| Partial eclipse | |||||||||||||
 The Moon's hourly motion shown right to left | |||||||||||||
| Date | August 19, 2035 | ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Gamma | 0.9433 | ||||||||||||
| Magnitude | 0.1049 | ||||||||||||
| Saros cycle | 119 (63 of 83) | ||||||||||||
| Partiality | 76 minutes, 31 seconds | ||||||||||||
| Penumbral | 289 minutes, 51 seconds | ||||||||||||
| |||||||||||||
A partiallunar eclipse will occur at the Moon’sdescending node of orbit on Sunday, August 19, 2035,[1] with an umbralmagnitude of 0.1049. A lunar eclipse occurs when theMoon moves into theEarth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. Unlike asolar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on thenight side of Earth. Occurring about 4.9 days beforeapogee (on August 14, 2035, at 2:10 UTC), the Moon's apparent diameter will be smaller.[2]
The eclipse will be completely visible overSouth America,Africa, andEurope, seen rising overNorth America and setting overwest,central, andsouth Asia.[3]
 |
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]
| Parameter | Value |
|---|---|
| Penumbral Magnitude | 1.15186 |
| Umbral Magnitude | 0.10490 |
| Gamma | 0.94339 |
| Sun Right Ascension | 09h52m42.8s |
| Sun Declination | +12°52'21.3" |
| Sun Semi-Diameter | 15'48.1" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 21h51m50.7s |
| Moon Declination | -12°01'40.6" |
| Moon Semi-Diameter | 15'05.5" |
| Moon Equatorial Horizontal Parallax | 0°55'23.4" |
| ΔT | 76.7 s |
This eclipse is part of aneclipse 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 afortnight.
| August 19 Descending node (full moon) | September 2 Ascending node (new moon) |
|---|---|
|  |
| Partial lunar eclipse Lunar Saros 119 | Total solar eclipse Solar Saros 145 |
This eclipse is a member of asemester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternatingnodes of the Moon's orbit.[5]
The penumbral lunar eclipses onJune 17, 2038 andDecember 11, 2038 occur in the next lunar year eclipse set.
| Lunar eclipse series sets from 2035 to 2038 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||||
| Saros | Date Viewing | Type Chart | Gamma | Saros | Date Viewing | Type Chart | Gamma | |
| 114 | 2035 Feb 22 | Penumbral | −1.0357 | 119 | 2035 Aug 19 | Partial | 0.9433 | |
| 124 | 2036 Feb 11 | Total | −0.3110 | 129 | 2036 Aug 07 | Total | 0.2004 | |
| 134 | 2037 Jan 31 | Total | 0.3619 | 139 | 2037 Jul 27 | Partial | −0.5582 | |
| 144 | 2038 Jan 21 | Penumbral | 1.0710 | 149 | 2038 Jul 16 | Penumbral | −1.2837 | |
This eclipse is a part ofSaros series 119, repeating every 18 years, 11 days, and containing 82 events. The series started with a penumbral lunar eclipse on October 14, 935 AD. It contains partial eclipses from May 18, 1296 through August 2, 1422; total eclipses from August 13, 1440 throughJune 15, 1927; and a second set of partial eclipses fromJune 25, 1945 throughAugust 19, 2035. The series ends at member 82 as a penumbral eclipse on March 25, 2396.
