query: when was the last time there was an eclipse in mexico

pos: Solar eclipse of July 11, 1991 Solar eclipse of July 11, 1991 A total solar eclipse occurred on July 11, 1991. 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 began over the Pacific Ocean and Hawaii moving across Mexico,

pos: Allais effect Allais effect during the solar eclipse of July 11, 1991 in Mexico and the eclipse of November 3, 1994 in Brazil. While he could not observe Allais' claim that there is a diurnal periodicity in the motion of a paraconical pendulum, he did, however, write: "The most interesting result of the Mexico and Brazil experiments is the increase of rotational velocity of the pendulum oscillation plane in the direction of the Foucault effect during the eclipse. It seems that we have some kind of special effect." Various other experiments using atomic clocks and gravimeters instead of pendulums also recorded significant

pos: Solar eclipse of July 11, 1991 down through Central America and across South America ending over Brazil. It lasted for 6 minutes and 53 seconds at the point of maximum eclipse. There will not be a longer total eclipse until June 13, 2132. This eclipse was the most central total eclipse in 800 years, with a gamma of -.0041. There will not be a more central eclipse for another 800 years. Its magnitude was also greater than any eclipse since the 6th century. Photos: Videos: Solar eclipse of July 11, 1991 A total solar eclipse occurred on July 11, 1991. A solar eclipse occurs when the

neg: El Tapado He was arrested at Cuetlaxcoapa (Puebla), accused of being in league with the pirates. From there he was conducted to Mexico City in fetters. In Mexico City, in a place called "Xico", he was taken to the scaffold (July 12, 1684). At the time of his execution, an eclipse of the sun was seen. The common people, who had given the marquis his nickname of "El Tapado" (the "covered-up", or "hidden"), viewed the eclipse as a sign from God that an innocent man was about to be executed. Nevertheless, the authorities continued with the hanging. Afterwards, the head of Benavides

neg: Transit of Venus infrequently. Such an event last occurred on 22 September 373,173 BC and will next occur on 26 July 69,163, and again on 29 March 224,508. The simultaneous occurrence of a solar eclipse and a transit of Venus is currently possible, but very rare. The next solar eclipse occurring during a transit of Venus will be on 5 April 15,232. The last time a solar eclipse occurred during a transit of Venus was on 1 November 15,607 BC. The day after the Venerean transit of 3 June 1769 there was a total solar eclipse, which was visible in Northern America, Europe

neg: Solar eclipse of May 30, 1984 Solar eclipse of May 30, 1984 An annular solar eclipse occurred on May 30, 1984. 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. Annularity was visible in Mexico, the United States,

neg: Solar eclipse of December 24, 1973 Solar eclipse of December 24, 1973 An annular solar eclipse occurred on December 24, 1973. 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. Annularity was visible from southern Mexico, southwestern Nicaragua,

neg: Solar eclipse of May 20, 2012 Solar eclipse of May 20, 2012 The solar eclipse of May 20, 2012 (May 21, 2012 local time in the Eastern Hemisphere) was an annular solar eclipse that was visible in a band spanning through Eastern Asia, the Pacific Ocean, and North America. As a partial solar eclipse, it was visible from northern Greenland to Hawaii, and from eastern Indonesia at sunrise to northwestern Mexico at sunset. The annular eclipse was the first visible from the contiguous United States since the solar eclipse of May 10, 1994, and the first in Asia since the solar eclipse of January 15, 2010.

neg: Eclipse Aviation Eclipse Aviation Eclipse Aviation Corporation was the Albuquerque, New Mexico-based manufacturer of the Eclipse 500 very light jet (VLJ) and also at one time proposed developing the Eclipse 400 single-engined jet. The company was founded in 1998 by early Microsoft employee and former Symantec CEO, Vern Raburn. Due to Raburn's relationship with Microsoft, Bill Gates was a major stake-holder in the Eclipse project. Production of the Eclipse 500 was halted in October 2008 due to lack of funding. The company entered an unsuccessful Chapter 11 bankruptcy in November 2008, which was converted into a Chapter 7 bankruptcy liquidation procedure in

