Big Bang produced mainly hydrogen and helium and only extremely trace amount of heavier elements. Yet there is abundant amount of carbon on Earth. The carbon atoms in your body were produced by A. Fusion in other stars that have already died B. Radiative decays inside the Earth C. Chemical reactions inside the Earth D. Fusion in the Sun
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Big Bang produced mainly hydrogen and helium and only extremely trace amount of heavier elements. Yet there is abundant amount of carbon on Earth. The carbon atoms in your body were produced by
A. Fusion in other stars that have already died
B. Radiative decays inside the Earth
C.
D. Fusion in the Sun
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- Aproximately what is the ratio of the sun's mass to that of the earth? a)10 b)10000 c)30000 d)300000 e)none of theseWhich of the following statements about the cosmic background radiation is NOT true? A. It has a temperature of about 3 degrees K above absolute zero. B. It is the result of a mixture of radiation from many independent sources, such as stars and galaxies. C. It had a much higher temperature in the past. D. It was discovered by Penzias and Wilson in the early 1960s E. It appears essentially the same in all directions (it is isotropic).Which particle has the largest mass? and How do nuclear decay reactions help explain the difference in the mass of the proton and neutron?
- Isotopes carbon-11 (116C) and carbon-14 (146C) are radioactive. How would each isotope decay? Write the decay equation for each isotope. I know that Carbon-11 decays by positron emission and carbon-14 by beta decay. I need help writing the decay equations for Isotope carbon-11 and carbon-14.K. Consider the following nuclear decay equation; the half-life of Carbon 14 is 5730 years. What is name given to the particle represented by How many neutrons does this isotope of Carbon have?2. Assume that the entire luminosity of the Sun is due to the PP chain reaction. The complete PP chain reaction converts 4 hydrogen nuclei into 1 helium nucleus, according to the following reaction: 4 H - He + 2e* + 2v. a. Estimate the amount of energy released by one complete reaction. b. Estimate how many of these reactions occur per second in the Sun, and how many neutrinos the Sun produces each second. c. Estimate the flux of neutrinos (in v's s' cm?) passing through the Earth.
- Why do the magnetic fields lines of the sun get warped? a. effects of the solar wind b. surface of the sun is cooler near the poles c. uneven fusion rates in the core d. equator rotates more rapidly than the poles21. Which of the following represents the notion that our observable Universe may be a part of a much larger whole? a. Big Bang Nucleosynthesis. b. Solar System. c. Galaxy. d. Multiverse.1. The mass of the Sun is about 2x10³0 kg. The Sun was about 72% hydrogen when it first formed. About 11% of the total amount of the Sun's hydrogen is available for fusion within the Sun's core. [3 points] (a) What is the total mass of hydrogen available for fusion, in kg? (b) The Sun fuses about 600 billion kg of hydrogen each second. Calculate how long the Sun's initial supply of hydrogen can last. Give your answer in both seconds and years. Hint: use the result you calculated in part (a). (c) We know that our Solar System is about 4.5 billion years old. Using your calculation above, how much longer do we have until the Sun runs out of hydrogen?
- 6.) A very old specimen of wood contained 10¹2 atoms of 14 C in 1986. (a) How many 14C atoms did it contain in the year 9474 B.C.2 (b) How many 14C atoms did it contain in 1986 B.C.?1. If a proton is moving at very high speed, so that its kinetic energy is much greater than its rest energy (mc²), can it then decay via p →n + n+? 2. What would an “antiatom," made up of the antiparticles to the constituents of normal atoms, consist of? What might happen if antimatter, made of such antiatoms, came in contact with our normal world of matter?23. The period during the early Universe in which the first atomic nuclei (not full atoms) formed is called: a. Cosmic Microwave Background. b. Inflation. c. Quantum Gravity Era. d. Big Bang Nucleosynthesis.