For ordinary stars like our sun, this energy loss would be too small to be detectable, but this energy loss was observed in 1974 in a binary pulsar called PSR1913 +16.
However, in 1974, this energy loss was observed in a binary pulsar called PSR1913 +16. For ordinary stars like our sun, this energy loss would be too small to be detectable.
For ordinary stars like our sun, this energy loss would be too small to be detectable. However, in 1974, this energy loss was observed in a binary pulsar called PSR1913 +16.
For ordinary stars like our sun, this energy loss would be too small to be detectable. However, in 1974, this energy loss was observed in a binary pulsar called PSR1913 +16.