neg: Solar eclipse of May 10, 1994 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), that is there is a ring of the sun around the dark moon. An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The path of annularity crossed four states of Mexico (Baja California Sur, Baja California, Sonora and Chihuahua), the United States, the Canadian provinces of Ontario, Nova Scotia and the southeastern tip of Quebec, Azores Islands except Santa Maria Island,

neg: Eclipse season a particular phase and about 29.5 days), the Moon will be new or full at least two, and up to three, times during the season. Eclipse seasons occur slightly shy of six months apart (successively occurring every 173.31 days - half of an eclipse year), the time it takes the Sun to travel from one node to the next along the ecliptic. If the last eclipse of an eclipse season occurs at the very beginning of a calendar year, it is possible for a total of seven eclipses to occur since there is still time before the end of the

neg: Solar eclipse of October 29, 1837 eclipse was in Antarctica at 61.9 S, 110.5 W at 11:19 UTC (4:19 AM local time). The subsolar marking was west of Angola in Africa. Solar eclipse of October 29, 1837 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

neg: Solar eclipse July 16, 2186, when totality will last 7 min 29 s. For comparison, the longest total eclipse of the 20th century at 7 min 8 s occurred on June 20, 1955, and there are no total solar eclipses over 7 min in duration in the 21st century. If the date and time of any solar eclipse are known, it is possible to predict other eclipses using eclipse cycles. The saros is probably the best known and one of the most accurate. A saros lasts 6,585.3 days (a little over 18 years), which means that, after this period, a practically identical

neg: Solar eclipse of April 7, 1940 (the part now belonging to Kiribati), Mexico and the United States. Solar eclipse of April 7, 1940 An annular solar eclipse occurred on April 7, 1940. 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

neg: Solar eclipse of June 10, 2002 Northern Mariana and the western tip of Jalisco, Mexico. Photos: Solar eclipse of June 10, 2002 An annular solar eclipse occurred on June 10, 2002. 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

neg: Solar eclipse of May 20, 2012 The eclipse continued to travel southeast, passing 30 miles (48 km) north of Las Vegas, Nevada, over St. George, Utah, and reaching the Grand Canyon by approximately 6:35 p.m MST. After passing over Albuquerque, New Mexico and Lubbock, Texas, the eclipse terminated above central Texas at sunset, 8:39 p.m. CST. An estimated 6.6 million people lived under the path of the antumbra. The penumbra was visible throughout most of North America, including the islands of Hawaii. Solar eclipse of May 20, 2012 The solar eclipse of May 20, 2012 (May 21, 2012 local time in the Eastern Hemisphere) was an

neg: Solar eclipse of November 10, 1844 9:51 UTC (7:58 PM local time on November 9). The subsolar marking was in the Great Zimbabwe (now Zimbabwe) in Africa. Solar eclipse of November 10, 1844 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. It was last of four partial eclipses that took place that year,

neg: Solar eclipse of August 16, 1841 of Antarctica at 61.9 S & 158 E at 21:20:24 UTC (8:20 AM local time). The subsolar marking was in the Pacific north of the 10th parallel north. Solar eclipse of August 16, 1841 A partial solar eclipse occurred on August 16, 1841 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. It was last of four

neg: Eclipse Aviation applications to replace halon, a greenhouse gas (GHG). It was developed by Eclipse Aviation for use aboard their Eclipse 500 jets, and is now being marketed to other aviation manufacturers. Eclipse Aviation Eclipse Aviation Corporation was the Albuquerque, New Mexico-based manufacturer of the Eclipse 500 very light jet (VLJ) and also at one time proposed developing the Eclipse 400 single-engined jet. The company was founded in 1998 by early Microsoft employee and former Symantec CEO, Vern Raburn. Due to Raburn's relationship with Microsoft, Bill Gates was a major stake-holder in the Eclipse project. Production of the Eclipse 500 was halted

neg: Solar eclipse of February 21, 1803 the totality was seen in Mexico. Solar eclipse of February 21, 1803 A total solar eclipse occurred on February 21, 1803. 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 eclipse was visible in

