May 2049 lunar eclipse explained

Type:penumbral
Date:17 May 2049
Gamma:-1.1337
Magnitude:0.7638[1]
Saros Ser:112
Saros No:67 of 72[2]
Cat Year:2001
Cat No:LE2049May17N
Penumbral:224 minutes 16 seconds
P1:09:33:02
Greatest:11:25:06
P4:13:17:18
Previous:December 2048
Next:June 2049

A penumbral lunar eclipse will take place on May 17, 2049.

Related lunar eclipses

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[3] This lunar eclipse is related to two partial solar eclipses of Solar Saros 119.

Tritos series

Tzolkinex

See also

Notes and References

  1. For a partial or total lunar eclipse, this value denotes the umbral magnitude. For a penumbral lunar eclipse, this denotes the penumbral magnitude.
  2. https://eclipse.gsfc.nasa.gov/LEsaros/LEsaros112.html Lunar Saros 112 - Fred Espenak's GSFC Eclipse Canon
  3. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros