Solar eclipse of June 1, 2030
Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, June 1, 2030,[1] with a magnitude of 0.9443. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 23 hours after apogee (on May 31, 2030, at 7:15 UTC), the Moon's apparent diameter will be smaller.[2]
The annular eclipse will start in northern Africa and will cross the Eurasian continent, including Algeria, Tunisia, Libya, Malta, Greece, northwestern Turkey, southeastern Bulgaria, southeastern Ukraine, Russia, northern Kazakhstan, northeastern China and northern Japan. It will also pass through a number of large cities such as Tripoli, Athens, Istanbul, Krasnodar, Rostov-on-Don, Volgograd, Omsk, Krasnoyarsk and Sapporo. The greatest eclipse will be near the border of Tomsk and Novosibirsk oblasts, ~200 km west of Tomsk. A partial eclipse will be visible for much of North Africa, Europe, Asia, Alaska, and northern Canada.
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Images
File:SE2030Jun01A.gif
Animated path
Eclipse details
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.[3]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2030 June 1 at 03:35:53.3 UTC |
| First Umbral External Contact | 2030 June 1 at 04:48:25.8 UTC |
| First Central Line | 2030 June 1 at 04:51:16.8 UTC |
| First Umbral Internal Contact | 2030 June 1 at 04:54:09.4 UTC |
| Ecliptic Conjunction | 2030 June 1 at 06:22:30.7 UTC |
| Greatest Eclipse | 2030 June 1 at 06:29:12.9 UTC |
| Greatest Duration | 2030 June 1 at 06:29:55.1 UTC |
| Equatorial Conjunction | 2030 June 1 at 06:31:58.0 UTC |
| Last Umbral Internal Contact | 2030 June 1 at 08:04:14.9 UTC |
| Last Central Line | 2030 June 1 at 08:07:06.9 UTC |
| Last Umbral External Contact | 2030 June 1 at 08:09:57.3 UTC |
| Last Penumbral External Contact | 2030 June 1 at 09:22:29.8 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.94426 |
| Eclipse Obscuration | 0.89163 |
| Gamma | 0.56265 |
| Sun Right Ascension | 04h37m01.2s |
| Sun Declination | +22°03'55.3" |
| Sun Semi-Diameter | 15'46.4" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 04h36m55.8s |
| Moon Declination | +22°34'11.5" |
| Moon Semi-Diameter | 14'42.7" |
| Moon Equatorial Horizontal Parallax | 0°53'59.6" |
| ΔT | 74.0 s |
Eclipse season
Script error: No such module "Labelled list hatnote". 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.
| June 1 Descending node (new moon) |
June 15 Ascending node (full moon) |
|---|---|
| File:SE2030Jun01A.png | File:Lunar eclipse chart close-2030Jun15.png |
| Annular solar eclipse Solar Saros 128 |
Partial lunar eclipse Lunar Saros 140 |
Related eclipses
Eclipses in 2030
- An annular solar eclipse on June 1.
- A partial lunar eclipse on June 15.
- A total solar eclipse on November 25.
- A penumbral lunar eclipse on December 9.
Metonic
- Preceded by: Solar eclipse of August 12, 2026
- Followed by: Solar eclipse of March 20, 2034
Tzolkinex
- Preceded by: Solar eclipse of April 20, 2023
- Followed by: Solar eclipse of July 13, 2037
Half-Saros
- Preceded by: Lunar eclipse of May 26, 2021
- Followed by: Lunar eclipse of June 6, 2039
Tritos
- Preceded by: Solar eclipse of July 2, 2019
- Followed by: Solar eclipse of April 30, 2041
Solar Saros 128
- Preceded by: Solar eclipse of May 20, 2012
- Followed by: Solar eclipse of June 11, 2048
Inex
- Preceded by: Solar eclipse of June 21, 2001
- Followed by: Solar eclipse of May 11, 2059
Triad
- Preceded by: Solar eclipse of August 1, 1943
- Followed by: Solar eclipse of April 2, 2117
Solar eclipses of 2029–2032
This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[4]
The partial solar eclipses on January 14, 2029 and July 11, 2029 occur in the previous lunar year eclipse set.
| Solar eclipse series sets from 2029 to 2032 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | June 12, 2029 File:SE2029Jun12P.png Partial |
1.29431 | 123 | December 5, 2029 File:SE2029Dec05P.png Partial |
−1.06090 | |
| 128 | June 1, 2030 File:SE2030Jun01A.png Annular |
0.56265 | 133 | November 25, 2030 File:SE2030Nov25T.png Total |
−0.38669 | |
| 138 | May 21, 2031 File:SE2031May21A.png Annular |
−0.19699 | 143 | November 14, 2031 File:SE2031Nov14H.png Hybrid |
0.30776 | |
| 148 | May 9, 2032 File:SE2032May09A.png Annular |
−0.93748 | 153 | November 3, 2032 File:SE2032Nov03P.png Partial |
1.06431 | |
Saros 128
This eclipse is a part of Saros series 128, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on August 29, 984 AD. It contains total eclipses from May 16, 1417 through June 18, 1471; hybrid eclipses from June 28, 1489 through July 31, 1543; and annular eclipses from August 11, 1561 through July 25, 2120. The series ends at member 73 as a partial eclipse on November 1, 2282. Its 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.
The longest duration of totality was produced by member 27 at 1 minutes, 45 seconds on June 7, 1453, and the longest duration of annularity was produced by member 48 at 8 minutes, 35 seconds on February 1, 1832. All eclipses in this series occur at the Moon’s descending node of orbit.[5]
| Series members 47–68 occur between 1801 and 2200: | ||
|---|---|---|
| 47 | 48 | 49 |
| File:SE1814Jan21A.gif January 21, 1814 |
File:SE1832Feb01A.gif February 1, 1832 |
File:SE1850Feb12A.gif February 12, 1850 |
| 50 | 51 | 52 |
| File:SE1868Feb23A.gif February 23, 1868 |
File:SE1886Mar05A.gif March 5, 1886 |
File:SE1904Mar17A.png March 17, 1904 |
| 53 | 54 | 55 |
| File:SE1922Mar28A.png March 28, 1922 |
File:SE1940Apr07A.png April 7, 1940 |
File:SE1958Apr19A.png April 19, 1958 |
| 56 | 57 | 58 |
| File:SE1976Apr29A.png April 29, 1976 |
File:SE1994May10A.png May 10, 1994 |
File:SE2012May20A.png May 20, 2012 |
| 59 | 60 | 61 |
| File:SE2030Jun01A.png June 1, 2030 |
File:SE2048Jun11A.png June 11, 2048 |
File:SE2066Jun22A.png June 22, 2066 |
| 62 | 63 | 64 |
| File:SE2084Jul03A.png July 3, 2084 |
File:SE2102Jul15A.png July 15, 2102 |
File:SE2120Jul25A.png July 25, 2120 |
| 65 | 66 | 67 |
| File:Saros128 65van73 SE2138Aug05P.jpg August 5, 2138 |
File:Saros128 66van73 SE2156Aug16P.jpg August 16, 2156 |
File:Saros128 67van73 SE2174Aug27P.jpg August 27, 2174 |
| 68 | ||
| File:Saros128 68van73 SE2192Sep06P.jpg September 6, 2192 | ||
Metonic series
The metonic 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 descending node.
Tritos series
Template:Solar Tritos series 2008 August 1
Inex series
Template:Solar Inex series 2001 June 21
References
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External links
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