Skip to main content

Gorgeous Webb image of Serpens Nebula shows a strange alignment

This image shows the centre of the Serpens Nebula as seen by the NASA/ESA/CSA James Webb Space Telescope’s Near-InfraRed Camera (NIRCam).
The Serpens Nebula, located 1,300 light-years from Earth, is home to a particularly dense cluster of newly forming stars (about 100,000 years old), some of which will eventually grow to the mass of our Sun. Webb’s image of this nebula revealed a grouping of aligned protostellar outflows (seen in the top left). These jets are identified by bright clumpy streaks that appear red, which are shock waves caused when the jet hits the surrounding gas and dust. NASA, ESA, CSA, STScI, K. Pontoppidan (NASA’s Jet Propulsion Laboratory), J. Green (Space Telescope Science Institute)

This stunning new image from the James Webb Space Telescope shows the famous Serpens Nebula, a dense star-forming region where new stars are being born amid clouds of dust and gas. Unlike some other nebulae, which are illuminated by radiation from stars that causes them to glow, this is a type called a reflection nebula, so it only shines due to the light that reflects from other sources.

As well as being visually striking, this image is also helping astronomers to learn about a special phenomenon related to newborn stars. When stars are first forming, they start as objects called protostars, and these protostars can give off extremely energetic jets of gas, which comes streaming off their north and south poles.

Recommended Videos

When this gas streaming off the protostar collides with nearby dust and gas, it creates shockwaves, which can be seen in the top left of the image. The red streaks of molecular hydrogen indicate these outflows, and one immediately noticeable thing about them is that they are all slanted at the same angle. This is the first time this phenomenon of aligned jets has been observed.

Normally, you would expect that a bunch of protostars would have outflows going in all different directions. So the fact these are all aligned suggests that there is something special going on in this region, which is affecting these young stars.

“Astronomers say there are a few forces that potentially can shift the direction of the outflows during this period of a young star’s life,” Webb scientists explain. “One way is when binary stars spin around each other and wobble in orientation, twisting the direction of the outflows over time.”

To learn more about the region, Webb scientists plan to use Webb’s NIRSpec instrument to understand what the cloud is made of, in addition to this data from Webb’s NIRCam instrument that was used to capture this image.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
Event Horizon Telescope can now take images of black holes that are 50% sharper
Illustration of the highest-resolution detections ever made from the surface of Earth

The Event Horizon Telescope project, the group that took the first-ever image of a black hole, has made another historic breakthrough, making the highest-ever resolution observations of space taken from the Earth's surface. The project uses facilities around the globe to turn the Earth itself into a giant observatory, which is capable of taking highly precise measurements of distant galaxies.

The latest observations made use of the Atacama Large Millimeter/submillimeter Array (ALMA), a large array of radio telescopes located in Chile, as well as other facilities in Spain, France, and Hawaii. To get higher-resolution images than previous observations, scientists weren't able to make the telescope bigger -- as it was already the size of the Earth -- so they observed at a higher frequency instead.

Read more
James Webb Telescope captures gorgeous galaxy with a hungry monster at its heart
Featured in this new image from the NASA/ESA/CSA James Webb Space Telescope is Messier 106, also known as NGC 4258. This is a nearby spiral galaxy that resides roughly 23 million light-years away in the constellation Canes Venatici, practically a neighbour by cosmic standards. Messier 106 is one of the brightest and nearest spiral galaxies to our own and two supernovae have been observed in this galaxy in 1981 and 2014.

A new image from the James Webb Space Telescope shows off a nearby galaxy called Messier 106 -- a spiral galaxy that is particularly bright. At just 23 million light-years away (that's relatively close by galactic standards), this galaxy is of particular interest to astronomers due to its bustling central region, called an active galactic nucleus.

The high level of activity in this central region is thought to be due to the monster that lurks at the galaxy's heart. Like most galaxies including our own, Messier 106 has an enormous black hole called a supermassive black hole at its center. However, the supermassive black hole in Messier 106 is particularly active, gobbling up material like dust and gas from the surrounding area. In fact, this black hole eats so much matter that as it spins, it warps the disk of gas around it, which creates streamers of gas flying out from this central region.

Read more
James Webb takes rare direct image of a nearby super-Jupiter
Artist’s impression of a cold gas giant orbiting a red dwarf. Only a point of light is visible on the JWST/MIRI images. Nevertheless, the initial analysis suggests the presence of a gaseous planet that may have properties similar to Jupiter.

Even with huge ground-based observatories and the latest technology in space-based telescopes, it's still relatively rare for astronomers to take an image of an exoplanet. Planets outside our solar system are so far away and so small and dim compared to the stars they orbit that it's extremely difficult to study them directly. That's why most observations of exoplanets are made by studying their host stars. Now, though, the James Webb Space Telescope has directly imaged a gas giant -- and it's one of the coldest exoplanets observed so far.

The planet, named Epsilon Indi Ab, is located 12 light-years away and has an estimated temperature of just 35 degrees Fahrenheit (2 degrees Celsius). The fact it is so cool compared to most exoplanets meant that Webb's sensitive instruments were needed to study it.

Read more