Most of us think we understand why Earth’s oceans have tides, but it turns out that there are some misconceptions in the common explanation. Yes, it’s true that the moon’s gravity pulls on water in the ocean, but it equally pulls on everything else, too, and we don’t levitate at high tide! In reality, it’s the distribution of tidal forces across the enormity of the ocean that causes the ocean to bulge along the Earth-moon line and create high and low tides. Lakes, puddles, and humans experience tides, too, but we’re so small that the tidal forces we experience are too tiny to be noticeable. For the full explanation, I encourage you to watch PBS Space Time’s video. Don’t let the 15 minute run-time deter you; the tidal explanation is contained within the first 9 minutes. (Video credit: PBS Space Time; via It’s Okay To Be Smart)
Videos
Weaponizing Water-Repellency
St. Pauli, a neighborhood in the German city of Hamburg, has demonstrated one of the most unusual applications of superhydrophobicity I’ve ever heard of. St. Pauli is known as a party district, and the residents of the area have grown understandably frustrated with inebriated visitors publicly urinating on their buildings and, yes, playgrounds. When fines failed to curb the issue, they took to treating walls chemically to make them superhydrophobic. As the targeted audience has discovered, water repellency tends to make liquid jets bounce off rather than run down a surface. Well played, St. Pauli. (Video credit: IG St. Pauli; submitted by entropy-perturbation)
Carbonation in Space
Astronauts don’t typically drink soda or other carbonated beverages while in space. The reason is probably apparent if you watch this new video of an effervescent tablet in water on the space station (or, you could watch the older classic one from Don Pettit). Unlike on Earth, where the carbon dioxide bubbles are buoyant and rise to the surface, the bubbles in a fluid in microgravity are randomly distributed. Those few bubbles that happen to be located along the edge of the water sphere will sometimes burst, creating the halo of tiny droplets you see in the video. In the case of sodas, though, the bubbles’ behavior creates a foamy mess, and, after ingestion, the bubbles are stuck travelling through the astronaut’s digestive system instead of getting burped out. Sounds rather unpleasant to me. (Video credit: NASA; submitted by entropy-perturbation and buckitdrop)
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LAST CALL: Help us do some science! I’ve teamed up with researcher Paige Brown Jarreau to create a survey of FYFD readers. By participating, you’ll be helping me improve FYFD and contributing to novel academic research on the readers of science blogs. It should only take 10-15 minutes to complete. You can find the survey here.
Soap Bubble Coalescence
Droplets falling onto a bath of the same liquid will sometimes coalesce via a series of increasingly smaller droplets in a process known as the coalescence cascade. Soap bubbles, it turns out, can exhibit a similar partial coalescence. When a bubble nears a soap film and the air between them drains away, coalesce can begin. If the the soap film beneath the bubble ruptures, some air from the inside of the bubble can escape. Part of the bubble coalesces with the soap film and a smaller daughter bubble is left behind. The researchers observed this process happen up to three times before the bubble coalesced completely. Alternatively, if the soap film did not rupture, the air inside the bubble had no escape, and the bubble would coalesce into a hemispherical lens atop the soap film. (Video credit: G. Pucci et al.; via KeSimpulan)
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Don’t forget about our FYFD survey! I’ve teamed up with researcher Paige Brown Jarreau to create a survey of FYFD readers. By participating, you’ll be helping me improve FYFD and contributing to novel academic research on the readers of science blogs. It should only take 10-15 minutes to complete. You can find the survey here. Please take a few minutes to participate and share!
Suppressing Instability
The Rayleigh Taylor instability is a common fluid phenomenon in which the interface between fluids of differing densities becomes unstable. It’s what’s responsible for all those awesome pictures of milk in ice coffee. For many years, fluid dynamicists theorized that the instability might be inhibited by rotation, which tends to suppress velocity changes along the axis of rotation. But actually creating an experiment demonstrating the effect was extremely difficult because any attempts to set a denser fluid over a lighter one before rotating it would kick off the instability. Recently, however, researchers succeeded in creating an experimental demonstration, seen in the video above. They did so by using magnetism. The initial set-up consists of two fluids of similar densities – a heavier, diamagnetic fluid on the bottom and a lighter, paramagnetic fluid floating on top. The tank was then spun up until both fluids were rotating like a rigid body. Then, the entire set-up was lowered into a vertically-oriented magnetic field. The paramagnetic fluid on top was attracted by the field while the diamagnetic fluid on the bottom was repelled. The end result is that the magnetic field created the effect of the upper fluid being heavier, thereby initiating the Rayleigh-Taylor instability. As you can see in the video, rotation does slow down–but not prevent–the instability. But it took some very clever and careful experimental design to show! (Video credit: K. Baldwin et al.)
