Table 3 contains information about two galaxies - AQA - A-Level Physics - Question 4 - 2019 - Paper 4
Question 4
Table 3 contains information about two galaxies.
Table 3
| Galaxy | Red shift, z | Distance from Earth / ly |
|-----------|----------------------|---... show full transcript
Worked Solution & Example Answer:Table 3 contains information about two galaxies - AQA - A-Level Physics - Question 4 - 2019 - Paper 4
Step 1
Discuss whether these data are consistent with Hubble's Law.
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Answer
To determine if the data for the two galaxies are consistent with Hubble's Law, we can use the formula:
v=H0imesd
where:
v is the recessional velocity of the galaxies,
H0 is Hubble's constant,
d is the distance of the galaxies from Earth.
For NGC 936:
Given redshift, z=4.8imes10−3 and using the relation v=cz, where c is the speed of light (c≈3×108m/s), we find:
vNGC936=4.8×10−3×3×108≈1.44×106m/s
The distance is d=6.8×107ly≈6.42×1020m (1 ly ≈9.46×1015m).
Now substituting in Hubble's law:
H0=dv≈6.42×10201.44×106≈2.24×10−15s−1
For NGC 3379:
Given redshift, z=3.0×10−3:
vNGC3379=3.0×10−3×3×108≈9.0×105m/s
The distance is d=3.2×107ly≈3.03×1020m.
Substituting in Hubble's law gives:
H0≈3.03×10209.0×105≈2.97×10−15s−1
In conclusion, both galaxies yield different estimates for Hubble's constant, but still reasonably consistent as they both indicate a positive correlation with distance, which supports Hubble's Law.
Step 2
Discuss one problem associated with the determination of the distance from the Earth to a quasar.
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One significant problem associated with determining the distance from the Earth to a quasar is the intrinsic brightness variability of quasars. Since quasars are incredibly distant and faint objects, distinguishing their actual luminosity and hence their distance can be complicated. They can vary in brightness due to several factors, such as changes in their accretion disks or interactions with nearby matter.
This variability can lead to errors when applying distance measurement techniques, such as the inverse square law of light, which assumes the object maintains a constant luminosity. Therefore, accurately gauging distances to quasars necessitates careful observation over time and can introduce uncertainties in cosmological models.