neg: HMS Eclipse (1807) at the Cape of Good Hope with 1600 barrels. She returned to Britain on 7 June 1845 with 1500 barrels [incomplete]. The last year for a "Lloyd's Register" listing for "Eclipse" is 1833. In 1834 there is an abbreviated entry for an "Eclipse", of London, of 401 tons (bm). This listing continues until 1838. That is the last mention of the vessel. After 1838, "Lloyd's Register" only carried vessels that had been surveyed. Notes Citations References HMS Eclipse (1807) HMS "Eclipse" was a Royal Navy built by John King at Dover and launched in 1807. She served off Portugal and

neg: Solar eclipse of December 13, 1898 Solar eclipse of December 13, 1898 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. It was the last of three solar eclipses that took place that year, the only one that was partial. It was the last three of solar saros 111, the last two eclipses of

neg: Solar eclipse of June 24, 1778 Solar eclipse of June 24, 1778 A total solar eclipse occurred on June 24, 1778. 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 total eclipse was visible in a path across Mexico, southeastern

neg: Solar eclipse of June 28, 1908 of North America including a part of Central Mexico around Mexico City and Orlando and Daytona Beach, Florida in the USA which occurred in the morning hours. In Africa, it included Rosso, Mauritania, the northernmost part of Senegal, Bamako and the southwestern French Sudan (now Mali), the southwesternmost part of Upper Volta (now Burkina Faso) and northern British Gold Coast (now Ghana) which occurred before sunset. Solar eclipse of June 28, 1908 An annular solar eclipse occurred on June 28, 1908. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the

neg: Solar eclipse special eye protection or indirect viewing techniques are used when viewing a solar eclipse. It is technically safe to view only the total phase of a total solar eclipse with the unaided eye and without protection; however, this is a dangerous practice, as most people are not trained to recognize the phases of an eclipse, which can span over two hours while the total phase can only last a maximum of 7.5 minutes for any one location. People referred to as "eclipse chasers" or "umbraphiles" will travel to remote locations to observe or witness predicted central solar eclipses. There are

neg: Lunar eclipse The Moon's average orbital speed is about , or a little more than its diameter per hour, so totality may last up to nearly 107 minutes. Nevertheless, the total time between the first and the last contacts of the Moon's limb with Earth's shadow is much longer and could last up to four hours. The relative distance of the Moon from Earth at the time of an eclipse can affect the eclipse's duration. In particular, when the Moon is near apogee,the farthest point from Earth in its orbit, its orbital speed is the slowest. The diameter of Earth's umbra does

neg: Solar eclipse of December 2, 1880 Solar eclipse of December 2, 1880 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. It was the last of four eclipses that took place that year, the last two that were partial. It was the last four of solar saros 111, the next eclipses of the cycle

neg: Solar Saros 139 it will produce the longest total eclipse calculated for the ten millennia from 3999 BCE to 6000 CE. The last eclipse to occur was a total eclipse on March 29, 2006, lasting 4 minutes 7 seconds and passing over portions of Africa and western Asia. The next eclipse will occur on April 8, 2024, lasting 4 minutes 28 seconds over central North America, entering in Mexico, crossing the United States, and leaving in eastern Canada. Solar Saros 139 Solar Saros 139 repeats every 18 years, 11 days. Saros 139 contains 71 events of which 16 will be partial eclipses, 12

neg: Eclipse 550 fuselage, empennage and wings, while final aircraft assembly will be carried out by Eclipse Aerospace at their Albuquerque, New Mexico plant. The initial price for the 550 in 2011 was US$2.695M and production was intended at that time to be 50-100 aircraft per year. The aircraft achieved an FAA production certificate in April 2012. In June 2013 the FAA approved the Eclipse 550 for a fatigue limit of 20,000 hours or 20,000 cycles with an unlimited calendar life. In August 2013 it was announced that the aircraft would incorporate autothrottles, new EFIS software, an anti-lock braking system and a high-resolution

neg: Eclipse Aerospace submit bids. Eclipse Aerospace indicated at the time that they intended to retain the company in Albuquerque, provide upgrades to the current Eclipse fleet and assess whether production can be restarted at some future point. Eclipse Aerospace opened for business in the old Eclipse Aviation facilities in Albuquerque, New Mexico on 1 September 2009, with 15 employees and was given the US Eclipse 500 type certificate by the Federal Aviation Administration on 30 September 2009. Prior to Eclipse Aerospace's acquisition of the Eclipse 500 type certificate, the European Aviation Safety Agency (EASA) had suspended the European type certificate, without giving

