July 1991 lunar eclipse
penumbral
DateJuly 26, 1991
Gamma1.4370
Magnitude−0.8109
Saros ser148
Saros no2 of 71
Penumbral152 minutes, 42 seconds
P 116:51:35
Greatest18:07:52
P 419:24:16
PreviousJune 1991
NextDecember 1991

A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Friday, July 26, 1991,[1] with an umbral magnitude of −0.8109. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 2.25 days after apogee (on July 24, 1991, at 12:10 UTC), the Moon's apparent diameter was smaller.[2]

This eclipse was the third of four lunar eclipses in 1991, with the others occurring on January 30 (penumbral), June 27 (penumbral), and December 21 (partial).

Visibility

The eclipse was completely visible over east Africa, much of Asia, Australia, and Antarctica, seen rising over much of Europe and west and central Africa and setting over northeast Asia and the central Pacific Ocean.[3]

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

July 26, 1991 Lunar Eclipse Parameters
ParameterValue
Penumbral Magnitude0.25425
Umbral Magnitude−0.81093
Gamma1.43698
Sun Right Ascension08h22m14.5s
Sun Declination+19°25'45.6"
Sun Semi-Diameter15'44.9"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension20h20m28.0s
Moon Declination-18°11'58.5"
Moon Semi-Diameter14'47.1"
Moon Equatorial Horizontal Parallax0°54'15.7"
ΔT58.0 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of June–July 1991
June 27
Ascending node (full moon)
July 11
Descending node (new moon)
July 26
Ascending node (full moon)
Penumbral lunar eclipse
Lunar Saros 110
Total solar eclipse
Solar Saros 136
Penumbral lunar eclipse
Lunar Saros 148

Eclipses in 1991

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 148

Inex

Triad

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[5] This lunar eclipse is related to two partial solar eclipses of Solar Saros 155.

July 20, 1982July 31, 2000

See also

Notes

  1. ^ "July 26–27, 1991 Penumbral Lunar Eclipse". timeanddate. Retrieved 8 January 2025.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 8 January 2025.
  3. ^ "Penumbral Lunar Eclipse of 1991 Jul 26". NASA. Retrieved 8 January 2025.
  4. ^ "Penumbral Lunar Eclipse of 1991 Jun 27". EclipseWise.com. Retrieved 8 January 2025.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros