Gravitational attraction of stars and cows
johndcook.com
johndcook.com
my attempt:
diameter of earth = 12742 km
sea level = distance from earth = 12742/2
weight of empire state building = 331000000 kg
resolution of BMA280 in the iPhone 6: 1/4096 g
mass of earth = 5.972e+24 kg
gravity of earth = 1 g
km to m = 1000x
(12742/2. * sqrt(331000000 / (5.972e+24 / 4096.))) * 1000
= 3 meters
So your phone should be able to register 1 bit of resolution when the empire state building is 3 meters away or less, otherwise it would be too far away to detect. Of course the empire state building would need to be compressed into a single point but that's a minor practical concern."minor" :)
That's great, have an upvote.
[1] http://sealevelstudy.org/sea-change-science/whats-in-a-numbe...
The locally detectable force is tidal. Which follows a cube law.
It turns out that every cow on Earth creates larger tidal forces on you than any star except the Sun. :-)
"a system which has spherical symmetry, and whose state is changing because of chemical reactions and diffusion ... cannot result in an organism such as a horse, which is not spherically symmetrical.”
http://www.dna.caltech.edu/courses/cs191/paperscs191/turing....
Under General Relativity what is commonly called gravity is a fictitious force or pseudo force and is purely an artifact of being in a non-inertial frame of reference.
While a very useful in most use cases, and accurate for most needs even Newton was bothered that under his model gravity acts Instanously. This superluminal communication makes the math work but is a spherical cow :)
As a direct comparison under Newtonian mechanics, the centrifugal force is a "inertial" or "fictitious" or "pseudo" force. Due to Einstein's equivalence principle, and under General Relativity gravity is also a "inertial" or "fictitious" or "pseudo" force.
To quote John Wheeler. "Mass tells space-time how to curve, and space-time tells mass how to move."
So if the cow is 5 cows away, you can get something like a get a 4% correction, that perhaps is measurable if you can measure the pull form the cow.
The cow representing Regulus is 4000 cows away, so the correction is less than 1/1000000 and it's safe to take it as a spherical cow.
[Side question: Can LIGO "hear" a nearby cow? It has filters to try to see the chirp of the merge of two black holes, and another filter to only consider the signals that appear in both detectors, so you probably need to train two synchronized dancing cows to fool LIGO. But, do they have enough precision?]
On the LIGO question: Two GPS-synchronized cows, standing near the end-masses, that mooed in the appropriate chirp (correcting amplitude for polarization) would make people nervous enough to do a few calculations and, out of an abundance of caution, put up a fence. I expect the gravitational effect from any mooing (it's a tiny quadrupolar deformation of the cow) to be extremely small.
In practice, even the end-station buildings are large enough to keep cow-moos from happening close-enough to bother the instrument gravitationally. Furthermore, there are no cows at Hanford, and I doubt that there are any near Livingston.
https://www.spsnational.org/the-sps-observer/fall/2017/consi...
The idea that everything in the universe is connected and pulling is mind blowing.
We only see a net attraction between current carrying parallel wires because the wires contain both electrons and protons in almost perfect balance, so that the electron/electron repulsions and proton/proton repulsions between the wires are almost perfectly canceled by the electron/proton attractions between the wires, leaving no net electrical attraction or repulsion.
That lets the weak magnetic attractions (or repulsions, depending on the directions of the currents) dominate.
As in, are we really feeling gravitational effects of mass that is 14 light years away, even if they are insignificantly tiny and we probably can't measure it, or is there a point where a force is so miniscule that the universe truncates the force to 0?
However, (and if I didn't screw up the math) since gravity scales linearly with mass, and the size of the visible universe is about 10^27 meters, then anything with mass greater than 10^15 protons -- or about the mass of a human cell -- has a "non zero" gravitational effect on you.
Other easily romantic notions in physics:
* we are all born of star stuff
* every breath we take has elements of the same breath as every human who ever lived (excluding some currently living ones, due to diffusion rates, but eventually...)
* (The current grav force between my partner and me is 1.9159965e-15 N)
Is it conceivable that some of the oxygen and nitrogen, etc, in the atmosphere today wasn’t present in the atmosphere, say, 40,000 years ago due to it being bound up in minerals or biological matter?
Select a planet, then touch the objects below. Eventually read the text at the end for the implementation details.
"Which has a greater gravitational pull on me: the Sun, or spiders?"
The main conclusion is sadly not that exciting, but the digressions are fun as always.
Tidal effects are caused by the gradient of the gravitational field across significant distances. And the gradient drops off in proportion to the inverse cube of the distance, not the inverse square. Which is why tidal effects are only observable from the moon and sun, not from other celestial bodies. (Jupiter's gravitational influence on the Earth is about 1% that of the moon, but it's so far away that the tidal effects are infinitesimal.)