How Far Back Into The Past Can We See In The Night Sky?

Table of Contents (click to expand)

Relativity tells us that looking at more distant objects allows us to look further back in time, but there is a limit to how far back we can go.

When we look into the night sky, we can see various types of astronomical objects. They range from planets, moons and stars to nebulae, star clusters, and nearby galaxies. With better and more sophisticated telescopes, we can also see more distant and compact objects, such as faraway galaxies, galaxy clusters, and neutron stars.

It should not surprise you that these objects are very far away!

Hubble Extreme Deep Field
This is an image take by the Hubble Space Telescope, called the Hubble Extreme Deep Field. Photographic attempts like these are made to capture the most distant parts of the universe. (Photo Credit : Flickr)


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Distances And Time

Einstein’s theory of relativity implies that when we look at distant objects, we see their historical versions, because light (and consequently information) takes time to reach us due to its limited speed. Thus, as we observe more distant objects, we are actually peering further back in time.

For example, light from the Sun takes eight and a half minutes to reach us. Thus, on Earth, we see the 8.5-minute-old version of the Sun, rather than the Sun in its present and immediate state. If the Sun were to suddenly explode (hypothetically, of course), we would only find out after more than eight minutes had passed.

Similarly, the light from the Large Magellanic Cloud (LMC) takes approximately 200,000 years to reach Earth. Thus, the Large Magellanic Cloud that we are currently observing is around 200,000 years old. In this case, the light takes a much longer time to reach Earth (since it is very far away, as compared to the Sun). Hence, we presently see an older version of the LMC than the Sun.

Large,Magellanic,Cloud
This is an image of the Large Magellanic Cloud. A satellite galaxy of the Milky Way, it is located nearly 200,000 light-years away from Earth. (Photo Credit : John A Davis/Shutterstock)

This is true for all objects out in the universe. Moreover, when the distance measurement is in the units of light-years, that figure is also the time taken by the light from that object to reach us. For example, the distance to the brightest star in the night sky, Sirius, is around 8.6 light-years. This means that, right now, any light emitted from there will take 8.6 years to reach us.

It is important to note that this time taken for light to reach us that we get from the light-years units, is an instantaneous figure. The space between the Earth and these distant objects is also continuously expanding. Thus, over time, light from these objects will need even more time to reach us, as the distance between the Earth and the objects increase. This becomes relevant when we talk about things like the most distant objects we have ever observed.

For example, the most distant individual star we have observed is designated WHL0137-LS, also called, Earendel. It is a star presently around 28 billion light-years away from us. That said, the photometric analysis of the light we observe from this star implies that it took approximately 12.9 billion years to reach us.

Expansion and Evolution of the Universe
An illustration of how the expansion of the Universe plays out. Over time, the expansion causes objects to get further away, causing the light from it to take more time to reach us. (Photo Credit : Designua/Shutterstock)

This discrepancy occurs due to the expansion of the universe. Furthermore, the light that is leaving Earendel at this very instant would take 28 billion years to reach us. Another effect of the universe’s expansion is that the light from the very farthest objects still would not have reached us yet. If the expansion rate is fast enough, it might never reach Earth. However, this article will focus on what is within the observable universe.

So, how far back in time can we see? The present estimates indicate that the universe is around 13.7 billion years old. Can we see the light that has been traveling for that long?

It turns out that there is a limit to this. We cannot see light that is 13.7 billion years old, formed at the instant of the Big Bang, nor during the immediate period after it. Simply speaking, this boundary suggests that we cannot directly see how the Big Bang looked or how the universe appeared way back then.

The most ancient time frame within which we can observe the universe is during the creation of cosmic background radiation (CMBR). It took place approximately 380,000 years after the Big Bang happened. So, to answer the original question: how far back into the past can we see in the night sky? The answer is the age of the universe minus 380,000 years. From our current estimates of the universe’s age, we get a value of around 13.32 billion years of “visibility” back in time.

