The duration of the oxygen-fusing stage in the core of a massive star is considerably shorter than the duration of the carbon-fusing stage. One main reason for this is that
A) carbon is a solid, while oxygen is a gas.
B) oxygen fusion does not begin until the contracting core has reached a higher temperature than the temperature at which carbon fusion is possible.
C) the electron degeneracy inhibits the carbon reaction, but it has been removed by the time oxygen fusion begins.
D) there are more fusion shells surrounding the oxygen fusion core than there are around the carbon fusion core. The shells prevent the escape of oxygen before it can fuse.
Correct Answer:
Verified
Q87: The center of the remnant of a
Q88: Which force induces the core to contract
Q89: A high-mass star goes through many fusion
Q90: The main product of silicon fusion reactions
Q91: Each successive stage of core nuclear reactions
Q93: In which order do the stages of
Q94: Which nuclear fusion cycle is the next
Q95: A Type Ia supernova is the
A) collapse
Q96: For a massive star (e.g., 25 solar
Q97: Which of these is MOST likely to
Unlock this Answer For Free Now!
View this answer and more for free by performing one of the following actions
Scan the QR code to install the App and get 2 free unlocks
Unlock quizzes for free by uploading documents