These clocks are accurate, they would lose just half a second if they lasted the age of the universe. That's 14 billion years.
But they will not be used to keep the train running on time. The clocks' exquisite precision, outlined in Nature today, means they can measure how space-time distorts under gravity forces.
Eventually, astrophysicists could enlist their help to detect mysterious dark matter.
More immediately, the clocks could tell us what's going on inside the earth by accurately mapping our planet's bumps and lumps – if the clocks are shrunk, that is.
Study co-author Will McGrew, a PhD student at the National Institute of Standards and Technology in the United States, said the "ticking" clocks is produced by oscillations of radiation emitted when electrons in ytterbium atoms are excited by lasers.
It turns out they tick, in almost perfect unison, 500 trillion times a second.
"Measuring time and frequency with such incredible precision provides a truly powerful lens to view the natural world," Mr McGrew said.
Atomic time 101
Measuring time was based on astronomy. For example, the length of a day was determined by one spin of the Earth on its axis.
But astronomical phenomena tend to slow down or speed up.
Our days are longerening, by an extra 1.7 milliseconds each century, thanks to our gravitational tango with the moon.
So while astronomical time can do for timetabling and such, science demands precision.
And this is where atomic time shines.
Rather than looking at the heavens, this form of time-keeping drills into the waves of radiation shrugged off by the atoms when they were bathed in a laser light.
They sound super futuristic, but atomic clocks have been around for more than 60 years.
The first atomic clock that was accurate enough to be used to set the time was built in 1955 at the UK's National Physical Laboratory.
It was accurate to a second in 300 years.
Some 12 years later, the caesium atomic clock became international time standard, and over time, atomic clocks became much more accurate.
Modern atomic clocks that use strontium or ytterbium instead of caesium lose one second every 300 million years or so.
More than time-keepers
Atomic clocks' precision means they have tested Albert Einstein's general theory of relativity, which predicted that time runs faster or slower under the influence of different gravitational forces.
In other words, a clock placed on a satellite orbiting Earth, which experiences higher gravity potential, will tick faster than a clock at sea level.
And there are already atomic clocks whizzing around the Earth on satellites that take advantage of this time dilation effect.
We would not have a global positioning system, or GPS, without them.
Another use of satellite-mounted atomic clocks is to accurately map Earth's size, shape, orientation in space and mass distribution, collectively called "geodesy".
Satellite geodesy usually involves timing how long light takes to make a trip between distant points, such as shining a laser to a satellite and timing how long it takes to bounce back to a receiver on Earth.
GPS geodesy is accurate to about a centimeter, said Matt King, who uses satellite geodesy at the University of Tasmania and was not involved with the study.
But clocks with a higher "tick" rate – that is, higher frequency – would not have to use light at all. They could use the relativistic effects of gravity.
This was what Mr McGrew and his colleagues wanted to achieve with their atomic clock.
Instead of caesium, they used ytterbium. The radiation waves emitted by ytterbium atoms oscillate almost five orders of magnitude faster than those from cesium atoms.
In their paper, the team showed that the clocks were exceptionally stable – losing or gaining time almost imperceptibly – ticking almost perfectly in unison.
So by comparing the ticking difference between the two ytterbium clocks placed on separate continents, a person could feasibly measure the height difference between the clocks to under a centimeter.
Harnessing precision of ultra-sensitive atomic clocks would be like having a "telescope looking inside", Professor King said.
"Let's say you have a earthquake," he said.
"If you can accurately measure this, you can learn about the fundamentals about the interior of the earth, like its viscosity or runniness."
How the Earth bounces back when glaciers melt or sinks when groundwater pumped out, too, could be tracked with atomic clocks.
And seeing how the ground around a volcano lifted and subsided, even on a sub-centimeter scale, could tell volcanologists how magma is moving around, Professor King added.
"Combine that with seismology, and you get a real picture of what's happening on the inside."
Big applications, compact clock
So what's stopping atomic clocks being wheeled out to volcanic and earthquake-risky places around the world?
Simply, the ytterbium clocks are big to move.
"[The clocks] basically take up a fairly large laboratory, "Mr McGrew said.
This is because they need a bunch of large lasers to work.
A couple of lasers cool the ytterbium atoms to a fraction over absolute zero (-273 degrees Celsius), while others hold the chilled atoms in place.
Mr McGrew and his colleagues have already begun working on the shrinking of the systems.
Professor King is optimistic that ultra-precise atomic clocks will be one day compact enough to be used on Earth as well as in space.
"Computers used to fill entire rooms as well.
"We might be 20 years away, it might be sooner, but if these [ytterbium clocks] can be miniaturised and if the precision keeps on increasing, then there is no shortage of applications. "
Weird and wonderful
Down the track, atomic clocks could be used for experiments that involve measuring the tiniest distortions in space-time, such as the incredibly subtle stretching and squashing of matter caused by a gravitational wave.
Take dark matter, for instance. Astrophysicists know that dark matter is out there, and that it forms around a quarter of all mass and energy in the universe.
But its "dark" nature – that does not seem to reflect, absorb or emit radiation – means it is very difficult to detect.
One model of dark matter suggests that it could interact with ordinary matter by changing the fundamental constants of nature, Mr McGrew said.
And this is where atomic clocks can help astrophysicists learn a little about the elusive stuff.
"Say there's a big dark matter object that passes through a laboratory that has a ytterbium clock and a strontium clock," Mr McGrew said.
"[The dark matter] would affect ytterbium by some factor, and then strontium by some other factor.
"By measuring the difference between the two clocks, you could detect the presence of the dark matter object.
"These are extremely subtle effects, but when you can make measurements with 18 digits of accuracy, you could detect them."
And, of course, there are purposes we have not yet dreamed of.
"The people who first made atomic clocks did not know they were building a GPS device," Mr McGrew said.
"I think there's something similar to say about atomic clocks – that their most salient, most important applications have not been thought of yet."