What Orbits the Milky Way? NASA Final sharing New Discoveries

What Orbits the Milky Way? NASA Final sharing New Discoveries
In an astonishing breakthrough, NASA has finally revealed what orbits our galaxy, the Milky Way. This video delves into the latest findings from NASA's astronomical research, uncovering the mysterious objects and phenomena that exist in the vast expanse of space surrounding our galaxy. From rogue planets and dark matter to dwarf galaxies and cosmic anomalies, we explore the incredible celestial bodies that coexist with us in the universe. Join us as we unpack these groundbreaking discoveries and discuss their implications for our understanding of the cosmos.
In This Video, You'll Discover:
1. New Discoveries: The latest revelations from NASA about objects orbiting the Milky Way.
2. Dwarf Galaxies: Insights into the small galaxies that are gravitationally bound to our own.
3. Dark Matter: How this elusive substance plays a role in what orbits our galaxy.
4. Rogue Planets: The mystery of planets not bound to any star, wandering through space.
5. Cosmic Phenomena: Unusual and unexplained phenomena detected near the Milky Way.
Why You Should Watch:
- Stay Informed: Get up-to-date information on recent astronomical discoveries.
- Expand Your Knowledge: Learn about the structures and objects beyond our solar system.
- Explore the Cosmos: Gain a deeper understanding of our galaxy and its surroundings.
- Join the Discussion: Engage with a community of space enthusiasts and share your thoughts.
Unveil the mysteries of our galaxy! *Like, comment, and subscribe* for more cosmic discoveries and space explorations! 🚀🌌
#NASA #MilkyWay #SpaceExploration #Astronomy #CosmicDiscoveries #DarkMatter #DwarfGalaxies #RoguePlanets #Astrophysics #SpaceScience

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The fundamental phenomenon of dilation explains galaxy rotation curves. Mass that is dilated is smeared through spacetime relative to an outside observer. It's the phenomenon behind the phrase "mass becomes infinite at the speed of light". A graph illustrates its squared nature, dilation increases at an exponential rate the closer you get to the speed of light. A time dilation graph illustrates the same phenomenon, it's not just time that gets dilated.
Dilation will occur wherever there is an astronomical quantity of mass because high mass means high momentum. This includes the centers of very high mass stars and the overwhelming majority of galaxy centers.
The mass at the center of our own galaxy is dilated. This means that there is no valid XYZ coordinate we can attribute to it, you can't point your finger at something that is smeared through spacetime. In other words, that mass is all around us. In other words, common spiral galaxies are centerless.
Dilation does not occur in galaxies with low mass centers because they do not have enough mass to achieve relativistic velocities. It has been confirmed in 6 very low mass galaxies including NGC 1052-DF2 and DF4 to have no dark matter, in other words they have normal rotation rates. All planets and all binary stars have normal rotation rates for the same reason.