# March 2016 lunar eclipse

A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, March 23, 2016, with an umbral magnitude of −0.3107. 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 days before apogee (on March 25, 2016, at 10:15 UTC), the Moon's apparent diameter was smaller.

## Visibility

The eclipse was completely visible over Australia and western North America, seen rising over much of Asia and setting over central and eastern North America and western South America.
| | Hourly motion shown right to left |
| Visibility map ||

## Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
March 23, 2016 Lunar Eclipse Parameters :
| Parameter | Value |
| Penumbral Magnitude | 0.77585 |
| Umbral Magnitude | −0.31071 |
| Gamma | 1.15916 |
| Sun Right Ascension | 00h12m02.0s |
| Sun Declination | +01°18'10.9" |
| Sun Semi-Diameter | 16'02.7" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 12h13m18.6s |
| Moon Declination | -00°18'21.4" |
| Moon Semi-Diameter | 14'46.0" |
| Moon Equatorial Horizontal Parallax | 0°54'11.6" |
| ΔT | 68.0 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.
Eclipse season of March 2016 :
| March 9 Descending node (new moon) | March 23 Ascending node (full moon) |
| Total solar eclipse Solar Saros 130 | Penumbral lunar eclipse Lunar Saros 142 |

## Related eclipses
### Eclipses in 2016

* A total solar eclipse on March 9.
* A penumbral lunar eclipse on March 23.
* A penumbral lunar eclipse on August 18.
* An annular solar eclipse on September 1.
* A penumbral lunar eclipse on September 16.

### Metonic

* Preceded by: Lunar eclipse of June 4, 2012
* Followed by: Lunar eclipse of January 10, 2020

### Tzolkinex

* Preceded by: Lunar eclipse of February 9, 2009
* Followed by: Lunar eclipse of May 5, 2023

### Half-Saros

* Preceded by: Solar eclipse of March 19, 2007
* Followed by: Solar eclipse of March 29, 2025

### Tritos

* Preceded by: Lunar eclipse of April 24, 2005
* Followed by: Lunar eclipse of February 20, 2027

### Lunar Saros 142

* Preceded by: Lunar eclipse of March 13, 1998
* Followed by: Lunar eclipse of April 3, 2034

### Inex

* Preceded by: Lunar eclipse of April 14, 1987
* Followed by: Lunar eclipse of March 3, 2045

### Triad

* Preceded by: Lunar eclipse of May 23, 1929
* Followed by: Lunar eclipse of January 23, 2103

### Lunar eclipses of 2013–2016

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.
The penumbral lunar eclipse on May 25, 2013 occurs in the previous lunar year eclipse set, and the penumbral lunar eclipse on August 18, 2016 occurs in the next lunar year eclipse set.
Lunar eclipse series sets from 2013 to 2016 :
| Ascending node | Ascending node | Ascending node | Ascending node | Descending node | Descending node | Descending node | Descending node |
| Saros | Date Viewing | Type Chart | Gamma | Saros | Date Viewing | Type Chart | Gamma |
| 112 | 2013 Apr 25 | Partial | −1.0121 | 117 | 2013 Oct 18 | Penumbral | 1.1508 |
| 122 | 2014 Apr 15 | Total | −0.3017 | 127 | 2014 Oct 08 | Total | 0.3827 |
| 132 | 2015 Apr 04 | Total | 0.4460 | 137 | 2015 Sep 28 | Total | −0.3296 |
| 142 | 2016 Mar 23 | Penumbral | 1.1592 | 147 | 2016 Sep 16 | Penumbral | −1.0549 |

### Saros 142

This eclipse is a part of Saros series 142, repeating every 18 years, 11 days, and containing 73 events. The series started with a penumbral lunar eclipse on September 19, 1709. It contains partial eclipses from May 5, 2088 through July 10, 2196; total eclipses from July 22, 2214 through April 21, 2665; and a second set of partial eclipses from May 3, 2683 through July 29, 2827. The series ends at member 73 as a penumbral eclipse on November 17, 3007.
The longest duration of totality will be produced by member 34 at 103 minutes, 54 seconds on September 15, 2304. All eclipses in this series occur at the Moon’s ascending node of orbit.
| Greatest | First | First | First | First |
| The greatest eclipse of the series will occur on 2304 Sep 15, lasting 103 minutes, 54 seconds. | Penumbral | Partial | Total | Central |
| The greatest eclipse of the series will occur on 2304 Sep 15, lasting 103 minutes, 54 seconds. | 1709 Sep 19 | 2088 May 05 | 2214 Jul 22 | 2250 Aug 13 |
| Last ||||
| The greatest eclipse of the series will occur on 2304 Sep 15, lasting 103 minutes, 54 seconds. | Central | Total | Partial | Penumbral |
| The greatest eclipse of the series will occur on 2304 Sep 15, lasting 103 minutes, 54 seconds. | 2448 Dec 10 | 2665 Apr 21 | 2827 Jul 29 | 3007 Nov 17 |
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.
Series members 7–28 occur between 1801 and 2200: :
| 7 | 7 | 8 | 8 | 9 | 9 |
| 1817 Nov 23 | 1817 Nov 23 | 1835 Dec 05 | 1835 Dec 05 | 1853 Dec 15 | 1853 Dec 15 |
| 10 | 10 | 11 | 11 | 12 | 12 |
| 1871 Dec 26 | 1871 Dec 26 | 1890 Jan 06 | 1890 Jan 06 | 1908 Jan 18 | 1908 Jan 18 |
| 13 | 13 | 14 | 14 | 15 | 15 |
| 1926 Jan 28 | 1926 Jan 28 | 1944 Feb 09 | 1944 Feb 09 | 1962 Feb 19 | 1962 Feb 19 |
| 16 | 16 | 17 | 17 | 18 | 18 |
| 1980 Mar 01 | 1980 Mar 01 | 1998 Mar 13 | 1998 Mar 13 | 2016 Mar 23 | 2016 Mar 23 |
| 19 | 19 | 20 | 20 | 21 | 21 |
| 2034 Apr 03 | 2034 Apr 03 | 2052 Apr 14 | 2052 Apr 14 | 2070 Apr 25 | 2070 Apr 25 |
| 22 | 22 | 23 | 23 | 24 | 24 |
| 2088 May 05 | 2088 May 05 | 2106 May 17 | 2106 May 17 | 2124 May 28 | 2124 May 28 |
| 25 | 25 | 26 | 26 | 27 | 27 |
| 2142 Jun 08 | 2142 Jun 08 | 2160 Jun 18 | 2160 Jun 18 | 2178 Jun 30 | 2178 Jun 30 |
| 28 ||
| 2196 Jul 10 ||

