Question

Globular clusters are spherical clusters of stars that orbit a galaxy, some of the older ones...

Globular clusters are spherical clusters of stars that orbit a galaxy, some of the older ones in the Milky Way are 13 Gyr old. At what distance would these globular clusters cease to spiral into the galactic nucleus due to the effects of dynamical friction if it has a mass of 6×106M⊙ and an orbital speed of 230 km/s?

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Answer #1

given

tmax = 13 Gyr ( 109 yr / Gyr )

= 13 x 109 x 3.14 x 107

= 40.8 x 1016 sec

M = 6 x 106 M

= 6 x 106 x 2 x 1030

= 1.2 x 1037 kg

vm = 230 km/sec

= 230000 m/sec

C = 76

G = 6.67 x 10-11 m3 / kg sec2

using equation

rmax = ( tmax C G M / 2 vm )1/2

= ( 40.8 x 1016 x 76 x 6.67 x 10-11 x 1.2 x 1037 / 2 x 3.14 x 230000 )1/2

= 1.31 x 1020 m

or

= 1.31 x 1020 / 3.1 x 1019

= 4.225 kpc

At 1.31 x 1020 m or 4.225 kpc distance would these globular clusters cease to spiral into

the galactic nucleus due to the effects of dynamical friction if it has a mass of 6 x 106M

and an orbital speed of 230 km/s.

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