| Annular eclipse | |
Annularity as seen fromBeigang, Yunlin, Taiwan | |
| Gamma | 0.1209 |
|---|---|
| Magnitude | 0.994 |
| Maximum eclipse | |
| Duration | 38 s (0 min 38 s) |
| Coordinates | 30°30′N79°42′E / 30.5°N 79.7°E /30.5; 79.7 |
| Max. width of band | 21 km (13 mi) |
| Times (UTC) | |
| Greatest eclipse | 6:41:15 |
| References | |
| Saros | 137 (36 of 70) |
| Catalog # (SE5000) | 9553 |
An annularsolar eclipse occurred at the Moon’sascending node of orbit on Sunday, June 21, 2020,[1][2][3][4][5][6][7] with amagnitude of 0.994. Asolar eclipse occurs when theMoon passes betweenEarth and theSun, thereby totally or partly obscuring the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon'sapparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like anannulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 6.2 days afterapogee (on June 15, 2020, at 1:55 UTC), the Moon's apparent diameter was smaller.[8]
The path of this annular eclipse passed through parts of theDemocratic Republic of the Congo,South Sudan,Ethiopia, andEritrea inAfrica; the southernArabian Peninsula, includingYemen,Oman, and southernSaudi Arabia; parts ofSouth Asia and theHimalayas, including southernPakistan and northernIndia; and parts ofEast Asia, includingSouth China andTaiwan.[9] A partial eclipse was visible throughout much of the rest ofAfrica,Southeast Europe, most ofAsia, and inNew Guinea and northernAustralia just before sunset. In Europe, the partial eclipse was visible to places southeast of the line passing through parts ofItaly,Hungary,Ukraine, and southwesternRussia.[9]

| Country or territory | City or place | Start of partial eclipse | Start of annular eclipse | Maximum eclipse | End of annular eclipse | End of partial eclipse | Duration of annularity (min:s) | Duration of eclipse (hr:min) | Maximum coverage |
|---|---|---|---|---|---|---|---|---|---|
| Impfondo | 05:43:11 (sunrise) | 05:48:05 | 05:48:40 | 05:49:14 | 06:52:20 | 1:09 | 1:09 | 95.68% | |
| Obo | 05:02:51 (sunrise) | 05:49:40 | 05:50:18 | 05:50:56 | 06:59:22 | 1:16 | 1:57 | 96.20% | |
| Lalibela | 06:52:22 | 07:59:40 | 08:00:14 | 08:00:48 | 09:20:02 | 1:08 | 2:28 | 97.06% | |
| Sukkur | 09:33:25 | 11:07:30 | 11:07:50 | 11:08:08 | 12:54:16 | 0:38 | 3:21 | 98.79% | |
| Pano Aqil | 09:34:04 | 11:08:21 | 11:08:40 | 11:09:00 | 12:55:06 | 0:39 | 3:21 | 98.79% | |
| New Mandi Gharsana | 10:12:30 | 11:50:12 | 11:50:27 | 11:50:42 | 13:37:08 | 0:30 | 3:25 | 98.89% | |
| Sirsa | 10:16:56 | 11:56:07 | 11:56:21 | 11:56:35 | 13:42:43 | 0:28 | 3:26 | 98.92% | |
| Dehradun | 10:24:10 | 12:05:19 | 12:05:30 | 12:05:40 | 13:50:46 | 0:21 | 3:27 | 98.96% | |
| New Tehri | 10:25:04 | 12:06:23 | 12:06:38 | 12:06:53 | 13:51:47 | 0:30 | 3:27 | 98.96% | |
| Xiamen | 14:43:43 | 16:10:26 | 16:10:54 | 16:11:22 | 17:24:21 | 0:56 | 2:41 | 97.75% | |
