File:PSR B1913+16 periastron shift graph.svg
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Summary
| Description | 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. | ||
| Date | Original 22 February 2010, modified version 16 March 2024 | ||
| Source |
This file was derived from: PSR B1913+16 period shift graph.svg |
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| Author | Original by Inductiveload, y-axis label changed by Howtonotwin | ||
| Permission (Reusing this file) |
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File history
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 22:34, 16 March 2024 | | 450 × 500 (109 KB) | Howtonotwin | {{Information |Description=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. |Source={{Derived from|PSR B1913+16 per... |
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