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Lesson 6.2 – Gravity, Time & Relativity

16 Dec 2025 Module 6: Black Holes and Extreme Space
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Part of a Module

This lesson is part of Module 6: Black Holes and Extreme Space. Take it in course mode for progress tracking and the end-of-module exam.

Gravity as Curved Space-Time

According to Einstein’s General Relativity, gravity is not just a force — it is the curvature of space and time caused by mass and energy.

Black holes curve space-time more extremely than any other known object.


Time Dilation Near Black Holes

As gravity increases:

  • Time slows down

  • Clocks near black holes tick more slowly compared to distant observers

From an outside observer’s perspective, an object falling into a black hole appears to freeze at the event horizon.


Orbits, Accretion Disks & Jets

Matter falling toward a black hole often forms an accretion disk:

  • Gas heats up due to friction

  • Emits powerful radiation

  • Can outshine entire galaxies

Some black holes produce relativistic jets, blasting particles outward at near light speed.


Why We Don’t Fall Into One

Despite popular fear:

  • Black holes are extremely rare nearby

  • Sagittarius A* has existed for billions of years without harming Earth

  • Normal gravity laws apply at safe distances


Key Takeaways

  • Gravity bends space and time

  • Time slows near massive objects

  • Black holes are observable via their effects

  • Relativity predicts these behaviours accurately

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