The Cosmic Setup
Imagine you are standing on Earth, looking up at the night sky. A distant galaxy is moving away from us at a staggering speed of 286 km/s. Because it is moving away, the light it emits gets stretched out as it travels through space towards us. This phenomenon is called redshift, which is a classic example of the Doppler effect for light.
To work with standard SI units, we first convert the given values. The velocity of the galaxy is v=286×103 m/s. The original wavelength of the red line is λ=630 nm=630×10−9 m.
The Master Equation
To find out exactly how much the wavelength stretches, we use the Doppler shift formula for light. When the velocity of the source is much less than the speed of light (v≪c), the fractional change in wavelength is equal to the ratio of the source's velocity to the speed of light:
Here, Δλ represents the shift in wavelength, and c=3×108 m/s is the speed of light in a vacuum. This is a fundamental relation used extensively in astrophysics to determine how fast galaxies are receding from us.
Final Calculation
Let's rearrange the formula to solve for Δλ and carefully substitute our known values:
Δλ=3×108286×103×630×10−9
To avoid silly mistakes, it is always best to group the numbers and the powers of ten separately. We can easily divide 630 by 3 to get 210:
Now, combining the powers of ten (3−9−8=−14) and multiplying the integers (286×210=60060):
The question asks for the answer in the format of x×10−10 m. To achieve this, we shift the decimal point four places to the left, which multiplies the coefficient by 104:
Comparing our result with the given expression x×10−10 m, we see that x=6.006. Rounding to the nearest integer, we get x=6.
Always remember to pay attention to the direction of motion. If the galaxy were moving towards us, the light waves would be compressed, resulting in a shorter wavelength. This is known as a blueshift.