What is the oldest light we have observed (and does it ever go out?)

There are phrases that we have become so accustomed to that our astonishment has worn off a little, but that if we rethink them, they can awaken curiosity.

“The oldest light in the Universe comes to us from the cosmic microwave background, emitted when the Universe was about 300,000 years old,” Matthew Middleton, an astronomer at the University of Southampton in the United Kingdom, told the BBC program CrowdScience.

The Universe began with the Big Bang about 13.8 billion years ago, but at first it was an extremely hot plasma.

During those ~300,000, photons, which are the elementary particles that make up light and all electromagnetic radiation, could not travel freely because they constantly collided with charged particles.

“But as the Universe expanded, it cooled, and as soon as it cooled enough for protons and electrons to combine and form a hydrogen atom, those photons were able to escape.

“That radiation has been traveling toward us ever since.”

That event is called “recombination,” and it marked the moment when “the Universe first became transparent.”

So there’s a kind of spike in the timeline of the Universe where suddenly a lot of energy is released, and now that energy is everywhere.

“It is very important because it tells us how the Universe developed its structure.

“It is the fingerprint of creation.”

That imprint is truly everywhere, and if you’re old enough to remember the static of old analog TVs, you’ve seen it.

That white noise comes, in part, from the cosmic microwave background radiation that Matthew describes, and it traveled through the cosmos for 13 billion years to reach you.

But beyond the cosmic microwave background, what is the oldest individual object we have been able to observe?

Astronomers have attempted to determine the age of individual stars in the vicinity of the Solar System, and HD 140283 has been the subject of detailed studies aimed at estimating it.

Nicknamed the “Methuselah Star,” it is located in our galactic environment and is considered one of the oldest stars whose age can be reliably measured.

It is estimated that its birth is close to that of the Universe itself, since it is part of the first generations of stars formed after the Big Bang.

But that refers exclusively to its intrinsic age as an object, and here we are talking about light.

From a cosmological point of view, its light is not particularly old: being located at a distance of approximately 190 light years, the photons we detect today were emitted just that number of years ago.

So our question really is: what is the oldest light we have ever observed coming from an individual object.

The answer, in this case, is not nearby stars, however old, but extremely distant primordial galaxies, whose light was emitted when the Universe was only a few hundred million years old and has traveled all that time before we could see them.

And the record for the most distant and oldest is held by JADES-GS-z14-0, whose light left when the Universe was approximately 300 million years old, which means that it is more than 13.4 billion years old.

However, in mid-2025, a contender appeared: MoM-z14, whose light would have been emitted about 20 million years earlier, that is, a little closer to the Big Bang.

Described as a “cosmic miracle” by the team of scientists who detected it with the James Webb Space Telescope, its discovery is awaiting peer review to be confirmed as the point detected by the most distant and, at the same time, oldest scientific instrument of all.

An echo of a very remote past, because we cannot forget that, since the Universe is so colossal, by the time those lights arrive, the objects that emitted them are no longer the same.

What astronomers observe is what it was: a point that indicates that a galaxy existed, which may now be a gigantic galaxy… or who knows what.

When we look at the lights in the sky, we travel through time.

But what about the future? Will the light have an expiration date?

If scientists have detected light that began its journey almost since the dawn of time, does that mean it never goes out?

“Photons are complicated,” answers astronomer Matthew Middleton.

“But you don’t have to go very deep to appreciate that energy is conserved in any closed system: that’s the first law of thermodynamics. So energy doesn’t disappear, it just changes form.

“A photon is a form of energy, and that energy will always exist in some form. Photons can change, but the energy remains.”

How can a photon transform into something else?

“You can get photons that produce matter and antimatter particles. So you can literally see light turning into matter. By the way, that’s why we exist.

“But photons can also be absorbed.”

When a photon hits an atom, its energy can be absorbed and cause an electron to rise to a higher energy level, Matthew explains.

In that case, the photon ceases to exist as an independent particle and the electron “jumps” to an excited state, taking with it the energy that the photon delivered. If the photon has enough energy, it can even completely knock the electron out of the atom (ionization).

“That energy is no longer in the form of a photon, but temporarily stored in the electron and the nucleus, but it still exists and can later be re-emitted as light, perhaps with a slightly different energy.

“It changes, it moves, but it is never completely destroyed.

“This is another way of looking at it: if I created something that released a photon into the Universe and it never interacted with anything, it would forever be a photon.

“It never turns off suddenly… if it did, it would drive many physicists crazy.

“So yes, in principle, light lasts forever.”

In conclusion: light has no expiration date.

If it traveled through empty space, it would continue to shine forever.

And even if it interacted with something, it wouldn’t be destroyed, it would just become a different form of energy.

By Editor

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