News
What Happens When Light Goes Boom? Part 3: Brad Bradington Sprints
(This is Part 3 of a series on Cherenkov radiation — the “light boom.” Read Part 1 and Part 2 first.)
We have our material — the crowd at the red carpet. We have our star particle — Brad Bradington. We have our paparazzi. Let’s watch what happens.
Brad steps out of his limo and walks at a nice, relaxed pace. The red carpet is absolutely packed — thousands of fans and photographers, crowding every inch. The people in the middle of the crowd and at the edges can’t see the limo from where they’re standing.
So when Brad appears, only the people right next to him know he’s arrived. And what do they do? They scream, they holler, they point their cameras and start snapping pictures. But only the ones nearest to him. The ones further back don’t even know he’s there yet.
As Brad walks slowly down the carpet, word of his presence spreads outward in all directions — a ripple of recognition, expanding like rings on a pond. If you had a bird’s-eye view, you’d see Brad moving through the crowd with these expanding rings of camera flashes around him, centered on wherever he happens to be.
Inside the material, this is a charged particle moving at a modest speed. It carries an electric field with it — a celebrity aura — and as it passes, it disturbs the atoms and molecules nearby. They stretch and squeeze and twist under the influence of that field, then snap back into place and release a tiny flash of light. These flashes radiate outward in all directions from wherever the particle is.
When the particle is moving slowly, the flashes from all directions are roughly in phase with each other. They overlap and interfere and largely cancel out. You don’t get a coherent glow. Nothing special happens.
But let’s say Brad Bradington is in a hurry.
Maybe he’s late. Maybe he hates crowds. Maybe he really has to pee. Whatever the reason — he leaps out of the limo and absolutely barrels for the entrance. Shoving people. Elbowing through. Zero regard for personal space.
The key: the paparazzi have a reaction time. Before they can snap a picture, they have to KNOW Brad is there. And the speed at which that knowledge travels — the speed at which the information “Brad Bradington is right here, right now” can reach a photographer’s eyes — is the speed of light in this material.
If Brad is moving slower than that speed, everything is orderly. He’s walking, light is running ahead of him, the paparazzi in front have plenty of warning, they fire from all directions, the flashes cancel out, no special glow.
But if Brad is moving FASTER than the local speed of light?
Then the paparazzi directly in front of him have no warning whatsoever. Zero. By the time any light from Brad reaches them, he’s already blown past. They only ever get a shot from behind, or from the side as he’s already gone.
Every single flash — the light released by every atom and molecule disturbed by Brad’s passage — is now entirely behind him. Instead of spreading out equally in all directions and canceling into nothing, they all pile up together. They reinforce each other. They add into a coherent wave, a shock front of light, spreading out behind the particle in a V-shaped cone.
It’s exactly like a sonic boom. When a jet aircraft exceeds the speed of sound, the sound waves it produces can no longer outrun it — they pile up into a pressure shock wave that you experience as a sudden violent crack. Cherenkov radiation is the same phenomenon, with light instead of sound. The particle drags a cone of coherent electromagnetic radiation behind it as it moves.
A sonic boom, but made of light.
A light boom.
THIS is what Pavel Cherenkov saw glowing blue in his bottle of water in 1934. The gamma rays hitting the water were knocking electrons loose and accelerating them to speeds faster than light moves in water — and those electrons were painting a cone of blue light as they went, over and over, billions of times per second, until the whole bottle glowed.
The blue color is not a coincidence, and it’s worth pausing on.
Cherenkov radiation produces light across a range of frequencies, but the intensity increases toward shorter wavelengths — toward blue and ultraviolet. The physics behind this involves the way different frequencies of light interact with a medium, but the short version is: the higher the frequency, the more coherently the radiation adds up, and the stronger the glow. Blue and violet win. Which is why every photograph of Cherenkov radiation you’ve ever seen — reactor pools, particle detectors, medical imaging — has that same particular, eerie, unmistakeable color. Not purple, not white, not green. Blue. Always blue.
Pavel Cherenkov got a Nobel Prize in 1958. Twenty-four years after he stared at a glowing bottle of water and decided, for no good reason except good scientific instinct, that it was worth understanding.
Not bad, Pavel.
In Part 4, we find out what Brad Bradington is actually good for — from the cores of nuclear reactors to a cubic kilometer of ice at the South Pole.
News
In Alabama, Opposition to Renewable Solar Energy Joins a Data Center Battle
Tuesday’s runoff for a slot on the Alabama Public Service Commission has a familiar ring to it, with talk of data centers and electricity costs. But in a southern twist, solar power has joined the list of villains.
