September_1996_lunar_eclipse

September 1996 lunar eclipse

September 1996 lunar eclipse

Total lunar eclipse September 27, 1996


A total lunar eclipse took place on Friday, September 27, 1996, the second of two lunar eclipses in 1996, the first being on Thursday, April 4. This is the 41st member of Lunar Saros 127. The previous event is the September 1978 lunar eclipse. The next event is the October 2014 lunar eclipse.

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

This eclipse was the second 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), 24 Mar 1997 (P) and 16 Sep 1997 (T).

Visibility

It was visible from all of North and South America, Europe and Africa.

Mid-infrared image of the Moon

The mid-infrared image of the Moon was taken during a September 1996 lunar eclipse by the SPIRIT-III instrument aboard the orbiting Midcourse Space Experiment (MSX) satellite.

During its totality, the Midcourse Space Experiment (MSX) satellite's SPIRIT-III instrument took the image of the Moon in mid-infrared. At these wavelengths, MSX was able to characterize the thermal (heat) distribution of the lunar surface during the eclipse. The brightest regions are the warmest, and the darkest areas are the coolest. The well-known crater Tycho is the bright object to the south of center. Numerous other craters are also seen as bright spots, indicating that their temperature is higher than in the surrounding dark mare.[1]

Eclipses of 1996

Lunar year series

This is the second of four lunar year eclipses at the descending node of the Moon's orbit.

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

Saros series

Lunar saros series 127, repeating every 18 years and 11 days, has a total of 72 lunar eclipse events including 54 umbral lunar eclipses (38 partial lunar eclipses and 16 total lunar eclipses). Solar Saros 134 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

More information Greatest, First ...
1901–2100
1906 Aug 04 1924 Aug 14 1942 Aug 26
1960 Sep 05 1978 Sep 16 1996 Sep 27
2014 Oct 08 2032 Oct 18 2050 Oct 30
2068 Nov 09

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 annular solar eclipses of Solar Saros 134.

More information October 3, 2005 ...

See also


References

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

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