MarketJune 1991 lunar eclipse
Company Profile

June 1991 lunar eclipse

A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, June 27, 1991, with an umbral magnitude of −0.7571. 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 only about 5 hours before apogee, the Moon's apparent diameter was smaller.

Visibility
The eclipse was completely visible over eastern North America, South America, west and southern Africa, and Antarctica, seen rising over western and northern North America and the eastern Pacific Ocean and setting over Europe, east and north Africa, and the Middle East. == Eclipse details ==
Eclipse details
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse. == Eclipse season ==
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. == Related eclipses ==
Related eclipses
Eclipses in 1991 An annular solar eclipse on January 15. • A penumbral lunar eclipse on January 30. • A penumbral lunar eclipse on June 27.A total solar eclipse on July 11. • A penumbral lunar eclipse on July 26. • A partial lunar eclipse on December 21. Metonic • Followed by: Lunar eclipse of April 15, 1995 Tzolkinex • Preceded by: Lunar eclipse of May 15, 1984 • Followed by: Lunar eclipse of August 8, 1998 Half-Saros • Preceded by: Solar eclipse of June 21, 1982 • Followed by: Solar eclipse of July 1, 2000 Tritos • Preceded by: Lunar eclipse of July 27, 1980 • Followed by: Lunar eclipse of May 26, 2002 Lunar Saros 110 • Preceded by: Lunar eclipse of June 15, 1973 • Followed by: Lunar eclipse of July 7, 2009 Inex • Preceded by: Lunar eclipse of July 17, 1962 • Followed by: Lunar eclipse of June 5, 2020 Triad • Followed by: Lunar eclipse of April 27, 2078 Lunar eclipses of 1991–1994 Metonic series Saros 110 Tritos series Inex series Half-Saros cycle A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two partial solar eclipses of Solar Saros 117. == See also ==
tickerdossier.comtickerdossier.substack.com