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Question: An astronomical unit \( \left( AU \right) \) is equal to the average distance from Earth to the Sun,...

An astronomical unit (AU)\left( AU \right) is equal to the average distance from Earth to the Sun, about 92.9×106mi92.9\times {{10}^{6}}mi . A parsec (pc)\left( pc \right) is the distance at which a length of 1AU1AU would subtend an angle of exactly 11 second of arc. A light-year (ly)\left( ly \right) is the distance that light, travelling through a vacuum with a speed of 186000mi/s186000mi/s , would cover in 1.01.0 year. Express the Earth-Sun distance is light-years

Explanation

Solution

Hint : Length of an arc =rθ\ell =r\theta
Where rr is the radius and θ\theta is the angle subtended by an arc on it’s centre.
θ\theta should be in radian. In case θ\theta is given in some other units then it needs to be consented first into radian.

Complete Step By Step Answer:
Distance between Earth and Sun =92.9×106=92.9\times {{10}^{6}} mi
A parsec is the distance at which a length of 1AU1AU subtend an angle of 11 second of arc so the distance at which 1AU1AU subtend only 11 second of arc r=θr=\dfrac{\ell }{\theta }
But first we need to convert 11 second of arc into radian.
11 sec of arc =160=\dfrac{1}{60} min of arc
11 min of arc =160=\dfrac{1}{60} degree
11 degree =π180=\dfrac{\pi }{180} radian
Therefore 1arcsec=(160×160×π180)1arc\sec =\left( \dfrac{1}{60}\times \dfrac{1}{60}\times \dfrac{\pi }{180} \right) radian
=4.85×106=4.85\times {{10}^{-6}} rad
thus 11 parsec =1AU4.85×106=2.06×105AU...............(i)=\dfrac{1AU}{4.85\times {{10}^{-6}}}=2.06\times {{10}^{5}}AU...............\left( i \right)
speed of light =186000mi/s=186000{}^{mi}/{}_{s}
thus in one year distance travelled by light
1y=186000×1\ell y=186000\times (seconds in 1year1year )
=186000×(365×24×60×60)=186000\times \left( 365\times 24\times 60\times 60 \right)
1y=5.9×1012mi1\ell y=5.9\times {{10}^{12}}mi
Now because 1AU=92.9×106mi1AU=92.9\times {{10}^{6}}mi
Given and in 1Mi=15.9×1012y1Mi=\dfrac{1}{5.9\times {{10}^{12}}}\ell y
So 1AU=92.9×106×15.9×1012y1AU=92.9\times {{10}^{6}}\times \dfrac{1}{5.9\times {{10}^{12}}}\ell y
=1.57×105y=1.57\times {{10}^{-5}}\ell y
And from equation (i)
1AU=12.06×105parsec1AU=\dfrac{1}{2.06\times {{10}^{5}}}par\sec
=4.85×106parsec=4.85\times {{10}^{-6}}par\sec
Thus distance between earth and sun =1AU=92.9×106mi=1.57×105y=1AU=92.9\times {{10}^{6}}mi=1.57\times {{10}^{-5}}\ell y
=4.85×106parsec=4.85\times {{10}^{-6}}par\sec .

Note :
In the formula =rθ\ell =r\theta , students must be careful that θ\theta should be kept in radian. Students should practice the unitary method for conversion questions.
1miles=1.6091 miles=1.609 kilometre
Students if want to solve the question in M.K.S unit standard, they can but it will just increase the number of steps. So students should be careful while working in other unit standards.