraviolet capabilities, along with its ability to see fine details, to better understand the environment where stars form in dwarf galaxies. The star-forming regions of UGC 5829 are readily visible in this image as bright-pink nebulae or clouds.”

While Hubble’s instruments operate primarily in the visible light range, which is the same range of wavelengths that can be seen by the human eye, they do also have the ability to look in some ultraviolet and infrared wavelengths. Using these different wavelengths allows scientists to observe features that would otherwise be hard to detect, as seen in this ultraviolet image of Jupiter taken by Hubble that shows off the planet’s great red spot.

You can get an idea of what the same object looks like at different wavelengths by comparing objects viewed by Hubble‘s visible light instruments with those viewed by the James Webb Space Telescope’s infrared instruments.

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