### 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.
Series members between 1801 and 2200 :
| 1808 Nov 03 (Saros 123) | 1808 Nov 03 (Saros 123) | 1819 Oct 03 (Saros 124) | 1819 Oct 03 (Saros 124) | 1830 Sep 02 (Saros 125) | 1830 Sep 02 (Saros 125) | 1841 Aug 02 (Saros 126) | 1841 Aug 02 (Saros 126) | 1852 Jul 01 (Saros 127) | 1852 Jul 01 (Saros 127) |
| 1863 Jun 01 (Saros 128) | 1863 Jun 01 (Saros 128) | 1874 May 01 (Saros 129) | 1874 May 01 (Saros 129) | 1885 Mar 30 (Saros 130) | 1885 Mar 30 (Saros 130) | 1896 Feb 28 (Saros 131) | 1896 Feb 28 (Saros 131) | 1907 Jan 29 (Saros 132) | 1907 Jan 29 (Saros 132) |
| 1917 Dec 28 (Saros 133) | 1917 Dec 28 (Saros 133) | 1928 Nov 27 (Saros 134) | 1928 Nov 27 (Saros 134) | 1939 Oct 28 (Saros 135) | 1939 Oct 28 (Saros 135) | 1950 Sep 26 (Saros 136) | 1950 Sep 26 (Saros 136) | 1961 Aug 26 (Saros 137) | 1961 Aug 26 (Saros 137) |
| 1972 Jul 26 (Saros 138) | 1972 Jul 26 (Saros 138) | 1983 Jun 25 (Saros 139) | 1983 Jun 25 (Saros 139) | 1994 May 25 (Saros 140) | 1994 May 25 (Saros 140) | 2005 Apr 24 (Saros 141) | 2005 Apr 24 (Saros 141) | 2016 Mar 23 (Saros 142) | 2016 Mar 23 (Saros 142) |
| 2027 Feb 20 (Saros 143) | 2027 Feb 20 (Saros 143) | 2038 Jan 21 (Saros 144) | 2038 Jan 21 (Saros 144) | 2048 Dec 20 (Saros 145) | 2048 Dec 20 (Saros 145) | 2059 Nov 19 (Saros 146) | 2059 Nov 19 (Saros 146) | 2070 Oct 19 (Saros 147) | 2070 Oct 19 (Saros 147) |
| 2081 Sep 18 (Saros 148) | 2081 Sep 18 (Saros 148) | 2092 Aug 17 (Saros 149) | 2092 Aug 17 (Saros 149) | 2103 Jul 19 (Saros 150) | 2103 Jul 19 (Saros 150) | 2114 Jun 18 (Saros 151) | 2114 Jun 18 (Saros 151) | 2125 May 17 (Saros 152) | 2125 May 17 (Saros 152) |
| 2136 Apr 16 (Saros 153) | 2136 Apr 16 (Saros 153) | | | | | 2169 Jan 13 (Saros 156) | 2169 Jan 13 (Saros 156) | | |
| 2190 Nov 12 (Saros 158) ||

### 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.
Series members between 1801 and 2200 :
| 1813 Aug 12 (Saros 135) | 1813 Aug 12 (Saros 135) | 1842 Jul 22 (Saros 136) | 1842 Jul 22 (Saros 136) | 1871 Jul 02 (Saros 137) | 1871 Jul 02 (Saros 137) |
| 1900 Jun 13 (Saros 138) | 1900 Jun 13 (Saros 138) | 1929 May 23 (Saros 139) | 1929 May 23 (Saros 139) | 1958 May 03 (Saros 140) | 1958 May 03 (Saros 140) |
| 1987 Apr 14 (Saros 141) | 1987 Apr 14 (Saros 141) | 2016 Mar 23 (Saros 142) | 2016 Mar 23 (Saros 142) | 2045 Mar 03 (Saros 143) | 2045 Mar 03 (Saros 143) |
| 2074 Feb 11 (Saros 144) | 2074 Feb 11 (Saros 144) | 2103 Jan 23 (Saros 145) | 2103 Jan 23 (Saros 145) | 2132 Jan 02 (Saros 146) | 2132 Jan 02 (Saros 146) |
| 2160 Dec 13 (Saros 147) | 2160 Dec 13 (Saros 147) | 2189 Nov 22 (Saros 148) | 2189 Nov 22 (Saros 148) |

### 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 149.
| March 19, 2007 | March 29, 2025 |