Astronoo - Back to homepage
X (new window) Bluesky (new window) Pinterest (new window)
English Français Español Português 日本語 Deutsch 中文
Last updated: February 2, 2022

Dark Night Paradox or Olbers' Paradox

Why is the night sky dark

Stars have a finite age and thus a finite lifespan. Their light source is too ephemeral to saturate space with their radiation. Credit: Stellarium image

Why is the night sky dark?

"The night is only night for us. It is our eyes that are dark." This quote from René Barjavel (1911-1985) in the science fiction novel "The Night of Times" could be the answer to the question: Why is the night sky dark?
Each of us might simply admit that the cause of the dark night is the absence of the Sun above the horizon, but this is not a good answer.
Indeed, the night is dark, and before the 20th century, the universe was assumed to be static, infinite, and populated with stars. For several centuries, these two ideas would remain paradoxical!
Evidently, the night has always been dark. But if the universe were infinite in space and time, no matter which direction you looked, your line of sight should intersect with a star, even a very distant one. The sky should therefore appear as bright as the Sun everywhere. However, we find that the night is essentially dark!
This assertion, known as Olbers' paradox, was studied in 1826 by Heinrich Olbers (1758-1840). However, the question had been posed since 1576 by Thomas Digges (1546-1595) in a publication where he distributed stars randomly throughout the celestial sphere. This view of the sky led him to ask, "Why do this infinity of stars not make the night sky bright?" His answer was that most of them were too far to be seen, but this is not a good answer.
In 1610, in his supportive letter to Galileo "Dissertatio cum Nuncio Sidereo" (Conversation with the Celestial Messenger), Johannes Kepler (1571-1630) seems to dismiss the notion of an infinite Universe.
Although many astronomers have pondered this question, the resolution of this paradox remained unresolved for three centuries.

Why Should an Infinity of Stars Illuminate the Night Sky?

Edmond Halley (1656-1742) and Jean-Philippe Loys de Chéseaux (1718-1751) provided a mathematical answer to this question. De Chéseaux, in 1744, inspired by Halley's work, imagined the sky as a series of concentric spherical layers of constant thickness centered on the observer. Thus, the number of stars in each layer is proportional to its surface area, hence the square of its radius. In other words, at a distance 2d there are 4 times more stars, at a distance 4d there are 16 times more stars, etc.
However, the brightness of a star is inversely proportional to the square of its distance. In other words, if a star has a certain brightness at a distance d, at a distance 2d, it is 4 times less bright. The flux from a star decreases as the inverse of the square of the distance ƒ(e)=L/4πr² (L=luminosity).
Thus, if the universe is infinite, we have an infinity of layers with the same brightness, and the observer receives the same amount of light energy from each layer. The total brightness should be infinite.
We now know that this assertion is incorrect because stars have a finite lifespan.

Why Not Simply Consider That the Cosmic Medium Is Not Transparent Everywhere?

Thus, light from stars could be blocked by interstellar dust and gas. This explanation is also incorrect because the medium would gradually heat up by absorbing light and become as bright as the surface of a star. This does not resolve Olbers' paradox.

Why Not Consider That Light from Distant Stars Has Not Had Time to Reach Us?

Indeed, in 1848 Edgar Allan Poe (1809-1849) intuitively presented this hypothesis in his essay on the material and spiritual universe titled "Eureka."
Indeed, the speed of light being finite (as known at that time), it takes a certain time to reach us. But this hypothesis is not correct in an infinite and eternal Universe. If the Universe is eternal, no matter how long it takes for light to reach us, it should already dazzle us.
In 1901, William Thomson, known as Lord Kelvin (1824-1907), demonstrated that in a transparent, uniform, and static universe, uniformly filled with stars, the finite age of stars prevented the visibility of distant stars.
To resolve this simple paradox of the black night, it was necessary to completely revise our conception of the Universe.
Behind the story of Olbers' paradox lay a disturbing cosmic reality from which several concepts emerged at the end of the 20th century.
- The Universe has not always existed; it has a history and is 13.77 billion years old.
- The speed of light (300,000 km/s) is finite, and thus the Universe has a finite size. In 13.77 billion years, photons have traveled 13.77 billion light-years.
- Stars have a finite age and thus a finite lifespan. Their light source is too ephemeral to saturate space with their radiation.
- The Universe is expanding at an accelerated rate. The sky is getting darker as light from distant galaxies is increasingly redshifted (Doppler effect). The most distant galaxies, losing their brightness, are extremely difficult to observe.

Conclusion

All these hypotheses must be combined to solve the Dark night paradox.
"The night is only night for us. It is our eyes that are dark."
In infrared observations, distant galaxies reveal gigantic glows that illuminate interstellar dust. For every point in the sky, our line of sight intersects the infrared flux of a galaxy.
But the most original brightness is found in the microwaves. This cooled fossil radiation is observed in all directions of the sky.

