Originally Posted By: MolaKule
There have been many fudge factors introduced in Astronomy to keep the status quo and to make the equations appear valid.
Dark Matter and Dark Energy are not new fudge factor concepts.
Around 1890, it was observed that Mercury’s orbit was being perturbed and some unknown agency was involved.
Specifically, Mercury’s perihelion (
https://en.wikipedia.org/wiki/Perihelion_and_aphelion ) was advancing 43 seconds of arc per century and could not be explained by Newtonian orbital mechanics.
The solution was to propose some form of “dark” matter which could not be seen, such as the planet “Vulcan” or an asteroid belt. Astronomers ignored the fact that a mass associated with Mercury would have a shorter orbital period than Earth.
In 1915 Einstein’s General Theory of Relativity solved the problem and was able to calculate precisely the anomalous 43 arc-seconds perturbation. Thus, Dark Matter was no longer needed.
Newton’s equation for mass, M = v^2*R/G, is still used by astronomers today to determine masses outside our solar system, where M = mass, v is the velocity of the orbital body, and R is the distance between the star and the orbiting body.
Masses can also be inferred from the amount of visible luminous material seen and measured from telescopes.
The problem is, Newton’s M and the mass inferred from visible luminous material doesn’t agree.
From Newton’s M (dynamical considerations) there appears to be more mass than from the “inferred” method, and this is called the M/L ratio. The problem with this ratio is that the calculated Mass/Luminosity ratio can vary between 2 and 600.
Since there is such a wide variation in this ratio, something was needed to make this wildly varying ratio fit the cosmological theories. So Dark Matter was re-introduced.
Mola, who came up with the idea to estimate mass based on luminous material visible? Isn't this just estimating the volume based on a diameter, then estimating the mass given some arbitrary density? No wonder this relationship varies so much. Even the density of the planets in our own solar system vary wildly. Earth is the most dense at ~5.51 g/cc with Saturn having the lowest density of ~0.687 g/cc...and that much variation is just in our own solar system. It doesn't seem like a wise idea to estimate the mass in this manner.