Skip to main content

James Webb is explaining the puzzle of some of the earliest galaxies

This image shows a small portion of the field observed by NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) for the Cosmic Evolution Early Release Science (CEERS) survey. It is filled with galaxies. The light from some of them has traveled for over 13 billion years to reach the telescope.
This image shows a small portion of the field observed by NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) for the Cosmic Evolution Early Release Science (CEERS) survey. It is filled with galaxies. The light from some of them has traveled for over 13 billion years to reach the telescope. NASA, ESA, CSA, Steve Finkelstein (UT Austin)

From practically the moment it was turned on, the James Webb Space Telescope has been shaking cosmology. In some of its very earliest observations, the telescope was able to look back at some of the earliest galaxies ever observed, and it found something odd: These galaxies were much brighter than anyone had predicted. Even when the telescope’s instruments were carefully calibrated over the few weeks after beginning operations, the discrepancy remained. It seemed like the early universe was a much busier, brighter place than expected, and no one knew why.

This wasn’t a minor issue. The fact early galaxies appeared to be bigger or brighter than model predicted meant that something was off about the way we understood the early universe. The findings were even considered “universe breaking.” Now, though, new research suggests that the universe isn’t broken — it’s just that there were early black holes playing tricks.

In the blackness of space, a bright object in the center of view is surrounded and partly obscured by a dark cloudArtist illustration of a black hole surrounded by extremely thick clouds of gas and dust
Artist illustration of a black hole surrounded by extremely thick clouds of gas and dust NASA/JPL-Caltech

The reason bright galaxies were surprising was that the obvious explanation would we that there were more stars, or brighter stars, in each galaxy. But stars can only appear and grow so fast, depending on the amount of matter around them. Trying to explain how galaxies could have grown to gargantuan proportions was difficult. Now, it seems that some of this extra brightness was caused by black holes, which gobble up nearby material. As they feed, that nearby material heats up and glows, giving off light that makes the galaxies brighter.

Recommended Videos

According to a new paper in The Astronomical Journal, this explains some — but not all — of that extra brightness. “We are still seeing more galaxies than predicted, although none of them are so massive that they ‘break’ the universe,” explained lead researcher Katherine Chworowsky of the University of Texas at Austin.

The research used data from the James Webb CEERS Survey, which identified some of these earliest galaxies. When researchers removed galaxies that were very red and compact from the analysis, based on the fact the redness could indicate black holes at work, the galaxies that are left behind fit more into what was expected.

“So, the bottom line is there is no crisis in terms of the standard model of cosmology,” said Steven Finkelstein, leader of CEERS. “Any time you have a theory that has stood the test of time for so long, you have to have overwhelming evidence to really throw it out. And that’s simply not the case.”

It isn’t a matter of case closed though. Even though the remaining galaxies aren’t wildly bright any more, they are still much more numerous than expected. There are roughly twice as many massive galaxies found as had been predicted. That does still suggest that early stars were forming faster than they do today, for reasons we don’t understand yet.

“And so there is still that sense of intrigue,” Chworowsky said. “Not everything is fully understood. That’s what makes doing this kind of science fun, because it’d be a terribly boring field if one paper figured everything out, or there were no more questions to answer.”

Please enable Javascript to view this content

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
James Webb spots ancient Spiderweb cluster that’s 10 billion years old
This image shows the Spiderweb protocluster as seen by Webb’s NIRCam (Near-InfraRed Camera).

A new image from the James Webb Space Telescope shows thousands of glittering galaxies that it spied by peering through clouds of dust and using its infrared instruments to reveal what lies beneath. In the center of the image is the Spiderweb protocluster, which is a group of galaxies in the early stages of forming a "cosmic city."

The light from the Spiderweb has been traveling for an astonishing 10 billion years to reach us, so looking at it is like looking back in time to the early stages of the universe. Astronomers are interested in studying this cluster of over 100 galaxies interacting together because it shows how galaxies clumped together to form groups when the universe was still young.

Read more
Webb and Hubble snap the same object for two views of one galaxy
Featured in this NASA/ESA/CSA James Webb Space Telescope Picture of the Month is the spiral galaxy NGC 2090, located in the constellation Columba. This combination of data from Webb’s MIRI and NIRCam instruments shows the galaxy’s two winding spiral arms and the swirling gas and dust of its disc in magnificent and unique detail.

With all the excitement over the last few years for the shiny and new James Webb Space Telescope, it's easy to forget about the grand old master of the space telescopes, Hubble. But although Webb is a successor to Hubble in some ways, with newer technology and the ability to see the universe in even greater detail, it isn't a replacement. A pair of new images shows why: with the same galaxy captured by both Webb and Hubble, you can see the different details picked out by each telescope and why having both of them together is such a great boon for scientists.

The galaxy NGC 2090 was imaged by Webb, shown above, using its MIRI and NIRCam instruments. These instruments operate in the mid-infrared and near-infrared portions of the electromagnetic spectrum respectively, which is why the arms of this galaxy appear to be glowing red. These arms are made of swirling gas and dust, and within them are compounds called polycyclic aromatic hydrocarbons that glow brightly in the infrared. The blue color in the center of the galaxy shows a region of young stars burning hot and bright.

Read more
Stunning view of the Sombrero Galaxy captured by James Webb
The NASA/ESA/CSA James Webb Space Telescope recently imaged the Sombrero galaxy with its MIRI (Mid-Infrared Instrument), resolving the clumpy nature of the dust along the galaxy’s outer ring. The mid-infrared light highlights the gas and dust that are part of star formation taking place among the Sombrero galaxy’s outer disk. The rings of the Sombrero galaxy produce less than one solar mass of stars per year, in comparison to the Milky Way’s roughly two solar masses a year. It’s not a particular hotbed of star formation. The Sombrero galaxy is around 30 million light-years from Earth in the constellation Virgo.

A new image from the James Webb Space Telescope shows a stunning and fashionable sight: the Sombrero Galaxy, named for its resemblance to the traditional Mexican hat. With its wide, flat shape reminiscent of the hat's wide brim, the galaxy, also known as Messier 104, has outer rings that are clearly visible for the first time.

The Sombrero Galaxy is located 30 million light-years away, in the constellation of Virgo, and it has been previously imaged by the Hubble Space Telescope. But while in the Hubble image, the galaxy appears as an opaque, pale disk, in the new Webb image you can see an outer blue disk, with a small bright core right at the center.

Read more