Tag: Spinning

  • A Spinning Universe Could Solve One of Physics’ Biggest Mysteries

    A Spinning Universe Could Solve One of Physics’ Biggest Mysteries

    Credit: Nasa

    When we observe the cosmos, a striking pattern emerges: Earth spins, the Sun spins, and even our Milky Way galaxy is rotating. Now, a bold new model proposes that the entire Universe might also be rotating. If proven, this revelation could resolve one of modern cosmology’s most persistent puzzles.

    We’ve long known that the Universe is expanding—but determining the precise rate of that expansion has proven to be a major challenge. Two different measurement methods yield two distinct values for the Hubble constant, and paradoxically, the more accurate these measurements become, the more confident scientists are in both. This discrepancy, known as the “Hubble tension,” has reached a critical point in the field.

    In an attempt to reconcile the difference, researchers from Hungary and the United States introduced a slight rotational component to a mathematical model of the Universe. Surprisingly, this small adjustment significantly reduced the discrepancy—offering a promising new perspective on the problem.

    The Unexpected Solution: Cosmic Rotation

    István Szapudi, an astronomer at the University of Hawai‘i and co-author of the study, expressed his astonishment at the outcome. According to Szapudi, the rotating Universe model aligns with current astronomical observations and complements other theoretical frameworks that also allow for cosmic rotation. “So maybe,” he says, “everything really is spinning.”

    Based on the team’s calculations, it would take the Universe trillions of years to complete a single rotation. Given that the cosmos is less than 14 billion years old, it’s still in the early stages of this cosmic spin—like watching the opening move of a vast, graceful ballet.

    While this rotational pace may seem imperceptibly slow to us, the researchers found that it’s near the maximum allowed speed without violating the cosmic speed limit set by light. Fortunately, this means there’s no need to worry about time loops or sci-fi-style paradoxes.

    A Familiar Idea with a New Twist

    The concept of a rotating Universe isn’t entirely new. Recent studies have suggested such motion might explain why galaxies seem to prefer spinning in one direction more than the other—something unexpected in a perfectly balanced, non-rotating cosmos.

    However, this is the first time rotation has been proposed as a direct solution to the Hubble tension, representing an innovative approach to one of cosmology’s most complex issues.

    In this chart, the curved line shows how the Hubble constant values align in a rotating Universe model, connecting local measurements (in blue) with distant ones (in orange).
    (Szigeti et al., Monthly Notices of the Royal Astronomical Society, 20259)

    To outsiders, this debate over a few kilometers per second per megaparsec might sound like semantics—but in reality, the implications are profound. At the heart of the debate is the Hubble constant, which plays a key role in calculating the Universe’s size, age, and the influence of dark energy.

    Why the Hubble Constant Matters

    The Hubble constant is essential for estimating cosmic distances, gauging the scale of the Universe, and understanding its rate of expansion. Altering it without caution risks undermining the entire Standard Model of Cosmology—like pulling a critical piece from a tower of blocks.

    One method for measuring the Hubble constant involves studying signals from the early Universe, such as the cosmic microwave background (CMB) and baryon acoustic oscillations. These yield a consistent value of around 67 km/s/Mpc.

    Closer to home, astronomers use “standard candles”—objects like specific stars and supernovae with known brightness levels—to measure distances and calculate expansion rates. This approach gives a higher value of about 73 km/s/Mpc.

    Two Numbers, One Universe—and a Rotational Fix

    It might seem tempting to split the difference between these two values and call it a day, but the precision of both measurements is so high that the discrepancy is statistically significant. Physicists are left grappling with two conflicting yet solid numbers.

    The new model proposes that both values could be correct within their own observational contexts. Rotation, the researchers argue, could affect how the expansion appears over distance—explaining the divergence between local and distant measurements.

    Their model’s curve shows how the Hubble constant varies in a rotating Universe, effectively bridging the gap between nearby (blue) and faraway (orange) observations. It offers a graceful explanation that links the two perspectives.

    The Deeper Meaning of a Spinning Cosmos

    If the Universe truly is rotating, it raises profound philosophical and scientific questions. What force could set the entire cosmos into motion? One intriguing theory speculates that our Universe might exist within the spinning interior of a black hole from another Universe—since black holes are known to rotate at near-relativistic speeds.

