Question #149642

 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)

Expert's answer

The diameter of that black hole's event horizon (doubled Schwarzschild radius, see https://en.wikipedia.org/wiki/Schwarzschild_radius) is given as


ds=4GMc2d_s = \dfrac{4GM}{c^2}

where G=6.67×1011m3kg1s2G = 6.67×10^{−11} m^3⋅kg^{−1}⋅s^{−2} is the gravitational constant, c=3108m/sc = 3\cdot 10^8m/s is the speed of light, and MM is the mass of the black hole. Since it is equal to 2.4e12 solar masses, obtain:


M=2.4×10121.99×1030kg=4.78×1042kgM = 2.4\times 10^{12}\cdot 1.99\times 10^{30}kg = 4.78\times 10^{42}kg

Thus, obtain:

ds=46.67×10114.78×1042(3108)22.31×1016md_s = \dfrac{4\cdot6.67×10^{−11}\cdot 4.78\times 10^{42}}{(3\cdot 10^8)^2} \approx 2.31\times 10^{16}m

The angular diameter (in radians) is:


θ=dsR\theta = \dfrac{d_s}{R}

where RR is the distance from the Earth to the black hole. Since this distance is 55 million light years, and one light year is approximately 9.46×1015m9.46\times 10^{15}m, the distance is:


R=551069.49×10155.2×1023mR = 55\cdot 10^6\cdot 9.49\times 10^{15} \approx 5.2\times 10^{23}m

Thus, the angular diameter is:


θ=2.31×1016m5.2×1023m4.4423×108rad\theta = \dfrac{2.31\times 10^{16}m}{5.2\times 10^{23}m} \approx 4.4423\times 10^{-8} rad

To convert it to arcseconds, calculate:

θ=4.4423×1083600180/π0.009\theta =4.4423\times 10^{-8}\cdot 3600\cdot 180/\pi \approx 0.009''

Answer. 0.009''.


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