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Astronomical observations of light from the Milky Way galaxy's stars indicate that it has a mass of about 8.0×10^11 solar masses. What should the orbital period of that star be? If its period is 6.0×10^7 years instead, what is the mass of the galaxy?

a) 2.6×10^8 years, 1.6×10^11 solar masses
b) 2.6×10^7 years, 1.6×10^12 solar masses
c) 6.0×10^7 years, 1.6×10^11 solar masses
d) 6.0×10^8 years, 1.6×10^12 solar masses

User Arx
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Final answer:

Using Kepler's third law of planetary motion, specifically a modified version suited for galactic scales, we can determine the orbital period of a star or the mass of the galaxy based on the star's orbital period. The calculations are intricate, involve conversions between light-years to years, and account for gravitational influences, including dark matter. This allows astronomers to infer the presence of dark matter and massive black holes.

Step-by-step explanation:

To determine the orbital period of a star in the Milky Way, or the mass of the Milky Way based on a star's orbital period, we use a form of Kepler's third law of planetary motion. This form states that the square of the orbital period (P) is directly proportional to the cube of the semi-major axis (a) of its orbit, multiplied by the sum of the masses (M) of the two bodies, usually in solar mass units when dealing with stars and galaxies.

For part (a), assuming that the orbital period is directly proportional to a^1.5 (since we're assuming M galaxy + M star is roughly equal to M galaxy), we can set up a ratio using known quantities: (P_new / P_old) = (a_new / a_old)^1.5. From our given, we know the Milky Way has a mass of 8.0 × 10^11 solar masses and the semi-major axis is given as 6.0 × 10^4 light-years, but we need to convert this distance into the same unit as the given galactic year, i.e., years. Knowing that light travels at approximately 9.461 × 10^12 km per year, and one light year equates to this distance, we can find out the approximate period.

For part (b), assuming the given period is 6.0 × 10^7 years, we use similar proportions to solve for the mass of the galaxy. We set the known period in relation to the known mass of the galaxy and can apply the rearranged form of Kepler's third law to find what the mass must be if the period is as given.

However, without going through the detailed calculations here, which would involve modifying Kepler's law to suit the context of a galaxy (including gravitational effects and dark matter considerations), we can recognize that these are complex physics calculations that generally yield results used to imply the existence of dark matter and suggest the presence of massive black holes.

User Introspective
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