Using a supercomputer, scientists have found that the matter of neutron stars with high isospin densities is superconducting.
The Perfect Cosmic Fireball
Astronomers have unveiled the extraordinary details of a nearly perfect spherical explosion—a kilonova—caused by the collision of two neutron stars. This dramatic event unfolded in 2017 in the galaxy NGC 4,993, located 140–150 million light years from Earth in the Hydra constellation. With a combined mass of 2.7 times that of the sun, the neutron stars had orbited each other for billions of years before their explosive merger.
Lead researcher Albert Sneppen of the Cosmic Dawn Center described the event as “a perfect explosion” due to its symmetry and scientific implications. The kilonova’s luminous fireball emitted a light equivalent to a billion suns for several days, dwarfing any earthly nuclear explosion in intensity.
Collapsed dead stars, known as neutron stars, are a trillion times denser than lead, and their surface features are largely unknown. Nuclear theorists have explored mountain building mechanisms active on the moons and planets in our solar system. Some of these mechanisms suggest that neutron stars are likely to have mountains.
Neutron star “mountains” would be much more massive than any on Earth—so massive that gravity just from these mountains could produce small oscillations, or ripples, in the fabric of space and time.
Mountains, or non-axisymmetric deformations of rotating neutron stars, efficiently radiate gravitational waves. In a study published in the journal Physical Review D, nuclear theorists at Indiana University consider analogies between neutron star mountains and surface features of solar system bodies.
The mechanisms resulting in particle acceleration to relativistic energies in space plasmas are an open question. Here, the authors show a reinforced shock acceleration model which enables electrons to efficiently achieve relativistic energies and reveal a low electron injection threshold.
Emily Simpson has loved space since she was a 10-year-old kid celebrating her birthday at a planetarium. Now a recent Florida Tech graduate, she leaves with not only a dual degree in planetary science and astronomy and astrophysics but with published research, too. She mapped our solar system’s “alternate fate” had it housed an extra planet between Mars and Jupiter instead of the existing asteroid belt.
Simpson’s paper, “How might a planet between Mars and Jupiter influence the inner solar system? Effects on orbital motion, obliquity, and eccentricity,” was published in Icarus, a journal devoted to the publication of research around solar system studies. It was co-authored by her advisor, assistant professor of planetary science Howard Chen.
They developed a 3D model that simulates how the solar system’s orbital architecture may have evolved differently with the formation of a planet that is at least twice the size of Earth’s mass—a super-Earth—instead of an asteroid belt.
More data releases are coming, and with it more discoveries, but many already wondering what’s next.
The amorphous state of matter is the most abundant form of visible matter in the universe, and includes all structurally disordered systems, such as biological cells or essential materials like glass and polymers.
An amorphous material is a solid whose molecules and atoms form disordered structures, meaning that they do not occupy regular, well-defined positions in space.
This is the opposite of what happens in crystals, whose ordered structure facilitates their mathematical description, as well as the identification of those “defects,” which practically control the physical properties of crystals, such as their plastic yielding and melting, or the way an electric current propagates through them.
Scientists are closer than ever to uncovering one of astronomy’s most elusive mysteries: Planet X. A groundbreaking telescope is set to revolutionize the search for the enigmatic ninth planet and challenge our understanding of the solar system’s boundaries.
Astronomers have made a remarkable discovery: a neutron star spinning at a staggering rate of 716 times per second, making it the fastest-spinning neutron star in the known universe, tied only with PSR J1748–2446. This stellar body, located in the binary system 4U 1820–30 within the NGC 6,624 globular cluster near the Milky Way’s center, is around 26 light-years from Earth in the constellation Sagittarius.
The discovery was made using NASA’s Neutron Star Interior Composition Explorer (NICER), an X-ray telescope mounted on the International Space Station. Gaurava K. Jaisawal from DTU Space shared that during observations of thermonuclear bursts, the team detected oscillations corresponding to a spin rate of 716 Hz, confirming the extreme speed.
Neutron stars, remnants of massive stars that have exhausted their nuclear fuel, are known for their rapid rotation and intense density. This newfound star is no exception, showcasing powerful thermonuclear blasts that briefly make it up to 100,000 times brighter than the Sun. These explosions occur as material from its companion star—a white dwarf in this case—accretes onto the neutron star’s surface, igniting under extreme pressure.
FRBs are so powerful that even after traveling billions of light-years, only around 50 have been traced back to their host galaxies.
