The ultimate goal of this work is to identify a kind of signature for CH5. Once we have it, we can compare it to what is observed from astronomical measurements to determine its abundance in different regions of space.
The ultimate goal of this work is to identify a kind of signature for CH5. Once we have it, we can compare it to what is observed from astronomical measurements to determine its abundance in different regions of space.
© 2020 Inspirational Stories
© 2020 Inspirational Stories