A person's hand is shown holding a glass flask in a dark room. An orange-red glow is emanating from the flask in a patches, forming a splash-like pattern near the base of the flask.

A Sloshing-Mercury-Powered Neon Light

In 1675, while transporting a barometer by night, the astronomer Jean Picard noticed a glow inside its glass tube, just above the mercury. As the mercury sloshed and splashed across the surface of the glass, a static electric charge had built up, which was discharging by ionizing the residual gas molecules inside the evacuated tube. [Styropyro] recreated this effect, and found that the dim glow could be made much stronger by adding some noble gas to the tube.

It starts with a simple recreation: he took a volumetric flask, attached a narrow glass stem to the mouth, added some mercury to the flask, evacuated it with a vacuum pump, and sealed off the glass stem. This produced a faint glow when shaken, but it was only really visible under very low light. When [Styropyro] brought it near a Tesla coil, however, it did glow much more brightly.

Backfilling an identical flask with neon to about 40 millitorr produced a much more spectacular result (a low pressure in the tube is necessary, but moderate pressure variations don’t significantly alter the effect). When shaken even slightly, this neon-containing flask produced a bright orange-red glow just above the surface of the mercury. Points of obstruction, such as those in a zig-zag tube, produced a brighter glow. A krypton-containing tube glowed blue, but less brightly than the neon tube.

Since this is, essentially, a triboelectric effect, other materials besides mercury should work; [Styropyro] tested several materials, and found that pieces of Teflon produced a faint glow, and copper beads a somewhat brighter glow. Unfortunately, Galinstan, the obvious replacement for mercury, wets and coats glass, preventing a charge buildup.

Without an added noble gas, the standard glow of barometric light comes from the excitation of mercury vapors, a glow which can also be seen in mercury rectifiers, and which excites the phosphors of fluorescent light bulbs.

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A rail sprayer somewhere on Union Pacific tracks

White Rails Are The Infrastructure Hack We Didn’t Know We Needed

Railroads might be a nineteenth century technology, but they’re still the backbone of cargo transportation in the 21st century. They’ve also far from run out of innovation, including this one which really just sounds like a hack: painting the rails white to beat the heat.

In the old days, when rails were short and riveted together, this might have been unecesssary; all those joints allowed for a lot of flex. But when you have kilometers of continously welded rail, the thermal expansion starts to matter. A lot. Even if the rails haven’t bent and buckled from excess heat, their capacity goes down. Trains must therefore slow way, way down in hot weather, reducing the overall amount of freight the system can handle.

So, how do you cool the million miles of metal that holds a country together? Paint. Simple white paint sprayed on the side of the rails can bring down temperatures 11 °C (20 °F), according to the Union Pacific Railroad, the first to try this in North America. It might not surprise you that this technique is also being rolled out on the other side of the pond during this summer’s European heat waves. Indeed, it was invented there; the Italians have been doing it for many years now.

If you think reducing solar heat with white paint is good, you can do better than that with special formulations that end up cooler than ambient. It passive cooling also comes in fibre form.

A USB Port By Any Other Color…

[Dr. Gough] bought a generic USB 3.0 hub on an Asian website. Surely, USB 3 is mature enough that even the cheapest hub will have some IC in it that will work well, right? You’d think so, but a little exploratory surgery showed that the only thing about this hub that was USB 3 were the blue port connectors.

We have a few problem USB hubs ourselves, so it might be worth doing this to any you have lying around. The first clue: most of the connectors on the PCB only have four pins. On closer examination, the hub appears to be a USB 3.0 extension cable with a USB 2.0 hub made from two HS8836A chips.

Not only are these USB 2-only, but all the ports on an HS8836A also share the same USB 1.1 bandwidth. Some hubs can provide multiple ports full 1.1 bandwidth, using the higher-speed USB protocol to the PC as a backhaul.

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Bad Apple On A Karaoke Machine

CD+Graphics was a format that never really caught on. It let music discs pack some graphics, maybe liner notes, and mostly song lyrics into the otherwise empty space on a CD. It was never intended for displaying full-motion video, but that didn’t stop [Adam Gashlin] from getting a Bad Apple, with lyrics, running on any device that will play CD+G.

The main challenge is that CD+G gives you 300 screen commands per second, which is plenty for updating text on the 48×16 blocks as the lyrics scroll by. But if you want to send custom blocks and draw images, that’s 2.5 seconds per screen: a lousy framerate.

