where λ_observed is the observed wavelength and λ_rest is the wavelength in the rest frame of emission. Note z is dimensionless number (i.e., it has no units).
Cosmological redshift is itself the most easily obtained high accuracy/precision direct-observable cosmological distance measure.
Thus, it the most basic direct-observable cosmological distance measure and astronomers customarily use it in preference to all others which harder to obtain and usually much less accurate/precise or are model-dependent which means NOT direct NOR indirect observables.
The upshot is that cosmological redshift is the natural independent variable for plots displaying the other cosmological distance measures as dependent variables which is why it is used for that purpose in Image 1 and Image 2.
A giga-light-year is the distance light travels in a gigayear moving at the vacuum light speed relative to an inertial frame of reference.
The vacuum light speed c = 2.99792458*10**8 m/s ≅ 3*10**8 m/s = 3*10**5 km/s ≅ 1 ft/ns is exactly 1 Gly/Gyr.
They are calculated for the Λ-CDM model (AKA concordance model) which is fitted to observations.
The Λ-CDM model currently fits all observations within uncertainty and is considered the most trustworthy cosmological model currently available.
Further improved observations may require it to be revised or abandoned, but for now it the best we have.
But even if the Λ-CDM model is revised or abandoned, it still fits the observable universe so well, the cosmological distance measures it predicts must still be correct to good accuracy/precision.
For a table correlating the cosmological distance measures, see the figure below (local link / general link: cosmological_redshift_lookup_table.html).
The free parameters of
Λ-CDM model used for
the plots are:
A remarkably simple result in
Friedmann-Lemaitre-Robertson-Walker (FLRW) models
is that
The cosmological redshift
is a direct observable since
intrisic spectral line
wavelengths are well known.
Well extinction can be neglected
or corrected for, but
the observable universe
is NOT static---we live in an
expanding universe.
So luminosity distance
is NOT in general true physical distance.
Note the true physical distance is called
proper distance
Relativityspeak.
However, luminosity distance
is a direct observable given that
you know intrinsic luminosity
(which sometimes you do),
you can measure flux F
(which is usually easy)
and
extinction can be neglected
or corrected for (which sometimes you do.)
In fact, observed
luminosity distances
are key observations in determining the
free parameters of the
Λ-CDM model.
However, z → 0:
luminosity distance
becomes proper distance to
1st order
in small z:
i.e., it becomes proper distance
asymptotically as
cosmological redshift → 0.
The naive Hubble distance would be the
proper distance if the
universal expansion were exponential:
i.e., if the cosmic scale factor a(t)
obeyed the formula:
The naive Hubble distance is NOT a direct observable.
It is plotted on the diagram just a simple reference case.
A cosmological model
with exponential expansion is the
De Sitter universe.
Comoving distance is a
time-independent measure of separation between
astronomical objects
participating in the mean
expansion of the universe.
Comoving distance r_c is related
to proper distance r_p
(which is true physical distance) by the formula
Since a(t=present) = 1 by convention,
comoving distance
and proper distance
are equal at present---and so both are shown
on the plot.
Neither comoving distance
nor proper distance
are direct observables.
They can only be calculated from
a cosmological model---in
the shown plots from the
Λ-CDM model as aforesaid.
We note that a z → ∞,
the comoving distance
asymptotically goes to a constant.
This constant is the comoving radius of the
observable universe.
The value for this comoving radius from the
Λ-CDM model
is ∼ 46.6 Gly = 14.3 Gpc
(see Wikipedia: Observable universe).
The edge of the
observable universe
is called the
particle horizon.
A light signal that started
at the particle horizon
at the mythical time zero of
the FLRW models
(which include the
Λ-CDM model)
would be reaching us just now.
No such light signal from
the particle horizon
can actually be reaching us since: (a) the
FLRW models
CANNOT actually be extrapolated back to time zero,
(b) the light signal
would be redshifted to zero energy if it came from
z = ∞.
Actually, the observable universe
was NOT transparent to light
until the recombination epoch
about 380,000 years after time zero
which corresponds to z ≅ 1100
(see Wikipedia: Recombination).
At present we can only observe to
to z ≅ 1100.
In the future, it may be possible to observe to higher z using
neutrinos or
gravitational waves.
We note that a z → ∞,
the comoving distance
asymptotically goes to a constant
which is just the
age of the observable universe = 13.797(23) Gyr (Planck 2018)
(see
Planck 2018: Age of the observable universe = 13.797(23) Gyr;
Wikipedia: Λ-CDM model: Parameters).
Neither lookback time
in general nor cosmic time are
direct observables.
They can only be calculated from
a cosmological model---in the
shown plots from the
Λ-CDM model as aforesaid.
Angular distance is
proper distance
if spatial geometry
is Euclidean (which it is within uncertainty) and
the observable universe is STATIC
(which it is NOT).
So angular distance is NOT
proper distance in general.
However, it is a direct observable in principle.
But you have to know s and θ.
Now θ can be often measured for
astronomical objects, but
s can usually be only estimated with poor accuracy for most
astronomical objects.
However s can be determined to
some accuracy/precision for
baryonic acoustic oscillations (BAO),
and thus these are very useful
standard rules
for cosmology.
Angular distances
can be used to fit cosmological models.
You may wonder why angular distance
in the log-log plot
reaches a maximum as z increases and then declines.
Well as you look out you look back in cosmic time
and eventually you look back far enough in
cosmic time that an
astronomical object
is seen when it was much closer than now and its
angular distance goes down.
In fact,
angular distance → 0 as z → ∞???.
To explain 1st order
agreement
in this context,
we note that the formulae
the cosmological distance measures
can be written in the
power series expansion form
The exponent z is raised to defines the
order of the term.
The coefficients of the terms are subscripted
by the order of the term.
To agree to 1st order
means that the f_1 coefficient
is the same in for the formulae, but the higher order
coefficients do NOT agree
in general.
However, as z → 0, lookback time
differs from the other
cosmological distance measures
only by a factor of the
vacuum light speed c.
The choice the units
gigayear (Gyr) for time and
giga-light-years (Gly) for distance
cause c = 1 Gly/Gyr which
lookback time agree with the distance-like
cosmological distance measures
to 1st order
in small z.
Yours truly has failed to find a compact general reference for the
1st-order for
the cosmological distance measures.
There is NO analytic formulae for the
cosmological distance measures,
except for the naive Hubble distance formula
which we gave above.
People choose whatever definition suits their needs.
One convenient choice of boundary is z = 0.5.
For z ≤ 0.5, the
cosmological distance measures
all agree to within ∼ 50, whereas for z > 0.5 they diverge more and more.
So z = 0.5 marks a qualitative line in the behavior of the
cosmological distance measures.
Another good feature is that the
lookback time for z = 0.5 is
∼ 5 Gyr.
The Sun
and Solar System is
4.6 Gyr
(see Wikipedia:
Formation and evolution of the Solar System: Timeline of Solar System evolution).
So if we want to consider the Sun itself
as a measure of the observable universe---and we
often do since it is our vantage point in time and space---then
a lookback time of 5 Gyr and z =0.5 are convenient
markers between the old and young
observable universe.
php require("/home/jeffery/public_html/astro/cosmol/cosmological_redshift_lookup_table.html");?>
UNDER CONSTRUCTION below, not required reading
     