| References:[1] | |||||||||
| Country or territory | City or place | Start of partial eclipse | Maximum eclipse | End of partial eclipse | Duration of eclipse (hr:min) | Maximum coverage | |||
|---|---|---|---|---|---|---|---|---|---|
| Mbandaka | 05:45:06 (sunrise) | 05:47:49 | 06:51:24 | 1:06 | 92.76% | ||||
| Bangui | 05:36:25 (sunrise) | 05:50:10 | 06:54:13 | 1:18 | 88.49% | ||||
| Juba | 06:47:57 | 07:50:34 | 09:02:49 | 2:19 | 87.91% | ||||
| Addis Ababa | 06:49:50 | 07:56:55 | 09:15:43 | 2:26 | 89.09% | ||||
| Khartoum | 05:57:24 | 07:01:08 | 08:14:38 | 2:17 | 75.56% | ||||
| Djibouti | 06:52:18 | 08:02:34 | 09:25:58 | 2:34 | 89.44% | ||||
| Asmara | 06:55:54 | 08:04:00 | 09:23:52 | 2:28 | 87.79% | ||||
| Sanaa | 06:56:15 | 08:08:01 | 09:33:15 | 2:37 | 97.33% | ||||
| Riyadh | 07:10:09 | 08:23:36 | 09:49:42 | 2:40 | 73.19% | ||||
| Doha | 07:12:49 | 08:30:35 | 10:02:12 | 2:49 | 79.67% | ||||
| Manama | 07:14:07 | 08:30:47 | 10:00:40 | 2:47 | 75.06% | ||||
| Dubai | 08:14:50 | 09:36:12 | 11:12:15 | 2:57 | 86.35% | ||||
| Muscat | 08:14:38 | 09:39:14 | 11:19:37 | 3:05 | 97.53% | ||||
| Karachi | 09:26:26 | 10:59:26 | 12:46:39 | 3:20 | 91.49% | ||||
| Kabul | 09:16:20 | 10:46:56 | 12:25:47 | 3:09 | 75.03% | ||||
| Islamabad | 09:50:29 | 11:25:11 | 13:06:30 | 3:16 | 82.01% | ||||
| Lahore | 09:48:49 | 11:26:19 | 13:10:29 | 3:22 | 91.21% | ||||
| New Delhi | 10:20:05 | 12:01:47 | 13:48:48 | 3:29 | 93.75% | ||||
| Kathmandu | 10:54:03 | 12:41:11 | 14:24:45 | 3:31 | 85.97% | ||||
| Thimphu | 11:21:23 | 13:09:30 | 14:49:24 | 3:28 | 84.78% | ||||
| Dhaka | 11:23:09 | 13:12:38 | 14:52:13 | 3:29 | 70.14% | ||||
| Lhasa | 13:26:49 | 15:13:16 | 16:50:51 | 3:24 | 93.78% | ||||
| Chongqing | 14:11:45 | 15:48:56 | 17:11:46 | 3:00 | 94.77% | ||||
| Hanoi | 13:16:18 | 14:55:55 | 16:18:27 | 3:02 | 70.98% | ||||
| Shanghai | 14:45:45 | 16:06:27 | 17:16:12 | 2:30 | 70.99% | ||||
| Hong Kong | 14:37:10 | 16:08:28 | 17:24:35 | 2:47 | 86.00% | ||||
| Taipei | 14:50:04 | 16:13:36 | 17:24:32 | 2:34 | 91.71% | ||||
| Manila | 15:01:12 | 16:23:03 | 17:31:43 | 2:31 | 68.37% | ||||
| Saipan | 17:25:21 | 18:29:57 | 18:49:42 (sunset) | 1:24 | 88.10% | ||||
| Hagåtña | 17:25:57 | 18:31:11 | 18:50:27 (sunset) | 1:25 | 95.18% | ||||
| References:[1] | |||||||||
Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the Moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[10]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2020 June 21 at 03:47:09.9 UTC |
| First Umbral External Contact | 2020 June 21 at 04:48:54.2 UTC |
| First Central Line | 2020 June 21 at 04:49:37.4 UTC |
| Greatest Duration | 2020 June 21 at 04:49:37.4 UTC |
| First Umbral Internal Contact | 2020 June 21 at 04:50:20.7 UTC |
| First Penumbral Internal Contact | 2020 June 21 at 05:52:48.7 UTC |
