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Solar eclipse of September 8, 1801
Partial solar eclipse September 8, 1801
Partial solar eclipse September 8, 1801
| Field | Value |
|---|---|
| previous | Solar eclipse of April 13, 1801 |
| next | Solar eclipse of October 7, 1801 |
A partial solar eclipse occurred at the Moon's descending node of orbit on Tuesday, September 8, 1801, with a magnitude of 0.1614. 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. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
The partial solar eclipse was visible for parts of modern-day eastern Russia and western Alaska.
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.
| Event | Time (UTC) |
|---|---|
| Equatorial Conjunction | 1801 September 8 at 04:23:25.3 UTC |
| First Penumbral External Contact | 1801 September 8 at 04:53:32.8 UTC |
| Ecliptic Conjunction | 1801 September 8 at 05:38:08.2 UTC |
| Greatest Eclipse | 1801 September 8 at 05:54:39.3 UTC |
| Last Penumbral External Contact | 1801 September 8 at 06:56:17.9 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.16147 |
| Eclipse Obscuration | 0.07489 |
| Gamma | 1.46568 |
| Sun Right Ascension | 11h04m58.3s |
| Sun Declination | +05°53'39.8" |
| Sun Semi-Diameter | 15'53.2" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 11h07m32.9s |
| Moon Declination | +07°04'46.3" |
| Moon Semi-Diameter | 15'03.7" |
| Moon Equatorial Horizontal Parallax | 0°55'16.6" |
| ΔT | 12.8 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. The first and last eclipse in this sequence is separated by one synodic month.
| September 8 | ||||
|---|---|---|---|---|
| Descending node (new moon) | ||||
| September 22 | ||||
| Ascending node (full moon) | ||||
| October 7 | ||||
| Descending node (new moon) | ||||
| [[File:SE1801Sep08P.png | 200px]] | [[File:SE1801Oct07P.png | 200px]] | |
| Partial solar eclipse | ||||
| Solar Saros 112 | Total lunar eclipse | |||
| Lunar Saros 124 | Partial solar eclipse | |||
| Solar Saros 150 |
References
References
- "Solar eclipse of September 8, 1801". [[NASA]].
- "Partial Solar Eclipse of 1801 Sep 08". EclipseWise.com.
- "NASA - Catalog of Solar Eclipses of Saros 112".
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