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The massive MJ0308 galaxy cluster in the foreground produces a gravitational lensing effect, which causes multiple images of SN Ares to appear. . | Credit: NASA\/ESA\/CSA\/image processing: Gavin Farley<\/p>\n
Two incredibly rare supernovas that erupted billions of years ago provide a unique opportunity to explain cosmology’s biggest mystery \u2014 How fast is the universe expanding?<\/p>\n
But there’s a twist: Even though astronomers have already observed these exploding stars, we will have to wait up to 60 years for their light to reach us again.<\/p>\n
A phenomenon called gravitational lensing has split the light from these obliterated stars into multiple images, each of which travels a different path through space-time to reach us. As a result, researchers will one day be able to measure the delay between these ghostly images to offer an unprecedented constraint on the expansion rate of the universe \u2014 a problem that has long bedeviled scientists, as the universe appears to be expanding at different rates depending on where they look.<\/p>\n
Conor Larison<\/a>, a postdoctoral researcher at the Space Telescope Science Institute, presented the discovery of the two gravitationally lensed supernovas, named SN Ares and SN Athena, at a news conference at the 247th meeting of the American Astronomical Society<\/a> in Phoenix.<\/p>\n Cosmic magnifying glasses reveal the invisible<\/p>\n These supernova observations are among the first results from the Vast Exploration for Nascent, Unexplored Sources (VENUS) treasury program. The VENUS survey employs the James Webb Space Telescope<\/a> (JWST) to observe 60 dense galaxy clusters, which act as cosmic lenses that split and focus the light from extremely distant, otherwise invisible sources such as supernovas.<\/p>\n Combined data from the Hubble Space Telescope and the James Webb Space Telescope capture the gravitationally lensed supernovas SN Ares and SN Athena. The researchers can predict when and where their images will reappear in the future. | Credit: NASA\/ESA\/CSA\/image processing: Gavin Farley<\/p>\n This cosmic phenomenon, called gravitational lensing, is a direct consequence of gravity’s effect on the fabric of space-time<\/a> and was first proposed by Albert Einstein in his theory of relativity<\/a>. It occurs when a massive celestial object, like a galaxy cluster, bends the light<\/a> from a more distant source that’s located behind it, thus magnifying the object.<\/p>\n “Strong gravitational lensing transforms galaxy clusters into nature’s most powerful telescopes,” Seiji Fujimoto<\/a>, principal investigator of the VENUS program and an astrophysicist at the University of Toronto, said in a statement<\/a>. “VENUS was designed to maximally find the rarest events in the distant Universe, and these lensed [supernovas] are exactly the kind of phenomena that only this approach can reveal.”<\/p>\n SN Ares is the first lensed supernova discovered via the VENUS program. The explosion occurred almost 10 billion years ago, when the universe was around one-third its current age. The warp in space-time caused by a foreground galaxy cluster, MJ0308, split the light from SN Ares into three images.<\/p>\n One image has already reached our telescopes. But the light from the other two images passes much closer to the massive center of MJ0308, so it experiences a much greater slowdown due to gravitational time dilation<\/a>. Therefore, the other two images of SN Ares will arrive in approximately 60 years \u2014 an unprecedented delay.<\/p>\n “Such a long anticipated delay between images of a strongly lensed supernova has never been seen before and could be the chance for a predictive experiment that could put unbelievably precise constraints on cosmological evolution,” Larison said in a statement<\/a>.<\/p>\n In the meantime, a delayed image of SN Athena, which erupted as a supernova when the universe was about half its current age, is anticipated to arrive in the next one to two years. Although it won’t be as cosmologically precise as its mythological half brother Ares, Athena will reveal how accurate our predictive powers have become.<\/p>\n A sorely needed natural experiment<\/p>\n The predicted reappearance of these supernovas, compared with their actual arrival times in the future, will provide precise constraints on the expansion rate of the universe, a value known as the Hubble constant<\/a>.<\/p>\n Curiously, when cosmologists measure the Hubble constant, they obtain different values<\/a> based on the measurement method \u2014 a disparity known as the Hubble tension<\/a>. Calculations based on the cosmic microwave background \u2014 the oldest light in the universe, emitted when the cosmos was only 380,000 years old \u2014 yield a universal expansion rate of 67 kilometers per second per megaparsec.<\/p>\n Yet calculations based on the Hubble Space Telescope’s observations of pulsating Cepheid stars<\/a>, used as “standard candles” for their specific luminosity patterns, yield a value of 73 kilometers per second per megaparsec.<\/p>\n Within the observable sphere of the cosmos, the delayed images from SN Ares and SN Athena may help reconcile the Hubble tension.<\/p>\n “If we can measure the difference in when these images arrive, we recover a measurement of the physical scale of the lensing system which spans the Universe between the supernova and us here on Earth,” Larison told Live Science via email. “Any distance measurement we can make like this in the Universe tells us how the Universe has been evolving over cosmic time, as these distances directly depend on this evolution.”<\/p>\n Equally importantly, the lensed supernovas allow astronomers to make this measurement in a “single, self-consistent step,” Larison added.<\/p>\n The time delays from these supernovas also allow an independent measurement method \u2014 unrelated to the cosmic microwave background or standard candles like Cepheid stars \u2014 at a time when such a measurement is “sorely needed” to test “possible unknown systematics\u201d governing cosmological expansion.<\/p>\n From Big Bang to big mystery<\/p>\n Coincidentally, 60 years have passed since the first formal suggestion to use lensed supernovas as a tool to explore the universe’s expansion. However, fewer than 10 such supernovas<\/a> had been discovered before the VENUS program observations.<\/p>\n “Since VENUS started last July, we have discovered 8 new lensed supernovae over 43 observations, almost doubling the known sample in a remarkably fast time frame,” Larison told Live Science. “It seems that, although lensed supernovae are certainly rare, the real limitation has been in observing capabilities. It is really only with JWST that we are achieving the depth and wavelength coverage necessary to find these en masse, which is exactly what VENUS was designed to do.”<\/p>\n related stories<\/p>\n \u2014James Webb telescope spots Milky Way’s long-lost ‘twin’ \u2014 and it is ‘fundamentally changing our view of the early universe’<\/a><\/p>\n \u2014‘I was astonished’: Ancient galaxy discovered by James Webb telescope contains the oldest oxygen scientists have ever seen<\/a><\/p>\n \u2014‘Totally unexpected’ galaxy discovered by James Webb telescope defies our understanding of the early universe<\/a><\/p>\n As a result, lensed supernovas may be the most exciting prospects in long-baseline cosmology, the study of how the universe has changed throughout its 13.8 billion years of existence.<\/p>\n The answer is up in the air; there’s no guarantee that the expansion of the universe will continue to accelerate, especially as dark energy may be weakening<\/a>. If it is, then the current expansion of the cosmos could one day become a contraction, having profound consequences on the ultimate fate of the universe.<\/p>\n![\"Two](\"https:\/\/www.newsbeep.com\/us\/wp-content\/uploads\/2026\/02\/e1a7a6dc9c145ac4b48f462e067b1f93.jpeg\"\/)
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