Artwork

Content provided by McDonald Observatory. All podcast content including episodes, graphics, and podcast descriptions are uploaded and provided directly by McDonald Observatory or their podcast platform partner. If you believe someone is using your copyrighted work without your permission, you can follow the process outlined here https://player.fm/legal.
Player FM - Podcast App
Go offline with the Player FM app!

Jets

 
Share
 

Archived series ("Inactive feed" status)

When? This feed was archived on June 22, 2017 20:15 (7y ago). Last successful fetch was on May 23, 2017 06:12 (7y ago)

Why? Inactive feed status. Our servers were unable to retrieve a valid podcast feed for a sustained period.

What now? You might be able to find a more up-to-date version using the search function. This series will no longer be checked for updates. If you believe this to be in error, please check if the publisher's feed link below is valid and contact support to request the feed be restored or if you have any other concerns about this.

Manage episode 179697185 series 1445573
Content provided by McDonald Observatory. All podcast content including episodes, graphics, and podcast descriptions are uploaded and provided directly by McDonald Observatory or their podcast platform partner. If you believe someone is using your copyrighted work without your permission, you can follow the process outlined here https://player.fm/legal.

Most of the matter that passes too close to a black hole will get a one-way trip to oblivion: It’ll vanish into the black hole. But some of that matter may instead get a quick trip back out into space. That’s because many black holes produce jets of charged particles. The biggest of them can span thousands of light-years, and can squirt away at close to the speed of light.

In fact, similar jets are found in other astronomical objects — from infant stars to dead stars.

Scientists still aren’t certain just how these jets form. But the process involves disks of gas and dust and strong magnetic fields. The material in a disk spirals toward the central object — a young star, for example, or a dead star such as a white dwarf, a neutron star, or a black hole.

Friction in the disk heats the material enough to rip atoms apart, creating streamers of charged particles. Magnetic fields then grab some of these particles and shoot them into space from the poles of the central object as narrow high-speed jets.

Those from young stars can stretch across billions of miles. But those from supermassive black holes at the hearts of galaxies can span thousands of light-years. And the black hole’s powerful gravity can accelerate them to much higher speeds — in some cases, just a bit below lightspeed.

As these jets ram into material in the galaxy around the black hole, they produce shockwaves and other dramatic effects — the fate of matter escaping from a black hole.

Script by Damond Benningfield

  continue reading

28 episodes

Artwork

Jets

StarDate Premium Audio

published

iconShare
 

Archived series ("Inactive feed" status)

When? This feed was archived on June 22, 2017 20:15 (7y ago). Last successful fetch was on May 23, 2017 06:12 (7y ago)

Why? Inactive feed status. Our servers were unable to retrieve a valid podcast feed for a sustained period.

What now? You might be able to find a more up-to-date version using the search function. This series will no longer be checked for updates. If you believe this to be in error, please check if the publisher's feed link below is valid and contact support to request the feed be restored or if you have any other concerns about this.

Manage episode 179697185 series 1445573
Content provided by McDonald Observatory. All podcast content including episodes, graphics, and podcast descriptions are uploaded and provided directly by McDonald Observatory or their podcast platform partner. If you believe someone is using your copyrighted work without your permission, you can follow the process outlined here https://player.fm/legal.

Most of the matter that passes too close to a black hole will get a one-way trip to oblivion: It’ll vanish into the black hole. But some of that matter may instead get a quick trip back out into space. That’s because many black holes produce jets of charged particles. The biggest of them can span thousands of light-years, and can squirt away at close to the speed of light.

In fact, similar jets are found in other astronomical objects — from infant stars to dead stars.

Scientists still aren’t certain just how these jets form. But the process involves disks of gas and dust and strong magnetic fields. The material in a disk spirals toward the central object — a young star, for example, or a dead star such as a white dwarf, a neutron star, or a black hole.

Friction in the disk heats the material enough to rip atoms apart, creating streamers of charged particles. Magnetic fields then grab some of these particles and shoot them into space from the poles of the central object as narrow high-speed jets.

Those from young stars can stretch across billions of miles. But those from supermassive black holes at the hearts of galaxies can span thousands of light-years. And the black hole’s powerful gravity can accelerate them to much higher speeds — in some cases, just a bit below lightspeed.

As these jets ram into material in the galaxy around the black hole, they produce shockwaves and other dramatic effects — the fate of matter escaping from a black hole.

Script by Damond Benningfield

  continue reading

28 episodes

All episodes

×
 
Loading …

Welcome to Player FM!

Player FM is scanning the web for high-quality podcasts for you to enjoy right now. It's the best podcast app and works on Android, iPhone, and the web. Signup to sync subscriptions across devices.

 

Quick Reference Guide