Cosmic Microwave Background

This complete map of the CMB (Cosmic Microwave Background) shows temperature fluctuations in the primitive Universe when it became transparent ~380,000 years after the Big Bang. The maximum temperature difference between the cold blue regions and the hot red regions is about 0.0001 °C. Credit: Montage of images taken by Planck (new window) (ESA satellite) over 9 years.

🏠

To explore in this category

Beyond Our Senses: What the Universe Still Hides from Us
Little Red Dots: The Compact Enigmas of the Early Universe
The Weak and Strong Anthropic Principles: Two Ways of Reading the Same Universe
The Universe: Matter... or Information?
Dark Energy: The Most Mysterious Force in the Universe
The Fountains of Creation: The Myth of White Holes
The Great Silence: 10 Insurmountable Walls to Meeting E.T.
The 5 Cosmic "End of the World" Scenarios (and Why They Won't Happen)
Why the Cause Always Precedes the Effect: The Order of the World is Written in This Principle
Absolute Zero and Nothingness: Two Limits the Universe Refuses to Reach
Economical Nature: The Secrets of Conserved Quantities
The Incredible Precision of the Universe's Laws: Chance or Necessity?
The Mystery of the Arrow of Time: Why Can't We Go Back?
The Big Bang: At the Frontiers of the Model
When Space Bends: The Tiny Slope That Guides the Universe
Nabataean Astronomy: Masters of the Desert Between Starry Skies and Stone Constructions
Polynesian Astronomy: The Art of Navigating the Pacific Ocean
Mesopotamian Astronomy: The Cradle of Celestial Observation
Andean Astronomy: A Sacred Link Between Sky and Earth
Ancient Persian Astronomy: Between Babylon and the Islamic Golden Age
Mayan Astronomy: Celestial Cycles Dictated Religious, Agricultural, and Political Time
Islamic Astronomy: When Baghdad Illuminated the Sky of Science
Indian Astronomy: From Sacred Poetry to Scientific Thought
Ancient Greek Astronomy: The Universe of Philosophers in Search of Cosmic Order
The Three Cosmic Shapes: A Hidden Geometry of the Universe
Egyptian Astronomy: Between Sky and Nile, the Secrets of Time
Babylonian Astronomy: When the Sky Predicted Destiny
Chinese Imperial Astronomy: A Millennial Scientific Legacy
Extreme Cosmic Objects: Where Physics Explodes
Mirror Universe: Coexistence of Two Worlds in a Cosmic Reflection
The first second of our history
Time Dilation: Relativistic Mirage or Reality?
Space Through Time: A Constantly Evolving Concept
The Expanding Universe: What Does "Creating Space" Really Mean?
From Nothingness to the Cosmos: Why Is There Something Rather Than Nothing?
How can the Universe measure 93 billion light-years?
How can we say that the Universe has an age?
First Proof of the Expansion of the Universe
Space-time slices of the observable Universe
When the Universe Was Blind: The Long Night Before the First Stars
Alternative theories to the accelerated expansion of the universe
The primitive atom: the first cosmological theory
Great walls and filaments: the great structures of the Universe
The Origins of the Universe: A History of Cosmic Representations
Lyman-alpha Blobs: Gaseous Traces of the First Galaxies
Gamma-Ray Bursts: The Ultimate Breath of Giant Stars
Perspective on the Inflation of the Universe
The Planck Universe: the Image of the Universe Becomes Clearer
The sky is immense with Laniakea
The Symmetries of the Universe: A Journey Between Mathematics and Physical Reality
The Geometry of Time: Exploring the Fourth Dimension of the Universe
How to measure distances in the Universe?
Why ‘nothing’ is impossible: Do nothingness and emptiness exist?
The Horizon Problem: Understanding the Uniformity of the Cosmos
What is Dark Matter? The Invisible Force Shaping the Universe
Metaverse, the next stage of evolution
Multiverse: An Ocean where each Spacetime Bubble has its own Physical Laws
Cosmological Recombination: When the Universe Became Transparent
The cosmological and physical constants of our Universe
The Thermodynamics of the Sandpile and the Avalanche Effect
The engine of the accelerated expansion of the Universe
The X-Ray Universe: When Space Becomes Transparent
The oldest galaxies in the universe
The Observable Universe as Seen Through the Cosmic Microwave Background
Hubble constant and expansion of the Universe
Dark Energy: When the Universe Defies Its Own Gravity
What is the Size of the Universe? Between Cosmological Horizon and Infinity
Quantum Vacuum and Virtual Particles: The Physical Reality of Nothingness
Paradox of the dark night
Journey into the Heart of Paradoxes: The Enigmas That Revolutionized Science
Enigma of the Missing Mass: Dark Matter and Dark Energy
The X-Ray Universe: When Space Becomes Transparent
Cosmic Microwave Background: The Thermal Echo of the Big Bang