Earth is hit by blast of energy from a dead star so powerful that scientists can’t explain it

Earth has been hit by a blast of energy from a dead star so powerful that scientists can’t fully explain it.

The intense gamma rays – detected using a huge system of telescopes in Namibia – would make people hiss to a crisp if we were exposed to them.

They come from the Vela Pulsar located about 1000 light years from Earth, which has already been compared in appearance to the mask from the Phantom of the Opera.

Pulsars are the remains of a massive star that blew up as a supernova an estimated 10,000 years ago and then collapsed on itself.

British astronomer Dame Jocelyn Bell Burnell was the first person to discover a pulsar in 1967, but this study marks the highest energy radiation from a pulsar yet observed.

The Vela Pulsar is located about 1,000 light-years from Earth in the southern sky in the constellation Vela

The Vela Pulsar is located about 1,000 light-years from Earth in the southern sky in the constellation Vela

What is a pulsar?

Pulsars are neutron stars, the shattered cores of massive suns that self-destructed when they ran out of fuel, collapsed and exploded.

The explosion simultaneously shattered the star and compressed its core into a body as small as a city but more massive than the sun.

The result is an object of incredible density, with a spoonful of matter weighing as much as a mountain on Earth.

Equally incredible is the rapid rotation of a pulsar, with typical rotation periods ranging from once every few seconds to hundreds of times per second.

Unfortunately, this doesn’t mean aliens are trying to contact us, according to study author Arache Djannati-Atai of the Astroarticle & Cosmology (APC) laboratory in France.

‘It’s true that when they were first discovered in 1967, the sources were called LGM1 and LGM2 for little green men, but that was almost a joke,’ he told MailOnline.

“We know for a fact that pulsars are corpses of massive stars and that no extraterrestrial intelligence is needed to produce the signals we see on Earth.”

Pulsars are described as remnants of stars that have exploded spectacularly in a supernova, the largest explosion to occur in space.

These pulsars emit rotating beams of electromagnetic radiation, a bit like cosmic lighthouses.

As their beam moves through our solar system, we see flashes of radiation at regular time intervals.

These flashes, also called radiation pulses, can be found in different energy bands of the electromagnetic spectrum.

“These dead stars are composed almost entirely of neutrons and are incredibly compact,” says HESS scientist and study author Emma de Oña Wilhelmi.

The Vela Pulsar makes more than 11 full rotations every second, faster than a helicopter rotor.  As the pulsar spins, it spits out a jet of charged particles that rush outward along the pulsar's axis of rotation at about 70 percent of the speed of light (artist's impression)

The Vela Pulsar makes more than 11 full rotations every second, faster than a helicopter rotor.  As the pulsar spins, it spits out a jet of charged particles that rush outward along the pulsar's axis of rotation at about 70 percent of the speed of light (artist's impression)

The Vela Pulsar makes more than 11 full rotations every second, faster than a helicopter rotor. As the pulsar spins, it spits out a jet of charged particles that rush outward along the pulsar’s axis of rotation at about 70 percent of the speed of light (artist’s impression)

The observations were made using the High Energy Stereoscopic System (HESS) telescope observatory in Namibia (photo).

The observations were made using the High Energy Stereoscopic System (HESS) telescope observatory in Namibia (photo).

The observations were made using the High Energy Stereoscopic System (HESS) telescope observatory in Namibia (photo).

“A teaspoon of their material has a mass of over five billion tons, or about 900 times the mass of the Great Pyramid of Giza.”

One specific pulsar that has long been of interest to scientists is the Vela Pulsar, located about 1,000 light-years in the southern sky in the constellation Vela.

Vela Pulsar is only about 20 kilometers in diameter and makes more than 11 full rotations per second, faster than a helicopter’s rotor.

As Vela Pulsar spins, it spits out a jet of charged particles that rush outward along the pulsar’s axis of rotation at about 70 percent of the speed of light.

Using the High Energy Stereoscopic System (HESS) telescope observatory in Namibia, the scientists studied gamma rays – which have the smallest wavelengths but the most energy of all waves in the electromagnetic spectrum – emitted by the Vela Pulsar.

The energy of this gamma ray was 20 teraelectron volts, or about 10 trillion times the energy of visible light.

This is an order of magnitude larger than in the case of the Crab pulsar, the only other pulsar detected in the tera-electronvolt energy range.

Scientists believe that the source of this radiation may be fast electrons produced and accelerated in the pulsar’s magnetosphere – the system of magnetic fields.

Like planets, including Earth, pulsars have a magnetosphere, an invisible force field that sends particles outward past the two magnetic poles.

The magnetosphere consists of plasma and electromagnetic fields that surround and rotate with the star.

The energy of this gamma ray was 20 teraelectron volts, or about 10 trillion times the energy of visible light (photo)

The energy of this gamma ray was 20 teraelectron volts, or about 10 trillion times the energy of visible light (photo)

The energy of this gamma ray was 20 teraelectron volts, or about 10 trillion times the energy of visible light (photo)

Pulsars have a magnetosphere, an invisible force field that sends particles outward past the two magnetic poles (photo)

Pulsars have a magnetosphere, an invisible force field that sends particles outward past the two magnetic poles (photo)

Pulsars have a magnetosphere, an invisible force field that sends particles outward past the two magnetic poles (photo)

According to the study authors, the Vela Pulsar now officially holds the record as the pulsar with the highest energy gamma rays discovered so far, which could revise existing astronomy models.

‘This discovery is important because we have made significant progress in investigating pulsars at their extreme energy limits,’ Djannati-Atai told MailOnline.

‘Within the zoo of cosmic beasts, pulsars are fantastic objects indeed – like neutron stars, they are extremely dense states of matter and have very intense magnetic fields.

‘Examining their energy limits of the phenomena taking place in pulsars and their environments helps us improve or even revise our theoretical models of the processes and physical conditions there.

‘It also provides a better understanding of other very dense and strongly magnetized objects that act as cosmic accelerators, for example the magnetospheres of black holes.’

The new study has been published in the journal Nature Astronomy.

SUPERNOVAE ARE CREATED WHEN A GIANT STAR EXPLODES

A supernova occurs when a star explodes, shooting debris and particles into space.

A supernova only burns for a short time, but can tell scientists a lot about how the universe began.

One type of supernova has shown scientists that we live in an expanding universe, a universe that is growing faster and faster.

Scientists have also determined that supernovae play a key role in the distribution of elements throughout the universe.

In 1987, astronomers discovered a 'titanic supernova' in a nearby galaxy, shining with the power of more than 100 million suns (pictured)

In 1987, astronomers discovered a 'titanic supernova' in a nearby galaxy, shining with the power of more than 100 million suns (pictured)

In 1987, astronomers discovered a ‘titanic supernova’ in a nearby galaxy, shining with the power of more than 100 million suns (pictured)

There are two known types of supernova.

The first type occurs in binary star systems when one of the two stars, a white carbon-oxygen dwarf, steals matter from its companion star.

Eventually, the white dwarf accumulates too much matter, causing the star to explode, resulting in a supernova.

The second type of supernova occurs at the end of a single star’s lifespan.

When the star runs out of nuclear fuel, some of its mass flows into the core.

Eventually the core is so heavy that it cannot support its own gravity and the core collapses, resulting in another gigantic explosion.

Many elements found on Earth are made in the cores of stars, and these elements travel on to form new stars, planets, and everything else in the universe.