25 Crazy Facts About Black Holes

Posted by , Updated on November 14, 2018

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Much like a black body in thermodynamics, a black hole is a region of space that pulls everything in but prevents anything from escaping, even light. The reason it is called a “black” hole is because it sucks up all the light that hits its border and reflects nothing. Formed when an amply compact mass deforms space and time, a black hole has a defined surface known as the “event horizon” which marks the point of no return. Little is known about black holes, but several scientists in history have developed their own theories about their properties and structures. Here is a list of 25 Crazy Facts About Black Holes.

25

Black holes affect time

clocks

Just as a clock runs a bit slower closer to sea level than up on a space station, clocks run really slow near black holes. It all has to do with gravity.

24

They can be infinitely big

black hole

There are a few theories that state they can be infinitely big. While not all scientists agree, there are several who believe that they can be infinitely big. 

23

The nearest black hole to the Earth is 1,600 light years away

black hole milky wayen.fonditos.com

Our galaxy is covered in black holes, but the one most likely to destroy our measly planet is still well beyond our solar system’s borders.

22

Stay away from the event horizon

black hole milkwaycentalblackhole.wordpress.com

The “Event Horizon” as it is called in physics, is the border of the black of hole. It’s the point of no return. Before that point, you can still escape. After that point…not a chance.

21

There is a massive black hole at the center of the Milky Way galaxy.

swirling black holecosmicsweaters.tumblr.com

It’s 30,000 light years away and is over 30 million times as massive as our sun.



Photo: Featured Image - User:Alain r, BH LMC, CC BY-SA 2.5 , 1. WikipediaCommons.com (Public Domain), 2. Nasa.gov (Public Domain), 3. WikipediaCommons.com (Public Domain), 4. ESO/L. Calçada/M.Kornmesser, A stellar black hole, CC BY 4.0 , 5. WikipediaCommons.com (Public Domain), 6. Pixabay.com (Public Domain), 7. jpg.nasa.gov (Public Domain), 8. James Spinks, Static Wallpaper, CC BY 2.0, 9. Maxwell Hamilton, Colliding Black Holes and Gravitational Waves, CC BY 2.0, 10. WikipediaCommons.com (Public Domain), 11. WikipediaCommons.com (Public Domain), 12. Simulating eXtreme Spacetimes, Black hole collision and merger releasing gravitational waves, CC BY-SA 4.0 , 13. Maxpixel.net (Public Domain), 14. jpl.nasa.gov (Public Domain), 15. ESO/WFI (Optical); MPIfR/ESO/APEX/A.Weiss et al. (Submillimetre); NASA/CXC/CfA/R.Kraft et al. (X-ray), ESO Centaurus A LABOCA, CC BY 4.0 , 16. jpl.nasa.gov (Public Domain), 17. WikipediaCommons.com (Public Domain), 18. WikipediaCommons.com (Public Domain), 19. Pixabay.com (Public Domain), 20. User:Alain r, BH LMC, CC BY-SA 2.5 , 21. jpl.nasa.gov (Public Domain), 22. Deutsch: Black_Hole_Milkyway.jpg: Ute Kraus, Physikdidaktik Ute Kraus, Universität Hildesheim, Tempolimit Lichtgeschwindigkeit, (Milchstraßenpanorama im Hintergrund: Axel Mellinger)
abgeleitetes Werk: Sponk (talk) English: Black_Hole_Milkyway.jpg: Ute Kraus, Physics education group Kraus, Universität Hildesheim, Space Time Travel, (background image of the milky way: Axel Mellinger)
derivative work: Sponk (talk), Black Hole Milkyway Event Horizon, CC BY-SA 2.5 , 23. WikipediaCommons.com (Public Domain), 24. WikipediaCommons.com (Public Domain), 25. PublicDomaintPictures.net (Public Domain)

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