How do you convert Hubble's constant?

Answer 1

The Hubble's constant #H_0# is 71 km/sec/mega parsec, nearly. See explanation for conversion.

#H_0# km/sec/mega parsec
#=H_0 X 10^(-6)# km/sec/parsec
#=(H_0 X 10^(-6)/206265)=4.85 x 10^(-12)H_0# km/sec/AU
#=(((H_0 X 10^(-6)/206265))/149597871)= 3.24 X 10^(-20)H_0# km/sec/km
#=(((H_0 X 10^(-6)/206265))/149597871)(365.25 X 24 X 3600)#
#=1.02 X 10^(-12)H_0# km/year/km

In this second edition, i convert #H_0 to age of our universe, in the

Hubble path.

The age of our universe is #1/H_0# years, where #H_0# is obtained

at your discretion, in u/year/u, with u representing a distance unit.

This invariant factor to be applied to the standard #H_0= 71#
km/sec/parsec is #1.02 X 10^(-12)#
Now, #1/(converted H_0)#
#=1/(71 X 1.02 X 10^(-12)) = 1.38 X 10^10# years.
#=13.8# billion years.
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Answer 2

Hubble's constant can be expressed in kilometers per second per megaparsec (km/s/Mpc). Conversion factors or dimensional analysis can be used to convert Hubble's constant to another unit. For example, multiplying by 1,000 will convert km/s/Mpc to km/s/pc, since there are 1,000 parsecs in a megaparsec.

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Answer from HIX Tutor

When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.

When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.

When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.

When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.

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