# Why is “gravitational” red-shift neglected in galaxy and galaxy cluster scales?

The red-shift of the light of a star in a galaxy or that of a galaxy in a cluster of galaxies is generally interpreted as how fast the star or the galaxy is moving, i.e. it is interpreted in a purely special-relativistic way. However, general relativity predicts that a light produced in a gravitational field gets red-shifted when comes out of the field. I wonder why the excess red-shift (over the Hubble red-shift) of stars and galaxies is only interpreted as how fast the object moves, not that how strong the ambient gravitational field is.

## 2 Answers

A Galaxy cluster could have $10^{14}$ solar masses within a radius of 5 Mpc.

In this case $GM/Rc^2 \sim 10^{-6}$, equivalent to a velocity shift of less than 1 km/s.

Our own Milky Way has a mass of around $10^{12}$ solar masses within 100 kpc. This gives a gravitational redshift of about 100 m/s.

These are completely negligible compared to cosmological redshifts and the peculiar velocities within clusters or groups of galaxies (the latter are of order 100-1000 km/s).

EDIT: To clarify, as a result of Lubos's comment (see below). Because the Earth is in the Milky Way, light is gravitationally blueshifted on it's way into the Milky Way and also into the "local group" of galaxies. However that light has emerged from a different galaxy in a different environment that will be redshifted as it makes its way out of that potential. These two shifts will not in general cancel because galaxies and galaxy clusters have a variety of masses, sizes and potential depths. Hence the numbers I give are the correct orders of magnitude for the errors introduced by ignoring gravitational redshift, but any exact correction needs to be calculated on a case-by-case basis.

FURTHER EDIT: The comment above is even more apt in the light of the literature referred to by Pulsar. For example Cappi (1995) model the (more realistic) potentials of rich clusters and show that the redshift is a strong function of where the galaxy is in the cluster, but could be anywhere in the range from less than 1 km/s to 300 km/s at the centres of the most massive clusters. This is a lot larger than my estimate above because densities in clusters vary more steeply than $r^{-2}$. However, this is still small compared to their velocity dispersions within the same clusters, because more massive clusters also have higher intrinsic velocity dispersions.

• No, Rob, it's your example that is wrong. A galaxy cluster could add $10^{-6}$ to the red shift but both the source of the light and we are at generic points of a galaxy cluster so the red shifts that you talk about basically cancel and we observe nothing. That's why I am talking about gravitational red shifts at places that significantly differ from the points on the surface of the Earth inside a galaxy, like on the surface of stars. – Luboš Motl Nov 3 '15 at 10:09
• @LubošMotl I agree with your comment, but not that my example is wrong. We are not in a dense Galaxy cluster but the Milky Way is a comparatively massive galaxy. In other words the redshifts do not exactly cancel and the numbers that I give do correspond to the order of magnitude for "errors" engendered by ignoring gravitational redshift. The correct corrections would have to be calculated on a case-by-case basis. – Rob Jeffries Nov 3 '15 at 10:23
• OK, I agree with those remarks. The potentials quantitatively differ. At the end, one doesn't find any particular examples in which the gravitational red shift from very extended blocs of matter would beat the Doppler or cosmological red shift. – Luboš Motl Nov 3 '15 at 11:33
• Going through the literature, it seems that gravitational redshift in clusters is of the order of 10 km/s. It's too small to be measured in individual clusters, but in principle it can be detected in a statistical ensemble of clusters by looking at the galaxy velocity distribution. See arxiv.org/abs/1109.6571 and references therein. – Pulsar Nov 3 '15 at 11:42
• @Pulsar I see the paper, but am finding it hard to reproduce of order 10 km/s with a simple calculation. What is going on here is that the density of clusters is quite centrally peaked, so that the redshift from a galaxy near the centre is much higher than one near the outskirts. – Rob Jeffries Nov 3 '15 at 12:00

The gravitational red shift is only significant for black holes – where the coefficient may grow arbitrarily large in the vicinity of the horizon – and the neutron stars – where the frequency drops to something comparable to 50%.

For all other celestial objects, the red shift is much smaller than one. And only planets and white dwarfs are objects for which the red shift may be easily detectable. It's helpful to calculate the red shift for the Sun. The red shift is given by the gravitational potential $$\frac{\Delta f}{f} = - \frac{GM}{Rc^2}$$ For the Sun, the relative decrease of the frequency may be calculated e.g. via Wolfram Alpha

http://www.wolframalpha.com/input/?i=Newton%27s+constant+times+solar+mass+over+solar+radius+over+c%5E2

and it is just $2\times 10^{-6}$; two parts per million. Note that the Hubble constant is about $10^{-10}$ per year – the inverse of 14 billion years, more precisely, so the distance needed to reduce the frequency relatively by two parts per million is $2\times 10^{-6}$ times 14 billion light years which is just 28,000 light years. That's still inside our galaxy!

For all other galaxies, the cosmological red shift is much greater than the gravitational red shift from Sun-like stars. The Sun is just too large, by radius, too diluted. This smallness of the gravitational potential becomes even more extreme if you consider the "groups" of stars such as galaxies themselves.

• Thank you Lubos. But isn't that there is a huge amount of dark matter around galaxies and galaxy clusters? Doesn't that produce a measurable amount of gravitational red-shift? – user65852 Nov 2 '15 at 19:13
• Dear @Kamran, the amount of visible or dark matter in a galaxy or cluster is huge but the gravitational red shift depends on the gravitational potential, and that decreases with the distance from the matter. And the distances in the galaxies and clusters are even more huge than the masses, and they win in the comparison. The visible and dark matter are very comparable in their effect - dark matter is just 5 times greater an energy density than the visible one in average, but it's even less concentrated than the visible one (greater typical distances). – Luboš Motl Nov 3 '15 at 10:06