How do we know how much visible matter exists?

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In summary, Baryonic Dark Matter is hypothetical matter that does not interact with the electromagnetic force, but whose presence can be inferred from gravitational effects on visible matter. There are three proposed explanations of this matter: Xezlec's MACHO, Wiki's definition of Dark Matter, and the 'baryonic' definition.
  • #1
Xezlec
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In discussions of how we infer the existence of dark matter, it always feels like people gloss over how exactly we know how much "visible matter" exists. I am led to believe that "visible matter" refers to any matter which can interact with things like photons, but doesn't that include things that might not be bright and flamey like stars? How can we tell there isn't just way more dirt, dust, gas, rock, rogue planets, space squirrels, icky black crud, and floating black velvet paintings of Elvis out there than what is close to stars and thereby illuminated?
 
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  • #4
Math Is Hard said:
No, I think the question is about plain old baryonic matter. Not dark. It's a good question.

It depends on how you define "dark matter". The proposed explanations from Xezlec are within the definitions on baryonic dark matter, (MACHO). The deifinition made by wiki article on Dark Matter "dark matter is hypothetical matter that does not interact with the electromagnetic force, but whose presence can be inferred from gravitational effects on visible matter." which already in the definition out rules the possibility of baryonic (in this context non leptonic, neutrino background are referred to as baryonic dark matter even thoug neutrinos are leptons)- and strong interacting dark matter.

The best definition of dark matter would be matter that can't be observed by telescopes due to their EM interactions but must exist due to its gravitational interaction. With this definition; both WIMPs, MACHOs, 'baryonic' and SIMPs (strongly interacting dark matter) are possible.
 
  • #5
Thanks, everyone! That answers my question six ways from Sunday, and gives me more to read about too.
 

FAQ: How do we know how much visible matter exists?

1. How do we measure the amount of visible matter in the universe?

To measure the amount of visible matter in the universe, scientists use a variety of methods such as observing the rotation of galaxies, analyzing the light emitted by stars and galaxies, and studying the cosmic microwave background radiation. These methods allow us to estimate the total amount of visible matter in the universe.

2. What is the difference between visible matter and dark matter?

Visible matter, also known as baryonic matter, is made up of the building blocks of atoms such as protons, neutrons, and electrons. Dark matter, on the other hand, is a type of matter that does not interact with light and cannot be seen directly. It is believed to make up about 85% of the total matter in the universe.

3. How do we know that the amount of visible matter is not the same everywhere in the universe?

Scientists use observations of the cosmic microwave background radiation, which is a remnant of the early universe, to study the distribution of matter in the universe. They have found that the amount of visible matter is not evenly distributed and varies across different regions of the universe.

4. Can we see all the visible matter in the universe?

No, we cannot see all the visible matter in the universe. Some of it may be hidden behind other objects, while some may be too far away for us to detect. Additionally, some matter may be in the form of gas or dust that is not easily visible to us.

5. How does the amount of visible matter affect the structure of the universe?

The amount of visible matter in the universe plays a crucial role in determining the structure of the universe. It is responsible for the formation of galaxies, stars, and other celestial bodies. The distribution of visible matter also affects the overall shape and evolution of the universe.

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