The spectrum of light from a star that is observed by the Hubble Space Telescope is not exactly the same as that star's spectrum observed by a telescope on Earth. Explain why this is so.

Short Answer

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The differences in the observed spectrum of light from a star observed by the Hubble Space Telescope and a telescope on Earth can be attributed to two main factors: the Earth's atmosphere and the Doppler effect. The Earth's atmosphere absorbs and scatters light, altering the observed spectrum for ground-based telescopes. Furthermore, differences in the relative motions between the star, Earth, and the Hubble Space Telescope can result in Doppler shifts, leading to different observed spectra. The Hubble Space Telescope, being outside of Earth's atmosphere and having a different relative motion, observes a spectrum of light that is closer to the star's actual spectrum compared to ground-based telescopes on Earth.

Step by step solution

01

Understanding the role of Earth's atmosphere

The Earth's atmosphere plays a significant role in altering the spectrum of light from a star viewed by a telescope on Earth. The atmosphere can absorb certain wavelengths of light, and this can change the observed spectrum. Additionally, turbulence in the atmosphere can cause the light to scatter, distorting the observed spectrum even further.
02

Explaining the Doppler effect

Another factor contributing to the difference in the observed light spectrum is the Doppler effect. When an object is moving relative to an observer (in this case, the star relative to the observer on Earth or the Hubble Space Telescope), the frequency (and hence the energy) of the light waves appears to change. Depending on the direction of the star's motion, its light can be "redshifted" (moving away from the observer) or "blueshifted" (moving towards the observer). This shift in frequency can change the observed spectrum.
03

Considering the Hubble Space Telescope's position

The Hubble Space Telescope orbits the Earth outside of its atmosphere. As a result, it does not experience the atmospheric effects discussed in Step 1. This means that the spectrum it observes is not interfered with by the atmosphere, giving a more accurate representation of the star's spectrum. Additionally, the Hubble Space Telescope's motion relative to the star might be different than that of an observer on Earth, which can lead to different Doppler effect impacts on the observed spectrum.
04

Conclusion

In summary, the differences in the observed spectrum of light from a star can be attributed to two main factors: the Earth's atmosphere and the Doppler effect. The Earth's atmosphere absorbs and scatters light, altering the observed spectrum for ground-based telescopes. Furthermore, relative motions between the star and the observer can cause Doppler shifts resulting in different observed spectra. The Hubble Space Telescope, being outside the Earth's atmosphere and having a different relative motion, observes a spectrum that is closer to the star's actual spectrum compared to ground-based telescopes on Earth.

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