The longest duration of totality was produced by member 49 at 102 minutes, 6 seconds on March 30, 1801. All eclipses in this series occur at the Moon’sdescending node of orbit.[6]
| Greatest | First | |||
|---|---|---|---|---|
| The greatest eclipse of the series occurred on1801 Mar 30, lasting 102 minutes, 6 seconds.[7] | Penumbral | Partial | Total | Central |
| 934 Oct 14 | 1296 May 18 | 1440 Aug 13 | 1512 Sep 25 | |
| Last | ||||
| Central | Total | Partial | Penumbral | |
| 1873 May 12 | 1927 Jun 15 | 2035 Aug 19 | 2396 Mar 25 | |
Eclipses are tabulated in three columns; every third eclipse in the same column is oneexeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
| Series members 49–71 occur between 1801 and 2200: | |||||
|---|---|---|---|---|---|
| 49 | 50 | 51 | |||
| 1801 Mar 30 | 1819 Apr 10 | 1837 Apr 20 | |||
| 52 | 53 | 54 | |||
| 1855 May 02 | 1873 May 12 | 1891 May 23 | |||
| 55 | 56 | 57 | |||
| 1909 Jun 04 | 1927 Jun 15 | 1945 Jun 25 | |||
 |  | |  |  |  |
| 58 | 59 | 60 | |||
| 1963 Jul 06 | 1981 Jul 17 | 1999 Jul 28 | |||
 |  |  |  |  |  |
| 61 | 62 | 63 | |||
| 2017 Aug 07 | 2035 Aug 19 | 2053 Aug 29 | |||
 |  | | |  | |
| 64 | 65 | 66 | |||
| 2071 Sep 09 | 2089 Sep 19 | 2107 Oct 02 | |||
| 67 | 68 | 69 | |||
| 2125 Oct 12 | 2143 Oct 23 | 2161 Nov 03 | |||
| 70 | 71 | ||||
| 2179 Nov 14 | 2197 Nov 24 | ||||
This eclipse is a part of atritos cycle, repeating at alternating nodes every 135synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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 1817 and 2200 | |||||||||
|---|---|---|---|---|---|---|---|---|---|
| 1817 May 01 (Saros 99) | 1828 Mar 31 (Saros 100) | 1839 Feb 28 (Saros 101) | 1850 Jan 28 (Saros 102) | 1860 Dec 28 (Saros 103) | |||||
| 1893 Sep 25 (Saros 106) | 1915 Jul 26 (Saros 108) | ||||||||
 |  | ||||||||
| 1926 Jun 25 (Saros 109) | 1937 May 25 (Saros 110) | 1948 Apr 23 (Saros 111) | 1959 Mar 24 (Saros 112) | 1970 Feb 21 (Saros 113) | |||||
 |  |  |  |  |  |  |  |  |  |
| 1981 Jan 20 (Saros 114) | 1991 Dec 21 (Saros 115) | 2002 Nov 20 (Saros 116) | 2013 Oct 18 (Saros 117) | 2024 Sep 18 (Saros 118) | |||||
 |  |  |  |  |  |  |  |  |  |
| 2035 Aug 19 (Saros 119) | 2046 Jul 18 (Saros 120) | 2057 Jun 17 (Saros 121) | 2068 May 17 (Saros 122) | 2079 Apr 16 (Saros 123) | |||||
| |  |  |  |  |  |  | ||
| 2090 Mar 15 (Saros 124) | 2101 Feb 14 (Saros 125) | 2112 Jan 14 (Saros 126) | 2122 Dec 13 (Saros 127) | 2133 Nov 12 (Saros 128) | |||||
| 2144 Oct 11 (Saros 129) | 2155 Sep 11 (Saros 130) | 2166 Aug 11 (Saros 131) | 2177 Jul 11 (Saros 132) | 2188 Jun 09 (Saros 133) | |||||
| 2199 May 10 (Saros 134) | |||||||||
This eclipse is a part of the long periodinex cycle, repeating at alternating nodes, every 358synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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 | |||||
|---|---|---|---|---|---|
| 1804 Jan 26 (Saros 111) | 1833 Jan 06 (Saros 112) | 1861 Dec 17 (Saros 113) | |||
| 1890 Nov 26 (Saros 114) | 1919 Nov 07 (Saros 115) | 1948 Oct 18 (Saros 116) | |||
 |  |  |  | ||
| 1977 Sep 27 (Saros 117) | 2006 Sep 07 (Saros 118) | 2035 Aug 19 (Saros 119) | |||
 |  |  |  | | |
| 2064 Jul 28 (Saros 120) | 2093 Jul 08 (Saros 121) | 2122 Jun 20 (Saros 122) | |||
| 2151 May 30 (Saros 123) | 2180 May 09 (Saros 124) | ||||
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (ahalf saros).[8] This lunar eclipse is related to two total solar eclipses ofSolar Saros 126.
| August 12, 2026 | August 23, 2044 |
|---|---|
 |  |
 | This lunar eclipse-related article is astub. You can help Wikipedia byexpanding it. |
_(cropped).jpg)