[Adam]’s first trick is to drop the resolution way down, which gets him into the 8 FPS range. Only update the blocks that change pushes this up to a respectable 17-20 FPS. But you can see the updates, and that’s distracting. It really needed buffering.

If you don’t know Bad Apple, it’s in black and white. And like many old graphics engines of the day, CD+G uses a dynamic palette of colors. [Adam] uses this to pack four frames into one, switching between them using palette swapping. (Absolutely check out his “rainbow” version of the video to see how the palette-swapping trick works.)

In the end, his demo has audio, triple-buffered video, and lyrics at 16.3 FPS. It’s slower than the fastest video-only version, but it looks so good, and [Adam]’s explanation of all of the graphics tricks he uses to get there is the real star of the show.

If you want to see Bad Apple running on yet more minimal hardware, how about a 16×2 LCD? Or a much more ridiculous implementation? How’s regexes in Vim for absurd? Got any Bad Apple hacks of your own? Let us know in the comments or the tips line. You can never have too many.

Even Chemical Bonds Obey Einstein’s Relativity

Although Einstein’s Theory of Relativity is typically associated with really large and really heavy things like planets in solar systems and big things in universes in general, it turns out that even at an atomic scale its effects can be measured. These are the findings of Brown University scientists, whose measurements on very heavy elements indicate the presence of relativistic bonds.

Unfortunately the paper by [Kirk A. Peterson] et al. in Science is paywalled without a convenient ArXiv version to ogle details beyond the supplemental, but the Brown press release gives quite a few details by itself, including the use of photoelectron spectroscopy to measure the strength of the bonds between the examined nuclei.

The essential summary is that our concept of how triple bonds work may be flawed, with the assumption that there are distinct sigma and pi bonds, the latter being the awkward, weaker ‘side bonds’ where the overlapping atomic orbitals do not directly line up as with a sigma bond. As it turns out, if there’s enough mass involved, relativistic effects smudge both types of bonds together into a hybrid type of bond.

Although the sigma-pi triple bond theory still seems to hold up for lighter atomic nuclei, in the case of the examined bismuth-carbon triple bond, the typical, slightly radioactive bismuth-209 nucleus with atomic number 83 is heavy enough to affect the orbital mechanics and with it the chemical bonds that these produce.

This is an important finding, as it affects our basic understanding of how strong the bonds between certain elements are. Pi bonds are after all significantly weaker than sigma bonds, so a hybrid form would effectively make triple bonds involving a heavier element stronger than one between lighter elements.

GOES-19 Goes Down, NOAA Investigating

Some breaking news from geostationary orbit, as the National Oceanic and Atmospheric Administration (NOAA) has announced that its newest Geostationary Operational Environmental Satellite (GOES) satellite unexpectedly went offline last night, and as of this morning, remains stuck in safe mode.

Launched in June of 2024, GOES-19 is one of four operational weather satellites that NOAA operates to provide forecast data and severe weather monitoring for the entire Western Hemisphere. The satellite is specifically responsible for covering the continental United States, Central and South America, as well as the Atlantic Ocean. This makes it a particularly critical asset even under normal circumstances, but the fact that it’s gone blind during the Atlantic hurricane season and while smoke from the raging Canadian wildfires is drifting over the Northeast and making the skies over Boston and New York City look like Mars is something of a worst-case scenario.

The good news is that two of the four satellites operate as orbital spares — the satellite that GOES-19 replaced in 2024, GOES-16, is still operational and can stand in as a backup for its coverage area. Obviously, it’s quite a bit older, having launched back in 2016, but it’s of the same design as GOES-19, and in good health, so there should be no degradation of service.

Still, getting GOES-19 back online will be critical for NOAA and the National Weather Service, and we expect they’ll be providing regular updates as the situation develops. Stay tuned.

Hackaday Europe 2026 – Build A Cable Modem For Your Arduino

Even for those of us that are quite technically minded, we spend precious little time thinking about the cables that carry our signals and do all the important work we need them to do on a daily basis. A great deal of theory and engineering goes into making things like telephone lines and HDMI cables work, but we mostly just plug them in and get on with whatever we’re doing.

If this is your experience, you might find the Hackaday Europe talk from [Michael Wiebusch] to be particularly interesting. He dives into transmission line theory from an accessible standpoint, explaining how two disparate signals can go in opposite directions on the very same wire. Then he demonstrates the theory by building a cable modem… well, sort of!

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