Solar eclipse of July 29, 1878 explained

A total solar eclipse occurred at the Moon's descending node of orbit between Monday, July 29 and Tuesday, July 30, 1878, with a magnitude of 1.0450. 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 2.4 days before perigee (on August 1, 1878, at 6:45 UTC), the Moon's apparent diameter was larger.[1]

The path of totality was visible from parts of modern-day eastern Russia, Alaska, western Canada, Washington, Idaho, Montana, Wyoming, Colorado, New Mexico, Kansas, Oklahoma, Texas, Louisiana, Cuba, Haiti, and the Dominican Republic. A partial solar eclipse was also visible for parts of Northeast Asia, North America, Central America, the Caribbean, and northern South America.

Newspapers in the United States reported of large migrations from the Midwest towards the path of totality to view the eclipse. Scientists observing from Pikes Peak in Colorado contended with altitude sickness and snowstorms, among other problems.[2] [3]

High-altitude astronomy

The 1878 eclipse was a turning point in modern astronomy, because it was the first time that many of the world's leading astronomers had the opportunity to make their observations from the higher altitudes provided by the Rocky Mountains. After the 1878 eclipse, astronomers began to build observatories at locations well above sea level, including on the sides and summits of mountains, a scientific trend which extended throughout the twentieth century and into the twenty-first.[4]

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.[5]

July 29, 1878 Solar Eclipse Times! Event! Time (UTC)
First Penumbral External Contact1878 July 29 at 19:18:31.9 UTC
First Umbral External Contact1878 July 29 at 20:23:40.9 UTC
First Central Line1878 July 29 at 20:24:46.4 UTC
First Umbral Internal Contact1878 July 29 at 20:25:52.4 UTC
Equatorial Conjunction1878 July 29 at 21:23:06.4 UTC
Ecliptic Conjunction1878 July 29 at 21:40:46.5 UTC
Greatest Duration1878 July 29 at 21:46:11.9 UTC
Greatest Eclipse1878 July 29 at 21:47:17.7 UTC
Last Umbral Internal Contact1878 July 29 at 23:08:56.0 UTC
Last Central Line1878 July 29 at 23:10:04.0 UTC
Last Umbral External Contact1878 July 29 at 23:11:11.6 UTC
Last Penumbral External Contact1878 July 30 at 00:16:08.9 UTC
July 29, 1878 Solar Eclipse Parameters! Parameter! Value
Eclipse Magnitude1.04495
Eclipse Obscuration1.09192
Gamma0.62323
Sun Right Ascension08h35m50.0s
Sun Declination+18°38'42.9"
Sun Semi-Diameter15'45.4"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension08h36m44.1s
Moon Declination+19°13'31.6"
Moon Semi-Diameter16'15.3"
Moon Equatorial Horizontal Parallax0°59'39.2"
ΔT-4.7 s

Eclipse season

See also: Eclipse cycle. 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.

Related eclipses

Eclipses in 1878

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 124

Inex

Triad

Solar eclipses of 1877–1880

The partial solar eclipses on March 15, 1877 and September 7, 1877 occur in the previous lunar year eclipse set, and the partial solar eclipse on December 2, 1880 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1877 to 1880
Descending node Ascending node
SarosMapGammaSarosMapGamma
114August 9, 1877

Partial
1.3277119February 2, 1878

Annular
−0.9071
124July 29, 1878

Total
0.6232129January 22, 1879

Annular
−0.1824
134July 19, 1879

Annular
−0.1439139January 11, 1880

Total
0.6136
144July 7, 1880

Annular
−0.9406146December 31, 1880

Partial
1.1591

Inex series

References

Further reading

External links

Notes and References

  1. Web site: Moon Distances for London, United Kingdom, England. timeanddate. 29 August 2024.
  2. Ruskin. Steve. 2008. 'Among the Favored Mortals of Earth': The Press, State Pride, and the Great Eclipse of 1878. Colorado Heritage.
  3. Waxman . Olivia B. . August 18, 2017 . Think This Total Solar Eclipse Is Getting a Lot of Hype? You Should Have Seen 1878 . . August 22, 2017.
  4. Book: America's first great eclipse : how scientists, tourists, and the Rocky Mountain eclipse of 1878 changed astronomy forever. Ruskin, Steven. 22 July 2017 . 9780999140901. [United States]. 992174591.
  5. Web site: Total Solar Eclipse of 1878 Jul 29. EclipseWise.com. 29 August 2024.