| Greatest Eclipse | 2020 June 21 at 06:41:15.4 UTC |
| Equatorial Conjunction | 2020 June 21 at 06:42:34.5 UTC |
| Ecliptic Conjunction | 2020 June 21 at 06:42:36.6 UTC |
| Last Penumbral Internal Contact | 2020 June 21 at 07:29:41.2 UTC |
| Last Umbral Internal Contact | 2020 June 21 at 08:32:11.3 UTC |
| Last Central Line | 2020 June 21 at 08:32:51.7 UTC |
| Last Umbral External Contact | 2020 June 21 at 08:33:32.0 UTC |
| Last Penumbral External Contact | 2020 June 21 at 09:35:13.9 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.99401 |
| Eclipse Obscuration | 0.98806 |
| Gamma | 0.12090 |
| Sun Right Ascension | 06h01m33.0s |
| Sun Declination | +23°26'09.7" |
| Sun Semi-Diameter | 15'44.2" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 06h01m30.2s |
| Moon Declination | +23°32'56.7" |
| Moon Semi-Diameter | 15'24.0" |
| Moon Equatorial Horizontal Parallax | 0°56'31.1" |
| ΔT | 70.0 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. The first and last eclipse in this sequence is separated by onesynodic month.
| June 5 Descending node (full moon) | June 21 Ascending node (new moon) | July 5 Descending node (full moon) |
|---|---|---|
| Penumbral lunar eclipse Lunar Saros 111 | Annular solar eclipse Solar Saros 137 | Penumbral lunar eclipse Lunar Saros 149 |
This eclipse is a member of asemester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternatingnodes of the Moon's orbit.[11]
The partial solar eclipses onFebruary 15, 2018 andAugust 11, 2018 occur in the previous lunar year eclipse set.
| Solar eclipse series sets from 2018 to 2021 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 117 Partial inMelbourne,Australia | July 13, 2018 Partial | −1.35423 | 122 Partial inNakhodka,Russia | January 6, 2019 Partial | 1.14174 | |
| 127 Totality inLa Serena,Chile | July 2, 2019 Total | −0.64656 | 132 Annularity inJaffna,Sri Lanka | December 26, 2019 Annular | 0.41351 | |
| 137 Annularity inBeigang, Yunlin,Taiwan | June 21, 2020 Annular | 0.12090 | 142 Totality inGorbea,Chile | December 14, 2020 Total | −0.29394 | |
| 147 Partial inHalifax, Canada | June 10, 2021 Annular | 0.91516 | 152 From HMS Protector offSouth Georgia | December 4, 2021 Total | −0.95261 | |
This eclipse is a part ofSaros series 137, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on May 25, 1389. It contains total eclipses from August 20, 1533 through December 6, 1695; the first set of hybrid eclipses from December 17, 1713 through February 11, 1804; the first set of annular eclipses from February 21, 1822 through March 25, 1876; the second set of hybrid eclipses from April 6, 1894 throughApril 28, 1930; and the second set of annular eclipses fromMay 9, 1948 through April 13, 2507. The series ends at member 70 as a partial eclipse on June 28, 2633. Its 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.