    Although these ideas sound like the stuff of science fiction, they’re grounded in cutting-edge mathematics and astrophysical data. Before drawing any dramatic conclusions, however, the team plans to develop a full computational model to explore testable predictions.

    In the meantime, we can imagine the Universe performing a grand, circular dance—just like everything within it, from electrons to galaxies. Perhaps rotation is a fundamental preference of nature itself.

    What Comes Next in Cosmic Research?

    Scientists must now search for observable evidence that supports—or contradicts—this rotating Universe model. If confirmed, it would revolutionize our understanding of the cosmos, requiring a major revision of our models of its structure and history.

    Ironically, the idea of a spinning cosmos echoes ancient, pre-Copernican views of the heavens. But today, those old notions are reborn with modern precision—proof that sometimes, the future of science lies in revisiting the past with new eyes.


    Read the original article on: Hype Science

    Read more: Astronomers Find Unusual Slow-Spinning Radio Source That ‘Shouldn’t Exist’

  • Wild Star Spinning at an Incredible 716 Times Per Second

    Wild Star Spinning at an Incredible 716 Times Per Second

    A neutron star located 27,400 light-years away is exhibiting one of the most remarkable rotational speeds ever observed.
    An artist’s impression of an accreting X-ray pulsar. (Dana Berry/NASA)

    Neutron Star Spins at Unbelievable Speed

    A neutron star located 27,400 light-years away is exhibiting one of the most remarkable rotational speeds ever observed.

    In the binary system 4U 1820-30, this dead star spins so rapidly around its axis that it completes an astounding 716 rotations per second. This marks the fastest spin observed, with the only other star known to spin at this speed being the famous pulsar PSR J1748-2446ad.

    According to astrophysicist Gaurava Jaisawal of the Technical University of Denmark and his team, this discovery supports the theoretical upper limit for neutron star spin, which is believed to be around 730 rotations per second.

    Jaisawal explains, “We were originally studying thermonuclear explosions from this system when we detected remarkable oscillations.”

    Potential for 4U 1820-30 to Become One of the Fastest Spinning Stars

    If further observations confirm these findings, the 4U 1820-30 neutron star will become one of the fastest-spinning objects ever observed in the universe.

    Neutron stars represent the final evolutionary phase of massive stars. When a star with a mass between 8 and 30 times that of the Sun exhausts its nuclear fuel, it undergoes a supernova explosion, ejecting its outer layers.

    The remaining core collapses under gravity, forming a neutron star. This dense object, with a mass between 1.1 and 2.3 times the Sun’s mass, has a radius of only about 20 kilometers (12 miles).

    An artist’s impression of a bursting X-ray pulsar. (Chris Smith/Walt Feimer/NASA’s Goddard Space Flight Center)

    Neutron stars display fascinating behaviors. Magnetars have extremely powerful magnetic fields, while pulsars, like this one, spin rapidly and emit beams of radio waves, creating a pulsing effect similar to a cosmic lighthouse.

    4U 1820-30’s Close Binary Orbit and Feeding Mechanism

    4U 1820-30, discovered in the 1980s, is a binary system in the constellation Sagittarius. It consists of a neutron star and a white dwarf star orbiting each other in a very tight orbit, completing one cycle every 11.4 minutes.

    Due to their close proximity, the neutron star can “feed” off its companion, stripping material away, which then accumulates on the neutron star’s surface. This material builds up, increasing both temperature and density until it triggers a thermonuclear explosion.

    Jaisawal and his team studied these explosions using NASA’s Neutron Star Interior Composition Explorer (NICER), an X-ray telescope mounted on the International Space Station.

    Astrophysicist Jerome Chenevez of the Technical University of Denmark explains, “During these bursts, the neutron star becomes up to 100,000 times brighter than the sun, releasing enormous amounts of energy.”

    The team recorded 15 thermonuclear explosions between 2017 and 2022. While analyzing the data, they noticed one explosion had an unusual signature—an oscillation at 716 Hertz, which indicated that the star was likely rotating as it erupted.

    This could suggest that the 4U 1820-30 neutron star is an X-ray pulsar, with a period of 716 rotations per minute, driven by thermonuclear explosions. If confirmed, this would make it the fastest known nuclear-powered pulsar, surpassing PSR J1748-2446ad.

    Additional observations will be needed to verify this hypothesis. If proven true, the discovery would provide new insights into neutron stars and their extreme behaviors before they reach the point of self-destruction.


    Read the origina article on: Science Alert

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