Concept explainers
(a)
The age of the universe.
Answer to Problem 21Q
The age of the universe is
Explanation of Solution
Given:
The value of the Hubble’s constant
The value of the Hubble’s costant
The value of the Hubble’s costant
Formula used:
The life of the universe is given by,
Calculation:
The life of the universe is calculated by,
Solve further,
Solve further,
Conclusion:
The age of the universe is
(b)
The age of the universe.
Answer to Problem 21Q
The age of the universe is
Explanation of Solution
Formula used:
The life of the universe is given by,
Calculation:
The life of the universe is calculated by,
Solve further,
Solve further,
Solve further,
Conclusion:
The age of the universe is
(c)
The age of the universe and how the age of globular cluster is used to place the limit on the maximum value of Hubble’s constant.
Answer to Problem 21Q
The age of the universe is
Explanation of Solution
Formula used:
The life of the universe is given by,
Calculation:
The life of the universe is calculated by,
Solve further,
Solve further,
Solve further,
Conclusion:
The age of the universe is
The age of the universe is decreasing as the value of the Hubble’s constant is increasing. Since. the age of the globular cluster cannot be less than the universe, as it is not possible that consist of the universe is older than the universe. So the age of the universe is more than the globular cluster and it apply the maximum limit on the value of the Hubble’s constant.
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Chapter 25 Solutions
Universe: Stars And Galaxies
- If the diameter of the Milky Way Galaxys visible disk, 80,000 ly, is represented in a model by a dinner plate with a diameter of 10 inches, what is the model distance to galaxy M31, 2.6 millionly away? What is the model distance to the Virgo galaxy cluster, 16 Mpc away? (Convert answers to feet.)arrow_forwardSuppose that stars evolved without losing mass-that once matter was incorporated into a star, it remained there forever. How would the appearance of the Galaxy be different from what it is now? Would there be population I and population II stars? What other differences would there be?arrow_forwardWe have said that the Galaxy rotates differentially; that is, stars in the inner parts complete a full 360° orbit around the center of the Galaxy more rapidly than stars farther out. Use Kepler’s third law and the mass we derived in Exercise 25.19 to calculate the period of a star that is only 5000 light-years from the center. Now do the same calculation for a globular cluster at a distance of 50,000 light-years. Suppose the Sun, this star, and the globular cluster all fall on a straight line through the center of the Galaxy. Where will they be relative to each other after the Sun completes one full journey around the center of the Galaxy? (Assume that all the mass in the Galaxy is concentrated at its center.)arrow_forward
- Suppose we could measure the distance to a galaxy using one of the distance techniques listed in Table 26.2 and it turns out to be 200 million light-years. The galaxy’s redshift tells us its recessional velocity is 5000 km/s. What is the Hubble constant?arrow_forwardAssume that the average galaxy contains 1011MSunand that the average distance between galaxies is 10 million light-years. Calculate the average density of matter (mass per unit volume) in galaxies. What fraction is this of the critical density we calculated in the chapter?arrow_forwardWhat evidence can you give that we live in a galaxy?arrow_forward
- Assume that the average galaxy contains 1011 MSun and that the average distance between galaxies is 10 million light-years. Calculate the average density of matter (mass per unit volume) in galaxies. What fraction is this of the critical density, 9.6 * 10-27?arrow_forwardRecall that Hubbleʹs law is written v = H0d, where v is the recession velocity of a galaxy located a distance d away from us, and H0 is Hubbleʹs constant. Suppose H0 = 80 km/s/Mpc. How fast would a galaxy located 800 megaparsecs distant be receding from us? A. 64 Mpc/s B. 64,000 km/s C. 0.1 times the speed of light D. 10 km/s E. 64 km/sarrow_forwardExplain how the Hubble constant, H0, can be used to make an estimate for the age of the Universe. Use the value of H0 = 0.07×103 kms-1/Mpc to estimate the Universe’s age. Comment on the significance of your answer.arrow_forward
- Using 22 km/s/million light-years for Hubble’s constant, what recessional velocity do we expect to find if we observe a galaxy at 600 million light-years?arrow_forwardImagine that an observed distant galaxy is measured to have a distance of 40 Mpc by a Type Ia supernovae and the redshift of the galaxy indicates the galaxy appears to be moving away from us at a speed of 2400 km/s. What would the Hubble constant be if measured solely based on this galaxy in units of km/s/Mpc?arrow_forwardIf a galaxy is 18 Mpc from Earth and the Hubble constant is 70 km/s/Mpc, what is the recession velocity of the galaxy (in km/s)? A galaxy is receding from Earth at a speed of 300 km/s and the Hubble constant is 70 km/s/Mpc. What is the distance to the galaxy (in Mpc)?arrow_forward
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