The observable universe — the part we can actually see and measure — is roughly 93 billion light-years across. That's the region from which light has had time to reach us since the universe became transparent.

That number isn't the size of the entire universe, though. Space itself has expanded while light from distant galaxies traveled toward us, so extremely distant objects are now much farther away than a simple age-times-speed-of-light calculation would suggest.

Scientists don't currently know the total size of the universe. It could be vastly larger than the observable universe — and it may even be infinite.

We don't know. Observations show the observable universe is extremely large and that space is very close to geometrically flat on the scales we can measure — but a flat universe doesn't automatically mean an infinite one.

The universe could be infinite, or it could be finite but so enormous that we simply can't detect its overall shape from our observable region. Scientists therefore distinguish carefully between what we can observe and what the entire universe actually contains.

We don't currently know whether the question "what happened before the Big Bang?" even has a meaningful answer in the conventional sense.

The Big Bang model describes the early hot, dense, expanding universe — it doesn't necessarily describe an ordinary explosion happening at one location in pre-existing space. Our current physical theories become incomplete when we try to describe the earliest moments, particularly where quantum mechanics and gravity must be treated together.

There are hypotheses involving inflation, quantum cosmology, and bouncing universes, among others — but none has been established as the definitive answer.

Dark matter is the name scientists give to an unseen form of matter whose presence is inferred from its gravitational effects. It doesn't appear to emit, absorb, or reflect light the way normal matter does, so we can't see it directly with ordinary telescopes.

Its gravitational effects help explain the motions of stars and galaxies, the behavior of galaxy clusters, and gravitational lensing. Current estimates suggest ordinary matter makes up about 5% of the universe, dark matter about 27%, and dark energy about 68%.

Scientists still don't know exactly what dark matter is made of.

Dark energy is the name scientists give to whatever is responsible for the universe's observed accelerated expansion. Astronomers discovered in the late 1990s that cosmic expansion is speeding up rather than simply slowing under gravity.

The leading explanation is a cosmological constant associated with the energy of empty space, but scientists don't yet know what dark energy fundamentally is. Other possibilities include evolving fields or modifications to our understanding of gravity itself. It's estimated to account for roughly 68% of the universe's mass-energy budget.

The observable universe is the portion of the universe from which light or other information has had time to reach Earth since the early universe. It's currently estimated to be roughly 93 billion light-years across.

The observable universe is centered on the observer — a civilization in a distant galaxy would have its own observable universe, centered on its own location. It's therefore not necessarily the entire universe.

We don't know. The idea of parallel or multiple universes appears in several theoretical frameworks in physics and cosmology, including some interpretations of quantum mechanics and certain models of cosmic inflation.

However, there is currently no direct observational evidence confirming that other universes exist. Parallel universes should be understood as a theoretical possibility being actively studied, not as an established discovery.

The ultimate fate of the universe depends on how cosmic expansion, dark energy, gravity, and the universe's contents behave over extremely long timescales.

The leading scenario under the simplest interpretation of today's observations is continued expansion, eventually leading to a very cold, dilute universe sometimes called the "Big Freeze" or heat death. Other possibilities — including a Big Rip or Big Crunch — have been studied under different assumptions about dark energy and cosmology. The exact fate isn't known with certainty.

We don't know. Earth is currently the only world known to host life. However, astronomers have discovered thousands of planets orbiting other stars, including worlds that may have environments capable of supporting some of the conditions associated with life.

Scientists are searching for signs of life through observations of planets, moons, atmospheres, radio signals, and other potential biosignatures. So far, there is no confirmed evidence of extraterrestrial life. This remains one of the biggest unanswered questions in science.