Solar eclipse of August 9, 1896

Last updated
Solar eclipse of August 9, 1896
SE1896Aug09T.png
Map
Type of eclipse
NatureTotal
Gamma 0.6964
Magnitude 1.0392
Maximum eclipse
Duration163 sec (2 m 43 s)
Coordinates 54°24′N132°12′E / 54.4°N 132.2°E / 54.4; 132.2
Max. width of band182 km (113 mi)
Times (UTC)
Greatest eclipse5:09:00
References
Saros 124 (48 of 73)
Catalog # (SE5000) 9272

A total solar eclipse occurred on August 9, 1896. 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. It was visible across Europe, Asia, and Japan.

Contents

It is a part of solar Saros 124.

This event was the subject of the first organized eclipse expedition by the British Astronomical Association. A group of 165 amateur and profession astronomers sailed from Tilbury, England on July 25, heading toward Vadsø, Norway. [1] This expedition failed to produce any usable results as they were frustrated by the weather conditions at the time of the eclipse. [2] However, a smaller expedition to Novaya Zemlya on Sir George Baden-Powell's yacht Otario met with success. [1]

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of May 28, 1900</span> Total solar eclipse

A total solar eclipse occurred on May 28, 1900. 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.

<span class="mw-page-title-main">Solar eclipse of April 16, 1893</span> Total solar eclipse April 16, 1893

A total solar eclipse occurred on April 16, 1893. 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.

<span class="mw-page-title-main">Solar eclipse of December 22, 1889</span> Total solar eclipse December 22, 1889

A total solar eclipse occurred on December 22, 1889. 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. It was visible from Cuba, to the coast of Brazil, and across southern Africa.

<span class="mw-page-title-main">Solar eclipse of September 7, 1858</span> Total solar eclipse September 7, 1858

A total solar eclipse occurred on September 7, 1858. 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. It was visible across South America.

<span class="mw-page-title-main">Solar eclipse of August 19, 1887</span> Total solar eclipse August 19, 1887

A total solar eclipse occurred on 19 August 1887. 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. It was visible across Europe, Asia, and Japan.

<span class="mw-page-title-main">Solar eclipse of January 1, 1889</span> Total solar eclipse January 1, 1889

A total solar eclipse occurred on January 1, 1889. 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. It was visible across western United States, and central Canada. Partiality was visible across the northern Pacific ocean including Hawaii, and all of the United States.

<span class="mw-page-title-main">Solar eclipse of August 18, 1868</span> Total eclipse named after Rama IV of Siam

A total solar eclipse occurred on August 18, 1868, also known as "The King of Siam's eclipse". 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.

<span class="mw-page-title-main">Solar eclipse of July 8, 1842</span> Total solar eclipse July 8, 1842

A total solar eclipse occurred on July 8, 1842. 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.

<span class="mw-page-title-main">Solar eclipse of July 18, 1860</span> Total solar eclipse July 18, 1860

A total solar eclipse occurred on July 18, 1860. 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.

<span class="mw-page-title-main">Solar eclipse of August 29, 1886</span> Total solar eclipse August 29, 1886

A total solar eclipse occurred on August 29, 1886. 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.

<span class="mw-page-title-main">Solar eclipse of May 26, 1854</span> Annular solar eclipse May 26, 1854

An annular solar eclipse occurred on May 26, 1854. 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.

<span class="mw-page-title-main">Solar eclipse of September 8, 1885</span> Total solar eclipse September 8, 1885

A total solar eclipse occurred on September 8, 1885. 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. The path of totality crossed New Zealand.

<span class="mw-page-title-main">Solar eclipse of January 22, 1898</span> Total solar eclipse January 22, 1898

A total solar eclipse occurred on January 22, 1898. 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. It was visible across central Africa, and into India and Asia.

<span class="mw-page-title-main">Solar eclipse of December 22, 1870</span> Total solar eclipse December 22, 1870

A total solar eclipse occurred on December 22, 1870. 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. Totality was visible from southern Portugal and Spain, across northern Algeria, then crossing Sicily, Greece, Bulgaria, and ending in the south-west of the Russian Empire.

<span class="mw-page-title-main">Solar eclipse of April 25, 1865</span> Total solar eclipse April 25, 1865

A total solar eclipse occurred on April 25, 1865. 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.

<span class="mw-page-title-main">Solar eclipse of August 29, 1867</span> Total solar eclipse August 29, 1867

A total solar eclipse occurred on August 29, 1867. 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. Totality occurred across central Argentina and the southern Atlantic ocean.

<span class="mw-page-title-main">Solar eclipse of December 12, 1871</span> Total solar eclipse December 12, 1871

A total solar eclipse occurred on December 12, 1871. 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.

<span class="mw-page-title-main">Solar eclipse of April 16, 1874</span> Total solar eclipse April 16, 1874

A total solar eclipse occurred on Thursday, April 16, 1874. 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.

<span class="mw-page-title-main">Solar eclipse of February 9, 1766</span> 18th-century total solar eclipse

A total solar eclipse occurred on Sunday, February 9, 1766. 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.

<span class="mw-page-title-main">Solar eclipse of November 30, 1853</span> Total Solar eclipse November 30, 1853

A total solar eclipse occurred on November 30, 1853. 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.

References

  1. 1 2 Marriott, R. A. (June 1991). "Norway 1896: the BAA's first organised eclipse expedition". Journal of the British Astronomical Association. 101 (3): 162–170. Bibcode:1991JBAA..101..162M.
  2. "Expedition for the Observation of the Total Solar Eclipse, August 9th, 1896". Memoirs of the British Astronomical Association. 6: 1–4. 1898. Bibcode:1898MmBAA...6....1.