Category Archives: Physics
It's Definitely not a Weak Interaction
What particle physics does to me
SFW, unless you’re dyslexic (or your boss is)
Check
I noticed a very important lesson in Rhett’s post July 4th and an example of work-energy: checking the answer.
Let me make some checks here. Will the acceleration be positive? Yes. The first term will always be positive and greater than g because (d+h)/d is greater than 1. What if a jumper jumps from a higher height (h). This would make the acceleration greater. What if the jumper stopped in less water, this would also make the acceleration greater. Finally, does this have the correct units? Yes.
Notice how Rhett isn’t checking the numerical answer — this is a check of the equation that leads to the numerical answer, to see if it’s reasonable. There’s a lot of power in doing this that one loses when the numbers are substituted too early in the process. While you can do the first and last checks — direction and units — the trends of what happens if a variable changes is removed. And checking the limiting behavior of an equation is a tremendously important tool as the questions, and resulting conclusions, get more complex.
Now, once you get the answer, you can check that for reasonableness, too. As I mentioned some time back, when I taught we stressed getting answers that made physical sense, else your math mistake be tagged as a conceptual error. You should not be deducing that a frog has a mass of 10^24 kg; one can check this by relating the mass to known objects (in this case, being a measurable fraction of the mass of the earth) which requires having some awareness of masses (or forces, energy, etc.) on different scales. Or can apply the long-lost art of estimating the answer from the number you put in. All numbers become 1,2 or 5 and you round aggressively — but the rounding often cancels, and you can get pretty close. At least close enough to be within a factor of 10 or less of the right answer.
And some of this is shown in sciencegeekgirl’s Teaching the gentle art of estimations which includes a simple estimation problem which was a complete disaster when asked of some teenage students.
The conclusion I draw from this? We’re doomed.
Interestingly (ironically?) the very last example has a number I question. The force of impact of an object falling under the influence of gravity is much larger than mg.
Acceleration goes as the velocity of impact divided by the time of contact. What is the time of contact? The bottom of the ball hits the ground, but the top keeps going until it gets the signal that the bottom has hit, that there’s no more room to move down, and it’s time to start moving up. That happens at the speed of sound.
And from that, a time of 10 microseconds is concluded, giving a force of 10,000 mg (i.e. an acceleration of 10,000 g’s. Wow!)
I balked at that (and commented in the post). The object doesn’t recoil that fast — that’s the limiting case for the top to know that there has been an impact. One needs to look at the spring constant of the material to know what’s going on. 10 microseconds is too short — the contact time is almost certainly much longer. How much longer, I wonder? A convenient scale with which I am becoming familiar is shutter speed. 10 microseconds wouldn’t be discernible on a high-speed camera, if I had access to one. Which I do.
This is at 420 frames/second, and since I have the advantage of being able to easily click through frame-by-frame on the original, I’ll tell you the answer: the ball is in contact for ~4 frames, or just under 10 milliseconds. IOW, almost three orders of magnitude longer than the speed-of-sound estimation.
Blame Feynman
Built on Facts: Failures of Cuteness in Physics
There’s a unit of cross-sectional area used in nuclear physics equal to a trillionth of a trillionth of a square centimeter. It’s roughly the cross-section of a heavy atomic nucleus, and it’s used to discuss interactions with incoming particles. You could say in some ways it’s a measure of how easy it is to hit a nucleus with a projectile like a neutron. A big nucleus is as easy to hit as the broad side of a barn. And the unit is called the barn, for exactly that reason. I have no evidence, but I blame Feynman anyway.
Sunny Side Up
If at first you don’t succeed … Fry, fry again
The Oatman sidewalk egg fry. Cook your eggs, using the sun.
The egg fry began at high noon, with temperatures coming in at 105 degrees at the start of the event, slightly cooler than organizers and contestants would have liked. The spectators, though, were appreciative.
Perhaps the most innovative – and certainly most effective – method of frying eggs on Saturday was that of Eric Schmidt and Xinaxiao Chou from Cibola, Ariz. Using a Frensel lens to intensify the heat, Schmidt was able to cook a perfect – and edible – sunny-side up egg in about 60 seconds.
(Some strange physics commentary, though, about sequestering Carbon.)
(note to self: bring Fresnel lens on vacation …)
Don't Be Such a Negative Nelly
Skulls in the Stars: Some musings on negative refraction
[I]s a negative refractive index necessary to have negative refraction? In fact, the answer is a resounding “no”, as apparently many researchers were aware even when Pendry’s first paper came out.
I Didn't Check with Houston
But I was ‘go’ for launch. A couple of antacid tablets in a pill bottle with a snap-cap. A shelf glued to the inside lets the tablets stay dry until you tip it over. Launch happens after ~15-30 seconds. Not really an indoor toy, but …
One Up on the Alpha Betas
Unlike the outcome in Revenge of the Nerds, my fireball did not result in the destruction of my residence.
(The source is a spray bottle containing rubbing alcohol, rather than me spitting grain alcohol)
Yes, it's Rocket Science
Basics of space flight: orbital mechanics
Orbital mechanics, also called flight mechanics, is the study of the motions of artificial satellites and space vehicles moving under the influence of forces such as gravity, atmospheric drag, thrust, etc. Orbital mechanics is a modern offshoot of celestial mechanics which is the study of the motions of natural celestial bodies such as the moon and planets. The root of orbital mechanics can be traced back to the 17th century when mathematician Isaac Newton (1642-1727) put forward his laws of motion and formulated his law of universal gravitation. The engineering applications of orbital mechanics include ascent trajectories, reentry and landing, rendezvous computations, and lunar and interplanetary trajectories.
Mad Max: Beyond Thunderhead
Besides being host to stunning lightning displays, thunderclouds also emit gamma rays, although researchers aren’t completely sure why. Last fall, detectors installed on a mountaintop in Japan captured the first simultaneous observations of this radiation along with the high-speed electrons thought to be their source. The results, detailed in the 26 June Physical Review Letters, support the prevailing model of thundercloud accelerators generating “runaway” electrons, which may sometimes initiate lightning.