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Astronomers Devise a New Way to Measure Cosmic Expansion with Lensed Supernovae
Superliminous supernovae are miraculous events. For astronomers, they also provide a vital tool for measuring cosmic distances and the rate at which the Universe is expanding. As part of the Cosmic Distance Ladder, these incredibly bright stellar explosions are the “standard candles” for objects billions of light-years away. In a rare event, researchers from the University of Munich, using the Large Binocular Telescope (LBT) in Arizona, witnessed a superluminous supernova 10 billion light-years away that was far brighter than most explosions of its kind.
What was especially amazing about this supernova was that it appeared five times in the night sky due to gravitational lensing by two foreground galaxies. These galaxies bent the path of the supernova’s light, causing it to take different paths. Because these paths have different lengths, the light appeared in different places around the galaxies at different times. By measuring the time delays between the multiple images, the researchers were able to obtain measurements of how fast the Universe is expanding – aka the Hubble-Lemaitre Constant.
The team consisted of researchers from the Technical University of Munich (TUM), the Max Planck Institute for Astrophysics (MPG), the Harvard & Smithsonian Center for Astrophysics (CfA), the E.O. Lawrence Berkeley National Laboratory, ETH Zurich, the Research Center for the Early Universe (RESCEU), the Cosmic Dawn Center (DAWN), the Ulugh Beg Astronomical Institute, the Chinese Academy of Sciences (CAS), Institute of Space Sciences (ICE, CSIC), the Excellence Cluster ORIGINS, the National Astronomical Observatory of Japan (NAOJ), the European Southern Observatory (ESO), the Space Telescope Science Institute (STScI), and multiple universities.
*Large Binocular Telescope on Mount Graham in Arizona, USA. Credit & ©: Dr. Christoph Saulder/MPE*
The paper describing their observations has been accepted for publication in Astronomy & Astrophysics
Only a few such measurements have been attempted to date because gravitationally lensed supernovae are so rare. It is also a challenging process, where astronomers must determine the masses of the lensing galaxies because this dictates how strongly the light from the background object is bent. To determine the masses of the two galaxies, the team obtained images with the LBT, using its two 8.4-meter (27.5 ft) mirrors and an adaptive optics system. The observations revealed two foreground lens galaxies at the center surrounded by five bluish images of the supernova explosion, making it look like fireworks!
Sherry Suyu, Associate Professor of Observational Cosmology at TUM and Fellow at the Max Planck Institute for Astrophysics, explained in an MPG press release:
We nicknamed this supernova SN Winny, inspired by its official designation SN 2025wny. It is an extremely rare event that could play a key role in improving our understanding of the cosmos. The chance of finding a superluminous supernova perfectly aligned with a suitable gravitational lens is lower than one in a million. We spent six years searching for such an event by compiling a list of promising gravitational lenses, and in August 2025, SN Winny matched exactly with one of them.
The image came as a surprise to the team since galaxy-scale lens systems normally produce only two or four copies. Using the positions of all five, junior researchers Allan Schweinfurth (TUM) and Leon Ecker (LMU) built the first model of the lens mass distribution. Said Allan Schweinfurth:
Until now, most lensed supernovae were magnified by massive galaxy clusters, whose mass distributions are complex and hard to model. SN Winny, however, is lensed by just two individual galaxies. We find overall smooth and regular light and mass distributions for these galaxies, suggesting that they have not yet collided in the past despite their close apparent proximity. The overall simplicity of the system offers an exciting opportunity to measure the Universe’s expansion rate with high accuracy.
This, in turn, could help astronomers and cosmologists relieve the ongoing issue of the Hubble Tension. To date, scientists have relied primarily on two methods to measure cosmic expansion: the Cosmic Distance Ladder and measurements of the Cosmic Microwave Background (CMB). The former is the local method, combining parallax, supernovae, and redshift measurements of bright objects to establish distances one step at a time. Since every step is dependent on the previous one, even small errors can add up and affect the final result.
In contrast, CMB measurements look back to the beginning of cosmic time by examining the “relic radiation” left over from the Big Bang. This approach is highly precise and relies on models of the early Universe to calculate its current rate of expansion. It relies heavily on assumptions about how the Universe evolved, however, which are still subject to debate. This study presents a third possible method in which astronomers use gravitationally lensed supernovae and measure the time delays between the multiple copies of the same image.
