Whizzing stars

The star S2 orbits the central region of our galaxy extremely quickly. The star has an orbital period of 15.5 years. The orbit is an ellipse, and the point of closest approach of S2 to the center of our galaxy is 17 light-hours, or 1.84 × 1 0 13 m 1.84 \times 10^{13}~m . To get an idea about how close this is in astronomical terms, this is about four times as far as the distance from the sun to Neptune.

Since the orbit is an ellipse the velocity of the star is not constant. However, we can get a rough estimate of the average speed by treating the orbit as a perfect circle. If the orbit of S2 was a perfect circle of radius 17 light-hours, what fraction of the speed of light is S2 going on average, i.e. what is v S 2 / v l i g h t v_{S2}/v_{light} ?

Details and assumptions

  • The speed of light is 3 × 1 0 8 m / s 3 \times 10^8~m/s .
  • There are 3.15 × 1 0 7 3.15 \times 10^7 seconds in a year.


The answer is 0.00079.

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4 solutions

Michael Tong
Oct 1, 2013

Formulas:

v a v e r a g e = d i s p l a c e m e n t t i m e v_{average} = \frac{displacement}{time}

C = 2 π r C = 2 \pi r

Information bank

t p e r i o d = 15.5 y t_{period} = 15.5y

y = 3.15 × 1 0 7 s y = 3.15 \times 10^7 s

r = 1.84 × 1 0 13 m r = 1.84 \times 10^{13} m

v l i g h t = 3 × 1 0 8 m / s v_{light} = 3 \times 10^8 m/s

Substitution

C = 2 π r = 2 π ( 1.84 × 1 0 13 m ) = 1.15 × 1 0 14 m C = 2 \pi r = 2\pi (1.84 \times 10^{13} m) = 1.15 \times 10^{14} m

t = 15.5 y = ( 15.5 ) ( 3.15 × 1 0 7 ) = 4.88 × 1 0 8 s t = 15.5y = (15.5)(3.15 \times 10^7) = 4.88 \times 10^8s

v S 2 = 1.15 × 1 0 14 4.88 × 1 0 8 = 2.36 × 1 0 5 m / s v_{S2} = \frac{1.15 \times 10^{14}}{4.88 \times 10^8} = 2.36 \times 10^5 m/s

v S 2 v l i g h t = 2.36 × 1 0 5 3 × 1 0 8 = 7.85 E 4 \frac {v_{S2}}{v_{light}} = \frac {2.36 \times 10^5}{3 \times 10^8} = 7.85E-4

total distance travelled in one revolution= 2.pi.R = D (where R=1.84x10^13 meters) total time taken=15.5 years= 15.5 x 3.15x10^7 seconds=T therefore; v = D/T and hence answer= v/speed of light = v / 3x10^8 = 0.00079

The ratio v star v light \dfrac{v_\text{star}}{v_\text{light}} can be written as 2 π R T v light \dfrac{2\pi R}{T v_\text{light}} , where R R is the star's orbit radius and T T is its period. Since T T is being expressed as 17 × 3600 seconds × v light 17 \times 3600 \: \text{seconds} \times v_\text{light} , we can simply the expression to 2 π R T \dfrac{2\pi R}{T} . By placing the adequate and correct numeric values, we find that our desired ratio is: 2 π × 17 × 3600 15.5 × 3.15 × 1 0 7 = 0.00079 \dfrac{2\pi \times 17 \times 3600}{15.5 \times 3.15 \times 10^7} = 0.00079

Orbital Radius of S2(R) = 17 light-hours = 1.84*(10**13) m

Therefore, Circumference of the orbit = 2*pi*R

Orbital period(t) = 15.5 years = 15.5*(3.15*(10**7)) s

c = 3*(10**8) m

Therefore, required ratio = ((2*pi*R)/t)/c = ((3.141592*2*(1.84*(10**13)))/(15.5*(3.15*(10**7))))/(3*(10**8)) = 0.00078928544529783238

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