News
New Study Assesses Titan’s Resources and their Potential Uses
Saturn’s largest moon, Titan, is a unique environment in our Solar System. It is the only moon (or body beyond Earth) to have a dense, nitrogen-rich atmosphere, and its methane cycle is very similar to Earth’s hydrological cycle, in which solid and liquid methane evaporates to form clouds and returns to the surface as precipitation. In addition, its prebiotic surface environment and rich organic chemistry make it a prime destination for astrobiology missions, such as NASA’s Dragonfly mission (set to launch no earlier than July 2028).
And as Robert Zubrin said in his book, Entering Space: Creating a Spacefaring Civilization, Saturn’s moons could become the “Persian Gulf” of the Solar System, with Titan being a major one because of its rich resource environment. In a recent NASA-supported study, a team of researchers compiled an inventory of Titan’s resources and their potential use by future generations of humans. When comparing this satellite to other destinations (i.e., the Moon and Mars), they conclude that Titan offers several potential benefits for human settlement.
The research was led by Conor A. Nixon, an astronomer and planetary scientist with the Solar System Exploration Division (SSED) at the NASA Goddard Space Flight Center and the Associate Laboratory Chief of their Planetary Systems Laboratory. He was joined by Ye Lu, a Professor of Aerospace Engineering at the Worcester Polytechnic Institute, and Jennifer E. Ruliffson, a Professor of Materials Science and Engineering at the University of Florida. The preprint of their paper has recently appeared online and is under review for publication in *Acta Astronautica*.
Artistic representation of Titan’s abundant resources and their possible uses. Credit: Nixon, C.A. et al (2026)
ISRU is a major aspect in all plans for long-duration missions to the Moon, Mars, and other locations far beyond Earth. To date, the vast majority of studies have focused on leveraging lunar and Martian resources to sustain crewed missions and eventual human settlement. With the exception of a recently proposed Titan ISRU Sample Return (TISR) mission, Titan has received considerably less attention, despite the possibilities this moon offers.
This includes opportunities for ISRU that would enable the construction of long-term habitats on the surface. In addition, they could also lead to Titan becoming a base for resupply missions traveling to and from the outer Solar System. Similarly, Titan could facilitate the exploration of Saturn’s other satellites, particularly the “Ocean Worlds” of Enceladus and Mimas, both of which are also rich in resources. Finally, its resources and products fashioned from them could be exported to other locations in the Solar System.
This includes fuel, feedstock, and basic necessities like food, water, nitrogen fertilizers, oxygen gas, and more. As Nixon told Universe Today via email:
Titan is gushing with hydrocarbons – what we call oil and natural gas on Earth. In the atmosphere, it has about 5% methane (what we call LNG and use in home heating and cooking). On the surface, we can find heavier hydrocarbons, such as propane used in BBQ tanks, butane used in lighters, and heavier liquids like kerosene and gasoline. Besides burning these hydrocarbons, we can also make a lot of products from them: plastics, synthetic rubber, and feedstocks for everything from solvents to pharmaceuticals, and even foods.
The previous study, led by Geoffrey Landis and the Compass Lab team from NASA’s John Glenn Research Center, looked at ISRU at Titan for one purpose: liquifying methane and producing liquid oxygen (LOX) and liquid hydrogen (LH2) from water to create propellant for a sample-return mission. Nixon and his colleagues cast a much wider net, looking further ahead by examining the many possible uses of all of Titan’s resources.
*A rendering of a notional spacecraft powered by nuclear thermal propulsion. Credit: General Atomics*
They also considered how a rich resource base could be used for a wider range of mission profiles. These include missions that need to return to Earth, as well as missions that plan to explore beyond Saturn. To this end, refueling stations on the surface could be accessed by landers from a larger spacecraft that would take on fuel and supplies. Alternately, refueling depots could be built in orbit – similar to what SpaceX is investigating for the Starship – that spacecraft would rendezvous on their way to other destinations.
And as Nixon noted, there’s the possibility of harvesting resources to build long-term settlements on Titan’s surface:
Basically you could envision either ‘refueling’ at Titan (in the manner of the Oleson/Landis study), or using the resources to sustain a more permanent settlement. [And] regarding refueling, it doesn’t just have to be for a return trip to Earth: it could be refueling a ship just arrived from the inner Solar System to go further out, say to Uranus or Neptune, or to explore the Saturnian moons. Or it could just be refueling a regular shuttle that traverses around the Saturn system between colonies on different moons.
Also, we can widen the definition from just ‘fuel’ to resources for a wide variety of purposes. So let’s imagine a permanent station on Titan that refines hydrocarbons and stores them as a variety of feedstocks and raw materials: everything from printer ink to fertilizer. Then, when a visiting ship comes to ‘refuel,’ it is restocking not just fuel but raw ingredients for food, perhaps for 3D printers used to make spare parts, textiles, utensils, and more.
