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Quasar Winds Race at One-Third Light Speed

Original: "The WISSHFUL program: the highest redshift UFO discovered in a non-lensed QSO"
arXiv:2606.05312v1 · 2026-06-03 · CC BY · ⏱ 1 min · High Energy Galaxies
An ancient quasar ejects gas at one-third the speed of light, unveiling the mystery of galaxy growth.
Abstract

Astronomers have peered at a distant supermassive black hole that's greedily gobbling matter while blasting out ferocious gas streams. These 'winds' race at up to a third of light speed — think cosmic engine exhaust. A single gust could scatter an entire galaxy. So what could possibly stop this hurricane?

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A quasar is a supermassive black hole at the center of a galaxy, consuming gas with a bright glow. In the era of “cosmic noon”, 12 billion years ago, such objects were not rare. Astronomers peered into that time with X-ray telescopes and for the first time saw two hurricane-like winds at quasar WISSH13. One gas stream races at one-third the speed of light — 100,000 km/s. It is not constant: in gusts it ejects as much matter as the black hole consumes. These winds blow out the building material for stars, preventing the galaxy from growing uncontrollably. The flows arise at the very edge of the abyss, near the Schwarzschild radius (the point of no return), and heat the surrounding gas to 200 million degrees, increasing disorder in the system. They also affect the distribution of dark matter — the invisible scaffolding of galaxies. The redshift, discovered by Edwin Hubble, helped measure the distance, and spectral analysis revealed the composition of the winds. This is reminiscent of black hole thermodynamics by Bekenstein.

🎯 If the fast wind particles traveled from Earth to the Sun, they would arrive in just over an hour — sunlight needs 8 minutes for the same journey.

🎬 The concept of ultra-fast winds steering the fate of a galaxy is reminiscent of the “Star Vortex” from Isaac Asimov’s novels, where the evolution of civilizations depended on global energy flows.

$$1+z_a = \sqrt{\frac{1+\beta}{1-\beta}},\quad \beta = v/c$$
Relation between the observed redshift of an absorption line (z_a) and the wind speed (v) in units of the speed of light (c)
$$\dot{M}_{out} = \Omega N_H m_p v_{out} r$$
Mass loss rate through the wind, where Ω is the covering factor, N_H is the column density, m_p is the proton mass, v_out is the speed, and r is the launch radius
Scientists
Adam RiessBrian SchmidtEdwin HubbleGeorges LemaîtreMaarten SchmidtSaul Perlmutter
Tags
quasar black hole galaxy spectroscopy expansion of the universe speed of light entropy dark matter
Laws
Hubble's lawsecond law of thermodynamicsDoppler effectHawking radiationgravitational lensingprinciple of constancy of the speed of light
Original: arXiv:2606.05312v1 · CC BY · bridge42worlds