object

star

A massive, luminous sphere of plasma held together by its own gravity.
12 related articles

Description

A star is a massive, luminous sphere of plasma held together by its own gravity. The immense pressure and temperature in its core trigger nuclear fusion, converting hydrogen into helium and releasing energy that counteracts the inward pull of gravity. Stars are the fundamental building blocks of galaxies, and their life cycles — from birth in nebulae to death as white dwarfs, neutron stars, or black holes — drive the chemical evolution of the universe, producing heavy elements that later form planets and life.

History

The understanding of stars as fusion-powered objects developed in the early 20th century. Arthur Eddington proposed in the 1920s that stars are powered by nuclear reactions, and Hans Bethe worked out the specific fusion chains in 1938-39, for which he later received the Nobel Prize.

How it works

Stars form from the gravitational collapse of dense regions in molecular clouds. As the core heats up, fusion ignites, creating an outward pressure that balances gravity in a state of hydrostatic equilibrium. The energy generated by fusion slowly works its way to the surface and is radiated into space. The star's mass determines its temperature, luminosity, and lifetime: more massive stars burn hotter and die faster, while smaller stars like our Sun can shine for billions of years.

In practice

Stars serve as natural laboratories for studying plasma physics, nuclear reactions, and extreme states of matter. They also act as 'cosmic furnaces' that produce the elements necessary for life, and their light is used to measure distances and the expansion of the universe.

Fun fact

The Sun alone converts about 600 million tons of hydrogen into helium every second, yet it has enough fuel to continue shining for another 5 billion years.

Concept graph →

Related articles · 12

Star Polymers Embrace Their Prey
An octopus waits with tentacles spread wide. No central controller directs its arms, but the moment prey touches one, all eight wrap around it. Physicists have recreated a similar trick in the lab with a body that has neither neurons nor muscles: a star polymer with self-propelled arms. The polymer was assembled from small cylindrical vibrobots on a vibrating plate.
HEP Phenomenology2026-07-212 minarXiv:2607.19469express
Why Bubbles Don't Immediately Turn into Matter
Boiling water in a pot is a good place to start. Bubbles of steam rise, pop, and the surface settles down. Something similar might have happened in the first moments of the universe's life with a special field filling space: bubbles of a new phase inflated and collided, like islands of steam in liquid.
Galaxies2026-07-083 minarXiv:2607.07973
High Energy2026-06-141 minarXiv:2606.15759express
The Law of Unified Cooling: What Links Blazars and Gamma-Ray Bursts
Blazars are long-lasting beams from black holes at the centers of galaxies. Gamma-ray bursts are the briefest flashes from supernova explosions or neutron star mergers. The former act like eternal spotlights, the latter like camera flashes.
HEP Theory2026-05-312 minarXiv:2606.01103express
Dark Matter as a Drop of Quantum Liquid
A lump of dark matter drifts through the void — invisible, almost intangible. No one knows what it's made of, but a new study suggests viewing it as a drop of quantum liquid. Two kinds of fermion particles — call them "heavy" (ψ) and "light" (χ)—exchange signals via a third mediator particle (φ), like floats tied to a single line.
Stellar2026-04-302 minarXiv:2605.00102express
How Cold Clouds Survive in the Fire of the Sun
In the scorching solar corona, where temperatures soar past a million degrees, float cold, dense clouds — solar prominences. They hang for weeks, neither falling nor dissolving, like icebergs in a boiling ocean. How they got there is a question that has puzzled astronomers for decades.
Galaxies2026-04-201 minarXiv:2604.17955express
Gas Jumps Over the Ring
A river flows toward a whirlpool, but a dam with a notch blocks the way. Most water piles up before the dam, but some, gaining height, leaps over it and falls straight into the funnel. So it is with gas in a galaxy: it streams toward the center but hits a ring of stars and gas, like a dam. Usually, everything stops there, swirling into a dense vortex.
Galaxies2026-03-052 minarXiv:2603.04784express
How black holes could have assembled galaxies
Dough rises faster when it already contains yeast. Similarly, galaxies may have assembled faster if they already had black holes inside. Astrophysicists considered a scenario where the universe contained primordial black holes from the very beginning — objects that could have formed in the first instants after the Big Bang.
Galaxies2026-01-161 minarXiv:2601.11515express
Galaxies2026-01-132 minarXiv:2601.08791express
Galaxies2026-01-081 minarXiv:2601.05316express
Black Holes as Unexpected Beacons of the Early Universe
A few hundred million years after the Big Bang, the universe resembled an endless dark ocean, shrouded in a thick fog of neutral (non-ionized) hydrogen. Then something dispersed the gloom: ultraviolet radiation knocked electrons out of atoms, making the gas as transparent as pure water.
Biological Physics2025-11-091 minarXiv:2511.08624express
Which Stars Can Give Birth to Life? The Answer's in the Color
Life began with molecules akin to natural sunscreen — based on carbon, they soaked up the mild ultraviolet of the young Sun and turned it into heat. This way of dissipating energy wasn’t just heating: it made molecules self-organize, like chefs kneading structured dough out of a chaos of ingredients. But ultraviolet is a finicky tool.