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Mathematics 17 Online
OpenStudy (anonymous):

Not sure if this can be considered suitable for the Mathematics forum; a calculation in Astrophysics :)

OpenStudy (anonymous):

The scale factor a(t) describes the expansion of the Universe. By considering how the redshift of light depends on the scale factor, calculate how the present-day physical separation of galaxies com- pares with their separation when light left galaxies we see today at redshift 1?

OpenStudy (anonymous):

What is it youre wanting to calculate?

OpenStudy (anonymous):

Maybe it's the z+1 = a_now/a_then....dunno.

OpenStudy (anonymous):

I cant tell if youre asking about the doppler effect making the galaxies appear redshifted since they are mostly moving away from us, or what

OpenStudy (anonymous):

Yeah, I think possibly I have to derive it? I take comfort in the fact that no one else really understands it either haha

OpenStudy (anonymous):

Doesn't say anything about the Doppler effect.... :S assignment question is just written as above :/

OpenStudy (anonymous):

Completely guessing here but if 2 = a_now/a_then -> implies doubling....

OpenStudy (anonymous):

What do u think, twice as far apart..?

OpenStudy (anonymous):

Is this formula z+1 = a_now/a_then in your course?

OpenStudy (anonymous):

Erm, if wavelengths have doubled (and lambda_now/lambda_then = a_now/a_then) then that implies the universe was half its present size when the light was emitted... Is that what you mean? And yep, thats the equation :)

OpenStudy (anonymous):

Well when did redshift 1 occur?

OpenStudy (anonymous):

/=equation - formula**

OpenStudy (anonymous):

I don't know when redshift = 1 was/is/will be :S

OpenStudy (anonymous):

So z is redshift-> 2 = a_now/a_then would seem to say that the "scale" is twice as big as it was then.

OpenStudy (anonymous):

Or it was half what is now, if u prefer...

OpenStudy (anonymous):

So the galaxies are twice as far apart now... Not my specialty this, I got that formula from http://en.wikipedia.org/wiki/Redshift

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