Popular

Maarten Schmidt

1929- · astronomy, astrophysics
Dutch-American astronomer who in 1963 deciphered the spectrum of the mysterious object 3C 273 and discovered quasars — the most distant and powerful sources of radiation in the Universe. This discovery radically changed ideas about the scale and evolution of the cosmos.

Biography

Born in Groningen, Netherlands. Studied astronomy at Leiden University under Jan Oort, one of the pioneers of radio astronomy. In 1959, moved to the USA and began working at the California Institute of Technology. Became professor of astronomy at Caltech, later directed the Hale Observatories. Member of the U.S. National Academy of Sciences. Awarded the Bruce Medal, the Henry Norris Russell Lectureship, and other honors. The asteroid 10430 Martschmidt is named after him.

Key discoveries

💡 Schmidt had long been unable to understand the spectrum of 3C 273 until he realized that the Balmer series lines were strongly redshifted. The insight came to him while driving home. He later said that the discovery process was like assembling a puzzle without a picture — the pieces suddenly came together into a single image.
Quote: "When I realized that the lines in the spectrum of 3C 273 were ordinary hydrogen lines, only shifted by 15%, I felt as if I had been struck by lightning. This meant the object was billions of light-years away from us."
Links in the knowledge graph 1
Related tags
active galactic nucleusexpansion of the universequasarspectroscopy
Related laws
Hubble's law
Related scientists
Robert HookeJohann Jakob BalmerJocelyn Bell BurnellArno PenziasCharles TownesJames Clerk MaxwellErwin SchrödingerCecilia Payne-Gaposchkin

Related articles

Weighing the Invisible: A Black Hole in the Early Universe

A team of scientists used light from carbon ions in a distant galaxy to determine the rotation speed of gas around the central object. A sharp acceleration of the gas toward the center pointed to a black hole with a mass of about 6.3 billion Suns. This is the first dynamical weighing of a black hole
arXiv:2504.13409 · 2025-04-18

Space Beacons: LST-1 Telescope Begins Tracking

For two years, the LST-1 prototype tracked the flickering of distant space beacons — blazars. At their centers, supermassive black holes act like giant spotlights, shooting out narrow beams of gamma rays. The telescope didn't catch the rays themselves, but their atmospheric footprints — faint blue f
arXiv:2510.03702 · 2025-10-04

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