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How far away are the most distance objects we can see?
What is currently the volume of space that we can study with the light that is reaching us?
You might want to look at this brief Cosmology FAQ paragraph:
http://www.astro.ucla.edu/~wright/cosmology_faq.html#DN
*******footnote stuff, background on distance scales used****
Cosmologists use several different indicators of distance and
for a discussion of the various sorts of distance, as well as
a Javascript calculator that converts between them (if you specify
what assumptions you are making about the model), see:
http://www.astro.ucla.edu/~wright/cosmo_02.htm
http://www.astro.ucla.edu/~wright/CosmoCalc.html
Among the most commonly used indices are redshift (z)
and "comoving distance".
The latter is measured at the present from rest with respect to the CMB and it is the type of distance that works in the
Hubble law relating distance to velocity
v = H0 D
the present comoving distance to an object multiplied by the
current value of the Hubble parameter is equal to the present radial comoving velocity
Other types of distance are "angular distance" (angular smallness of an object of known size) and "luminosity distance"
(dimness of a source of known brightness) and "light travel time".
The last does not work in the Hubble law and may be difficult to determine because different parts of the light's path have undergone different amounts of stretching---the travel time is hard to relate consistently to other measures of distance. But it is one of the indices that is calcuated by the "Cosmo Calculator" at Ned Wright's site.
What is currently the volume of space that we can study with the light that is reaching us?
You might want to look at this brief Cosmology FAQ paragraph:
http://www.astro.ucla.edu/~wright/cosmology_faq.html#DN
*******footnote stuff, background on distance scales used****
Cosmologists use several different indicators of distance and
for a discussion of the various sorts of distance, as well as
a Javascript calculator that converts between them (if you specify
what assumptions you are making about the model), see:
http://www.astro.ucla.edu/~wright/cosmo_02.htm
http://www.astro.ucla.edu/~wright/CosmoCalc.html
Among the most commonly used indices are redshift (z)
and "comoving distance".
The latter is measured at the present from rest with respect to the CMB and it is the type of distance that works in the
Hubble law relating distance to velocity
v = H0 D
the present comoving distance to an object multiplied by the
current value of the Hubble parameter is equal to the present radial comoving velocity
Other types of distance are "angular distance" (angular smallness of an object of known size) and "luminosity distance"
(dimness of a source of known brightness) and "light travel time".
The last does not work in the Hubble law and may be difficult to determine because different parts of the light's path have undergone different amounts of stretching---the travel time is hard to relate consistently to other measures of distance. But it is one of the indices that is calcuated by the "Cosmo Calculator" at Ned Wright's site.