neg: Solar eclipse of June 28, 1889 and Indian Ocean. This was the 47th solar eclipse of Solar Saros 125. It is a part of solar Saros 125. The last seven annular solar eclipses of Solar Saros 125 without a penumbra southern limit (six after 1889) !August 1, 1943 !August 11, 1961 !August 22, 1979 Solar eclipse of June 28, 1889 An annular solar eclipse occurred on June 28, 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. An annular solar eclipse occurs when the Moon's apparent

neg: Eclipse season calendar year for two full eclipse seasons, each having up to three eclipses. In each sequence below, each eclipse is separated by a fortnight. The first and last eclipse in each sequence is separated by one synodic month. See also "Eclipse cycles". The partial lunar eclipse of August 7-8, 2017 was followed by the solar eclipse of August 21, 2017. Eclipse season An eclipse season is one of only two periods during a year when eclipses can occur, due to the orbital inclination of the Moon. Each season lasts for approximately 35 days and repeats just short of six months,

neg: Eclipse Aviation February 2009. In the final Chapter 7 procedure, completed on August 20, 2009, there was only one bidder, a new company formed to acquire the assets, Eclipse Aerospace. Eclipse operated service centers at Albuquerque International Sunport, Gainesville Regional Airport in Florida, and Albany International Airport in New York. Eclipse Aviation was founded by Vern Raburn in 1998 in Scottsdale, Arizona, and the company started to design the twin-engined Eclipse 500 very light jet. Due to investments by the State of New Mexico and incentives and concessions from the City of Albuquerque, the company decided to set up its production facilities

neg: HMS Eclipse (1807) ("San Blas" may have been San Blas, Nayarit, Mexico.) "Lloyd's List" for 21 September reported that "Eclipse" had been lost on the Tre Maria Islands. She had last been reported "all well" on 15 April going into "San Blas" with 820 barrels of oil. The September report came from her bosun and four crew members who had deserted in one of her boats. However, by 16 November she was reported to be "all well" and heading to San Blas with 820 barrels. Between 17 August and 3 September she was at Honolulu with 200 barrels. "eclipse" returned on 15 February

neg: Solar eclipse of October 29, 1837 Solar eclipse of October 29, 1837 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

neg: Solar eclipse of November 10, 1844 Solar eclipse of November 10, 1844 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. It was last of four partial eclipses that took place that year, two in the space of two months each, the last one was on July 1819 and covered a part of the

neg: Solar eclipse of August 16, 1841 Solar eclipse of August 16, 1841 A partial solar eclipse occurred on August 16, 1841 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. It was last of four partial eclipses that took place that year, two in the space of two months each, the last one was on July 1819 and covered a part of the

neg: Solar eclipse of March 7, 1970 remainder of the southern states. There will not be an eclipse with a greater duration of totality over the contiguous U.S. until April 8, 2024, a period of 54 years. This eclipse slowed a radio transmission of atomic time from North Carolina to Washington, D.C. <BR>Animation of eclipse path (3 minutes per frame) CBS broadcast the first total eclipse in color. "Maps": "News": "Photos and observations" Solar eclipse of March 7, 1970 A total solar eclipse occurred on Saturday, March 7, 1970, visible across most of North America and Central America. A solar eclipse occurs when the Moon passes between

neg: Eclipse Aerospace Eclipse Aerospace Eclipse Aerospace was an American aircraft manufacturer, maintenance and upgrade company. The company provided maintenance and upgrades to the Eclipse 500 fleet and was the manufacturer of the Eclipse 550. The company was formed specifically to purchase the assets of bankrupt Eclipse Aviation, for which it paid US$20M in cash and US$20M in promissory notes in August 2009. In April 2015 the company was merged with Kestrel Aircraft to form One Aviation. Eclipse Aviation, the Albuquerque, New Mexico-based manufacturer of the Eclipse 500 very light jet and the company that was developing the Eclipse 400 single-engine jet, was

