Deep Space Synergy: Webb, Hubble Telescopes Combine For Unprecedented Image Of Universe

NASA’s James Webb Space Telescope and the Hubble Space Telescope are providing astronomers with one of the most detailed and colorful images of the universe yet. They’ve focused their gaze on an enormous galaxy cluster named MACS0416, located about 4.3 billion light-years away from Earth, where two galaxy clusters are in the midst of a colossal collision. This event is significant as it offers a glimpse into the processes that lead to the formation of even larger galaxy clusters.

The combined image is remarkable for its panchromatic view, which melds visible and infrared light to reveal features of the universe that were previously undetectable. This includes not only the galaxies within the cluster but also those that lie far beyond it, as well as various celestial objects whose brightness changes over time. The latter phenomenon, likely a result of gravitational lensing, occurs when massive objects like galaxy clusters bend and amplify the light from more distant objects behind them.

This celestial tableau is part of a series from the Frontier Fields program, which began in 2014 with Hubble leading the charge to locate some of the faintest and youngest galaxies known. The James Webb Space Telescope enhances this exploration with its advanced infrared capabilities, enabling an even deeper look into the early universe.

This panchromatic view of galaxy cluster MACS0416 was created by combining infrared observations from NASA’s James Webb Space Telescope with visible-light data from NASA’s Hubble Space Telescope.
This panchromatic view of galaxy cluster MACS0416 was created by combining infrared observations from NASA’s James Webb Space Telescope with visible-light data from NASA’s Hubble Space Telescope. The resulting wavelength coverage, from 0.4 to 5 microns, reveals a vivid landscape of galaxies whose colors give clues to galaxy distances: The bluest galaxies are relatively nearby and often show intense star formation, as best detected by Hubble, while the redder galaxies tend to be more distant, or else contain copious amount of dust, as detected by Webb. The image reveals a wealth of details that are only possible to capture by combining the power of both space telescopes. (Credit: NASA, ESA, CSA, STScI, J. Diego (Instituto de Física de Cantabria, Spain), J. D’Silva (U. Western Australia), A. Koekemoer (STScI), J. Summers & R. Windhorst (ASU), and H. Yan (U. Missouri).

“We are building on Hubble’s legacy by pushing to greater distances and fainter objects,” says Rogier Windhorst, principal investigator of the PEARLS program, in a statement.

The colors in the image are not just for show; they carry significant meaning. The shortest wavelengths of light are shown as blue, and these often represent galaxies closer to us with active star formation. The longest wavelengths appear red, pointing to more distant galaxies. Some galaxies appear red due to cosmic dust, which absorbs the blue light from stars.

In an affectionate nod to the holiday season and the vibrant image, the cluster has been dubbed the “Christmas Tree Galaxy Cluster.” The research team, scouring through data, discovered 14 transients, or objects varying in brightness, some likely being individual or multiple-star systems magnified by gravitational lensing, while others are probable supernovae.

This side-by-side comparison of galaxy cluster MACS0416 as seen by the Hubble Space Telescope in optical light (left) and the James Webb Space Telescope in infrared light (right) reveals different details.
This side-by-side comparison of galaxy cluster MACS0416 as seen by the Hubble Space Telescope in optical light (left) and the James Webb Space Telescope in infrared light (right) reveals different details. Both images feature hundreds of galaxies, however the Webb image shows galaxies that are invisible or only barely visible in the Hubble image. This is because Webb’s infrared vision can detect galaxies too distant or dusty for Hubble to see. (Light from distant galaxies is redshifted due to the expansion of the universe.) The total exposure time for Webb was about 22 hours, compared to 122 hours of exposure time for the Hubble image. (Credit: NASA, ESA, CSA, STScI)

One transient, in particular, has caught the astronomers’ attention. A star system they’ve nicknamed “Mothra,” due to its immense brightness and magnification, is thought to be magnified by at least a factor of 4,000. This follows another significant find by the team, a lensed star they named “Godzilla”.

The prolonged visibility of Mothra, despite the necessary precise alignment for such magnification, suggests an additional object in the foreground cluster contributing to the effect. This object, potentially a faint globular star cluster, has been termed a “milli-lens” by the researchers.

Jose Diego, who led the study on this intriguing find, suggests that a globular star cluster might be responsible, though the exact nature of this lensing object remains a mystery.

This image of galaxy cluster MACS0416 highlights one particular gravitationally lensed background galaxy, which existed about 3 billion years after the big bang.
This image of galaxy cluster MACS0416 highlights one particular gravitationally lensed background galaxy, which existed about 3 billion years after the big bang. That galaxy contains a transient, or object that varies in observed brightness over time, that the science team nicknamed “Mothra.” Mothra is a star that is magnified by a factor of at least 4,000 times. The team believes that Mothra is magnified not only by the gravity of galaxy cluster MACS0416, but also by an object known as a “milli-lens” that likely weighs about as much as a globular star cluster. (Credit: NASA, ESA, CSA, STScI, J. Diego (Instituto de Física de Cantabria, Spain), J. D’Silva (U. Western Australia), A. Koekemoer (STScI), J. Summers & R. Windhorst (ASU), and H. Yan (U. Missouri).)

These findings, poised to advance our understanding of the universe, are documented in two scientific papers, one accepted for publication in The Astrophysical Journal and the other already published in Astronomy & Astrophysics. The data from Webb was acquired as part of the PEARLS GTO program 1176, marking yet another milestone in space exploration and astrophysics.


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