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Hubble's law describes the observed relationship between the recession velocities of galaxies and their distances from us. It states that the recession velocity of a galaxy is proportional to its distance from us. However, Hubble's law does not directly account for time dilation.

Time dilation is a phenomenon predicted by the theory of special relativity, which states that the passage of time can be influenced by relative motion and gravitational fields. Time dilation occurs when an observer in one reference frame measures a different passage of time compared to an observer in a different reference frame.

In the context of cosmology, time dilation becomes relevant when considering the expansion of the universe. As the universe expands, galaxies recede from each other, and their recession velocities increase with distance. According to Hubble's law, the velocity-distance relationship holds true for these receding galaxies.

Time dilation comes into play when we consider the effect of this expansion on the perceived passage of time for distant objects. As light travels from distant galaxies to us, it traverses an expanding universe. The expansion of space itself affects the wavelength and frequency of the light waves, leading to a phenomenon known as cosmological redshift.

Cosmological redshift causes the light emitted by distant galaxies to be "stretched" to longer wavelengths, shifting it towards the red end of the electromagnetic spectrum. This redshift is a consequence of the expansion of the universe and can be interpreted as a change in the frequency of the light.

The observed redshift of light from distant galaxies is related to the relative motion between the emitting galaxy and our reference frame. This relative motion can result in time dilation effects. Specifically, the time experienced by objects in the distant galaxies appears to pass more slowly relative to our time due to their relative motion away from us.

So, while Hubble's law itself does not explicitly account for time dilation, the observation of redshift in distant galaxies, which is a consequence of the expanding universe, does involve time dilation effects. The redshift provides valuable information about the relative motion and time dilation of these objects in the context of cosmic expansion.

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