Solar eclipse of April 3, 1848 | |
---|---|
Type of eclipse | |
Nature | Partial |
Gamma | -1.2264 |
Magnitude | 0.5834 |
Maximum eclipse | |
Coordinates | 71°48′S89°00′W / 71.8°S 89°W |
Times (UTC) | |
Greatest eclipse | 22:49:07 |
References | |
Saros | 146 (18 of 76) |
Catalog # (SE5000) | 9158 |
A partial solar eclipse occurred on April 3, 1848, during fall. 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 second of four partial eclipses that took place that year, each two in two months, the last one was on March 5 in the Northern Hemisphere, the next one was in a smaller portion of the same location on August 28, 1848. [1] It was a solar saros 146 cycle [2]
The eclipse was visible in the Pacific Ocean and included the northeast and northwestern Antarctica especially a part of the west of the Antarctic Peninsula.
The eclipse started at sunrise offshore from Antarctica where the Indian and the Pacific Ocean divide and ended at sunset in the peninsula and offshore from Chile.
It showed about up to 15-30% obscuration in northern Antarctica within the 180th meridian, and from 48% to 58% obscuration in the peninsular portion.
10% obscurity in northern Antarctica and 20% at the Antarctic peninsula. The greatest eclipse was at the Antarctic Peninsula at 71.8 S, 89 W at 22:49 UTC (4:49 PM local time). [1]
The subsolar marking was north of the 5th parallel north in the Pacific around the Palmyra Atoll.
A partial solar eclipse occurred on March 14, 1801 just days before autumn. 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.
A very small partial solar eclipse occurred on August 28, 1848, during late winter. 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. This was the 71st and final solar eclipse from Solar Saros 113.
A partial solar eclipse occurred on August 18, 1830, during winter. 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.
A partial solar eclipse occurred on March 25, 1819 in the first days of fall. 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.
A partial solar eclipse occurred on April 5, 1837, during fall. 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.
A partial solar eclipse occurred on February 3, 1859 during summer. 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.
A partial solar eclipse occurred on October 31, 1826 during spring, also known as the 1826 Halloween 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A annular solar eclipse occurred on January 11, 1842 during summer. 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.
A partial solar eclipse occurred on January 21, 1852 during summer. 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.
An annular solar eclipse occurred on January 23, 1860 during summer. 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.
A partial solar eclipse occurred on November 21, 1862 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. As is shown under 6% obscuration, the center of the Moon's shadow was missed by about 2,670 km above the area south of the Antarctic Circle.
A partial solar eclipse occurred on November 10, 1844 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.
A partial solar eclipse occurred on January 31, 1870 during summer. 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.
A partial solar eclipse occurred on November 20, 1873 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.
A partial solar eclipse occurred on December 2, 1880, 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.
An annular solar eclipse occurred on November 21, 1881 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. 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.
A partial solar eclipse occurred on December 13, 1898, before summer. 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.
A partial solar eclipse occurred on February 11, 1888, during summer. 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.
A partial solar eclipse occurred on December 1, 1891, during late 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.
An annular solar eclipse occurred on December 3, 1899, during late 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. 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.