Which of the following is most likely to occur when mass is continually added to a 1.5 solar mass neutron star? Group of answer choices The star's radius will increase. The star will rejoin the main sequence. The star will turn into white dwarf. The star will eventually become a black hole. The star will erupt as a supernova.
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Q: Effective Temperature (K) 25,000 10,000 -10 6,000 3,000 10 102 A +10- D 10-2 +15 B A 104 M F…
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A: After a supernova explosion, the remaining core will collapse to form a neutron star if the mass of…
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A: Correct answer is Emission nebula
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A: Given , Temperature = 3000 K Solar Luminosity = 100,000 Now , mass and luminosity are related by…
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A: Required : Steps involved in star cycle.
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A: Required : Spectral type, absolute magnitude, temperature and luminosity of star E.
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A: We need to find what happens to a neutron star that accretes too much matter.
Q: sequence
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A: A white dwarf is a stellar core remnant that is highly dense and made of electron-degenerate matter.…
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Q: You discover a binary star system in which one member is a 15 solar-mass main-sequence star and the…
A: Required : The correct option.
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A: Answer: A high or low a star is on the main sequence is dictated primarily is discussed below:
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A: Zebulon is a binary star system composed of a 10 M sun main sequence star and a 1 M sun red giant.
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A: Question 32: Among O star, F star, and K star each with a magnitude of 2 . which one is most…
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Q: Indicate whether the following statements are true or false (Select T-True, F-False. If the first is…
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- A main sequence star of mass 25 M⊙has a luminosity of approximately 80,000 L⊙. a. At what rate DOES MASS VANISH as H is fused to He in the star’s core? Note: When we say “mass vanish '' what we really mean is “gets converted into energy and leaves the star as light”. Note: approximate answer: 3.55 E14 kg/s b. At what rate is H converted into He? To do this you need to take into account that for every kg of hydrogen burned, only 0.7% gets converted into energy while the rest turns into helium. Approximate answer = 5E16 kg/s c. Assuming that only the 10% of the star’s mass in the central regions will get hot enough for fusion, calculate the main sequence lifetime of the star. Put your answer in years, and compare it to the lifetime of the Sun. It should be much, much shorter. Approximate answer: 30 million years.Betelgeuse is a nearby supergiant that will eventually explode into a supernova. Let's see how awesome it would look. At peak brightness, the supernova will have a luminosity of about 10 billion times the Sun. It is 600 light-years away. All stellar brightnesses are compared with Vega, which has an intrinsic luminosity of about 60 times the Sun, a distance of 25 light-years, an absolute magnitude of 0.6 and an apparent magnitude of 0 (by definition). a) At peak brightness, how many times brighter will Betelgeuse be than Vega? b) Approximately what apparent magnitude does this correspond to? c) The Sun is about -26.5 apparent magnitude. What fraction of the Sun's brightness will Betelgeuse be?List the following 5 terms in order through a stars life cycle (starting with the sun), through the remainder of its lifetime: a. Black dwarf b. Planetary nebula c. Red giant d. Star (Sun) e. White dwarf
- What happens to a white dwarf when a normal star dumps mass to a white dwarf? Group of answer choices The white dwarf get smaller, causing its temperature and density to decrease. The white dwarf get smaller, causing its temperature and density to increase. The white dwarf get larger, causing its temperature and density to decrease. The white dwarf get larger, causing its temperature and density to increase.Do this in 10 min. I will give like on answer8) A neutron star is found with a radius of 10 km and has a surface temperature of 1,000,000 K. Calculate its luminosity with respect to that of the Sun. nts)