Photo AI

A teacher uses a buzzer attached to a string to demonstrate the Doppler effect to a group of students - Scottish Highers Physics - Question 5 - 2022

Question icon

Question 5

A-teacher-uses-a-buzzer-attached-to-a-string-to-demonstrate-the-Doppler-effect-to-a-group-of-students-Scottish Highers Physics-Question 5-2022.png

A teacher uses a buzzer attached to a string to demonstrate the Doppler effect to a group of students. The buzzer produces a sound of constant frequency. The teacher... show full transcript

Worked Solution & Example Answer:A teacher uses a buzzer attached to a string to demonstrate the Doppler effect to a group of students - Scottish Highers Physics - Question 5 - 2022

Step 1

Explain, in terms of wavefronts, why the frequency of the sound heard by the students is lower...

96%

114 rated

Answer

As the buzzer moves away from the students, the wavefronts are stretched, leading to fewer wavefronts passing a given point per second, resulting in a lower frequency. Conversely, when the buzzer moves towards the students, the wavefronts are compressed, which means more wavefronts arrive per second, increasing the frequency.

Step 2

Calculate the redshift of star B.

99%

104 rated

Answer

The redshift ( ext{z}) is calculated using the formula:

z=λobservedλrestλrestz = \frac{\lambda_{observed} - \lambda_{rest}}{\lambda_{rest}}

Given: ( ext{\lambda_{observed}} = 610, nm) and ( ext{\lambda_{rest}} = 580, nm):

z=610580580=305800.0517z = \frac{610 - 580}{580} = \frac{30}{580} \approx 0.0517

Step 3

Determine the approximate distance from Earth to the binary star system.

96%

101 rated

Answer

Using the redshift formula along with the relationship of distance and redshift, the distance (D) can be calculated from the redshift:

D=zcH0D = z \cdot \frac{c}{H_0}

Where (c = 3.00 \times 10^8 m/s) and assuming a Hubble constant (H_0) for calculation, we find:

If (z \approx 0.0517):

D \approx 0.0517 \cdot \frac{3.00\times10^8}{67.8 \times 10^3} \approx 2.3 \times 10^8 m\

Step 4

Calculate the gravitational force between star A and star B at this instant.

98%

120 rated

Answer

The gravitational force (F) is calculated using Newton's law of gravitation:

F=Gm1m2r2F = G \frac{m_1 m_2}{r^2}

Where:

  • (G = 6.67 \times 10^{-11} \frac{N m^2}{kg^2})
  • (m_1 = 2.19 \times 10^{30} kg)
  • (m_2 = 1.80 \times 10^{30} kg)
  • (r = 3.44 \times 10^{12} m)

Substituting these values yields:

F=6.67×1011(2.19×1030)(1.80×1030)(3.44×1012)22.22×1020NF = 6.67 \times 10^{-11} \frac{(2.19 \times 10^{30})(1.80 \times 10^{30})}{(3.44 \times 10^{12})^2} \approx 2.22 \times 10^{20} N

Step 5

State how many times greater the gravitational force between star A and star B is at this point, compared to that in (i).

97%

117 rated

Answer

If the distance between the stars is halved, the gravitational force increases by a factor of (4). This is because gravitational force is inversely proportional to the square of the distance: (F \propto \frac{1}{r^2}), so halving the distance results in: (4 \times F_{original}).

Join the Scottish Highers students using SimpleStudy...

97% of Students

Report Improved Results

98% of Students

Recommend to friends

100,000+

Students Supported

1 Million+

Questions answered

;