Why Do Galaxy Clusters Look Stretched in Redshift Maps?

Galaxy clusters can look stretched toward the observer in redshift maps because the galaxies’ internal motions alter the redshifts used to estimate their distances. If every redshift difference is treated as a distance difference, galaxies in one compact cluster are placed at artificially spread-out positions along the line of sight.

Astronomers call this pattern the fingers-of-God effect. It is a distortion in a map inferred from spectra, not proof that clusters form long physical spikes aimed at Earth. The underlying motions are real; their translation into apparent depth creates the misleading shape.

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A sky position does not supply the third coordinate

A telescope image gives angular positions: which direction each galaxy occupies on the sky. A three-dimensional map also needs depth. Galaxy surveys often obtain that information by measuring spectral redshifts and applying a cosmological distance model.

That is useful because cosmic expansion relates distance to redshift. But a galaxy can also move relative to the average expansion around it. This additional motion is called a peculiar velocity; “peculiar” is a technical label, not a claim that the motion violates ordinary gravity.

Peter Coles’s explanation hosted by NED writes the low-redshift approximation as v = H₀d + vₚ, where vₚ is the line-of-sight peculiar component. The observed velocity-like quantity combines the expansion term with local motion.

Our guide to measuring cosmic distances introduces that limitation. The specific consequence here appears when a map mistakes the local-motion contribution for extra or missing distance.

Give one compact cluster an artificial depth

Consider a hypothetical nearby cluster centered approximately 100 megaparsecs away. For illustration, adopt H₀ = 70 kilometers per second per megaparsec and neglect its physical depth compared with the effect being demonstrated. A megaparsec is one million parsecs.

The expansion contribution in this simplified model is 70 × 100 = 7,000 km/s. Now give three member galaxies line-of-sight peculiar velocities of −700, 0, and +700 km/s relative to that mean.

Their observed velocity-like values become 6,300, 7,000, and 7,700 km/s. A naive conversion that divides each by H₀ places them at 90, 100, and 110 megaparsecs.

The map has invented a 20-megaparsec spread for galaxies assigned approximately the same actual distance in this example. It has not created extra separation on the sky: the wrong placement is along the radial coordinate inferred from redshift.

These are chosen numbers, not measurements of a named cluster or a new determination of H₀. The additive velocity and linear distance relation are low-redshift approximations; a map of the distant universe needs the appropriate cosmological conversion instead.

Why the fingers point toward the map’s observer

Cluster galaxies have substantial motions in different directions within the gravitationally bound system. The part of each motion toward or away from the observer changes its measured redshift.

Alison Coil’s review of real and redshift space explains how those differing redshifts stretch a cluster along the line of sight. On a map centered on the observer, that direction changes from one part of the sky to another. The resulting features can therefore look like radial fingers all pointing back toward the map’s origin.

Nothing needs to align the physical clusters toward us. The common alignment follows from the measurement direction used to infer each cluster’s depth.

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Real clusters are not necessarily perfect spheres, and real filaments exist. The effect does not mean every elongated structure is false. It means shape inferred from redshift alone must be distinguished from independently established spatial structure.

This is measured, not just a drawing trick

In their 2002 study of early Sloan Digital Sky Survey data, Idit Zehavi and colleagues measured galaxy clustering separately along and across the line of sight. Their small-scale correlation pattern showed the elongation expected from internal velocity dispersion. The sample contained 29,300 galaxies; it was a specific early survey sample, not a census of every galaxy or today’s entire SDSS archive.

That comparison also showed why one explanation does not cover every scale. Random motions in collapsed systems produce the small-scale stretching, while coherent large-scale flows can produce a different distortion: an apparent compression along the line of sight. The latter is often called the Kaiser effect.

Both patterns contain information about gravitational motion. Treating them solely as image errors would throw away useful evidence; treating them as literal physical shapes would misread the measurement.

How to read a map without overinterpreting it

Check whether the radial coordinate is redshift, an inferred distance, or a distance corrected using a peculiar-velocity model. Look for the assumed cosmology and the description of any corrections. Removing fingers is a model-dependent reconstruction, not a fresh direct observation of each galaxy’s position.

Also distinguish the map from a normal photograph. A redshift wedge or clustering contour is a constructed representation; its axes and selection limits carry information the picture alone cannot supply. The cluster and supercluster overview introduces the structures themselves, but interpreting their plotted shapes requires this additional measurement step.

The essential distinction is between where a galaxy is and where its redshift places it under an assumed conversion. Fingers of God are what happens when those two coordinates diverge systematically inside a moving cluster.

AI-generated illustration for Galileo Whispers of a generic galaxy cluster. This is not a photograph, a redshift map or a reconstruction of measured galaxy positions.

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Newsroomhttp://galileowhispers.com
Newsroom is the editorial byline of Galileo Whispers, an English-language astronomy publication. Our focus is explaining stars, planets, galaxies, and the science behind them, alongside practical observing guides and celestial events.

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