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Deep-Space Tech Shrinks Down: Compton Camera Peers into the Atom's Heart

Deep-Space Tech Shrinks Down: Compton Camera Peers into the Atom’s Heart

March 14, 2024
This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

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Deep-Space Tech Shrinks Down: Compton Camera Peers into the Atom’s Heart

by nasaspacenews
March 14, 2024
in News, Others
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Deep-Space Tech Shrinks Down: Compton Camera Peers into the Atom's Heart
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Scientists have repurposed a powerful astronomical tool, the Compton Camera, to investigate the minuscule world of atoms. Originally designed to study distant celestial objects, the camera has proven adept at revealing the inner workings of atomic nuclei.

From Deep Space to the Atomic Nucleus

Developed for the Hitomi satellite to observe high-energy cosmic phenomena, the Compton Camera wasn’t intended for atomic investigations. However, researchers realized its potential to measure the polarization of gamma rays – a key element in understanding the structure of atomic nuclei.

Compton Camera: Unveiling the Atomic Landscape

Compton cameras utilize the “Compton scattering” phenomenon to determine the direction and energy of gamma rays. This involves high-energy light particles bouncing off electrons within an atom, revealing details about the atom’s structure.

Unstable Nuclei: A Scientific Mystery

While numerous stable atomic nuclei exist, thousands of unstable ones remain a scientific enigma. Scientists have observed unique phenomena around these unstable nuclei, including anomalies in electron energy levels and the appearance/disappearance of “magic numbers” (specific electron shell configurations).

A New Tool for Unveiling the Secrets

Conventional methods struggle to analyze changes in unstable nuclei due to limitations in sensitivity and detection efficiency. This is where the repurposed Compton Camera steps in.

The Power of Polarization

The camera’s Cadmium Telluride (CdTe) sensor excels at measuring the polarization of gamma rays emitted by unstable nuclei. This polarization, arising from the scattering angle of the light, offers insights into the properties of particles within the atom, including their “spin” and “parity” (quantum mechanical characteristics).

Experiments Validate the Repurposed Tech

Researchers at RIKEN conducted experiments by bombarding iron nuclei with protons, causing them to emit gamma rays. The Compton Camera successfully measured the scattering angle and polarization of these gamma rays, revealing valuable information about the nucleus’ internal structure.

Beyond Expectations: A New Era of Discovery

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The bright star at the center of NGC 3132, Southern Nebula Ring, while prominent when viewed by NASA's Webb Telescope in near-infrared light, plays a supporting role in sculpting the surrounding nebula. A second star, barely visible at lower left along one of the bright star's diffraction spikes, is the nebula's source. It has ejected at least eight layers of gas and dust over thousands of years.

The Future: A Universe of Possibilities

The experiment’s success surpassed even the researchers’ expectations. This paves the way for utilizing space-grade instruments like the Compton Camera to unlock the secrets of the atomic world.

Takahashi, the lead researcher, suggests that various astronomical Compton cameras hold similar potential for measuring the polarization of photons, opening doors to further exploration of the atomic realm.

Tags: NASAspace discoveryspace exploration

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This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

Star Meets Doom: Hubble Reveals Wandering Black Hole’s Deadly Snack

May 10, 2025
A storm is pictured in the Arabian Sea less than 700 miles off the coast of Oman as the International Space Station orbited 260 miles above. NASA / Jasmin Moghbeli

Storm Warning: JWST Detects Violent Weather on Nearby Substars

May 7, 2025
Image captured by Juno during its 66th perijove, then further processed with color enhancement by Gerald Eichstädt and Thomas Thomopoulos. NASA / JPL / SwRI / MSSS / Gerald Eichstädt / Thomas Thomopoulos CC BY 3.0

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This artist's illustration shows a protoplanetary disk swirling around a young star. New research showing how a young star can send some material back into the disk helps explain an observational discrepancy. Image Credit: NASA/JPL-Caltech/T. Pyle (SSC)

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This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

Star Meets Doom: Hubble Reveals Wandering Black Hole’s Deadly Snack

May 10, 2025
A storm is pictured in the Arabian Sea less than 700 miles off the coast of Oman as the International Space Station orbited 260 miles above. NASA / Jasmin Moghbeli

Storm Warning: JWST Detects Violent Weather on Nearby Substars

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