•P60 Buckminsterfullerene, C60, is a large molecule consisting of 60 carbon atoms connected to form a hollow sphere. The diameter of a C60 molecule is about 7 x 10¬10m. It has been hypothesized that C60 molecules might be found in clouds of interstellar dust, which often contain interesting chemica compounds. The temperature of an interstellar dust cloud may- be very low, around 3 K. Suppose you are planning to try to detect the presence of C60 in such a cold dust cloud by detecting photons emitted when molecules undergo transitions from one rotational energy state to another. Approximately, what is the highest-numbered rotational level from which you would expect to observe emissions? Rotational levels are l=0,1,2,3,..

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.•P60 Buckminsterfullerene, C60, is a large molecule
consisting of 60 carbon atoms connected to form a hollow sphere.
The diameter of a C60 molecule is about 7 x 10–10 m. It has
been hypothesized that C60 molecules might be found in clouds
of interstellar dust, which often contain interesting chemical
compounds. The temperature of an interstellar dust cloud may
be very low, around 3 K. Suppose you are planning to try to
detect the presence of C60 in such a cold dust cloud by detecting
photons emitted when molecules undergo transitions from one
rotational energy state to another.
Approximately, what is the highest-numbered rotational level
from which you would expect to observe emissions? Rotational
levels are l= 0,1,2,3,..
Transcribed Image Text:.•P60 Buckminsterfullerene, C60, is a large molecule consisting of 60 carbon atoms connected to form a hollow sphere. The diameter of a C60 molecule is about 7 x 10–10 m. It has been hypothesized that C60 molecules might be found in clouds of interstellar dust, which often contain interesting chemical compounds. The temperature of an interstellar dust cloud may be very low, around 3 K. Suppose you are planning to try to detect the presence of C60 in such a cold dust cloud by detecting photons emitted when molecules undergo transitions from one rotational energy state to another. Approximately, what is the highest-numbered rotational level from which you would expect to observe emissions? Rotational levels are l= 0,1,2,3,..
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