Astronomy: abundance, concentration, density

In summary, the equation d(surface density * concentration)/dt represents the rate of change of the nuclide's abundance in the interstellar medium.
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Puchinita5
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Homework Statement



Hi. I feel like this is probably very basic. Basically, I'm trying to understand how

surface density * concentration = abundance


I'm reading about gas surface density in the galaxy and its relationship to star formation, gas ejection etc. And we are given an equation that states

d(gas surface density)/ dt = rate of gas ejection - rate of star formation

then it goes on to say that the "abundance of a nuclide in the Interstellar Medium is the concentration times the density"

and now they do a proof where d(surface density * concentration)/dt is supposed to be the rate of change of the element's abundance.


I'm not understanding how multiplying a concentration by surface density would give an abundance. Can someone help explain this?


Homework Equations





The Attempt at a Solution

 
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  • #2
Abundance is defined as the relative amount of a given element or compound in a particular environment. In the context of interstellar medium, it refers to the relative amount of nuclide present in the gas clouds. Surface density is the amount of mass per unit area. It is a measure of the thickness of a material on a surface. Concentration can be thought of as the amount of a certain element or compound within a given volume. When you multiply the surface density by the concentration, you get the amount of the element or compound per unit area. This is the same as the abundance of the nuclide in the interstellar medium.
 

1. What is the definition of abundance in astronomy?

Abundance in astronomy refers to the amount or proportion of a specific element or molecule present in a celestial object, such as a star or a planet.

2. How is the concentration of elements determined in the universe?

The concentration of elements in the universe is determined by analyzing the spectral signatures of celestial objects. This involves measuring the amount of light emitted at different wavelengths, which can reveal the presence and abundance of various elements.

3. What is the relationship between abundance and density in astronomy?

In astronomy, abundance and density are related in that the abundance of elements or molecules in a celestial object can contribute to its overall density. However, density can also be affected by other factors such as temperature, pressure, and gravitational forces.

4. How do astronomers measure the density of celestial objects?

Astronomers use various techniques, such as spectroscopy, to measure the density of celestial objects. They can also calculate density by determining the mass and size of the object, or by studying its gravitational effects on surrounding objects.

5. How does the abundance of elements vary in different parts of the universe?

The abundance of elements can vary greatly in different parts of the universe. For example, the early universe was primarily composed of hydrogen and helium, while heavier elements like carbon and oxygen are more abundant in later stages of star formation. Additionally, the abundance of elements can vary within different types of galaxies and even within individual stars.

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