just b 1. In this question, you may assume that the core temperature in the Sun...
choose correct answer. no explanation needed QUESTION 10 How do astrophysicists account for neutrino emission from the Sun? Solar flares create neutrinos with very energetic magnetic fields. Convection releases neutrinos, which random walk through the radiation zone. Fission in the Sun's core creates neutrinos when protons turn into neutrons. The annihilation of positrons and electrons in the core produces neutrinos. Fusion in the Sun's core creates neutrinos when protons turn into neutrons, QUESTION 11 How does the interstellar medium impact...
#2 please ! Ro le Astronomy 1F03 Problem Set 3 Thursday, Nov 10th, 2019 Write your answers on a separate sheet and show your work 1. The protesproton chain effectively c erta hyre en into hem according to 4 He. A Helium wus weighs 6.64518 x 10 IT kg and Hydrogen mucha proton) welches 1.67262 x 10 Workout the change in a when I kg of Hydrogen is converted completely into Helium 4. Convert the change in mass Per burning...
Question 1) When does a protostar become a true star? Select one: a. when the star is 1 million years old b. when the central temperature reaches 1 million Kelvin c. when nuclear fusion begins in the core d. when the thermal energy becomes trapped in the center Question 2: On average, what is the greatest mass a newborn star can have? Select one: a. 10 solar masses b. 50 solar masses c. 150 solar masses d. 300 solar masses...
choose correct answer. no explanation needed QUESTION 31 اماں VIII w mu VII 11 OBA FG KM This figure depicts the evolutionary track of a 2 Mo star, with the various evolutionary changes indicated. During which stage does the star have an inert (non-fusing) helium core? iv vil Hi ООО viii vi QUESTION 32 VI V и VE IV 1 OBA FG KM This figure depicts the evolutionary track of a 2 Mo star, with the various evolutionary changes indicated....
Question 2 (1 point) The Weak Interaction is weak because Question 2 options: To interact weakly requires the creation of a heavy gauge boson Not many particles participate in it Particles that interact weakly do so at a great distance The weak interaction involves neutrinos which are rare Question 3 (1 point) All other things being equal, which of the following conditions would result in more nuclear reactions taking place each second inside the Sun than is currently the case...
choose correct answer. no explanation needed QUESTION 36 What does the apparent magnitude of a star tell us about that star? its mass how bright it appears from Earth its radius how much energy it is emitting QUESTION 37 What is the reason sunspots appear darker than surrounding regions on the Sun's surface? They actually are fairly bright, but appear dark against the even brighter background of the surrounding photosphere. They are too cold to emit any visible light. They...
Question: Write at least two paragraphs discussing things that you learned from the background portion of this lab. Be sure to include your interpretation of why nuclear fusion does not occur naturally on the Earth as well as why we do not yet have the technology to replicate the process. lab/Background Information: Nuclear fusion is a very important physical process that governs how the Universe evolves. It occurs naturally in stars, but has not been observed to occur naturally anywhere...
i need help with 3-9 pret uie ale he appluly dlagonal line of data points. For reference, the values for the Sun are M +4.85, B-V +0.63. 2. Theoretical Stellar Models and Evolutionary Tracks The theoretical Zero-Age Main Sequence' (-ZAMS) is defined as the set of computer models representing stars that have just started converting H to He in their cores via thermonuclear fusion. a. Plot the 4 ZAMS data points for each mass from Table 3. Then connect those...