An annular
solar eclipse
A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of Earth, totally or partially. Such an alignment occurs approximately every six months, during the eclipse season i ...
occurred at the Moon's
ascending node
An orbital node is either of the two points where an orbit intersects a plane of reference to which it is inclined. A non-inclined orbit, which is contained in the reference plane, has no nodes.
Planes of reference
Common planes of referenc ...
of orbit on Sunday, August 1, 1943, with a
magnitude
Magnitude may refer to:
Mathematics
*Euclidean vector, a quantity defined by both its magnitude and its direction
*Magnitude (mathematics), the relative size of an object
*Norm (mathematics), a term for the size or length of a vector
*Order of ...
of 0.9409. A
solar eclipse
A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of Earth, totally or partially. Such an alignment occurs approximately every six months, during the eclipse season i ...
occurs when the
Moon
The Moon is Earth's only natural satellite. It Orbit of the Moon, orbits around Earth at Lunar distance, an average distance of (; about 30 times Earth diameter, Earth's diameter). The Moon rotation, rotates, with a rotation period (lunar ...
passes between
Earth
Earth is the third planet from the Sun and the only astronomical object known to Planetary habitability, harbor life. This is enabled by Earth being an ocean world, the only one in the Solar System sustaining liquid surface water. Almost all ...
and the
Sun
The Sun is the star at the centre of the Solar System. It is a massive, nearly perfect sphere of hot plasma, heated to incandescence by nuclear fusion reactions in its core, radiating the energy from its surface mainly as visible light a ...
, 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. Occurring about 25 minutes before
apogee
An apsis (; ) is the farthest or nearest point in the orbit of a planetary body about its primary body. The line of apsides (also called apse line, or major axis of the orbit) is the line connecting the two extreme values.
Apsides perta ...
(on August 1, 1943, at 4:40 UTC), the Moon's apparent diameter was near its minimum. Apogee did occur as the eclipse was just before its greatest eclipse.
Annularity was visible in the southern
Indian Ocean
The Indian Ocean is the third-largest of the world's five oceanic divisions, covering or approximately 20% of the water area of Earth#Surface, Earth's surface. It is bounded by Asia to the north, Africa to the west and Australia (continent), ...
, with the only land being
ÃŽle Amsterdam
(), also known as Amsterdam Island or New Amsterdam (), is an island of the French Southern and Antarctic Lands in the southern Indian Ocean that together with neighbouring ÃŽle Saint-Paul to the south forms one of the five districts of the t ...
in
French Madagascar
The Colony of Madagascar and Dependencies () was a French colony off the coast of Southeast Africa between 1897 and 1958 in what is now Madagascar. The colony was formerly a protectorate of France known as Malagasy Protectorate. The protecto ...
(now belonging to
French Southern and Antarctic Lands
The French Southern and Antarctic Lands (, TAAF) is an overseas territory ( or ) of France. It consists of:
* Adélie Land (), the French claim on the continent of Antarctica.
* Crozet Islands (), a group in the southern Indian Ocean, south ...
). A partial solar eclipse was visible from
Australia
Australia, officially the Commonwealth of Australia, is a country comprising mainland Australia, the mainland of the Australia (continent), Australian continent, the island of Tasmania and list of islands of Australia, numerous smaller isl ...
,
Indonesia
Indonesia, officially the Republic of Indonesia, is a country in Southeast Asia and Oceania, between the Indian Ocean, Indian and Pacific Ocean, Pacific oceans. Comprising over List of islands of Indonesia, 17,000 islands, including Sumatra, ...
,
Malaysia
Malaysia is a country in Southeast Asia. Featuring the Tanjung Piai, southernmost point of continental Eurasia, it is a federation, federal constitutional monarchy consisting of States and federal territories of Malaysia, 13 states and thre ...
, eastern
Madagascar
Madagascar, officially the Republic of Madagascar, is an island country that includes the island of Madagascar and numerous smaller peripheral islands. Lying off the southeastern coast of Africa, it is the world's List of islands by area, f ...
,
Antarctica
Antarctica () is Earth's southernmost and least-populated continent. Situated almost entirely south of the Antarctic Circle and surrounded by the Southern Ocean (also known as the Antarctic Ocean), it contains the geographic South Pole. ...
's
Wilkes Land.
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.
Eclipse season
This eclipse is part of an
eclipse season
An eclipse season is a period, roughly every six months, when eclipses occur. Eclipse seasons are the result of the axial parallelism of the Orbit of the Moon, Moon's orbital plane (orbital inclination, tilted five degrees to the ecliptic, Earth ...
, 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
A fortnight is a unit of time equal to 14 days (two weeks). The word derives from the Old English term , meaning "" (or "fourteen days", since the Anglo-Saxons counted by nights).
Astronomy and tides
In astronomy, a ''lunar fortnight'' is hal ...
.
Related eclipses
Eclipses in 1943
*
A total solar eclipse on February 4.
*
A partial lunar eclipse on February 20.
* An annular solar eclipse on August 1.
*
A partial lunar eclipse on August 15.
Metonic
* Preceded by:
Solar eclipse of October 12, 1939
* Followed by:
Solar eclipse of May 20, 1947
Tzolkinex
* Preceded by:
Solar eclipse of June 19, 1936
file:1936 uludag.jpg, left, Astronomers in Turkey observing the 1936 eclipse
A total solar eclipse occurred at the Moon's Lunar node, descending node of orbit on Friday, June 19, 1936, with a Magnitude of eclipse, magnitude of 1.0329. A solar ecl ...
* Followed by:
Solar eclipse of September 12, 1950
A total solar eclipse occurred at the Moon's Lunar node, descending node of orbit between Monday, September 11, 1950 and Tuesday, September 12, 1950, with a Magnitude of eclipse, magnitude of 1.0182. A solar eclipse occurs when the Moon passes bet ...
Half-Saros
* Preceded by:
Lunar eclipse of July 26, 1934
* Followed by:
Lunar eclipse of August 5, 1952
Tritos
* Preceded by:
Solar eclipse of August 31, 1932
* Followed by:
Solar eclipse of June 30, 1954
Solar Saros 125
* Preceded by:
Solar eclipse of July 20, 1925
* Followed by:
Solar eclipse of August 11, 1961
Inex
* Preceded by:
Solar eclipse of August 21, 1914
* Followed by:
Solar eclipse of July 10, 1972
Triad
* Preceded by:
Solar eclipse of September 29, 1856
* Followed by:
Solar eclipse of June 1, 2030
Solar eclipses of 1942–1946
Saros 125
Metonic series
Tritos series
Inex series
Notes
References
{{Solar eclipses
1943 8 1
1943 in science
1943 8 1
August 1943