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Starts With A Bang

The Universe is disappearing, and we’re powerless to stop it

There are an estimated two trillion galaxies within the observable Universe. Most are already unreachable, and the situation only gets worse.
big bang
There is a large suite of scientific evidence that supports the expanding Universe and the Big Bang. At every moment throughout our cosmic history for the first several billion years, the expansion rate and the total energy density balanced precisely, enabling our Universe to persist and form complex structures. Whether the entropy of any part (or the whole) of the Universe increases, decreases, or remains the same, time always runs forward at the same rate.
Credit: NASA / GSFC
Key Takeaways
  • As the Universe expands, it also gravitates, so the expansion rate has slowed down tremendously since the hot Big Bang occurred some 13.8 billion years ago.
  • However, about six billion years ago, distant galaxies started speeding up in their recession from us: an effect caused by the relentless presence of dark energy.
  • Today, some ~94% of the galaxies we can observe are already unreachable by us, and in the far future, only the Local Group will remain.

It’s been nearly a century since scientists first theorized that the Universe is expanding, and that the farther away a galaxy is from us, the faster it appears to recede. This isn’t because galaxies are physically moving away from us, but rather because the Universe is full of gravitationally-bound objects, and the fabric of space that those objects reside in is expanding.

But this picture, which held sway from the 1920s onward, has been recently revised. It’s been only 20 years since we first realized that this expansion was speeding up, and that as time goes on, individual galaxies will appear to recede away from us faster and faster. In time, they’ll become unreachable, even if we journey toward them at the speed of light. The Universe is disappearing, and there’s nothing we can do about it.

The Milky Way, as seen at La Silla observatory, is a stunning, awe-inspiring sight to anyone, and offers a spectacular view of a great many stars in our galaxy. Beyond our galaxy, however, are trillions of others, nearly all of which are expanding away from us. (Credit: ESO/Håkon Dahle)

When you look out at a star whose light arrives after traveling toward you for 100 years, you’re seeing a star that’s 100 light years away, due to the fact that the speed of light is finite. But when you look out at a galaxy whose light arrives after traveling toward you for a journey of 100 million years, you’re not looking at a galaxy that’s 100 million light years distant. Rather, you’re seeing a galaxy that’s significantly farther away than that!

The reason for this is that on the largest scales — objects that aren’t gravitationally bound together into galaxies, groups or clusters — the Universe is expanding. The longer it takes a photon to travel from a distant galaxy to your eyes, the greater the role of the Universe’s expansion, implying that the most distant galaxies are even farther away than the amount of time the light from them has been traveling.

expanding universe
This simplified animation shows how light redshifts and how distances between unbound objects change over time in the expanding Universe. The farther a galaxy is, the faster it expands away from us, and the more its light appears redshifted. A galaxy moving with the expanding Universe will be even a greater number of light years away, today, than the number of years (multiplied by the speed of light) that it took the light emitted from it to reach us. (Credit: Rob Knop)

This shows up as a cosmic redshift. Since light is emitted with a particular energy, and hence a particular wavelength, we fully expect that it will arrive at its destination with a particular wavelength as well. If the fabric of the Universe were neither expanding nor contracting, but rather were constant, that wavelength would be the same. But if the Universe is expanding, the fabric of that space is stretching as shown in the video above, and hence the wavelength of that light becomes longer. The great redshifts we’ve observed for the most distant galaxies have absolutely verified this picture.

Distant galaxies, like those found in the Hercules galaxy cluster, are not only redshifted and receding away from us, but their apparent recession speed is accelerating. Eventually, we will cease to receive light from beyond a certain point from them. (Credit: ESO/INAF-VST/OmegaCAM. Acknowledgement: OmegaCen/Astro-WISE/Kapteyn Institute)

But we can do much more than determine that the Universe has expanded and continues to expand. We can use all the information we gather to conclude how the Universe has expanded over its history, which in turn tells us what the Universe is composed of.

Once the light leaves a distant, cosmic source, the expanding Universe stretches the wavelength of that light. This leads to a redshift, where the more distant objects will have their light redshift for longer amounts of time, when different components of the Universe (like dark energy, matter, or radiation/neutrinos) were more important.

expansion of the Universe
Two of the most successful methods for measuring great cosmic distances are based on either their apparent brightness (L) or their apparent angular size (R), both of which are directly observable. If we can understand the intrinsic physical properties of these objects, we can use them as either standard candles (L) or standard rulers (R) to determine how the Universe has expanded, and therefore what it’s made of, over its cosmic history. (Credit: NASA/JPL-Caltech)

By measuring sources at a whole slew of distances, discovering their redshift and then either measuring their intrinsic vs. apparent size or their intrinsic vs. apparent brightness, we can reconstruct the entire expansion history of the Universe.

