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