Use the inverse square law for light to answer each of the following questions. a) Suppose a star has the same luminosity as our Sun (3.8×10^26 watts) but is located at a distance of 10 light-years. What is its apparent brightness? Express your answer using two significant figures. b) Suppose a star has the same apparent brightness as Alpha Centauri A (2.7×10^-8 watt/m^2) but is located at a distance of 300 light-years. What is its luminosity? Express your answer using two significant figures. c) Suppose a star has a luminosity of 7.0×10^26 watts and an apparent brightness of 3.0×10^-12 watt/m^2. How far away is it? Give your answer in both kilometers and light-years. Express your answer using two significant figures.
Added by Alba L.
Step 1
Given: Luminosity, L = $3.8 \times 10^{26}$ watts Distance, D = 10 light-years = $9.461 \times 10^{15}$ meters Using the inverse square law formula: $F = \frac{L}{4\pi D^2}$ Show more…
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Suppose a star has the same luminosity as our Sun (3.8x10^26 watts) but is located at a distance of 10 light-years. What is its apparent brightness? Suppose a star has the same apparent brightness as Alpha Centauri A (2.7x10^-8 watt/m^2) but is located at a distance of 300 light-years. What is its luminosity? Suppose a star has a luminosity of 6.0x10^26 watts and an apparent brightness of 4.5x10^-12 watt/m^2. How far away is it? Give your answer in both kilometers and light-years. Suppose a star has a luminosity of 9.0x10^29 watts and an apparent brightness of 4.0x10^-15 watt/m^2. How far away is it? Give your answer in both kilometers and light-years.
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Suppose a star has a luminosity of 8.0×10^26 watts and an apparent brightness of 3.5×10^-12 watt/m^2. How far away is it? Give your answer in both kilometers and light-years. Express your answer using two significant figures. Suppose a star has a luminosity of 6.0×10^29 watts and an apparent brightness of 5.0×10^-15 watt/m^2. How far away is it? Give your answer in both kilometers and light-years. Express your answer using two significant figures.
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Visual Magnitude of a Star If all stars were at the same distance, it would be a simple matter to compare their brightness. However, the brightness that we see, the apparent visual magnitude $m,$ depends on a star's intrinsic brightness, or absolute visual magnitude $M_{V},$ and the distance $d$ from the observer in parsecs ( 1 parsec $=3.262$ light years), according to the formula $m=M_{V}-5+5 \cdot \log (d) .$ The values of $M_{V}$ range from $-8$ for the intrinsically brightest stars to $+15$ for the intrinsically faintest stars. The nearest star to the sun, Alpha Centauri, has an apparent visual magnitude of 0 and an absolute visual magnitude of 4.39 . Find the distance $d$ in parsecs to Alpha Centauri.
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