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Image: Solar eclipses 1995-2035

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Description: In this graph we see various series of eclipses. The steeply sloping series are eclipses one semester (six synoptic months) apart, with inex number decreasing by 8 each time. The series that rise gently toward the right are eclipses separated by octons (47 synoptic months), with inex number decreasing by 3 each time. The series going gently downwards to the right are eclipses separated by heptons (41 synoptic months), with inex number increasing by 5 each time.
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