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Supermassive black hole

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Our own galaxy, the Milky Way, is home to anywhere from 100 to 400 billion stars, and at least as many planets.

At the center of the galaxy is an intense radio source known as Sagittarius A*, a supermassive black hole that has incredible, incomprehensible mass and power. 

Scientists have revealed new imagery of the black hole  looming at the center of the Milky Way. Seen through polarization, we see an incredible image that looks computer generated. But indeed, it’s the powerful magnetic fields spiraling outward from the center.

Two new research papers document how these amazing images were captured, and give us a bit more of a glimpse into the awesome power of these astronomical forces.

Taken by an array of radio telescopes called the Event Horizon Telescope, the image we see shows the radio waves that are then interpreted as visible light.

The M87* galaxy black hole compared to our own Sgr A* black hole.

Every bit of about a ‘runaway supermassive black hole‘ sounds exciting. The idea of something so massive on the run, the visual of it leaving behind a trail of newly formed stars, and the sheer power of such a force is something that makes our brain feel sparkly.

Astronomers using Hubble telescope recently spotted a strange ‘blemish’ that turned out to be an amazing sight – a supermassive black hole trailing a 200,000-light-year-long chain of young blue stars. After being ejected from a galaxy, this near unfathomable force is tearing across the interstellar space at breakneck speed.

Artists have visualized what this anomaly looks like, which is, frankly, incredible. Nothing like this has ever been seen in the universe before.

From Hubblesite:

“The universe is so capricious that even the slightest things that might go unnoticed could have profound implications. That’s what happened to Yale astronomer Pieter van Dokkum when he was looking through Hubble Space Telescope images and noticed a suspected blemish that looked like a scratch on photographic film. For Hubble’s electronic cameras, cosmic rays skimming along the detector look like “scratches.” But once spectroscopy was done on the oddball streak van Dokkum realized it was really a 200,000-light-year-long chain of young blue stars located over halfway across the universe! van Dokkum and his colleagues believe that it stretches between a runaway monster back hole and the galaxy it was ejected from. The black hole must be compressing gas along its wake, which condenses to form stars. Nothing like it has ever been seen anywhere else in the universe before.”

Visuals by NASA, ESA, Leah Hustak.

“This is an artist’s impression of a runaway supermassive black hole that was ejected from its host galaxy as a result of a tussle between it and two other black holes. As the black hole plows through intergalactic space it compresses tenuous gas in front to it. This precipitates the birth of hot blue stars. This illustration is based on Hubble Space Telescope observations of a 200,000-light-year-long “contrail” of stars behind an escaping black hole.”

Black Hole

 

Outer space is incredible. This artist’s rendering of a black hole is just so amazing, I wanted to share. Via NASA:

This artist’s concept illustrates a supermassive black hole with millions to billions times the mass of our sun. Supermassive black holes are enormously dense objects buried at the hearts of galaxies. (Smaller black holes also exist throughout galaxies.) In this illustration, the supermassive black hole at the center is surrounded by matter flowing onto the black hole in what is termed an accretion disk. This disk forms as the dust and gas in the galaxy falls onto the hole, attracted by its gravity.

Also shown is an outflowing jet of energetic particles, believed to be powered by the black hole’s spin. The regions near black holes contain compact sources of high energy X-ray radiation thought, in some scenarios, to originate from the base of these jets. This high energy X-radiation lights up the disk, which reflects it, making the disk a source of X-rays. The reflected light enables astronomers to see how fast matter is swirling in the inner region of the disk, and ultimately to measure the black hole’s spin rate.

Image credit: NASA/JPL-Caltech

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