Concept explainers
(a)
The total number of interstellar gas atoms in the Coma Cluster.
Answer to Problem 55Q
The number of interstellar gas atoms in the Coma Cluster is
Explanation of Solution
Given:
The mass of the Coma Cluster is,
Formula used:
The number of atoms in the Coma Cluster is given by,
Calculation:
The mass of Sun is,
The mass of one atom of hydrogen is,
The number of atoms in the Coma Cluster is calculated as,
Conclusion:
The number of interstellar gas atoms in the Coma Cluster is
(b)
The total number of intracluster gas atoms per cubic centimeters in the Coma Cluster.
Answer to Problem 55Q
The number of atoms per centimeter cube is
Explanation of Solution
Given:
The radius of the Coma Cluster is,
Formula used:
The volume of the cluster is given by,
The number of atoms per centimeter cube is given by,
Calculation:
The volume of cluster is calculated as,
The number of atoms per centimeter cube is calculated as,
Conclusion:
The number of atoms per centimeter cube is
(c)
The comparison between the intracluster gas in the Coma Cluster with the gas in the atmosphere, a typical gas cloud in our own galaxy and the corona of the Sun.
Answer to Problem 55Q
The number of molecules in the Earth’s atmosphere per centimeter cube is
Explanation of Solution
Given:
The number of molecules per centimeter cube in Earth’s atmosphere is,
The number of molecules in the typical gas cloud in the Milky way galaxy is,
The number of molecules in the corona of the Sun is,
Calculation:
The ratio of the number of molecules in Coma Cluster and the molecules in the Earth’s atmosphere is calculated as,
The ratio of the number of molecules in Coma Cluster and the molecules in the Milky Way galaxy is calculated as,
The ratio of the number of molecules in Coma Cluster and the molecules in the corona of the Sun is calculated as,
Conclusion:
The number of molecules in the Earth’s atmosphere per centimeter cube is
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Chapter 23 Solutions
Universe: Stars And Galaxies
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- As we have discussed, Sirius B in the Sirius binary system is a white dwarf with MB ∼ 1M , LB ∼ 0.024L ,and rB ∼ 0.0084r . For such a white dwarf, the temperature at the center is estimated to be ∼ 107 K.If Sirius B’s luminosity were due to hydrogen fusion, what is the upper limit of the mass fraction of thehydrogen in such a white dwarf?Step 1: Calculate the observed energy production rate per unit mass (remember luminosity is energy outputper unit time).Step 2: Use the per unit mass energy generation rate of hydrogen fusion (via PP chain) to estimate thepossible hydrogen mass fraction given the condition at the center of the white dwarf.arrow_forwardIf we plot the apparent brightnesses of stars in a globular cluster versus their surface temperatures in a similar way as in the HR diagram , there will be a horizontal branch . Which of the following statements about these horizontal branch stars is wrong ? (A)They have the same absolute magnitude . (B)They have different sizes . (C)Their sole source of energy is hydrogen shell burning . (D)They can help us estimate the distance of the globular cluster from us .arrow_forward5arrow_forward
- Convert the average mass density in gm/cm-3 of a M = 0.5 Msun R = 0.015 Rsun white dwarf to the average number density of electrons, ne , in cm-3. Let Z/A = 0.5. What is the uncertainty in their momentum, Δp, in g-cm/s? (Hint: you'll need to find the average separation, Δx, between the electrons)arrow_forward(Astronomy) PSR1913+16 Problem II. Using only the Figure, what are the maximum radial velocities as found from the redshift and blueshift, respectively? Note: redshifts have positive radial velocities values in the figure, whereas blueshifts have negative radial velocity values. (Answer in km/s)arrow_forwardCan you please help with Part 2 of 2? Thank you.arrow_forward
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