Top Qs
Timeline
Chat
Perspective

August 2009 lunar eclipse

Penumbral lunar eclipse 6 August 2009 From Wikipedia, the free encyclopedia

August 2009 lunar eclipse
Remove ads

A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, August 6, 2009,[1] with an umbral magnitude of −0.6642. 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 2.1 days after apogee (on August 3, 2009, at 22:40 UTC), the Moon's apparent diameter was smaller.[2]

Quick Facts Date, Gamma ...

This eclipse was the third of four lunar eclipses in 2009, with the others occurring on February 9 (penumbral), July 7 (penumbral), and December 31 (partial).

Remove ads

Visibility

The eclipse was completely visible over South America, Africa, and Europe, seen rising over much of North America and setting over central and south Asia.[3]

Thumb Thumb
Hourly motion shown right to left
Thumb
The Moon's hourly motion across the Earth's shadow in the constellation of Capricornus.
Thumb
Visibility map

Eclipse details

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

More information Parameter, Value ...

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.[5][6][7]

More information July 7Ascending node (full moon), July 22Descending node (new moon) ...
Remove ads
Summarize
Perspective

Eclipses in 2009

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 148

Inex

Triad

  • Preceded by: Lunar eclipse of October 6, 1922
  • Followed by: Lunar eclipse of June 6, 2096

Lunar eclipses of 2006–2009

This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[8]

The lunar eclipses on July 7, 2009 (penumbral) and December 31, 2009 (partial) occur in the next lunar year eclipse set.

More information Lunar eclipse series sets from 2006 to 2009, Descending node ...

Saros 148

This eclipse is a part of Saros series 148, repeating every 18 years, 11 days, and containing 70 events. The series started with a penumbral lunar eclipse on July 15, 1973. It contains partial eclipses from October 10, 2117 through May 5, 2460; total eclipses from May 17, 2478 through September 14, 2676; and a second set of partial eclipses from September 25, 2694 through May 25, 3091. The series ends at member 70 as a penumbral eclipse on August 9, 3217.

The longest duration of totality will be produced by member 37 at 104 minutes, 29 seconds on July 10, 2568. All eclipses in this series occur at the Moon’s ascending node of orbit.[9]

More information Greatest, First ...

Eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

More information Series members 1–13 occur between 1973 and 2200: ...

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

More information Series members between 1801 and 2096 ...

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

More information Series members between 1801 and 2154 ...

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[11] This lunar eclipse is related to two partial solar eclipses of Solar Saros 155.

More information July 31, 2000 ...
Remove ads

See also

Notes

Loading related searches...

Wikiwand - on

Seamless Wikipedia browsing. On steroids.

Remove ads