March_1997_lunar_eclipse

March 1997 lunar eclipse

March 1997 lunar eclipse

Partial lunar eclipse March 30, 1997


A partial lunar eclipse took place on Monday, March 24, 1997, the first of two lunar eclipses in 1997.

More information Partial Lunar Eclipse, Duration (hr:mn:sc) ...

This partial lunar eclipse was nearly total; however, it occurred 3 days after the lunar apogee, so the umbral shadow is smaller.

This was the 29th member of Lunar Saros 132, and the last of the first set of partial eclipses. The next event was the April 2015 lunar eclipse, which was the first of 12 total eclipses.

This eclipse was the third of an almost tetrad (that occurred when there were 4 consecutive lunar eclipses that had an umbral eclipse magnitude of 0.9 or greater). The others were 04 Apr 1996 (T), 27 Sep 1996 (T) and 16 Sep 1997 (T).

Visibility

This eclipse was completely visible from North and South America, and visible setting over Western Europe and Africa.

This simulated view of the Earth from the Moon at greatest eclipse shows the visibility.

Eclipses of 1997

Lunar year series

This was the third of four lunar year eclipses at the ascending node of the Moon's orbit.

The lunar year series repeats after 12 lunations or 354 days (Shifting back about 10 days in sequential years). Because of the date shift, the Earth's shadow will be about 11 degrees west in sequential events.

More information Lunar eclipse series sets from 1995–1998, Ascending node ...

Saros series

Lunar saros series 132, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 44 umbral lunar eclipses (32 partial lunar eclipses and 12 total lunar eclipses).

More information Greatest, First ...

There are 11 series events between 1901 and 2100, grouped into threes (called an exeligmos), each column with approximately the same viewing longitude on earth.

1901–2100
1907 Jan 29 1925 Feb 8 1943 Feb 20
1961 Mar 2 1979 Mar 13 1997 Mar 24
2015 Apr 4 2033 Apr 14 2051 Apr 26
2069 May 6 2087 May 17

Inex series

The inex series repeats eclipses 20 days short of 29 years, repeating on average every 10571.95 days. This period is equal to 358 lunations (synodic months) and 388.5 draconic months. Saros series increment by one on successive Inex events and repeat at alternate ascending and descending lunar nodes.

This period is 383.6734 anomalistic months (the period of the Moon's elliptical orbital precession). Despite the average 0.05 time-of-day shift between subsequent events, the variation of the Moon in its elliptical orbit at each event causes the actual eclipse time to vary significantly. It is a part of Lunar Inex series 35.

More information Descending node, Ascending node ...

Tritos series

Tzolkinex

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[2] This lunar eclipse is related to two total solar eclipses of Solar Saros 139.

March 18, 1988 March 29, 2006

See also


Notes

  1. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros



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