![]() Live-webcast of the lunar eclipse on 15 June 2011, University of Applied Sciences Offenburg/Germany.Wikimedia Commons has media related to Lunar eclipse of 2011 June 15. Bao-Lin Liu, Canon of Lunar Eclipses 1500 B.C.-A.D.^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros.^ "Longest lunar eclipse for a decade turns moon blood red", Terry Brown.List of lunar eclipses and List of 21st-century lunar eclipses.This lunar eclipse is related to two annular solar eclipses of Solar Saros 137. It is a part of Lunar Inex series 39.Īll events in this series listed below and more are total lunar eclipses.Ī lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). Despite the average 0.05 time-of-day shift between subsequent events, the variation of the Moon in its elliptical orbit at each event causes the actual eclipse time to vary significantly. This period is 383.6734 anomalistic months (the period of the Moon's elliptical orbital precession). Saros series increment by one on successive Inex events and repeat at alternate ascending and descending lunar nodes. This period is equal to 358 lunations ( synodic months) and 388.5 draconic months. The inex series repeats eclipses 20 days short of 29 years, repeating on average every 10571.95 days. This series produces 23 total eclipses between Jand August 9, 2120. Sequential events have incremental Saros cycle indices. The tritos series repeats 31 days short of 11 years at alternating nodes. The greatest eclipse of the series will occur on 2029 Jun 26, lasting 102 minutes. Solar Saros 137 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series. Lunar saros series 130, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 56 umbral lunar eclipses (42 partial lunar eclipses and 14 total lunar eclipses). Each eclipse in the series repeats after one semester (6 lunations or 177 days) occurring at alternating nodes. This eclipse is the center of nine lunar eclipses in a short-lived series. It was preceded by the partial solar eclipse of January 4, 2011, and the partial solar eclipse of 1 June 2011. A partial solar eclipse on 25 November. ![]() ![]() The next central total lunar eclipse was on Jover South America, western Africa, and Europe, and setting over eastern Asia. The last time a lunar eclipse was closer to the center of the earth's shadow was on July 16, 2000. This was a relatively rare central lunar eclipse, in which the center point of Earth's shadow passes across the moon. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. The second occurred on December 10, 2011. It was the first of two such eclipses in 2011. The moon's hourly motion across the Earth's shadow in the constellation of Ophiuchus (north of Scorpius)Ī total lunar eclipse took place on 15 June 2011. The moon passes right to left through the Earth's shadow ( April 2021) ( Learn how and when to remove this template message) Please help to improve this article by introducing more precise citations. This article includes a list of general references, but it lacks sufficient corresponding inline citations.
0 Comments
Leave a Reply. |
AuthorWrite something about yourself. No need to be fancy, just an overview. ArchivesCategories |