Question

Suppose that star formation stops today, everywhere in the universe. a. At what time t_die will...

Suppose that star formation stops today, everywhere in the universe.

a. At what time t_die will the last stars die out?

b. What will be the scale factor a(t_die) at that time?

Homework Answers

Answer #1

Well their is no actual end to a star's life so stars will never die. Most of them will end up being black dwarf stars, a white dwarf star that has cooled down and no longer commits heat or light. The majority of the stars will become black dwarfs, some will become black holes though. So assuming a black dwarf is the end of a star life, we can now determine how long it will take for every star to get to the end.

So lets take the beginning stage of a star's life, a nebula. Now we want to find the youngest nebula because that will be the last star to brcome a black dwarf.

So for a nebula to become a black dwarf would take around 20-30 billion years. Seems like a big number? Well the white dwarf cooling down into a black dwarf takes over 10 billion years!

Know the answer?
Your Answer:

Post as a guest

Your Name:

What's your source?

Earn Coins

Coins can be redeemed for fabulous gifts.

Not the answer you're looking for?
Ask your own homework help question
Similar Questions
The first major star formation in the universe occurred in “proto-galaxies” soon after the Big Bang,...
The first major star formation in the universe occurred in “proto-galaxies” soon after the Big Bang, ∼13 billion years ago. Could any of those stars still be surviving on the Main Sequence today, i.e., still burning H into He in their cores? If yes, approximately what range of Main Sequence spectral types and stellar masses should still be surviving? Express the stellar masses relative to the Sun’s mass. Hint: In class we noted that stellar lifetimes scale with mass due...
Stellar nurseries are massive regions of star formation much like the region in which our own...
Stellar nurseries are massive regions of star formation much like the region in which our own star formed. Once these baby stars form they eventually get gravitationally ejected from the region and move into interstellar space. Stars are formed in bundles in this regard and our Sun likely has numerous brothers and sisters that formed from the same cloud as ours. They are out there independently revolving around the center of the Milky Way as we are. Our Sun's sister...
1. what is singularity a. place where you could leave universe b. center of black hole...
1. what is singularity a. place where you could leave universe b. center of black hole , infinite density c. we dont know 2. summarize the varios ways stars (law mass and high mass ) could die and describe them .
Expansion of the universe Q: What is the Cosmological Principle? Why is it not an exact...
Expansion of the universe Q: What is the Cosmological Principle? Why is it not an exact statement? In what sense could it be true (on large scales a good approximation)? Q: What is Hubble’s Law? What does it say in simple terms? What is the pattern of galaxy motions relative to us? What are possible interpretations of this motion? Q: What is the cosmic scale factor? What does it measure? What is its value today? in the past? the future?
Consider a star 1 of mass m1 = 2 * 10^30kg located at r1= <-2*10^11,-1*10^11,0>m and...
Consider a star 1 of mass m1 = 2 * 10^30kg located at r1= <-2*10^11,-1*10^11,0>m and another star 2 of mass m2 = 3 *10^30kg located at r2 =<2*10^11,3*10^11,0>m that are isolated from all the other objects in the universe. a) What is the vector that points from star 1 to star 2? b) What is the unit vector that points from star 1 to star 2? c) What is the gravitational Fg on 1 by 2? (Draw picture) d)Suppose...
Stars and galaxies in the distance universe are receding from us with a speed proportional to...
Stars and galaxies in the distance universe are receding from us with a speed proportional to their distance away, v = Hr, where H ≈ 73 m/s/Mpc is the Hubble constant. (a) What is the value of H in SI units? SR units? (Mpc = Mega parsec.) (b) Because they are receding from us, light received from distant stars will be red-shifted. It is common to define the dimensionless red-shift parameter z as λ/λ0 ≡ 1 + z. There is...
(8 pts) Answer each of the following questions: (a) When did the Big Bang occur and...
(8 pts) Answer each of the following questions: (a) When did the Big Bang occur and what was the result? (b) Is "string theory" a proven scientific theory? Why or why not? (c) Where does the Strong Nuclear Force come into play? (d) What is Cosmology? (5 pts) If our Sun and solar system had formed at the same time as the very first stars in the universe, describe how and why our solar system would be different than the...
Suppose today is Dec 31st, 2020, and as always, today is time t=0. Prithu wants to...
Suppose today is Dec 31st, 2020, and as always, today is time t=0. Prithu wants to buy a $20 million yacht. The dealer is offering the following scheme. Pay $2 million as down payment today and borrow $18 million from the dealership at 18% per year and payoff the loan in 4 yearly installments, the first installment is due one year from now, meaning December 31, 2021. If he agrees to the scheme, he will receive the delivery of the...
Suppose the difference between matter and antimatter in the early universe were 1 part in 108...
Suppose the difference between matter and antimatter in the early universe were 1 part in 108 instead of 1 part in 109. (a.) Evaluate the temperature at which deuterium begins to form. (b.) At what age does this occur? (c.) Evaluate the temperature and the corresponding time of radiation decoupling (when hydrogen atoms form).
The distance to the North Star, Polaris, is approximately 6.44 1018 m. (a) If Polaris were...
The distance to the North Star, Polaris, is approximately 6.44 1018 m. (a) If Polaris were to burn out today, how many years from now would we see it disappear? y (b) What time interval is required for sunlight to reach the Earth? (The average Earth–Sun distance is 1.50 1011 m.) min (c) What time interval is required for a microwave signal to travel from the Earth to the Moon and back? (The average Earth–Moon distance is 3.84 108 m.)...