Cosmic Background Radiation Left After the Big Bang
This is an image of the Cosmic Microwave Background radiation obtained using the Planck satellite. The color coding represents the tiny temperature variations in the CMBR. (Photo Credit : – Flickr)

Also Read: Are You Looking Into The Past When You Look At The Stars?

Epoch Of Recombination

The creation of the CMBR occurred during a period that scientists call the epoch of recombination. Before this epoch, the universe had such a high temperature that matter only existed as plasma, consisting of ionized atoms and free electrons.

The light (or photons) that existed before the recombination epoch contains information about the very early universe, and probably even the Big Bang! However, the ionized plasma would have scattered these photons quite effectively. The photons would bounce from one charged particle to the next, keeping them trapped and altering their properties. As a result, these photons are not available for us to see, as they did not be able to travel freely back then.

Compton scattering diagram in physics
A diagram showing the scattering of photons by a free electron. This phenomena would have been prevalent before the epoch of recombination.  (Photo Credit : zizou7/Shutterstock)

During the epoch of recombination, the universe cooled to about 2700 degrees Celsius. At this temperature, the ions and electrons combined (hence the term ‘recombination’) to form the first atoms.

The photons present at that time would not have been scattered by the newly-formed atoms, and were thus allowed to travel freely for the first time. These photons are what we see as the CMBR. Hence, CMBR is the relic of the radiation left from the Big Bang. We see it in microwave wavelengths, since the universe’s expansion over time would stretch its wavelength to longer values. It also gains the prestigious distinction as the oldest thing we can see in the universe.

Also Read: What Is The Cosmic Microwave Background?

The Dark Age

Big Bang Expansion
This is a schematic diagram of the evolution of the universe, with the CMBR represented as the ‘Afterglow Light Pattern,’ with the Dark Age following it. (Photo Credit : Flickr)

Even though we have observed the CMBR, not much is known about the universe after that point. What followed the CMBR is what scientists refer to as the Dark Age. Once the wavelength of the CMBR shifted towards the infrared section of the spectrum, the universe would have appeared dark to the human eye. Not much is known about the universe during this stage, as the production of new photons did not happen. Only after the formation of the first stars would new photons begin forming again.

In summary, this is the current information we have about the early universe. This knowledge has enabled us to develop theories and cosmological models that explain how the universe became what it is today. However, with telescopes like JWST, which can discover more distant stars and galaxies, we might be able to learn about the aftermath of the epoch of re-ionization. The CMBR, however, will remain the oldest observable feature of our incredible universe!

References (click to expand)
  1. Epoch Of Recombination | COSMOS. Centre for Astrophysics and Supercomputing
  2. Large Magellanic Cloud. Tration
  3. Welch, B., Coe, D., Zackrisson, E., Mink, S. E. de ., Ravindranath, S., Anderson, J., … Vikaeus, A. (2022, November 1). JWST Imaging of Earendel, the Extremely Magnified Star at Redshift z = 6.2. The Astrophysical Journal Letters. American Astronomical Society.
  4. Hubble Telescope Spots the Most Distant Star Ever .... Smithsonian Institution
  5. Then vs. Now: The Age of the Universe. Tration
  6. ESA - Planck and the cosmic microwave background. esa.int
  7. J Miralda-Escude. (2003) [astro-ph/0307396] The Dark Age of the Universe. arXiv
  8. Welch, B., Coe, D., Diego, J. M., Zitrin, A., Zackrisson, E., Dimauro, P., … Broadhurst, T. (2022, March 30). A highly magnified star at redshift 6.2. Nature. Springer Science and Business Media LLC.
About the Author

Anand has a MSc Physics degree NIT Surathkal (India), and is currently undertaking a research project on galaxy evolution. He is passionate about nature and structures of the universe, and hopes to call himself a cosmologist one day. He likes to explore various genres in music; however, he is a metal-head and his favorite bands are Bring Me The Horizon and Deftones. His other interests include swimming and taking road trips.

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