Penumbral Lunar Eclipse 24 June 2002 | |
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The moon grazed the southern penumbral shadow of the Earth. | |
Series (and member) | 149 (2 of 72) |
Gamma | -1.4439 |
Duration (hr:mn:sc) | |
Penumbral | 2:09:05 |
Contacts (UTC) | |
P1 | 20:22:28 |
Greatest | 21:27:09 |
P4 | 22:31:33 |
The moon's hourly motion across the Earth's shadow in the constellation of Scorpius. |
A penumbral lunar eclipse took place on Monday 24 June 2002, the second of three lunar eclipses in 2002. This penumbral eclipse was visibly imperceptible due to the small entry into the southern penumbral shadow.
This lunar eclipse was during the 2002 FIFA World Cup, occurring only 6 days before the 2002 FIFA World Cup Final, which was won by Brazil.
This is the third eclipse this season.
First eclipse this season: 26 May 2002 Penumbral Lunar Eclipse
Second eclipse this season: 10 June 2002 Annular Solar Eclipse
Lunar eclipse series sets from 1998–2002 | ||||||||
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Descending node | Ascending node | |||||||
Saros | Date Viewing | Type Chart | Gamma | Saros | Date Viewing | Type Chart | Gamma | |
109 | 1998 Aug 08 | penumbral | 1.4876 | 114 | 1999 Jan 31 | penumbral | −1.0190 | |
119 | 1999 Jul 28 | partial | 0.7863 | 124 | 2000 Jan 21 | total | −0.2957 | |
129 | 2000 Jul 16 | total | 0.0302 | 134 | 2001 Jan 09 | total | 0.3720 | |
139 | 2001 Jul 05 | partial | −0.7287 | 144 | 2001 Dec 30 | penumbral | 1.0732 | |
149 | 2002 Jun 24 | penumbral | −1.4440 | |||||
Last set | 1998 Sep 06 | Last set | 1998 Mar 13 | |||||
Next set | 2002 May 26 | Next set | 2002 Nov 20 |
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). [1] This lunar eclipse is related to one partial solar eclipse of Solar Saros 156.
1 July 2011 |
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A penumbral lunar eclipse took place on Sunday 24 April 2005, the first of two lunar eclipses in 2005. At maximum eclipse, 86.5% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 6 minutes overall, and was visible from east Asia, Australia, and the Americas.
A penumbral lunar eclipse took place on 9 February 2009, the first of four lunar eclipses in 2009, and being the deepest of three penumbral eclipses. It also happened on the Lantern Festival, the first since 20 February 1989. The tables below contain detailed predictions and additional information on the Penumbral Lunar Eclipse of 9 February 2009.
A penumbral lunar eclipse took place on 7 July 2009, the second of four lunar eclipses in 2009. This eclipse entered only the southernmost tip of the penumbral shadow and thus was predicted to be very difficult to observe visually. This lunar eclipse was the predecessor of the solar eclipse of 22 July 2009.
A penumbral lunar eclipse took place on 6 August 2009, the third of four lunar eclipses in 2009. The Moon's small entry into the Earth's penumbral shadow produced an extremely subtle dimming of the Moon's southern edge, difficult to observe visually.
A penumbral lunar eclipse took place on Wednesday 20 November 2002, the last of three lunar eclipses in 2002.
A penumbral lunar eclipse took place on Sunday 26 May 2002, the first of three lunar eclipses in 2002.
A penumbral lunar eclipse occurred on 28 November 2012, the second of two lunar eclipses in 2012.
A penumbral lunar eclipse took place on Sunday, January 31, 1999, the first of two lunar eclipses in 1999.
A penumbral lunar eclipse took place at the Moon's ascending node on 11 February 2017, the first of two lunar eclipses in 2017. It was not quite a total penumbral lunar eclipse. It occurred the same day as comet 45P/Honda–Mrkos–Pajdušáková made a close approach to Earth. It also occurred on the Lantern Festival, the first since 9 February 2009. Occurring only 4.4 days after perigee, the moon's apparent diameter was larger.
A penumbral lunar eclipse took place on Thursday, June 27, 1991, the second of four lunar eclipses in 1991. The moon entered the Earth's penumbra for about 3 hours, and was difficult to see. This lunar eclipse is the predecessor of the Solar eclipse of July 11, 1991.
A penumbral lunar eclipse took place on Friday, July 26, 1991, the third of four lunar eclipses in 1991. This was the 2nd member of Lunar Saros 148. The previous event was on 15 July 1973, and the 1st eclipse of the series. The next event was on 6 August 2009.
A penumbral lunar eclipse took place on Tuesday, May 15, 1984, the first of three lunar eclipses in 1984. This was a deep penumbral eclipse, with the southern limb of the Moon close to the Earth's shadow.
A penumbral lunar eclipse took place on Tuesday, January 20, 1981, the first of two lunar eclipses in 1981. In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth, and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours and 24 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see. The moon's apparent diameter was larger because the eclipse occurred 5.2 days after perigee.
A penumbral lunar eclipse took place on 30 November 2020. A penumbral lunar eclipse occurs at full moon when the Moon passes through Earth's penumbral shadow.
A penumbral lunar eclipse took place at the Moon's descending node of the orbit on Tuesday, August 26, 1980, the last of three penumbral lunar eclipses in 1980 with a penumbral magnitude of 0.70891. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 70.891% of the Moon's disc was partially shaded by the Earth, which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours, 34 minutes and 26 seconds.
A partial lunar eclipse took place on Thursday, May 13, 1976, the first of two lunar eclipses in 1976, the second being a penumbral lunar eclipse on November 6, 1976. At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour, 15 minutes and 23.8 seconds, with just 12.17% of the Moon in shadow at maximum. Occurring only 1.1 days after perigee, the Moon's apparent diameter 5.4% larger than average.
A partial lunar eclipse took place on Monday, December 10, 1973, the last of four lunar eclipses in 1973, the first was a penumbral lunar eclipse on January 18, the second was a penumbral lunar eclipse on June 15, and the third was a penumbral lunar eclipse on July 15. It occurred near perigee, and as described, such event was known as a supermoon.
A penumbral lunar eclipse took place on Friday, June 15, 1973, the second of four lunar eclipses in 1973, the first was a penumbral lunar eclipse on Thursday, January 18, the third being with a penumbral lunar eclipse on Sunday, July 15, and the last being with a partial lunar eclipse on Monday, December 10.
A penumbral lunar eclipse took place on Thursday, January 18, 1973, the first of four lunar eclipses in 1973, the second being with a penumbral lunar eclipse on Friday, June 15, the third being with a penumbral lunar eclipse on Sunday, July 15, and the last being with a partial lunar eclipse on Monday, December 10.
A penumbral lunar eclipse took place on Sunday, July 15, 1973, the third of four lunar eclipses in 1973, the first was a penumbral lunar eclipse on Thursday, January 18, the second was a penumbral lunar eclipse on Friday, June 15, and the last being with a partial lunar eclipse on Monday, December 10.