By calculating the mass distribution of the lensing galaxy, scientists can directly calculate the Hubble-Lemaitre Constant. “Unlike the cosmic distance ladder, this is a one-step method, with fewer and completely different sources of systematic uncertainties,” said Stefan Taubenberger, a leading member of Professor Suyu’s team and first author on their study.
Meanwhile, astronomers worldwide are observing SN Winny in detail with ground-based and space-based telescopes. Their results will provide new insights into cosmic expansion that could help resolve the Hubble Tension.
Further Reading: MPG
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Surveillance Prices. Hidden Fees. Shifting Costs. This Madness Must Stop.
It’s time to combat commercial surveillance with stronger laws on fair pricing.
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Dry Martian Meteorite Reveals Early Water in Mars’s Crust
Billions of years ago, Mars was hypothesized to have been a habitable world with flowing liquid water and the potential for life. But directly studying its ancient past is currently limited to orbiters and rovers, as scientists have yet to obtain direct samples from Mars. However, meteorites have been found on Earth to have potentially originated from Mars during large impacts that flung chunks of the Red Planet into space, eventually being grabbed by Earth’s gravity and crashing into the Earth’s surface.
Now, an international team of scientists might be one step closer to piecing together Mars’ watery ancient past, and specifically how much water could have flowed across the Red Planet’s surface long ago. In findings recently published in the Geophysical Research Letters, a collaborative team of researchers led by the Technical University of Denmark investigated an intriguing meteorite with an even more intriguing name, “Black Beauty”, with the scientific designation of Northwest Africa 7034 (NWA 7034). What makes Black Beauty so intriguing is its designation as the only known meteorite that originated from the crust of Mars, having been blasted away during an impact billions of years ago, as Black Beauty is estimated to be about 4.4 to 4.5 billion years old.
Using a combination of X-ray and neutron tomography, the researchers analyzed Black Beauty with the goal of ascertaining if the ancient meteorite contained traces of water, also called hydrous materials in the scientific community. While X-ray tomography is used to identify the densest parts of Black Beauty while focusing on iron and silicon, neutron tomography was used to identify that previous “holes” found by normal X-rays were actually hydrous materials.
“Neutrons are particularly sensitive to hydrogen,” said Dr. David Mannes, who is a scientist at the Paul Scherrer Institute (PSI), a co-author on the study. Dr. Mannes collaborated with fellow study co-author, Dr. Anders Kaestner, on the neutron tomography at PSI. “In combination with X-ray tomography, we were not only able to detect tiny hydrated minerals, but also, for the first time, visualize larger, macroscopic hydrogen deposits.”
Essentially, the researchers identified that early Mars contained a water reservoir large enough to engage with the Martian surface and crust, resulting in water deposits into crustal rocks that eventually became Black Beauty. The researchers also note these materials are similar to materials found in Jezero Crater by NASA’s Perseverance rover. Therefore, Black Beauty continues to add a growing pile of evidence that Mars was a much warmer and wetter planet billions of years ago.
While Black Beauty has revealed intricate details regarding ancient Mars and its watery past, arguably the most famous meteorite from Mars is the Allan Hills 84001 (ALH84001) meteorite, which was recovered in Antarctica on December 27, 1984. However, it wasn’t until 1996 before scientists discovered it was potentially from Mars, as ALH84001 had initially been designated as an asteroid chunk, which are frequently discovered on Earth. Once scientists studied ALH84001, they discovered it contained unique structures they hypothesized could indicate signs of ancient Martian life.
While their 1996 study published in Science gained worldwide attention, including an official address from President Bill Clinton, the scientific community was quick to claim these features could have formed from non-biological processes. Regardless of its specific origin, both Black Beauty and ALH84001 demonstrate the importance of bringing back samples from Mars to reduce relying on ancient meteorites.
Unfortunately, the long-anticipated NASA-ESA Mars Sample Return mission was canceled by Congress due to ballooning costs, meaning all the sample tubes that NASA’s Perseverance rover has been depositing on the Martian surface is potentially for nought. For now, scientists have to rely on meteorites to unlock the secrets of ancient Mars, but China’s planned Tianwen-3 might be the first to return Mars samples to Earth sometime next decade.
What new insights into the “Black Beauty” meteorite and ancient Mars will researchers make in the coming years and decades? Only time will tell, and this is why we science!
As always, keep doing science & keep looking up!
