#black-holes

#black-holes

The gamma-ray outburst from black hole M87* offers vital insights into the phenomena surrounding supermassive black holes and their energetic flares.

Primordial black holes could explain dark matter and may influence the solar system's planets by causing measurable wobbles.

The newly discovered black hole LID-568 devours matter 40 times faster than the theoretical limit, challenging previous understandings of black hole growth mechanisms.

Gravitational waves can pass through many objects, but black holes present a unique challenge with their event horizon.

Supermassive black holes merge by overcoming the final parsec problem, possibly aided by dark matter affecting angular momentum.

Black holes can form through collapsing gas disks without the need for star formation.

Discovery of unexpected massive stars in early universe challenges existing cosmological models, revealing insights into the role of black holes in galaxy formation.

A newly discovered black hole is consuming matter at 40 times the Eddington limit, demonstrating extraordinary brightness beyond expected limits.

Astronomers discovered a black hole, LID-568, consuming matter at 40 times the theoretical limit shortly after the Big Bang.

The JWST reveals new insights into the Sombrero galaxy, showcasing complex dust structures and a supermassive black hole.

A newly discovered black hole, 400 million times the Sun's mass, shows periods of hyperactivity followed by long dormancy, challenging black hole growth models.

Black holes may possess even more mysteries than previously understood, particularly with the recent discovery involving jets and unidentified objects.

The supermassive black hole at the center of our galaxy, Sagittarius A*, is spinning so fast that it warps spacetime and takes on the shape of a football.

Researchers used a new method, called the 'outflow method', to estimate the mass and spin rate of Sagittarius A*, using data from NASA's Chandra X-ray Observatory and the National Science Foundation's Karl G. Jansky Very Large Array (VLA).

Black holes could be 'frozen stars,' resolving the black hole information paradox and challenging existing theories of general relativity.

The concept of Hawking radiation might apply to all massive objects, not just black holes, challenging our understanding of mass and decay.

Astronomers have discovered an object that falls into a 'black hole mass gap,' too heavy to be a neutron star but too light to be a black hole.

This discovery challenges current theories about the formation and classification of celestial objects, and could lead to a reevaluation of Einstein's theory of general relativity.

Hawking radiation challenges black hole theory

Interplay of quantum physics and general relativity

Astronomers discovered record-breaking plasma jets from a supermassive black hole, which play a critical role in the evolution of the universe.

Astronomers discovered the largest black hole jets ever seen, stretching 23 million light years, defying previous theoretical limits.

A supermassive black hole is preventing the galaxy GS-10578 from forming new stars, effectively rendering it 'dead.'

A black hole named Porphyrion ejects energy across 23 million light-years, creating the largest cosmic jets ever discovered.

Black hole jets may influence galaxy evolution over immense distances.

Discovery sheds light on cosmic structure and the growth of galaxies.

Supermassive black holes can emit jets that cause nearby stars to explode, revealing gaps in our understanding of black hole interactions.

Early universe black holes are more numerous than previously estimated, reshaping our understanding of cosmic formation and evolution.

Creating a black hole with light alone is impossible.

Black holes warp spacetime drastically. Approaching one, classical mechanics break down, and objects plunge uncontrollably, revealing the mystery of the plunging region.

The European Space Agency has approved the construction of the Laser Interferometer Space Antenna (LISA), the first space experiment to measure gravitational waves.

LISA will be able to observe gravitational waves of lower frequency than those detected on Earth, allowing it to spot phenomena such as black holes orbiting each other.

Gravitational waves detection in 2015 revolutionized physics, offering new insights into the universe and black hole origins.

The discovery of heavier black holes challenges previous assumptions about their formation and existence, highlighting the importance of gravitational wave data and observational evidence from missions like Gaia in expanding our understanding of black holes.