How can I identify the appropriate spectral line for Doppler calculation?

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Discussion Overview

The discussion revolves around identifying the appropriate spectral line for Doppler shift calculations in astrophysics, particularly in the context of measuring the velocity of stars using spectral lines. Participants explore the implications of using different spectral lines and the accuracy of velocity calculations based on observed shifts.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant summarizes a method for calculating the velocity of Alpha Centauri using spectral lines and discusses the implications of using different lines for Doppler calculations.
  • Another participant questions the accuracy of the calculated velocity of 24.25 km/s derived from a shift of 4 pixels and asks for the formula relating Doppler shift to velocity.
  • Concerns are raised about the variability in pixel shift measurements, suggesting that a shift of 4 pixels could represent a range of values, thus affecting the precision of the velocity calculation.
  • Participants discuss the dependence of Doppler shift on wavelength, indicating that shifts are not uniform across different wavelengths.
  • One participant expresses a realization that the assumption of uniform shift across the spectrum may not hold true, acknowledging the complexity of the calculations involved.

Areas of Agreement / Disagreement

Participants express differing views on the accuracy of velocity calculations based on pixel shifts, with some suggesting that the precision may not be as high as initially presented. There is no consensus on the best approach to identify the appropriate spectral line for Doppler calculations, and the discussion remains unresolved.

Contextual Notes

Participants note that the accuracy of velocity calculations is influenced by the specific spectral lines chosen and the inherent variability in pixel shift measurements. The discussion highlights the complexity of Doppler shift calculations and the need for careful consideration of the assumptions involved.

jagadeeshr
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Hi,

I was looking into Doppler shift calculations, and I came across this blog post. It gives a very simple and straight forward account of calculating the velocity of a star.

Following is the summary the blog post:

Spectrum of Alpha Centauri (A. Cen.) is obtained through Lhires III spectroscope. Spectrum of the sky/sun is used as a reference for calculations since A. Cen. and Sun are G2V type stars.

When the A. Cen.'s spectrum is superimposed on the Sun's spectrum, A. Cen's lines have shifted to the left (blue). Shift is 4 pixels.

From the spectrum, two Iron (Fe) lines are identified at 5371.5 Å and 5424.1 Å. They are 52.58 Å apart, and number of pixels between them is 258 pixels. Therefore 1 pixel = 0.2 Å.

Shift between A. Cen. and Sun is is 4 pixels. Therefore, shift in terms of wavelength is 0.8 Å (-0.8 Å, because of blue shift).

Radial Velocity is calculated using the formula: V = C * (Δλ / λ). Where: C ( speed of light) is 3*10^5 km/s, Δλ is 0.8 Å and λ is 5424.1 Å. The equation gives velocity as -44.25 km/s. Taking into account Earth's heliocentricity of 20 km/s, the final velocity of A. Cen. is -44.25 + 20 = -24.25 km/s. This is very close to the astronomical database value of -22.3 km/s.

Here is what I'm confused about: If we use the other Fe line (at 5371.5 Å) as the rest wavelength, the velocity will be -44.68 + 20 = 24.68 km/s (0.4 km/s increase). If we consider spectral lines towards the left (blue region) of the spectrum, the velocity will be higher.

For example, consider an object that emits lines at 4000 Å, 5500 Å and 7000 Å. The shift in wavelength due to Doppler is 1 Å. The Doppler calculations will indicate velocity of 75 km/s at 4000 Å; 54.54 km/s at 5500 Å and 42.85 km/s at 7000 Å.

Therefore, how to identify the appropriate spectral line for Doppler calculation?
 
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Hello there,

Do I understand correctly that you conclude a velocity of 24.25 km/s from a shift of 4 pixels ? What is your estimate for the accuracy of this calculated velocity ?

Re your last paragraph: what is the formula for doppler shift as a function of velocity ?
 
BvU said:
Hello there,

Do I understand correctly that you conclude a velocity of 24.25 km/s from a shift of 4 pixels ? What is your estimate for the accuracy of this calculated velocity ?

Re your last paragraph: what is the formula for doppler shift as a function of velocity ?
BvU said:
Hello there,

Do I understand correctly that you conclude a velocity of 24.25 km/s from a shift of 4 pixels ? What is your estimate for the accuracy of this calculated velocity ?

Re your last paragraph: what is the formula for doppler shift as a function of velocity ?

24.25 km/s from a shift of 4 pixels in that particular spectral image. 1 pixel is 0.2 Å, shift is 4 pixels or 0.8 Å.

3*10^5*(-0.8/5424.1) = -44.25 km/s+ 20 km/s = -24.25 km/s

Formula of Doppler shift as function of velocity: Δλ / λ = V/ C (Calculations)
 
jagadeeshr said:
24.25 km/s from a shift of 4 pixels in that particular spectral image. 1 pixel is 0.2 Å, shift is 4 pixels or 0.8 Å.

3*10^5*(-0.8/5424.1) = -44.25 km/s+ 20 km/s = -24.25 km/s
So what if the actual shift is 4.43 pixels ? Or 3.85 ?
Formula of Doppler shift as function of velocity: Δλ / λ = V/ C (Calculations)
So not all frequencies will shift the same 1 Angstrom
 
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jagadeeshr said:
Formula of Doppler shift as function of velocity: Δλ / λ = V/ C (Calculations)
To make it clearer:
$$
\Delta \lambda = \frac{v \lambda}{c}
$$
i.e., the shift is not the same for all wavelengths, since it depends on ##\lambda##.
 
BvU said:
So what if the actual shift is 4.43 pixels ? Or 3.85 ?
My point is that from the given 4 pixels (which can mean anything between 3.5 and 4.5 pixels, I must assume), you can not calculate a velocity in 4 digits accuracy. You get ##44\pm 5## km/s. And the same absolute error in the final ##24\pm 5## km/s (provided the 20 km/s correction has a considerably smaller error)
 
BvU said:
So what if the actual shift is 4.43 pixels ? Or 3.85 ?

So not all frequencies will shift the same 1 Angstrom

DrClaude said:
To make it clearer:
$$
\Delta \lambda = \frac{v \lambda}{c}
$$
i.e., the shift is not the same for all wavelengths, since it depends on ##\lambda##.

Ah. Based on the image in the blog, I had assumed that the shift will be uniform across the entire spectrum.

Thank you.
 

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