z = (λ_observed-λ_rest_frame)/λ_rest_frame = a_0/a(t) - 1
      ,
where λ_observed is the observed wavelength
for an object participating in the mean expansion of the universe
λ_rest_frame is the rest-frame wavelength
(which is known for spectral lines),
a_0 is the cosmic scale factor
for the current cosmic time t,
a(t) is the cosmic scale factor
for the cosmic time when a
light was emitted that
is reaching us at the
at the current cosmic time t = present.
     
a_0/a(t) = z +1
      ,
is the factor
by which the
observable universe
has expanded since the
cosmic time when a
light was emitted.
     
F = L/(4*πr**2)
     
which inverted for r gives
     
r = sqrt[L/(4*πF)]
      ,
the luminosity distance.
The luminosity distance would be the
proper distance
(distance measurable at one instant in time with a ruler) if the
observable universe
were static and if extinction
can be neglected or corrected for.
     
r = (c/H_0)*z = L_H * z
      ,
where c is the vacuum light speed,
H_0 is the
Hubble constant
taken to be a constant in cosmic time
(which it isn't),
L_H = c/H_0 is called the
Hubble length
(note the
Hubble length = L_H = c/H_0 = 4.2827 Gpc/h_70 = 13.968 Gly/h_70)
and
z is the cosmological redshift again.
     
a(t) = a_0*exp(t/t_0 - 1)
      ,
where a_0 = 1 is the current
cosmic scale factor,
exp is exponential function,
and t_0 is the present cosmic time
cosmic time
which is also the
age of the observable universe = 13.797(23) Gyr (Planck 2018)
(see Planck 2018: Age of the observable universe = 13.797(23) Gyr;
Wikipedia: Λ-CDM model: Parameters, but
recall the
expansion of the universe
is NOT exponential expansion).
r_p = r_c * a(t)
where a(t) is the cosmic scale factor
again.
     
r=s/θ
      ,
where is the perpendicular-to-line-of-sight
size of an astronomical object
and θ is the angular size of the
astronomical object
as measured at
Earth.
This item is UNDER RECONSTRUCTION when time allows.
The reason for this is that they agree to
1st order in small z.
     
f(z) = f_1*z + f_2*z**2 + f_3*z**3 + ... as long as z ≤ ∼ 1
      .
Note the lookback time
is a time quantity and the
cosmological distance measures
are distance quantities.
As z → 0, the differences between formulae for the
cosmological distance measures
eventually start decreasing like z**2
and the relative differences like z because the terms of order ≥ 3 become smaller at a faster rate than
lower order terms.
f_1 = L_H = c/H_0 = (13.968 ... Gly)/h_70 for the distance-like quantities
and
f_1 = t_H = 1/H_0 = (13.968 ... Gyr)/h_70 for lookback time,
where t_H=1/H_0 is called the Hubble time.