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Detection of Hydrogen Hydrogen is prev...

Detection of Hydrogen
Hydrogen is prevalent in the universe. Life in the universe is ultimately based on hydrogen.
The are about `1xx 10^(23)` atars in the universe. Assume that they are like our sun (radius `700.000 km`, density, `1.4 g//cm^(-3) 3//4` hydrogen and `1//4` helium by mass). Estimate the number of stellar protons in the universe to one significant figure.
In the `1920s`, Cecilia Payne discovered, by spectral analysis of starlight , that hydrogen is the most abundant element in most stars.

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To estimate the number of stellar protons in the universe, we will follow these steps: ### Step 1: Calculate the Volume of a Typical Star The volume \( V \) of a star can be calculated using the formula for the volume of a sphere: \[ V = \frac{4}{3} \pi r^3 \] Given that the radius \( r \) of the sun is \( 700,000 \) km, we first convert this to centimeters: \[ r = 700,000 \, \text{km} = 700,000 \times 10^5 \, \text{cm} = 7 \times 10^8 \, \text{cm} \] Now, substituting this value into the volume formula: \[ V = \frac{4}{3} \pi (7 \times 10^8)^3 \] ### Step 2: Calculate the Mass of a Typical Star The mass \( M \) of the star can be calculated using the formula: \[ M = \text{Density} \times \text{Volume} \] Given that the density of the star is \( 1.4 \, \text{g/cm}^3 \): \[ M = 1.4 \, \text{g/cm}^3 \times V \] ### Step 3: Estimate the Mass of Protons in a Typical Star The mass of protons in a star can be estimated based on the composition of the star. We know that the star is composed of \( \frac{3}{4} \) hydrogen and \( \frac{1}{4} \) helium by mass. The mass of hydrogen contributes one proton per atom, while helium contributes two protons per atom. Therefore, the total mass of protons can be calculated as: \[ \text{Mass of protons} = M \times \left(\frac{3}{4} + \frac{1}{4} \times \frac{1}{2}\right) \] ### Step 4: Calculate the Total Number of Protons in the Universe To find the total number of protons in the universe, we multiply the number of protons in one star by the total number of stars in the universe: \[ \text{Total protons} = \text{Mass of protons} \times \text{Number of stars} \] Given that there are approximately \( 1 \times 10^{23} \) stars in the universe. ### Step 5: Final Calculation After calculating the mass of a typical star and the mass of protons in that star, we can estimate the total number of protons in the universe. 1. Calculate the volume: \[ V \approx \frac{4}{3} \times 3.14 \times (7 \times 10^8)^3 \approx 1.44 \times 10^{27} \, \text{cm}^3 \] 2. Calculate the mass: \[ M \approx 1.4 \times 1.44 \times 10^{27} \approx 2.016 \times 10^{27} \, \text{g} \] 3. Calculate the mass of protons: \[ \text{Mass of protons} \approx 2.016 \times 10^{27} \times \left(\frac{3}{4} + \frac{1}{8}\right) \approx 1.8 \times 10^{27} \, \text{g} \] 4. Total protons in the universe: \[ \text{Total protons} \approx 1.8 \times 10^{27} \times 1 \times 10^{23} \approx 1.8 \times 10^{50} \] ### Conclusion Thus, the estimated number of stellar protons in the universe is approximately \( 1 \times 10^{80} \).
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