Solar eclipse of March 10, 2100
Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse will occur at the Moon's ascending node of orbit between Wednesday, March 10 and Thursday, March 11, 2100,[1] with a magnitude of 0.9338. 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 2.9 days before apogee (on March 13, 2100, at 21:10 UTC), the Moon's apparent diameter will be smaller.[2]
The path of annularity will be visible from parts of northeastern Australia, Papua New Guinea, the Solomon Islands, Tuvalu, and Hawaii, California, Oregon, northwestern Nevada, Idaho, Montana, Wyoming, North Dakota, South Dakota, and Minnesota in the United States. A partial solar eclipse will also be visible for parts of Australia, Oceania, and North America.
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 | 2100 March 10 at 19:26:43.1 UTC |
| First Umbral External Contact | 2100 March 10 at 20:33:05.4 UTC |
| First Central Line | 2100 March 10 at 20:36:01.0 UTC |
| First Umbral Internal Contact | 2100 March 10 at 20:38:57.2 UTC |
| First Penumbral Internal Contact | 2100 March 10 at 21:52:49.6 UTC |
| Greatest Duration | 2100 March 10 at 22:21:55.8 UTC |
| Greatest Eclipse | 2100 March 10 at 22:28:11.0 UTC |
| Ecliptic Conjunction | 2100 March 10 at 22:31:51.0 UTC |
| Equatorial Conjunction | 2100 March 10 at 22:48:12.9 UTC |
| Last Penumbral Internal Contact | 2100 March 10 at 23:03:03.0 UTC |
| Last Umbral Internal Contact | 2100 March 11 at 00:17:11.1 UTC |
| Last Central Line | 2100 March 11 at 00:20:09.1 UTC |
| Last Umbral External Contact | 2100 March 11 at 00:23:06.7 UTC |
| Last Penumbral External Contact | 2100 March 11 at 01:29:34.7 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.93384 |
| Eclipse Obscuration | 0.87205 |
| Gamma | 0.30770 |
| Sun Right Ascension | 23h24m46.6s |
| Sun Declination | -03°47'43.4" |
| Sun Semi-Diameter | 16'06.4" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 23h24m14.3s |
| Moon Declination | -03°33'06.4" |
| Moon Semi-Diameter | 14'49.6" |
| Moon Equatorial Horizontal Parallax | 0°54'24.7" |
| ΔT | 123.8 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.
| February 24 Descending node (full moon) |
March 10 Ascending node (new moon) |
|---|---|
| File:SE2100Mar10A.png | |
| Penumbral lunar eclipse Lunar Saros 115 |
Annular solar eclipse Solar Saros 141 |
Related eclipses
Eclipses in 2100
- A penumbral lunar eclipse on February 24.
- An annular solar eclipse on March 10.
- A penumbral lunar eclipse on August 19.
- A total solar eclipse on September 4.
Metonic
- Preceded by: Solar eclipse of May 22, 2096
- Followed by: Solar eclipse of December 29, 2103
Tzolkinex
- Preceded by: Solar eclipse of January 27, 2093
- Followed by: Solar eclipse of April 23, 2107
Half-Saros
- Preceded by: Lunar eclipse of March 5, 2091
- Followed by: Lunar eclipse of March 17, 2109
Tritos
- Preceded by: Solar eclipse of April 10, 2089
- Followed by: Solar eclipse of February 8, 2111
Solar Saros 141
- Preceded by: Solar eclipse of February 27, 2082
- Followed by: Solar eclipse of March 22, 2118
Inex
- Preceded by: Solar eclipse of March 31, 2071
- Followed by: Solar eclipse of February 18, 2129
Triad
- Preceded by: Solar eclipse of May 10, 2013
- Followed by: Solar eclipse of January 9, 2187
Solar eclipses of 2098–2101
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 eclipse on October 24, 2098 occurs in the previous lunar year eclipse set.
| Solar eclipse series sets from 2098 to 2101 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 121 | April 1, 2098 File:SE2098Apr01P.png Partial |
−1.1005 | 126 | September 25, 2098 File:SE2098Sep25P.png Partial |
1.14 | |
| 131 | March 21, 2099 File:SE2099Mar21A.png Annular |
−0.4016 | 136 | September 14, 2099 File:SE2099Sep14T.png Total |
0.3942 | |
| 141 | March 10, 2100 File:SE2100Mar10A.png Annular |
0.3077 | 146 | September 4, 2100 File:SE2100Sep04T.png Total |
−0.3384 | |
| 151 | February 28, 2101 File:SE2101Feb28A.png Annular |
0.9964 | 156 | August 24, 2101 File:Saros156 06van69 SE2101Aug24P.jpg Partial |
−1.1392 | |
Saros 141
This eclipse is a part of Saros series 141, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on May 19, 1613. It contains annular eclipses from August 4, 1739 through October 14, 2640. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on June 13, 2857. 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 annularity was produced by member 20 at 12 minutes, 9 seconds on December 14, 1955. All eclipses in this series occur at the Moon’s ascending node of orbit.[5]
| Series members 12–33 occur between 1801 and 2200: | ||
|---|---|---|
| 12 | 13 | 14 |
| File:SE1811Sep17A.png September 17, 1811 |
File:SE1829Sep28A.png September 28, 1829 |
File:SE1847Oct09A.png October 9, 1847 |
| 15 | 16 | 17 |
| File:SE1865Oct19A.png October 19, 1865 |
File:SE1883Oct30A.png October 30, 1883 |
File:SE1901Nov11A.png November 11, 1901 |
| 18 | 19 | 20 |
| File:SE1919Nov22A.png November 22, 1919 |
File:SE1937Dec02A.png December 2, 1937 |
File:SE1955Dec14A.png December 14, 1955 |
| 21 | 22 | 23 |
| File:SE1973Dec24A.png December 24, 1973 |
File:SE1992Jan04A.png January 4, 1992 |
File:SE2010Jan15A.png January 15, 2010 |
| 24 | 25 | 26 |
| File:SE2028Jan26A.png January 26, 2028 |
File:SE2046Feb05A.png February 5, 2046 |
File:SE2064Feb17A.png February 17, 2064 |
| 27 | 28 | 29 |
| File:SE2082Feb27A.png February 27, 2082 |
File:SE2100Mar10A.png March 10, 2100 |
File:SE2118Mar22A.png March 22, 2118 |
| 30 | 31 | 32 |
| File:SE2136Apr01A.png April 1, 2136 |
File:SE2154Apr12A.png April 12, 2154 |
File:SE2172Apr23A.png April 23, 2172 |
| 33 | ||
| File:SE2190May04A.png May 4, 2190 | ||
Metonic series
Template:Solar Metonic series 2054–2145
Tritos series
Template:Solar Tritos series 2001 December 14
Inex series
Template:Solar Inex series 2013 May 10
References
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External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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