There’s also the large volume of water on Titan, which accounts for 50% of its mass (the rest being rocky material in its core) and exists in both solid and liquid states. The liquid portion exists largely beneath the surface, where ammonia and salinity (two natural antifreeze compounds) maintain its liquid state. Water also exists in abundance as surface ice, which could be harvested and used to provide everything from drinking water to hydrogen fuel, oxygen gas, and (as noted) to manufacture LOX/LH2 propellant.
*This mosaic of Saturn’s moon Enceladus was created with images captured by NASA’s Cassini spacecraft. Credit: NASA/JPL/Space Science Institute*
After considering Titan’s resource base and the opportunities for resupply, settlement, and exploration, Nixon and his colleagues compared Titan with the Moon, Mars, and several NEAs. They determined that while Titan is much more distant and would require nuclear propulsion to enable transits, its potential is unrivaled. “There is simply no other world (that we know of) like Titan,” said Nixon. “Titan is unique in multiple respects: it’s the only moon with an atmosphere, and it’s the only planet/moon other than Earth to have hydrocarbons available in the atmosphere and on the surface.”
While the idea of crewed missions to Titan, or the settlement of this and other Cronian moons, is a far-off prospect, the potential is obvious. By establishing infrastructure and outposts in and around Saturn’s moons, humanity would have access to a huge resource base. Beyond Titan, Saturn’s atmosphere contains massive reserves of the rare isotope helium-3 (³He), considered the ideal fuel for fusion reactors and fusion propulsion. With so much water, hydrocarbons, and precious gases available, Saturn could very well become the “Persian Gulf” of the Solar System.
But as Nixon indicated, the benefits go far beyond refueling and include the means to build a manufacturing base capable of meeting all the needs of a human population. With the abundant plastics, feedstock for 3-D printers, fuel, and food that could be produced in-situ, a human settlement on Titan could endure for generations. It may be a far-off possibility, but it’s good to know that it’s there and could be fulfilled someday as part of humanity becoming an interplanetary civilization.
Further Reading: arXiv
News
California high surf and coastal flooding risk continues until Wednesday

The risk of flooding and dangerous surf at California beaches will continue until Wednesday, weather officials said Sunday.
Waves are not expected to be as big as those that pounded the shore last week and led to the deaths of two people.
The National Weather Service said San Francisco recorded its highest-ever summer ocean water level late Saturday.
At 1.83 feet above normal high tide, the level was the highest recorded outside of those occurring from November to March, when winter storms cause surges, officials said. Water level records go back to 1898.
A coastal flood advisory remains in effect through Wednesday morning, the weather service said.
The highest tides will be in the evening, officials said.
Over the last week, the greatest threat of dangerous rip currents and sneaker waves has been on the beaches facing south or southwest, officials said.
The city of Newport Beach warned residents to prepare for a series of king tides, continuing through Tuesday.
City employees have been distributing sandbags to residents to help protect their property from flooding. Officials urged those going to the beach not to park in low-lying areas.
“Motorists are urged to drive slowly through flooded areas to avoid creating wakes that can worsen flooding and impact nearby properties,” the city said in a statement.
Last week’s ocean swell brought historic 20-foot waves to the Wedge, the Newport surf break at the tip of the Balboa Peninsula.
On Wednesday, rescuers attempted to save two women who were swept out to sea from a beach in Santa Cruz. One of the women died. The other was in critical condition, officials said Friday.
The body of missing 5-year-old Amada Mia Brown of San Bernardino was recovered in Laguna Beach on Thursday, two days after she vanished in high surf.
Officials urge beachgoers to stay off rocks and jetties at times of high surf and keep an eye on the ocean.
If caught in a rip current, don’t panic, officials advised. Swim along the shoreline, rather than directly back to the beach, until free of the current’s pull.
If needed, tread water and call for help.
-
News3 weeks agoTrump administration sues UCLA, alleging antisemitic environment festered
-
News2 weeks ago
Iran War Live Updates: Israel Strikes Southern Lebanon After Pulling Back From Threat to Beirut
-
News1 week agoNew Cloud-Detecting Method Will Help Astronomers Characterize Exoplanets
-
Trending2 weeks agoSF Giants’ familiar script sees Casey Schmitt homer, loss to Arizona
-
Trending3 weeks agoSpurs’ Mitch Johnson Finishes Third in Coach of the Year Voting
-
News3 weeks ago
Iran War Live Updates: U.S. and Iran Trade Strikes, Further Threatening Negotiations
-
Trending2 weeks agoStripping U.S. citizenship for some is harder than Trump vowed : NPR
-
Entertainment2 weeks agoBlack Crowes singer Chris Robinson booed after mocking Florida fans’ ‘USA’ chant
