A massive structure recently observed in our galaxy is located about 55,000 light-years away on the other side of the Milky Way. This filament, called Maggie, is just shy of 4,000 light-years long and 130 light-years wide, extending about 1,600 light-years below the galactic plane.
The diffuse nature of Maggie and lack of a carbon monoxide signal, except on the smallest scale along the axis, suggest a juvenile filament. An examination of the centroid velocity sees it speed up and slow down—an indication that electromagnetic pinching is occurring—and probably where most star formation is happening.
Gareth Samuel, creator of "See the Pattern” and EU advocate, reinforces the idea that it's the movement of material in the filaments which powers the stars that reside in them.
Gareth Samuel | See the Pattern
• YouTube [ Ссылка ]
• Facebook [ Ссылка ]
• Twitter [ Ссылка ]
--
If you see a CC with this video, it means that subtitles are available. To find out which ones, click on the Gear Icon in the lower right area of the video box and click on “subtitles” in the drop-down box. Then click on the subtitle that you would like.
The Thunderbolts Project — a Voice for the Electric Universe
[ Ссылка ]
Become a Producer through the PATREON Rewards program...
[ Ссылка ]
Subscribe to Thunderbolts eNewsletter [ Ссылка ]
Guides to the Electric Universe [ Ссылка ]...
Electric Universe Books & Merch [ Ссылка ]
Electric Universe by Wal Thornhill [ Ссылка ]
Instagram [ Ссылка ]...
Facebook [ Ссылка ]
Twitter @tboltsproject
Ideas and/or concepts presented in this program do not necessarily express or represent the Electric Universe model or the views of The Thunderbolts Project or T-Bolts Group Inc.
The Thunderbolts Project™
Trademark of T-Bolts Group Inc. a non-profit 501(c)(3) organization.
Copyright © 2022 T-Bolts Group Inc. All rights reserved.
