Popular

quasar

13
A quasar is a lighthouse at the center of a distant galaxy. There, a supermassive black hole devours gas and stars, causing a blinding light to flash that is visible across the entire universe.

History

The first quasars were noticed in the 1950s as point-like radio sources. In 1963, Dutch astronomer Martin Schmidt measured the redshift of 3C 273 and realized: the object is incredibly distant and therefore monstrously bright. Calculations were based on Hubble's law, discovered by Edwin Hubble.

How it works

Gravity accelerates infalling matter to near-light speeds. When particles collide, kinetic energy turns into heat — the accretion disk glows white-hot. Excess energy escapes as narrow jets shooting from the poles of the rotating hole.

💡 Quasars shine brighter than a trillion stars, but are no larger than our solar system!
Links in the knowledge graph 1
Scientists
Edwin HubbleKarl Schwarzschild
Related tags
Accretion diskactive galactic nucleusactive galactic nucleusblack holegalaxyjetradio astronomyredshift
Laws
Einstein field equations

Related articles

Black Holes: The Perfect Mask of the Abyss

All the headline discoveries — from mergers detected by LIGO to the image of M87*’s shadow — are interpreted as direct proof of black holes’ existence. But a careful analysis shows that the same signatures arise from any ultracompact horizonless object, if its radius differs from the gravitational r
arXiv:2605.13901v1 · 2026-05-12

Phantom Glow: A Wormhole's Shadow Shines Brighter Than a Black Hole's

Scientists compared images of an Ellis-Bronnikov wormhole and a Schwarzschild black hole with accreting plasma. It turns out the central shadow and photon ring of the wormhole are noticeably brighter—light passes through the throat, adding from the far side of the disk. The result matches Event Hori
arXiv:2606.01699v1 · 2026-06-01

Cradle for a Black Hole: Dark Matter and the Mystery of Red Dots

Observations by the JWST have revealed a population of compact, anomalously red and bright sources in the early Universe — the so-called 'little red dots' (LRDs). Their nature remains a mystery: standard models of stars or active galactic nuclei cannot explain their spectra. One candidate is quasi-s
arXiv:2606.02539v1 · 2026-06-01

Roots from the Abyss: The Secret Growth of Supermassive Black Holes

Astronomers are increasingly finding giant black holes in the early universe, with masses reaching a billion suns. Ordinary gas accretion can't 'fatten' them up fast enough. A new hypothesis introduces an extra dimension: our brane-universe and an invisible donor brane intersect at a shared horizon.
arXiv:2606.03414v1 · 2026-06-02

Red Lanterns of the Cosmos: What Compact Objects from the Early Universe Conceal

Analysis of a hundred 'little red dots' (LRDs) with JWST has shown that their ultraviolet light is redder and more compact than that of ordinary galaxies. Spectral lines of carbon, helium, and hydrogen point to extreme conditions around a black hole, whose radiation seeps through a clumpy envelope.
arXiv:2606.03522v1 · 2026-06-02

Scarlet Invisible Cores: How Hydrogen Fog Conceals Black Holes

Scientists spectroscopically studied 14 'little red dots' (LRD) — compact objects at high redshifts. They decomposed the hydrogen Balmer series lines and found that the anomalously high Balmer decrement values are not due to dust absorption, but to extreme gas density (above 10⁹ cm⁻³). This led to a
arXiv:2606.04711v1 · 2026-06-03

A Cosmic Sketch Without Smudges: JWST Confirms Cold Dark Matter

The JWST peered into the hearts of gravitational lenses — and found not a single smudge expected from lightweight dark matter particles. New data shut down many warm dark matter models and bolster the standard cold scenario. Limits on the half-mode mass and thermal relic mass are among the tightest
arXiv:2606.05277v1 · 2026-06-03

Winds of Cosmic Noon: How Quasar WISSH13 Halts Star Formation

At the peak of star formation, 12 billion years ago, quasar WISSH13 was ejecting two streams of matter at near-light speeds. Analysis of XMM-Newton and NuSTAR data revealed a cold corona and powerful reflection—a sure sign of accretion at the Eddington limit. These ultrafast winds, with kinetic powe
arXiv:2606.05312v1 · 2026-06-03

Quiet Quasar: Ultraviolet Storm at a Third of Light Speed

The quasar SDSS J2318, pretending to be a quiet one with weak emission lines, concealed inside a furious wind accelerated to 0.3 the speed of light. This outflow is capable of sweeping the interstellar medium out of its host galaxy, forever halting star birth. The discovery, made through spectroscop
arXiv:2606.06226v1 · 2026-06-04

Quasi-stars: The Furnaces Where Supermassive Black Holes Are Born

The James Webb Space Telescope has spotted mysterious "Little Red Dots" in the early universe—compact objects that don't fit standard models. A new study suggests they may be quasi-stars: black holes shrouded in a dense gas cocoon that thermalizes radiation like a giant furnace. Calculations using t
arXiv:2606.06575v1 · 2026-06-04

The Rapids of a Black Hole: The Birth and Death of Blanets

In the turbulent disks of active galactic nuclei, blanets form—giant planets of incredible density. Drifting toward the central black hole, they are torn apart by tidal forces, generating brief but dazzling flares in optical and ultraviolet light. Their density allows them to approach the horizon of
arXiv:2606.06884v1 · 2026-06-05