Each of the two Voyager spacecraft, launched in 1977, carries a phonograph record. The records hold sounds and images chosen to represent Earth, assembled by a committee led by Carl Sagan. The records themselves are the part most people know about. The cover is the part worth a closer look.
Electroplated onto the aluminium cover of each record is an ultra-pure sample of uranium-238. It sits in a small area about two centimetres across, and it is there to serve a single function. It is a clock.
The reasoning is straightforward. Uranium-238 decays into a chain of daughter products at a fixed, known rate. A finder who measures how much uranium-238 remains, against how much of the daughter material has accumulated, can calculate how long the decay has been running. That figure is the time elapsed since the sample was placed on the spacecraft. It tells the finder how old the record is.
Why uranium-238
The choice of isotope is the whole point. Uranium-238 has a half-life of about 4.5 billion years, meaning that after that span roughly half of any given quantity has decayed. That is a slow clock, and a slow clock is what a message of this kind needs.
A fast-decaying isotope would be useless here. If the half-life were measured in years or centuries, the sample would have decayed away to almost nothing long before any plausible finder encountered it, leaving nothing to measure. A half-life of billions of years means the clock stays readable across the kind of timescales the Voyager spacecraft will actually be drifting.
NASA gives the sample’s radioactivity as about 0.00026 microcuries, a very small amount. It is a reference quantity to be measured, not a power source or a hazard.
The other clock on the cover
The uranium is not the only timekeeping device on the record cover. It is one of two, and the two are meant to be checked against each other.
The cover also carries a pulsar map, the same basic diagram used earlier on the Pioneer 10 and 11 plaques. It shows the position of the Sun relative to 14 pulsars, with each pulsar’s rotation period written in binary. Pulsars spin down slowly and predictably over time. A finder who knows how fast those 14 pulsars are spinning when the record is found, and compares that to the periods recorded on the cover, can also work out roughly how much time has passed.
So the cover gives a finder two independent ways to date the record. One is the decay of the uranium. The other is the slowing of the pulsars. If both methods point to a similar launch epoch, a finder can have more confidence in the answer. The redundancy is deliberate.
What “a billion years” actually refers to
The Voyager record is often described as a message built to last around a billion years, and the figure is worth handling carefully.
It is an estimate of the physical survival of the record itself, not a guarantee and not a precise prediction. The record is gold-plated copper in an aluminium cover, mounted on the spacecraft body. In interstellar space it faces erosion mainly from micrometeoroid impacts and cosmic rays, both of which act slowly. Estimates of how long the record’s grooves would remain physically readable run to a timescale of that order, hundreds of millions to a billion-plus years. These are estimates of material durability, and they carry wide uncertainty.
The uranium clock is well matched to that lifespan. With a half-life of about 4.5 billion years, the uranium-238 sample will still be measurable, still a working clock, long after a billion years have passed. The clock is designed to outlast the message it dates.
What none of this depends on is the record being found. The Voyager spacecraft were not aimed at any recipient, and the distances between stars are such that neither craft will pass close to another star for tens of thousands of years at least. The record cover is built the way it is not because a finder is expected, but so that the information is complete and self-checking if, against very long odds, one ever exists.
That is the quiet logic of the uranium spot. It is two centimetres of metal added to a cover, on the assumption that the most useful thing you can give a hypothetical finder, along with the message, is an honest way to know how old the message is.