American astronomers have stumbled across one of the farthest quasars
ever seen. The light from the quasar, which has a red shift of 4.21, was
emitted when the Universe was less than a fifth of its current size.
Donald Schneider of the Institute for Advanced Study in Princeton, New
Jersey, Maarten Schmidt of the California Institute of Technology in Pasadena,
and James Gunn of Princeton University discovered the object while searching
for distant quasars with the 200-inch telescope on Palomar Mountain in California.
On an image of the constellation of Pisces, they found an object they thought
might be a distant quasar.
But when they obtained better spectra, they found that the suspicious
object was only a star in our Galaxy. Beside the star, however, was another
object whose spectrum had been recorded by chance. This second object turned
out to be a quasar with an extremely large red shift.
The new quasar is one of the most distant known. In the time its light
has been travelling to the Earth, the Universe has become 5.21 times larger,
stretching the wavelength of the quasar’s light by the same factor.
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To date, astronomers have published reports of only 15 other quasars
with a red shift greater than 4. The farthest-known quasar, discovered by
Schneider’s team in 1991, has a red shift of 4.897. But of all known quasars
with red shifts greater than 4, the new one is the faintest. It is 2.5 million
times dimmer than any object visible to the naked eye.
In 1987, another group of astronomers also accidentally discovered a
quasar with a red shift greater than 4. Schneider con-siders it amazing
that more than 10 per cent of the 16 known quasars with red shifts greater
than 4 have been found by accident as astronomers have mounted intense searches
for such objects.
Schneider and his colleagues will report their discovery in the March
issue of The Astronomical Journal.
![Astronomers have long known that understanding how star clusters come to be is key to unlocking other secrets of galactic evolution. Stars form in clusters, created when clouds of gas collapse under gravity. As more and more stars are born in a collapsing cloud, strong stellar winds, harsh ultraviolet radiation and the supernova explosions of massive stars eventually disperse the cloud, and their light can bear down on other star-forming regions in the galaxy. This process is called stellar feedback, and it means that most of the gas in a galaxy never gets used for star formation. Researching how star clusters develop can answer questions about star formation at a galactic scale. Now, the state of the art has been further developed with both Hubble and Webb working together to provide a broad-spectrum view of thousands of young star clusters. An international team of astronomers has pored over images of four nearby galaxies from the FEAST observing programme (#1783), trying to solve this mystery. Their results show that it is the most massive star clusters that clear away their gaseous shroud the fastest, and begin lighting their galaxy the earliest. The team identified nearly 9000 star clusters in the four galaxies in different evolutionary stages: young clusters just starting to emerge from their natal clouds of gas, clusters that had partially dispersed the gas (both from Webb images), and fully unobstructed clusters visible in optical light (found in Hubble images). With Webb???s ability to peer inside the gas clouds, they were able to then estimate the mass and age of each cluster from its light spectrum. This image shows a section of one of the spiral arms of Messier 51 (M51), one of the four galaxies studied in this work, as seen by Webb???s Near-Infrared Camera (NIRCam). The thick clumps of star-forming gas are shown here in red and orange, representing infrared light emitted by ionised gas, dust grains, and complex molecules such as polycyclic aromatic hydrocarbons (PAHs). Within these gas complexes, each tens or hundreds of light years across, Webb reveals the dense, extremely bright clusters of massive stars that have just recently formed. The countless stars strewn across the arm of the galaxy, many of which would be invisible to our eyes behind layers of dust, are also laid bare in infrared light. [Image description: A large, long portion of one of the spiral arms in galaxy M51. Red-orange, clumpy filaments of gas and dust that stretch in a chain from left to right comprise the arm. Shining cyan bubbles light up parts of the gas clouds from within, and gaps expose bright star clusters in these bubbles as glowing white dots. The whole image is dotted with small stars. A faint blue glow around the arm colours the otherwise dark background.]](https://images.newscientist.com/wp-content/uploads/2026/05/13114322/SEI_296271016.jpg)


