Universe Expansion

Universe Expansion

Six square images show different spiral galaxies: NGC 5247, Messier 100, NGC 1300, NGC 4030, NGC 2987, and NGC 1232, each with bright centers and spiral arms.
At and beyond the current frontiers of knowledge, many physicists have strongly held opinions. Can surveys point the way to breakthroughs?
A digital illustration exploring the origin of the universe—depicting a blue energy burst on the left and a geometric white grid forming a funnel shape on a purple background, evoking one of the biggest mysteries in science.
The original idea of the Big Bang was synonymous with a singularity: a point of zero volume. In this Universe, things never got that small.
A cartoon tooth fairy holds a tooth and magic wand, standing before colorful cosmic microwave background maps, blending whimsy with the wonders of theoretical physics.
Theoretical physics is notorious for wild ideas that seem, at first, to be nonsensical fantasies. That's where the tooth fairy comes in.
Illustration of multiple spiral galaxies and stars being pulled toward a central black hole in deep space, with blue and purple light streaks tracing the motion along a dark energy curve that shapes the universe.
Today, in the here-and-now, a full 13.8 billion years have elapsed since the start of the hot Big Bang. But would that be true for everyone?
atom quantum
In physics, we reduce things to their elementary, fundamental components, and build emergent things out of them. That's not the full story.
A dense star field and distant galaxies with bright galaxy clusters and several white squares highlighting specific points in the image.
Only nearby objects appear to the naked eye. With telescopes of all types, especially in space, we've smashed those records many times over.
A deep space image showing numerous distant galaxies of various shapes and sizes scattered across a dark background, revealing just how empty is space between these cosmic islands.
There's a lot of room in interplanetary, interstellar, and intergalactic space, but just how low the densities go is truly mind-boggling.
two particles different wavelength speed of light
Contrary to common experience, not everything needs a medium to travel through. Overcoming that assumption removes the need for an aether.
An Ishihara color blindness test with colored dots, showing letters “u” and “d” in black, and a magnified section highlighting the dot pattern—inviting viewers to observe proton decay through subtle visual cues.
"Color" with respect to the strong force is just an analogy. Here's how to understand it without colors, group theory, or any advanced math.
Two highways, "Early Route" and "Late Route," marked 67.2 and 73.5, traverse a cosmic background with gradients and data—highlighting the Hubble tension and potential bad measurement in determining universal expansion rates.
The distance ladder and the CMB give incompatible values for the expansion rate. A new study shows just how robust the Hubble tension is.
Known as the "past hypothesis" problem, the Universe's initially low entropy has long puzzled scientists. Now, cosmic inflation solves it.
apollo 8 earthrise
As the world teeters on the brink of nuclear war, distant, advanced civilizations would never know it. Earth appears peaceful from far away.
black hole merger
As light travels across the Universe, it's subject to cosmic expansion, changing fields, and relative motion. How about gravitational waves?
A colorful map shows the distribution of nearby galaxies, with distances and redshift factors labeled, created by DESI; NSF, NOIRLab, and Kitt Peak logos are visible.
Is dark energy evolving with at least 99.99% confidence? Despite the quality of recent data, scientists have every reason to be skeptical.
logarithmic history of universe
In a 13.8 billion year old Universe, a few seconds hardly seems like it matters. But these minuscule changes sure do add up over time.
Two peculiar galaxies collide in deep space, forming bright clusters and swirling dust clouds—a striking scene that reveals the beauty and violence of the cosmos against a dark background.
Most massive galaxies are spiral or elliptical shaped. But peculiar galaxies showcase the beautiful violence that helps explain our cosmos.
Illustration of multiple spiral galaxies and stars being pulled toward a central black hole in deep space, with blue and purple light streaks tracing the motion along a dark energy curve that shapes the universe.
Early on, the Universe needed near-perfect flatness, or atoms, stars, and galaxies couldn't form. What happens once dark energy takes over?
bok globule barnard 68 dust wavelength
The image you're seeing isn't a hole in the Universe, and the cosmic voids that do exist aren't hole-like at all.
A person sits on a chair against a white backdrop with abstract black dotted patterns, set against a yellow background.
1hr 16mins
NASA astronomer Michelle Thaller makes the case that quantum entanglement may be the underlying fabric from which spacetime itself emerges. 
Looking up at the night sky gives us a glimpse of the Universe beyond our terrestrial concerns. Here's the science of what's out there.
No matter what physical system we consider, nature always obeys the same fundamental laws. Must it be this way, and if so, why?
Bald man in a blue shirt gestures with both hands in front of him, palms facing each other, against a plain white background.
7mins
Jim Al-Khalili explains how the past and future are more fluid than we may think.
travel straight line
In theory, the fabric of space could have been curved in any way imaginable. So why is the Universe flat when we measure it?
Binary black holes eventually inspiral and merge. That's why the OJ 287 system is destined for the most energetic event in history.
M81 Group
Over billions of years, fewer stars form, galaxies mutually recede, and the Universe becomes ever darker. Here's how fast it all happens.
Millikan Lemaitre and Einstein
Not everyone accepts the scientific consensus; some even make careers out of challenging it. But only a select few do it the right way.
Side-by-side images of a nebula in space, showing colorful, wispy gas and dust shells surrounding a bright central region with numerous stars in the background.
Resembling a cosmic brain, the Exposed Cranium Nebula instead shows a dying, massive star, as JWST reveals. Its fate remains uncertain.
warm-hot intergalactic medium sculptor wall
In traveling through the expanding Universe, particles slow down while light and gravitational waves redshift. What degrades and what won't?
particle physics destroy universe
Smashing things together at unprecedented energies sounds dangerous. But it's nothing the Universe hasn't already seen, and survived.
No civilization, no matter how successful, can last forever. What does the non-detection of intelligent aliens mean for our own longevity?