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Illinois and UChicago Physicists Develop a New Method for Measuring Cosmic Expansion
For about a century, scientists have known that the Universe is in a state of constant expansion. In honor of the scientists who definitively showed this, this expansion has come to be known as the Hubble Constant (or Hubble-Lemaitre Constant). Today, scientists use two main techniques to measure the rate of expansion: the Cosmic Microwave Background (CMB) and the Cosmic Distance Ladder. The former relies on redshift measurements of the CMB, the relic radiation left over from the Big Bang, while the latter relies on parallax and redshift measurements using variable stars and supernovae (aka “standard candles”).
The only problem is that the two methods don’t agree, leading to what is known as the “Hubble Tension.” This problem is considered one of the greatest cosmological mysteries facing scientists today. Luckily, new methods are emerging that could help resolve this “tension” and bring order to the Standard Model of Cosmology. In a recent study, a team of astrophysicists, cosmologists, and physicists from the University of Illinois and the University of Chicago has proposed a new method using the tiny ripples in spacetime known as gravitational waves (GWs).
The study was led by Bryce Cousins, an NSF Graduate Research Fellow from the Institute of Gravitation and the Cosmos (IGC) at the University of Illinois Urbana-Champaign. He was joined by multiple colleagues from the IGC, as well as researchers from the Kavli Institute for Cosmological Physics and the Enrico Fermi Institute at the University of Chicago. Their study, “Stochastic Siren: Astrophysical gravitational-wave background measurements of the Hubble constant,” appeared on Jan. 16th in the Physical Review Letters.
Scientists hoping to resolve the Hubble Tension have proposed several solutions, ranging from Early Dark Energy (EDE) and interactions between Dark Matter (DM) and neutrinos to evolving dark-energy dynamics. In recent years, the discovery of gravitational waves has also emerged as a means of resolving the Tension by providing a new way to measure cosmic expansion. Originally predicted by Einstein’s Theory of General Relativity, gravitational waves are ripples caused in the fabric of spacetime caused by the merger of massive objects (neutron stars and/or black holes).
They were first confirmed in 2016 by scientists at the Laser Interferometer Gravitational wave Observatory (LIGO). Thanks to upgraded instruments and international cooperation, the LIGO-Virgo-KAGRA (LVK) collaboration has detected more than 300 GW events. In that time, astronomers have found ways to use events to explore cosmological phenomena, including measuring the expansion of the cosmos. In the current research, the team found a way to improve these measurements by leveraging the gravitational-wave background (GWB), which is caused by astrophysical collisions that the LVK network is not yet sensitive enough to detect.
They call it the “stochastic standard siren” method, since the collisions that make up the gravitational-wave background occur stochastically. Daniel Holz, a UChicago Professor and study co-author, explained in a UIUC press release:
It’s not every day that you come up with an entirely new tool for cosmology. We show that by using the background gravitational-wave hum from merging black holes in distant galaxies, we can learn about the age and composition of the universe. This is an exciting and completely new direction, and we look forward to applying our methods to future datasets to help constrain the Hubble constant, as well as other key cosmological quantities.
*Artist’s impression of the electromagnetic signal from the merger of two neutron stars. Credit: NSF/LIGO/Sonoma State University/A. Simonnet*
As a proof of principle, the team applied their method to current LVK Collaboration data. They found that the non-detection of the GWB provides evidence against slow cosmic expansion rates. They then combined their method with measurements of the Hubble Constant based on individual black hole collisions to obtain a more accurate rate. “Because we are observing individual black hole collisions, we can determine the rates of those collisions happening across the Universe,” said Cousins. “Based on those rates, we expect there to be a lot more events that we can’t observe, which is called the gravitational-wave background.”
This showed that at lower values of the Hubble constant, the total volume of space within which collisions occur is smaller. This would imply that the density of object collisions is higher, increasing the strength of the GWB signal to the point that current instruments could detect it. “This result is very significant—it’s important to obtain an independent measurement of the Hubble constant to resolve the current Hubble tension,” added co-author Nicolás Yunes, the founding director of the Illinois Center for Advanced Studies of the Universe (ICASU). “Our method is an innovative way to enhance the accuracy of Hubble constant inferences using gravitational waves.”
With LVK’s improved architecture, scientists estimate that the GWB is likely to be detected within the next six years. If and when this happens, the team’s method could be used to improve measurements of the Hubble Constant further. Until then, the stochastic siren method could be used to constrain higher values of the Hubble Constant, thereby establishing upper limits on the GWB and allowing scientists to study it before a full detection is made.
“This should pave the way for applying this method in the future as we continue to increase the sensitivity, better constrain the gravitational-wave background, and maybe even detect it,” says Cousins. “By including that information, we expect to get better cosmological results and be closer to resolving the Hubble tension.”
Further Reading: University of Illinois
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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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