Is Dark Matter Really Necessary in Our Understanding of the Universe?

In summary: So, in summary, the bulge of the Milky Way has a radius of 40 parsecs and a total stellar mass of 25 billion Solar masses. At this density, the spacetime within the bulge is severely distorted, providing sufficient force to hold onto solar mass objects at the edge of the Milky Way disk. However, this force alone is not enough to explain the observed rotation rate of galaxies, as shown by the need for dark matter to account for other observed phenomena. Additionally, the mass of the Milky Way within a radius of 60,000 light years is estimated to be 210 billion solar masses, with the majority of this mass being made up of dark matter. This suggests that dark matter is necessary
  • #1
neonred
4
0
The bulge of the milky way is 40 parsecs in radius.
There is 288.218 stars per cubic light-year in the milky way bulge.
At the density, spacetime for the entire 40 parsec radius should be severely distorted.
The total stellar mass of the bulge is about 25 billion Solar masses.
The Milky Way has an approximate radius of 50 000 light years

F = (6.67 x 10^-11)(25 x 10^9)(1,989E30) (1,989E30) / [ (50,000)(9.4605284 × 10^15) ]^2
F = (6.5968 X 10^60) / (2.2375 x 10^41)
F = 2.94829 x 10^19 Newtons

Let's calculate the gravitational attraction between Ceres (dwarf planet) and Sun

F = 6.67 x 10^-11)(1,989E30)(8,958 x 10^20) / (414 x 10^9)^2
F = (1.884 x 10^41) / 1.7139 x 10^23)
F = 1.099 x 10 ^ 18 Newtons

We can see that the gravitational force exerted by the distorted space the bulge of the milky way provides sufficient force hold onto solar mass objects at the edge of the milky way disk.

I ask again, why is Dark Matter needed?
The closer you are to the Sun, the greater the depression in spacetime.
But if you have a 40 parsec radius spacetime depression relative to disk and arms...
A depression in spacetime is a depression in spacetime period.
There is no need for dark matter.
Imagine two people pulling a blanket, and a third person putting a small bowling ball in the middle.
How can you say, the bulge or bowling ball does not curve the spacetime around it? It does.
The blanket is the milky way, and the bowling ball is the bulge.
 
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  • #2
neonred said:
We can see that the gravitational force exerted by the distorted space the bulge of the milky way provides sufficient force hold onto solar mass objects at the edge of the milky way disk.
But is that force sufficient to explain the observed rotation rate? For all the galaxies that we can observe? It's not enough to calculate the force (I haven't checked your calculations, but we can assume for the moment that they're correct) between the core of a galaxy and the rim and say that it is looks to be enough to hold an object in orbit around the core. You also have to show that the force Implies an orbital velocity consistent with what we observe; and when we do that we find that there's not enough visible matter to produce the necessary force.

There are many other observed phenomena that cannot be explained by the gravitational attraction of all the matter that we can see; you'll find a partial list in the Wikipedia article on dark matter.
 
  • #3
The people who assembled WMAP data and this paper https://arxiv.org/abs/1703.09233,Mapping dark matter on the celestial sphere with weak gravitational lensing, would be very surprised and disappointed to discover that DM is not needed. It really strains credibility to even suggest these prominent scientists have managed to overlook these and similarly naive objections to DM.
 
  • #4
neonred said:
There is 288.218 stars per cubic light-year in the milky way bulge.

You know this number to six decimal places? Really?

If I were going to kick off a thread arguing that everybody else is wrong, I wouldn't start it this way.
 
  • #5
"So the team used this data to determine the mass of our galaxy. What they found was that within a radius of 60,000 light years the mass is about 210 billion solar masses. It should be emphasized that this is only the mass of our galaxy within a 120,000 light year diameter, which is about the diameter of the visible galaxy. Beyond this region our galaxy is dominated by https://briankoberlein.com/2014/08/15/five-facts/, which makes up most of the total mass of our galaxy. So we can say that the Milky Way has roughly 200 billion stars."

I did the math and the velocity works to be 221542 m/s which is consistent with observed data. In other words, if we define the milky way to be 120, 000 light years in diameter and the mass of the galaxy is 210 billion solar masses, then the milky way does not violate Newton's law of gravitation. In other words, there sufficient stellar matter not only to hold onto Stars in the galaxy, but also to explain the mean velocity of stars at the edge of the disk. The way it has ever been described to me at any corner of the web is, "there is insufficient stellar matter to explain galactic star retention and orbital speed of stars in the disk". This statement appears incredibly incorrect in lieu of Newton's gravity laws and Einstein's general relativity (spacetime).

However, I what about the orbital velocities of clusters which the milky way holds onto outside of the disk, right? I am having difficulty finding a good dataset for this. Please provide so that I can continue my analysis.
 
  • #6
neonred said:
I did the math and the velocity works to be 221542 m/s which is consistent with observed data.

The velocity of what? Consistent with what observed data?

Note that if you're calculating the velocity of the solar system around the galactic center, the solar system is within the radius that your quote explicitly says is not dominated by dark matter, so you would not expect the solar system's velocity calculated on the basis of visible matter to be different from observation. You would have to find an object significantly further out from the center than 60,000 light years, which the solar system is not (it's only about 30,000 light years from the center).

neonred said:
what about the orbital velocities of clusters which the milky way holds onto outside of the disk, right? I am having difficulty finding a good dataset for this. Please provide so that I can continue my analysis.

In other words, you don't even have the data you need to back up the extreme claims you are making. And rather than go get it yourself, you want us to provide it? Sorry, it doesn't work that way.

Thread closed.
 

1. What is dark matter?

Dark matter is a type of matter that makes up about 85% of the total matter in the universe. It does not emit or absorb light, which is why it is "dark" and cannot be directly observed. Its presence can only be inferred through its gravitational effects on visible matter.

2. How is dark matter needed in our understanding of the universe?

Dark matter is needed in our understanding of the universe because it plays a crucial role in the formation and evolution of galaxies. Without dark matter, the current theories and models of the universe cannot explain the observed structure and dynamics of galaxies.

3. What evidence supports the existence of dark matter?

There are several lines of evidence that support the existence of dark matter. These include the rotation curves of galaxies, the gravitational lensing effect, and the cosmic microwave background radiation. These observations cannot be explained by visible matter alone and require the presence of dark matter.

4. How is dark matter different from regular matter?

Dark matter is different from regular matter in several ways. It does not interact with light, it does not emit or absorb any electromagnetic radiation, and it does not have an electric charge. Additionally, it is much more abundant than regular matter, making up about 27% of the total matter in the universe.

5. Can we detect or directly observe dark matter?

Currently, we do not have the technology to directly detect or observe dark matter. However, scientists are working on experiments and technologies that may be able to detect dark matter indirectly through its interactions with regular matter. These include experiments using underground detectors and particle accelerators.

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