Solar eclipse of May 6, 1883


A total solar eclipse occurred at the Moon's descending node of orbit between Sunday, May 6, and Monday, May 7, 1883, with a magnitude of 1.0634. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.1 days after perigee, the Moon's apparent diameter was larger.
The path of totality was visible from parts of the South Pacific Ocean. A partial solar eclipse was also visible for parts of eastern Australia, Oceania, Hawaii, Central America, and western South America.

Observations

An expedition of American astronomers traveled from Peru to Caroline Island aboard the to observe the total solar eclipse. A French expedition also observed the eclipse from Caroline, and the United States Navy mapped the atoll. Johann Palisa, a member of the expedition, discovered an asteroid later that year which he named Carolina "in remembrance of his visit to island".

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.
EventTime
First Penumbral External Contact1883 May 6 at 19:21:10.1 UTC
First Umbral External Contact1883 May 6 at 20:18:44.5 UTC
First Central Line1883 May 6 at 20:20:08.5 UTC
First Umbral Internal Contact1883 May 6 at 20:21:32.7 UTC
First Penumbral Internal Contact1883 May 6 at 21:34:45.7 UTC
Equatorial Conjunction1883 May 6 at 21:45:09.2 UTC
Greatest Eclipse1883 May 6 at 21:53:48.9 UTC
Greatest Duration1883 May 6 at 21:56:03.6 UTC
Ecliptic Conjunction1883 May 6 at 21:58:10.3 UTC
Last Penumbral Internal Contact1883 May 6 at 22:13:04.8 UTC
Last Umbral Internal Contact1883 May 6 at 23:26:12.7 UTC
Last Central Line1883 May 6 at 23:27:35.7 UTC
Last Umbral External Contact1883 May 6 at 23:28:58.4 UTC
Last Penumbral External Contact1883 May 7 at 00:26:34.2 UTC

ParameterValue
Eclipse Magnitude1.06341
Eclipse Obscuration1.13085
Gamma−0.42503
Sun Right Ascension02h54m04.8s
Sun Declination+16°37'58.2"
Sun Semi-Diameter15'50.7"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension02h54m25.5s
Moon Declination+16°12'38.1"
Moon Semi-Diameter16'35.5"
Moon Equatorial Horizontal Parallax1°00'53.6"
ΔT-5.6 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months 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.
April 22
Ascending node
May 6
Descending node
Partial lunar eclipse
Lunar Saros 110
Total solar eclipse
Solar Saros 136

Related eclipses

Eclipses in 1883

Metonic

  • Preceded by: Solar eclipse of July 19, 1879
  • Followed by: Solar eclipse of February 22, 1887

Tzolkinex

  • Preceded by: Solar eclipse of March 25, 1876
  • Followed by: Solar eclipse of June 17, 1890

Half-Saros

Tritos

  • Preceded by: Solar eclipse of June 6, 1872
  • Followed by: Solar eclipse of April 6, 1894

Solar Saros 136

Inex

Triad

Solar eclipses of 1880–1884

The solar eclipses on January 11, 1880, July 7, 1880, and December 31, 1880 occur in the previous lunar year eclipse set, and the partial solar eclipse on March 27, 1884 occurs in the next lunar year eclipse set.