PSR B1913+16 periastron shift graph
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Original by Inductiveload, y-axis label changed by Howtonotwin
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450 x 500 Pixel (111975 Bytes)
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Shift in time of periastron of PSR B1913+16 relative to a hypothetical system with a constant orbital period. The slow decrease in the real system's period is due to the emission of gravitational radiation and causes the parabolic shape of the graph. Red points are experimental data, and the blue line is the shift predicted by relativity. Error bars are shown, but are generally too small to be seen as distinct for most points.
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This work is based on a work in the public domain. It has been digitally enhanced and/or modified. This derivative work has been (or is hereby) released into the public domain by its author, Howtonotwin. This applies worldwide.
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Tento soubor byl odvozen z: PSR B1913+16 period shift graph.svg
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