| 词条 | Solar eclipse of October 29, 1837 |
| 释义 |
A partial solar eclipse occurred on October 29, 1837 during spring. 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. It was the last of three partial eclipses that took place that year, the first of two in two months, the last was on May 4 which covered a part of the Northern Hemisphere.[1] It was part of solar saros 150.[2] DescriptionThe eclipse was visible in much of Antarctica with the exception of most of the northern and northeastern parts, it included most of southern South America, the South Zetland Islands and the South Orkney Islands. The edge of the eclipse included Paraguay (parts are now in Argentina) and southern Brazil. The eclipse started at sunrise in Chile south of Antofagasta and finished at sunset in Antarctica. It showed about up to 10% obscurity in the South Pole area and in Uruguay, 20 to 35% at the Antarctic Peninsula and Patagonia. The greatest eclipse was in Antarctica at 61.9 S, 110.5 W at 11:19 UTC (4:19 AM local time).[1] The subsolar marking was west of Angola in Africa. See also
References1. ^1 {{cite web|title=Solar eclipse of October 29, 1837|url=http://eclipse.gsfc.nasa.gov/5MCSEmap/1801-1900/1837-10-29.gif|publisher=NASA|accessdate=March 13, 2017}} 2. ^{{cite web|url=http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros150.html|title=Solar Saros 150|publisher=NASA|accessdate=March 13, 2017}} External links
2 : 1837 in science|19th-century solar eclipses |
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