phénomène

rayon X

High-energy electromagnetic radiation with wavelengths shorter than ultraviolet light.
4 articles liés

Description

X-rays are a form of high-energy electromagnetic radiation with wavelengths shorter than ultraviolet light, typically ranging from about 0.01 to 10 nanometers. They are produced when high-speed electrons collide with matter or when electrons transition between inner atomic shells. X-rays are famous for their ability to penetrate soft tissue but are absorbed by dense materials like bone, making them invaluable in medical imaging and materials science.

Histoire

X-rays were discovered by Wilhelm Röntgen in 1895, who observed them as an unknown type of radiation that could expose photographic plates. He named them 'X-rays' to signify their mysterious nature, and he received the first Nobel Prize in Physics in 1901 for this discovery.

Comment ça marche

X-rays are generated when charged particles, usually electrons, are accelerated and then decelerated rapidly, or when they knock inner-shell electrons out of atoms, causing higher-energy electrons to fill the vacancy and emit photons. Because of their short wavelength, X-rays can pass through many materials, but their absorption depends on the atomic number and density of the material. In detectors, X-rays are captured by converting their energy into electrical signals, often using scintillators or semiconductor sensors.

En pratique

X-rays are used in medical radiography, computed tomography (CT) scans, airport security scanners, and in astronomy to observe high-energy phenomena like black holes and supernovae, as mentioned in the article about invisible light from young galaxies.

Anecdote

X-rays were first used for medical imaging within months of their discovery, and the first X-ray image ever taken was of Röntgen's wife's hand, showing her bones and wedding ring.

Concept graph →

Articles liés · 4

Optique2026-09-063 minarXiv:2609.06454
Un orchestre attoseconde à l'échelle du kiloélectronvolt : comment accorder les harmoniques à l'unisson
Accorder une corde à la bonne note : on ajuste l'impulsion laser pour que les harmoniques résonnent à l'unisson à des fréquences de l'ordre du kiloélectronvolt. La lumière que nous voyons oscille à des centaines de milliers de milliards de fois par seconde.
Un trou noir invisible tapi après un festin cosmique
Dans une galaxie lointaine, à environ 290 millions d'années-lumière de nous, se cache l'objet HLX-1. Autrefois, il brillait plus fort que des centaines de milliards de soleils ; aujourd'hui, il s'est tu. De 2018 à 2022, les télescopes spatiaux Hubble, Chandra et Swift ont observé son déclin.
La lumière invisible des jeunes galaxies
Une ampoule tamisée qui se met soudain à éclairer des motifs invisibles sur le mur : c'est un peu ainsi que les astronomes observent les galaxies naines lointaines, ces minuscules îles d'étoiles pauvres en éléments lourds. Dans certaines d'entre elles, on a remarqué une faible lueur violette d'hélium ionisé (la raie spectrale particulière He II 4686 Å).