Recent findings from the University of Kansas have unraveled a long-standing astrophysical mystery, revealing how the intricate interplay of gravity and magnetospheric plasma divides the radio emissions of a club pulsar—a remnant of the supernova witnessed by ancient astronomers in 1054 AD—into perfectly aligned “stripes.”

In 1054 AD, Chinese astronomers documented an exceptionally bright new star, the most luminous object in the night sky after the moon, visible even in broad daylight for 23 days. This spectacular celestial event was also noted by Japanese, Arabian, and Native American astronomers.

Today, the Crab Nebula, found where this bright star once shone, is cataloged as Messier 1 (M1) or NGC 1952, located approximately 6,500 light-years away in the Taurus constellation.

Initially identified in 1731 by British physician and astronomer John Beavis, the Crab Nebula was later rediscovered in 1758 by French astronomer Charles Messier. Its name, reflecting its appearance, is derived from a painting by Irish astronomer Lord Rose in 1844.

The central star of the Crab Nebula is the Crab Pulsar, scientifically known as PSR B0531+21.

Due to their proximity and visibility, studying the Crab Nebula and its pulsars offers astronomers vital insights into the nature of nebulae, supernovae, and neutron stars.

“Gravity alters the shape of spacetime,” states Professor Mikhail Medvedev, one of the study’s authors.

“In the presence of a gravitational field, light does not travel in straight lines because space itself is curved,” he explains.

“What seems straight in flat spacetime appears curved under strong gravitational influence. Hence, gravity functions as a lens in curved spacetime.”

While gravitational lensing has often been discussed in relation to black holes, this case uniquely illustrates a “tug of war” between plasma and gravity creating the observed signals.

“In black hole imagery, gravity solely shapes the structure,” notes Professor Medvedev.

“In contrast, both gravity and plasma are at play in the club pulsar. This research presents a novel application of this combined effect.”

“An intriguing pattern emerges in the pulsar’s spectrum,” Professor Medvedev adds.

“Unlike a conventional broad spectrum like sunlight—which offers a continuous range of colors—the Crab’s high-frequency interpulses display discrete spectral bands. It’s like observing a rainbow with only selected ‘colors’ visible, leaving significant gaps in between.”

A large mosaic image of the Crab Nebula, a six-light-year wide remnant of a supernova explosion. Documented by Japanese, Chinese, and Native American astronomers around 1054 AD. Image credit: NASA / ESA / J. Hester / A. Loll, Arizona State University.

Typically, pulsar radio emissions are broader, noisier, and less organized compared to those from club pulsars.

“In the case of club pulsars, the stripes are exceptionally distinct, contrasting sharply with the complete darkness that separates them,” explains Professor Medvedev.

“There are shining bands and voids in between, with no gradual transition. No other pulsar displays this kind of banding. This uniqueness makes the club pulsar both intriguing and complex to comprehend.”

While former models could replicate the striped pattern, they failed to account for the high contrast actually seen in club pulsars.

Professor Medvedev has found that the plasma material surrounding the club pulsar contributes to the diffraction of electromagnetic pulses, which significantly influences the neutron star’s distinct zebra pattern.

By integrating Einstein’s theory of gravity into his analysis, Medvedev discovered its crucial role in shaping the club pulsar’s zebra stripe pattern.

“Prior theoretical models could reproduce the striped pattern, but not the observed contrast. Including gravity bridged that gap,” asserts Professor Medvedev.

“The plasma in a pulsar’s magnetosphere acts as a defocusing lens, while gravity serves as a focusing lens. Plasma tends to scatter light rays, whereas gravity draws them inward. When these dual effects converge, certain paths will offset each other.”

The synergy between defocused magnetospheric plasma and focusing gravity creates in-phase and out-of-phase interference bands of radio intensity, producing zebra stripes in club pulsars.

“The nature of symmetry suggests there are at least two pathways for light,” Medvedev observes.

“When two nearly identical paths converge on an observer, they create an interferometer. The signals amalgamate, reinforcing each other at specific frequencies (in phase) to yield bright bands, while at others (out of phase), they cancel each other out, generating darkness. This concept encapsulates the essence of interference patterns.”

“Little additional physics appears necessary to qualitatively explain the stripes.”

“Yet, quantitative enhancements could be implemented; the current model includes gravity in a static, lowest-order approximation.”

“Since pulsars rotate, incorporating rotational effects might lead to significant quantitative, if not qualitative, changes.”

The new research is set to be published in the Plasma Physics Journal.

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Mikhail V. Medvedev. 2026. Theory of the dynamic spectrum of club pulsar high-frequency interpulse stripes. Plasma Physics Journal, in press. arXiv: 2602.16955