The observable universe contains the mass of 75 billion trillion Suns. Yet if you could somehow put the entire cosmos on a scale, it would weigh exactly zero.
While weight and mass are often used interchangeably on Earth, they measure entirely different things in astrophysics. Weight is the gravitational force exerted on an object by another massive body. An object has weight because a planet or star's gravity pulls it downward. Because the universe encompasses everything that exists, there is no outside body to exert a gravitational pull on it. Without an external gravitational field, the concept of weight ceases to exist.
Mass, however, is an intrinsic property of matter. It measures how much physical substance is present, regardless of gravity. While the universe has no weight, it absolutely has mass.
Determining that total mass comes with a cosmic caveat: astronomers can only calculate the mass of the observable universe. Because light travels at a finite speed, telescopes can only detect objects whose light has had time to reach Earth since the Big Bang. If the entire universe beyond that horizon is infinite, as many cosmologists suspect, its total mass is also infinite.
To estimate the mass of the finite, observable portion, astrophysicists rely on the universe's critical density. By studying the cosmic microwave background and the expansion rate of space, they have calculated the total mass-energy density of the universe to be roughly kilograms per cubic meter. That is equivalent to about five hydrogen atoms in a volume the size of a standard washing machine.
Multiplying that density by the total volume of the observable universe—a sphere roughly 93 billion light-years across—yields a total mass-energy of approximately kilograms.
This calculation—a 3 followed by 54 zeros—includes everything. However, ordinary matter—the protons, neutrons, and electrons that make up stars, planets, and gas clouds—accounts for only 5% of that total. About 27% is dark matter, an invisible substance that binds galaxies together. The remaining 68% is dark energy, the force driving the universe's accelerating expansion, which contributes to the total mass via Einstein's mass-energy equivalence ().
Isolating just the ordinary matter, the mass of the observable universe is roughly kilograms. This 5% fraction of reality accounts for every star, planet, and gas cloud astronomers have ever detected.
