Hubble discovered a Titanic star collision that shakes space and time

This is an artist’s impression of the collision of two neutron stars. The collision between two dense stellar remnants unleashes the energy of 1,000 standard starbursts. In the aftermath of the collision, a jet of radiation is released from a blowtorch at nearly the speed of light. The jet is directed along a narrow beam confined by strong magnetic fields. The roaring jet slammed into and swept away material in the surrounding interstellar medium. Credit: Elizabeth Wheatley (STScI)

Over 299,000,000 meters per second – a super-fast jet blasting from a star crash.

Neutron stars are the leftover cores “compacted in the trash” of massive stars that have exploded. Although it weighs more than our Sun, it would fit right into New York City. With such an unimaginable density, one teaspoon of surface matter could weigh no less than 4 billion tons on Earth.

If that doesn’t make your mind spin, just imagine what happens when two of those intense cannonballs collide head-on. Ripple the fabric of time and space in a phenomenon called

gravitational waves
Gravitational waves are distortions or ripples in the fabric of space and time. They were first detected in 2015 by LIGO’s advanced detectors and are caused by catastrophic events such as the collision of black holes, supernovae, or the merger of neutron stars.

“data-gt-translate-attributes=”[{” attribute=””>gravitational waves, which can be measured by detectors on the ground on Earth.

The explosive event, named GW170817, was observed in August 2017. The blast released energy comparable to that of a supernova explosion. It was the first combined detection of gravitational waves and gamma radiation from a

Two neutron stars collided, the remaining cores of massive stars that exploded, sending ripples through the fabric of space-time in a phenomenon called gravitational waves. In the aftermath, a blowtorch jet of radiation is shot out at nearly the speed of light, slamming into the material surrounding the obliterated pair. Astronomers used Hubble to measure the motion of a mass of matter that the jet hit. attributed to him:

Founded in 1958, the National Aeronautics and Space Administration (NASA) is an independent agency of the United States federal government that is the successor to the National Advisory Committee for Aeronautics (NACA). It is responsible for the civilian space program, as well as aviation and space research. see it is “To discover and expand knowledge for the benefit of mankind.” its core values “Safety, integrity, teamwork, excellence and inclusion.”

“data-gt-translate-attributes=”[{” attribute=””>NASA’s Goddard Space Flight Center; Lead Producer: Paul Morris

Astronomers using NASA’s Hubble Space Telescope have made a unique measurement indicating that a jet was blasted across space at speeds faster than 99.97% the speed of light by a titanic collision between two neutron stars.

The explosive event, dubbed GW170817, occurred in August 2017. The blast generated energy comparable to a supernova explosion. It was the first time gravitational waves and gamma rays were detected together from a binary neutron star merger.

This was a significant turning point in the research of these extraordinary collisions. In addition to the discovery of gravitational waves, 70 observatories across the world and in space saw the aftermath of this merger across a large swath of the electromagnetic spectrum. This signaled an important development in the area of Time Domain and Multi-Messenger Astrophysics, which makes use of a number of “messengers” including gravitational waves and light to analyze the progression of the universe through time.

Just two days later, scientists quickly aimed Hubble toward the explosion’s location. The neutron stars collapsed into a

The authors used Hubble data together with data from ESA’s (the European Space Agency) Gaia satellite, in addition to VLBI, to achieve extreme precision. “It took months of careful analysis of the data to make this measurement,” said Jay Anderson of the Space Telescope Science Institute in Baltimore, Maryland.

By combining the different observations, they were able to pinpoint the explosion site. The Hubble measurement showed the jet was moving at an apparent velocity of seven times the speed of light. The radio observations show the jet later decelerated to an apparent speed of four times faster than the speed of light.

In reality, nothing can exceed the speed of light, so this “superluminal” motion is an illusion. Because the jet is approaching Earth at nearly the speed of light, the light it emits at a later time has a shorter distance to go. In essence, the jet is chasing its own light. In actuality, more time has passed between the jet’s emission of the light than the observer thinks. This causes the object’s velocity to be overestimated – in this case seemingly exceeding the speed of light.

“Our result indicates that the jet was moving at least at 99.97% the speed of light when it was launched,” said Wenbin Lu of the University of California, Berkeley.

The Hubble measurements, combined with the VLBI measurements, announced in 2018, greatly strengthen the long-presumed connection between neutron star mergers and short-duration gamma-ray bursts. That connection requires a fast-moving jet to emerge, which has now been measured in GW170817.

This work paves the way for more precision studies of neutron star mergers, detected by the


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