How does dark matter relate to the expansion of the universe?
It's the Dark Energy.
The Newton Law of Gravitation states that the force of gravity weakens as the square of the distance, meaning that the farther away you are, the weaker the force of gravity; conversely, the closer an object is to the center of mass, the faster it moves around it. Using the solar system as an example, the orbital periods of all the planets increase as we move from Mercury towards Neptune. These findings and the observed irregularities in the orbits of objects around galaxies sparked the debate over dark matter.
On a much grander scale, however, this is not the case. What scientists observed was that, in the majority of galaxies, objects at the periphery were moving nearly as fast as those within, suggesting that some sort of force was at work on those objects, a force they named Dark Matter.
The universe is made up of two main components: Dark Matter, which makes up 25% of the total, and Dark Energy, which is mysterious and accounts for the remaining 5% of the universe. The expansion of the universe is caused by Dark Energy. Until recently, scientists thought that the universe would eventually stop expanding and contract again into a singularity, but recent observations have predicted that the universe is expanding continuously due to this mysterious energy, which they have named Dark Energy and which accounts for almost 68% of the universe.
By signing up, you agree to our Terms of Service and Privacy Policy
Due to its contribution to the total mass density, dark matter's gravitational pull on the universe influences the dynamics of cosmic expansion that are seen in the universe and influences the rate of expansion.
By signing up, you agree to our Terms of Service and Privacy Policy
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
- How many cubic nanometers are in a cubic parsec?
- What does cosmic background radiation tell us about the universe?
- Are there experiments in which scientists can recreate aspects of the Big Bang?
- How do you calculate the energy of light that has a wavelength of 10 cm?
- In relation to the size of a galaxy, how do you convert arcminute into distance?
- 98% accuracy study help
- Covers math, physics, chemistry, biology, and more
- Step-by-step, in-depth guides
- Readily available 24/7