Solar eclipse of 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.
Solar eclipse of August 29, 1867 | |
---|---|
![]() Map | |
Type of eclipse | |
Nature | Total |
Gamma | −0.794 |
Magnitude | 1.0344 |
Maximum eclipse | |
Duration | 171 sec (2 m 51 s) |
Coordinates | 41.1°S 34.9°W |
Max. width of band | 189 km (117 mi) |
Times (UTC) | |
Greatest eclipse | 13:13:07 |
References | |
Saros | 123 (45 of 70) |
Catalog # (SE5000) | 9205 |
Observations
José J. Vergara and Luis Grosch observed the eclipse from a small hill close to Santiago.[1]
Related eclipses
It is a part of solar Saros 123.
References
- L. Grosch (1869). "Beobachtung der Sonnenfinsterniss am 29. August 1867". Astronomische Nachrichten. 73 (9): 137–138. Bibcode:1869AN.....73..137G. doi:10.1002/asna.18690730903.
- NASA chart graphics
- Mabel Loomis Todd (1900). Total Eclipses of the Sun. Little, Brown.

Wikimedia Commons has media related to Solar eclipse of 1867 August 29.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.