The longest duration of totality was produced by member 11 at 2 minutes, 55 seconds on September 10, 1569, and the longest duration of annularity will be produced by member 59 at 7 minutes, 5 seconds on February 28, 2435. All eclipses in this series occur at the Moon’sascending node of orbit.[12]
| Series members 24–46 occur between 1801 and 2200: | ||
|---|---|---|
| 24 | 25 | 26 |
February 11, 1804 | February 21, 1822 | March 4, 1840 |
| 27 | 28 | 29 |
March 15, 1858 | March 25, 1876 | April 6, 1894 |
| 30 | 31 | 32 |
April 17, 1912 | April 28, 1930 | May 9, 1948 |
| 33 | 34 | 35 |
May 20, 1966 | May 30, 1984 | June 10, 2002 |
| 36 | 37 | 38 |
June 21, 2020 | July 2, 2038 | July 12, 2056 |
| 39 | 40 | 41 |
July 24, 2074 | August 3, 2092 | August 15, 2110 |
| 42 | 43 | 44 |
August 25, 2128 | September 6, 2146 | September 16, 2164 |
| 45 | 46 | |
September 27, 2182 | October 9, 2200 | |
Themetonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's ascending node.
| 21 eclipse events between June 21, 1982 and June 21, 2058 | ||||
|---|---|---|---|---|
| June 21 | April 8–9 | January 26 | November 13–14 | September 1–2 |
| 117 | 119 | 121 | 123 | 125 |
June 21, 1982 | April 9, 1986 | January 26, 1990 | November 13, 1993 | September 2, 1997 |
| 127 | 129 | 131 | 133 | 135 |
June 21, 2001 | April 8, 2005 | January 26, 2009 | November 13, 2012 | September 1, 2016 |
| 137 | 139 | 141 | 143 | 145 |
June 21, 2020 | April 8, 2024 | January 26, 2028 | November 14, 2031 | September 2, 2035 |
| 147 | 149 | 151 | 153 | 155 |
June 21, 2039 | April 9, 2043 | January 26, 2047 | November 14, 2050 | September 2, 2054 |
| 157 | ||||
June 21, 2058 | ||||
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 1801 and 2200 | ||||
|---|---|---|---|---|
March 4, 1802 (Saros 117) | February 1, 1813 (Saros 118) | January 1, 1824 (Saros 119) | November 30, 1834 (Saros 120) | October 30, 1845 (Saros 121) |
September 29, 1856 (Saros 122) | August 29, 1867 (Saros 123) | July 29, 1878 (Saros 124) | June 28, 1889 (Saros 125) | May 28, 1900 (Saros 126) |
April 28, 1911 (Saros 127) | March 28, 1922 (Saros 128) | February 24, 1933 (Saros 129) | January 25, 1944 (Saros 130) | December 25, 1954 (Saros 131) |
November 23, 1965 (Saros 132) | October 23, 1976 (Saros 133) | September 23, 1987 (Saros 134) | August 22, 1998 (Saros 135) | July 22, 2009 (Saros 136) |
June 21, 2020 (Saros 137) | May 21, 2031 (Saros 138) | April 20, 2042 (Saros 139) | March 20, 2053 (Saros 140) | February 17, 2064 (Saros 141) |
January 16, 2075 (Saros 142) | December 16, 2085 (Saros 143) | November 15, 2096 (Saros 144) | October 16, 2107 (Saros 145) | September 15, 2118 (Saros 146) |
August 15, 2129 (Saros 147) | July 14, 2140 (Saros 148) | June 14, 2151 (Saros 149) | May 14, 2162 (Saros 150) | April 12, 2173 (Saros 151) |
March 12, 2184 (Saros 152) | February 10, 2195 (Saros 153) | |||
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 | ||
|---|---|---|
November 9, 1817 (Saros 130) | October 20, 1846 (Saros 131) | September 29, 1875 (Saros 132) |
September 9, 1904 (Saros 133) | August 21, 1933 (Saros 134) | July 31, 1962 (Saros 135) |
July 11, 1991 (Saros 136) | June 21, 2020 (Saros 137) | May 31, 2049 (Saros 138) |
May 11, 2078 (Saros 139) | April 23, 2107 (Saros 140) | April 1, 2136 (Saros 141) |
March 12, 2165 (Saros 142) | February 21, 2194 (Saros 143) | |