Do we have to worry about relativity when studying galactic objects? (Intermediate)

I'm puzzled by the implication of the Einstein's theory about time being in a way a function of speed and/or acceleration. Doesn't it mean that time must be actually different on the bodies with different speed if this speed is big enough to notice it? Might be not noticeable on Mars compared to Earth, since the rotation of the Solar System probably compensates or balances somehow and their speed isn't big anyway. But what about time in the whole of the Solar System which rotates with a really huge speed around the centre of the Galaxy compared to time around Antares? What about time in our Local Group compared to the time in the M83, for instance, ot M31?

You ask a good question; it turns out that astronomers do have to worry about the time effects implied by Einstein's theories in certain circumstances.

As you mention, the time measured by an observers in two different reference frames depends on their relative speeds; in short, an observer that is observing an event in a reference frame moving at speed v will measure the time in that frame to move slower than in his frame by a factor gamma=square root of (1-(v/c)2), where c is the speed of light. So, we only need to worry about these effects when (v/c) squared is comparable to 1. To be safe, let's assume that no correction is needed if v is 20% the speed of light.

Now, the speed of light is 300000 km/s, and so only objects with velocities of 60 000 km/s relative to the Earth need to take relativity into account. The Solar system does move quickly around the galactic centre by Earth standards at 220 km/s, but this is nowhere near fast enough to require a correction for relativistic effects. So, the speed with which time elapses in the Solar System and in Antares are very, very nearly the same. Astronomers do have to worry about these relativistic effects when studying so called "high energy phenomena" in the Universe, however. A good example is in the study of jets that are emitted in the vicinity of black holes, both at the centre of distant galaxies and in stellar systems in the solar neighbourhood. These jets are often observed to propagate through the interstellar medium in these systems at substantial fractions of the speed of light (some are even observed to move faster than c, but this is just an illusion caused by relativity). Estimates of the propagation speed and energetics of the jets may require substantial corrections for relativistic effects. Look here for a pretty picture of a jet in a nearby galaxy.

This page was last updated June 27, 2015.

About the Author

Kristine Spekkens

Kristine Spekkens

Kristine studies the dynamics of galaxies and what they can teach us about dark matter in the universe. She got her Ph.D from Cornell in August 2005, was a Jansky post-doctoral fellow at Rutgers University from 2005-2008, and is now a faculty member at the Royal Military College of Canada and at Queen's University.

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http://www.astro.queensu.ca/people/Kristine_Spekkens/main.php
http://www.rmc.ca/aca/phy/per/spekkens-k-eng.php

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