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Darth Vader to San Diego City Council: The Emperor liked Flock cameras

In a galaxy not so far, far away — well, in San Diego — the controversial police use of Flock surveillance cameras that photograph and record license plate numbers has at least one prominent supporter.
Darth Vader.
“The Emperor is a fan of Flock,” a person wearing a full-body costume of the “Star Wars” villain told a committee of the San Diego City Council this week, referencing Darth Vader’s evil, power-hungry boss, Emperor Palpatine, ruler of the Galactic Empire.
“And we must continue utilizing Flock technologies so that we can follow and surveil the Rebel scum as they move from playground to playground, from playground to pool, from pool to gymnasium,” the person said during public comments at a Wednesday meeting of the Public Safety and Livable Neighborhoods Committee.
The cosplayer, who breathed heavily into the microphone a la the movie villain, was formally called to the podium by the name Darth Vader.
It was a stance a bit out of sync with silver screen Darth, who famously told an Imperial stooge who got too braggadocious about the Empire’s planet-destroying Death Star: “Don’t be too proud of this technological terror you’ve constructed.”
But in a twist not quite as big as Darth telling Luke Skywalker he was his daddy, the bad guy in black showed up to the government meeting in San Diego to be sarcastic about Flock cameras. He didn’t actually support them at all.
Nor, it turns out, did a lot of people in the audience, who hoisted signs from the American Civil Liberties Union reading: “Get the Flock Out!”
The cosplayer’s sarcastic endorsement comes as Flock Safety — the company whose more than 120,000 artificial intelligence-enabled license plate readers can be found along roadsides in every state but Alaska — comes under increasing scrutiny by lawmakers, civil rights groups and members of the public who have expressed privacy concerns.
Dozens of mostly smaller cities have deactivated their Flock cameras or ended contracts with the company over concerns that it provides data to the Trump administration that can be used to track down immigrants for deportation.
And recent reporting by the Washington Post uncovered at least 50 instances nationwide in which law enforcement officials were accused of misusing their access to the cameras, largely to stalk former romantic partners or citizens.
Last month, the Los Angeles Police Department announced it was pausing its relationship with Flock, but police officials later said they were in the process of negotiating a new deal with the company that would include more data-sharing safeguards.
Both Mayor Karen Bass and her opponent in the November mayoral election, Councilmember Nithya Raman, have said the city should stop working with Flock.
The company, whose automated license readers document plate data as vehicles drive past, says it has partnerships with 5,000 law enforcement agencies nationwide.
Amid public backlash, the company announced this month several platform changes, including a shorter data retention window and audit tools for law enforcement customers intended to flag abnormal search behavior.
In San Diego, Flock cameras are affixed to streetlights in about 500 locations, according to the 2025 Annual Surveillance Report by the San Diego Police Department.
In addition to plate numbers, the report states, the cameras record the date, time and location of the scan, as well as vehicle descriptors such as make, model and color.
The information is encrypted and transmitted to a secure database that can be accessed only by San Diego police personnel, according to the department. The data is saved for 30 days and automatically deleted unless it is being used as evidence in an active investigation, according to the department.
The report says San Diego police officers last year conducted more than 244,000 investigative searches of the data and that it played a “key role in advancing 361 cases.”
The data, per the department, helped officers recover 259 stolen vehicles and find four missing people, as well as aiding the investigations of around nine of the city’s 28 homicides in 2025.
In a presentation to the Public Safety and Livable Neighborhoods Committee in November, San Diego Police Capt. Charles Lara said the technology “has been truly game-changing for our department, especially while we continue to operate with hundreds of officers below ideal staffing levels.”
Lt. Kristopher McAndrew said the “vast majority of data is never viewed” and that the police department does not share data with federal or out-of-state law enforcement agencies or private entities.
At the meeting this week, Darth Vader — who, like everyone else who approached the podium, was allotted two minutes of speaking time — said of the Flock camera system: “I need this so I can stalk my ex-girlfriend.”
He asked the City Council members how residents will continue to trust them when they continue to vote “for surveillance technology that imprisons them.”
He advised one of the council members to work on her Jedi mind tricks to fool them, then raised his hand to the audience, saying: “Do it like this.”
“This technology will help us find the Rebel scum and their hidden base on Hoth,” he said, referencing the ice planet in the “Star Wars” universe. “This technology will help us find Luke Skywalker as he traverses the universe in his X-wing. This technology is a necessary, necessary force.”
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