In addition, since the way the Universe expands is determined by the various types of matter and energy present within it, we can learn what our Universe is made out of:

  • 68% dark energy, equivalent to a cosmological constant,
  • 27% dark matter,
  • 4.9% normal (protons, neutrons and electrons) matter,
  • 0.1% neutrinos and antineutrinos,
  • about 0.008% photons, and
  • absolutely nothing else, including no curvature, no cosmic strings, no domain walls, no cosmic textures, etc.
Friedmann equation
The relative importance of different energy components in the Universe at various times in the past. Note that when dark energy reaches a number near 100% in the future, the energy density of the Universe (and, therefore, the expansion rate) will remain constant arbitrarily far ahead in time. Owing to dark energy, distant galaxies are already speeding up in their apparent recession speed from us. (Credit: E. Siegel)

Once we know the components of the Universe to this degree of precision, we can simply apply this to the laws of gravity (given by Einstein’s General Relativity), and determine the future fate of our Universe. What we discovered, when we first applied this to the discovery of a dark energy-dominated Universe, was shocking.

First off, it meant that all the galaxies that weren’t already gravitationally bound to us would eventually disappear from view. They would speed away from us at an ever-increasing rate as the Universe continued to expand and expand and expand, unchecked by gravitation or any other force. As time went on, a galaxy would get more distant, meaning that there was an increasing amount of space between that galaxy and ourselves. The galaxy appears to move away at greater and greater speeds, due to the expansion of space.

The GOODS-North survey, shown here, contains some of the most distant galaxies ever observed, some of which have had their distances independently confirmed. A great many the galaxies imaged in this image are already unreachable by us, even if we left today at the speed of light. (Credit: NASA, ESA, and Z. Levay)

But this leads to an inevitable conclusion that is even more disturbing. It means that, at a particular, key distance from us, due to the expansion of the fabric of space itself, a photon either leaving our galaxy toward a distant one or approaching ours from a distant galaxy will never reach us. The expansion rate of the Universe is so great that distant galaxies become unreachable to our own, even if we were to move at the speed of light!

At present, that distance is “only” about 18 billion light years away, as the matter and radiation density is still dropping, and so is the overall expansion rate (when measured in km/s/Mpc).

If you consider that our observable Universe is some 46 billion light years in radius, and that all regions of space contain (on average and on the largest scales) the same number of galaxies as one another, it means that only about 6% of the total number of galaxies in our Universe are presently reachable by us, even if we left today, and traveled at the speed of light.

The size of our visible Universe (yellow), along with the amount we can reach (magenta). The limit of the visible Universe is 46.1 billion light-years, as that’s the limit of how far away an object that emitted light that would just be reaching us today would be after expanding away from us for 13.8 billion years. However, beyond about 18 billion light-years, we can never access a galaxy even if we traveled toward it at the speed of light. (Credit: Andrew Z. Colvin and Frederic Michel, Wikimedia Commons; Annotations: E. Siegel)

It also means that, on average, between twenty and sixty thousand stars transition every second from being reachable to being unreachable. The light they emitted a second ago will someday reach us, but the light they emit this very second never will.

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It’s a disturbing, sobering thought, but there’s also a more optimistic way to view it: this is the Universe reminding us how precious every second is. It’s the Universe telling us that if we ever want to travel beyond our own Local Group — beyond the gravitationally bound set of objects made up of Andromeda, the Milky Way and about 60 small, satellite galaxies — that every moment we delay is another opportunity being lost.

dark energy
The different possible fates of the Universe, with our actual, accelerating fate shown at the right. After enough time goes by, the acceleration will leave every bound galactic or supergalactic structure completely isolated in the Universe, as all the other structures accelerate irrevocably away. After another few tens of billions of years, only the Local Group will be reachable any longer. We can only look to the past to infer dark energy’s presence and properties, which require at least one constant, but its implications are larger for the future. (Credit: NASA & ESA)

Of the estimated two trillion galaxies in our Universe today, only about 6% of them are still reachable from the point of view of the Milky Way, and that number is getting smaller all the time. This also means that 94% of the galaxies in our observable Universe are already out of humanity’s reach, owing to the accelerated expansion of the Universe caused by dark energy. Every galaxy beyond our Local Group, as time goes on, is destined for that same fate.

Unless we develop the capacity for intergalactic travel and head out to other galaxy groups and clusters, humanity will forever be stuck in our Local Group. As time goes on, our ability to send or receive signals to what lies beyond in the great cosmic ocean will fade from view. The accelerated expansion of the Universe is relentless, and the gravity we have isn’t strong enough to overcome it. The Universe is disappearing, and we’re absolutely powerless to stop it.


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