Black Holes - The supermassive black hole imaged by the Event Horizon Telescope (EHT) is one of the largest black holes in the nearby Universe.  At a distance of 55 million light years from Earth, and with a mass equal to 2.4e12 solar masses, calculate the angular diameter of that black hole's event horizon as viewed from the Earth. (express your answer in arcseconds)

Applications and Investigations in Earth Science (9th Edition)
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ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
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Black Holes - The supermassive black hole imaged by the Event Horizon Telescope (EHT) is one of the largest black holes in the nearby Universe.  At a distance of 55 million light years from Earth, and with a mass equal to 2.4e12 solar masses, calculate the angular diameter of that black hole's event horizon as viewed from the Earth. (express your answer in arcseconds)

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Step 1

The points in the space that are very dense and forms deep sinks for gravity are called black holes. The gravitational field of such black holes is very intense that even the light which have such a huge speed can't pass through them.

Step 2

The diameter of the black hole's event Horizon telescope is given by,

d=4GMc2

G= the gravitational constant having value 6.67×10-11m3/kg sec2  , c= speed of the light having value 3×108m/sec  , and M is the black hole's mass. It is given the mass of the black hole is 2.4e12 solar masses. As, 1 solar mass=1.99×1030kg . So, on calculating its mass in the kilograms, we get,×1015m

M=  2.4×1012×1.99×1030kg=4.78×1042kg

So on putting the values on the above formula, the diameter obtained is,

d=4×6.67×10-11×4.78×1042(3×108)2=2.31×1016m

We know  the angular distance in radians is calculated by the formula,

θ=dR

R is the distance from the earth to the black hole=55 million light-years. We know, One light year=9.46×1015m . So,

R=55×106×9.46×1015=5.2×1023m  

Thus,  the angular diameter is,

θ=2.31×1016m5.2×1023m=4.44×108radians

For converting radians to arc seconds, we will multiply it by 3600×180π

so, θ=4.44×108×3600×180π=0.009arcseconds

 

   

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