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3C 273 was the first quasar to be discovered - AQA - A-Level Physics - Question 3 - 2022 - Paper 4

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3C 273 was the first quasar to be discovered. IC 1101 is one of the largest galaxies known. Table 2 shows some information about these objects. Table 2 Absolute ma... show full transcript

Worked Solution & Example Answer:3C 273 was the first quasar to be discovered - AQA - A-Level Physics - Question 3 - 2022 - Paper 4

Step 1

State the property of the quasar that led to its discovery.

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Answer

The quasar 3C 273 is characterized as a high power and powerful radio emitter, indicating its significant energy output, which led to its discovery.

Step 2

Show that the absolute magnitude X of quasar 3C 273 is about −27.

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Answer

To determine the absolute magnitude, we use the formula: M=m5imesextlog10(d)+5M = m - 5 imes ext{log}_{10}(d) + 5 Where:

  • M is the absolute magnitude,
  • m is the apparent magnitude (12.8), and
  • d is the distance in parsecs (760 Mpc = 760,000,000 parsecs).

Plugging in the numbers: M=12.85imesextlog10(760000000)+5M = 12.8 - 5 imes ext{log}_{10}(760000000) + 5 Calculating ext{log}_{10}(760000000), we find: M=12.85imes8.880+5M = 12.8 - 5 imes 8.880 + 5 Mextresultinginapproximately27.M ext{ resulting in approximately } -27.

Step 3

Explain which would be the brighter object.

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Answer

Quasar 3C 273 would be the brighter object due to its more negative absolute magnitude compared to IC 1101. In celestial terms, a lower (more negative) absolute magnitude indicates a higher intrinsic brightness.

Step 4

Go on to calculate the ratio brightness of brighter object / brightness of dimmer object.

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Using the absolute magnitudes:

  • For quasar: M = -27
  • For IC 1101: M = -22.8

The difference in absolute magnitudes is: extDifference=22.8(27)=4.2 ext{Difference} = -22.8 - (-27) = 4.2

Using the formula for brightness ratio: rac{B_1}{B_2} = 10^{0.4 imes ext{Difference}}

Calculating: rac{B_1}{B_2} = 10^{0.4 imes 4.2} ext{ which is approximately } 2.51^{3.33}.

Step 5

Calculate the average density within the event horizon of the black hole.

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Answer

The volume of the black hole's event horizon can be calculated using the formula for the volume of a sphere: V=43πr3V = \frac{4}{3} \pi r^3

Where the radius r can be derived from the mass of the black hole: r=2GMc2r = \frac{2GM}{c^2} Substituting in values:

  • G (gravitational constant) is approximately 6.67imes1011extm3/extkgs26.67 imes 10^{-11} ext{ m}^3/ ext{kg s}^2,
  • M = 7.1imes1011M7.1 imes 10^{11} M_⊙ (where MM_⊙ mass of the Sun is 1.989imes10301.989 imes 10^{30} kg).

Calculating: M=7.1imes1011imes(1.989imes1030)extkgM = 7.1 imes 10^{11} imes (1.989 imes 10^{30}) ext{ kg}

Then substituting values to find the volume and density: average density=massV\text{average density} = \frac{\text{mass}}{V}

This will yield the average density in kg/m³.

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