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Don’t forget about our FYFD survey! I’ve teamed up with researcher Paige Brown Jarreau to create a survey of FYFD readers. By participating, you’ll be helping me improve FYFD and contributing to novel academic research on the readers of science blogs. It should only take 10-15 minutes to complete. You can find the survey here. Please take a few minutes to participate and share!
Magnus Effect
Putting a little bit of spin on an object can have a big aerodynamic effect, thanks to the Magnus effect. As demonstrated in the video above, backspin on a basketball dropped from a big height will send it flying out and away. The reason spinning objects generate these counterintuitive motions is because the air flow over them creates differential pressures. On the side of the ball spinning with the flow, air is accelerated, dropping the local pressure; whereas on the opposite side, the ball spinning against the direction of flow makes the flow separate and no longer flow smoothly along that side. This causes a high pressure on that side. Like the difference in pressure on either side of an airfoil, the pressure difference across the ball creates a force that pushes the ball toward the low pressure side. Check out some of the other places Magnus effect shows up! (Video credit: Veritasium; submitted by Andrew C.)
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Help us do some science! I’ve teamed up with researcher Paige Brown Jarreau to create a survey of FYFD readers. By participating, you’ll be helping me improve FYFD and contributing to novel academic research on the readers of science blogs. It should only take 10-15 minutes to complete. You can find the survey here.
The Kelvin-Helmholtz Instability
The Kelvin-Helmholtz instability is a pattern frequently found in nature. It has a distinctive shape, like a series of breaking ocean waves that curl over on themselves to create a string of vortices. The instability shows up when there is a velocity difference between two fluid layers. The unequal shear between the two layers magnifies any disturbance to their interface, which manifests in the fractal, overturning whorls seen in the numerical simulation above. You can find the Kelvin-Helmholtz instability in the lab, in the sky, in the ocean, on Jupiter and Mars–even on the sun! For more information on the methods used to create the simulation above, check out the full paper. (Video and research credit: K. Schaal et al.)
How the Grand Canyon Formed
The Grand Canyon is a monument to the power of water, air, and time. In this video from It’s Okay To Be Smart, Joe Hanson describes the formation of the Grand Canyon – from the ancient oceans that created its many layers to the tectonic upthrusts that eventually created the Colorado River that continues to cut through the Canyon’s rocks today. Fluid dynamics play a major role in the geology of the Grand Canyon, whether it’s in the mantle convection that helps drive plate tectonics or the sedimentation that builds and erodes rock layers. (Video credit: It’s Okay To Be Smart)
Air Pressure in Flight
We live at the bottom of a sea of air, surrounded by a constant pressure equal to 101 kPa (14.7 psi) over our entire bodies. For the most part, we don’t notice the pressure air exerts on us. But if you’ve flown on a commercial airplane, you may have noticed some of the effects of changing that air pressure. Flexible sealed containers, like bags of chips or bottles of water, change their shape dramatically over the course of a flight because the air pressure inside them can be greater than the air cabin pressure at altitude. In the video above, Nick Moore measured his in-flight cabin pressure as 84 kPa (12psi), which is equivalent to about 1500 m (5000 ft) above sea level. Why do airlines keep the cabin pressure lower in flight? The biggest reason is because the airplane, like the in-flight snack, is a pressure vessel. At cruising altitudes the outside air pressure is about 24 kPa (3.5 psi). To keep the interior of the cabin habitable, the fuselage of the airplane has to hold a higher pressure. The larger the difference between the interior and exterior pressures, the greater the stress the airplane must withstand. Keeping the air pressure in flight a little lower makes the engineering a little easier and does the occupants no harm. (Video credit: N. Moore)
Making Lava
In this video, NPR’s Adam Cole takes a trip to upstate New York to find out how to make lava – and not the kind with vinegar and baking soda! We’ve featured footage from this duo before. Since most lava flows don’t occur in predictable or controlled circumstances, it can be tough for scientists to study their fluid properties and flow behaviors. Set-ups like this one allow more precise experimentation, as well as opportunities to test other wild ideas. For more, check out the full video and the Syracuse University Lava Project. (Video credit: NPR Skunk Bear/A. Cole; via skunkbear)