neg: Tomás de la Cerda, 3rd Marquis of la Laguna there he was taken to Mexico City in chains. On 12 July 1684 he was conducted to the scaffold, but when he appeared there was an eclipse of the sun. Although the people viewed this as Heaven's displeasure at the execution of an innocent, he was executed anyway. Viceroy's de la Cerda's term was extended three years by king Charles II. On 16 November 1686 he turned over authority to his successor, Melchor Portocarrero, 3rd Count of Monclova. The viceroy and his wife, María Luisa Manrique de Lara y Gonzaga, had a friendly relationship with the great Mexican poet Sor

neg: Solar eclipse of October 19, 1865 included the Cape Verdean Islands of Sotavento and Boa Vista Island, at the time a Portuguese colony. In Africa, it included most of Senegal, at the time a French colony, southern Agawedj (or Agaouedj, now Mauritania) and parts of Mali. In many parts of Brazil except for the south, it was the third consecutive solar eclipse that took place, all of it appeared as partial, the last two were on October 30, 1864 and April 25, 1865, both with an umbral portion in one part. Solar eclipse of October 19, 1865 An annular solar eclipse occurred on October 19, 1865.

neg: Solar eclipse of January 4, 1639 Arctic Circle. It was the first eclipse of solar saros 145 with the moon's penumbra touching the earth for just under 8 minutes, sometimes, it was called a micro-eclipse. The greatest eclipse was in the land of the Samoyeds at 64.6 N and 80 E at 4:56 UTC (9:56 AM local time) at the fourth minute. All of the eclipse occurred at or after sunrise. It was the first of three partial eclipses that took place that year, the last occurred in the Southern Hemisphere on December 5, 1638, the next was on June 1. It was the last solar

neg: Solar eclipse of November 21, 1862 three partial eclipses that took place that year, the last occurred in the same hemisphere on June 27, nearly on the opposite side of the previous eclipse. It was the last three of the solar saros 111, the next was on December 2, 1880 and the last was on January 5, 1935. The eclipse took place in a part of Northern Antarctica (in areas that had a 24-hour daylight at the time) to the area separating the Indian and Pacific Ocean, to the range of 170th meridian east and up to around the 50th meridian east. The eclipse started at

neg: Solar eclipse By the 8th millennium, the longest theoretically possible total eclipse will be less than 7 min 2 s. The last time an eclipse longer than 7 minutes occurred was June 30, 1973 (7 min 3 sec). Observers aboard a Concorde supersonic aircraft were able to stretch totality for this eclipse to about 74 minutes by flying along the path of the Moon's umbra. The next total eclipse exceeding seven minutes in duration will not occur until June 25, 2150. The longest total solar eclipse during the 11,000 year period from 3000 BC to at least 8000 AD will occur on

neg: Solar eclipse of June 30, 1973 was the last total solar eclipse that exceeds 7 minutes in this series. The last total eclipse over 7 minutes was on July 1, 1098 which lasted 7 minutes and 5 seconds. There will not be a longer total solar eclipse until June 25, 2150. The greatest eclipse occurred in the Agadez area in the northwest of Niger not far from Algeria inside the Sahara Desert somewhat 40 km east of the small mountain of Ebenenanoua at 18.8 N and 5.6 E and occurred at 11:38 UTC. The umbral portion of the path started near the border of Guyana and

neg: Solar eclipse of August 6, 1823 Solar eclipse of August 6, 1823 A partial solar eclipse occurred on August 6, 1823 in the midwinter season. 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 eclipse of solar saros 152. It was one of four partial eclipses that took place that year, each two in two months, the last one was on

neg: Solar eclipse of September 10, 1923 in Japan (now in Russia) on September 11, and crossed the Pacific Ocean, southwestern California including the whole Channel Islands, northwestern and northern Mexico, Yucatan Peninsula, British Honduras (today's Belize), Swan Islands, Honduras, and Serranilla Bank and Bajo Nuevo in Colombia on September 10. The eclipse was over 90% in Los Angeles, San Diego and Santa Barbara in the Southern California coast. Solar eclipse of September 10, 1923 A total solar eclipse occurred on September 10, 1923. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun

neg: Solar eclipse of November 20, 1873 Solar eclipse of November 20, 1873 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. It was the last of two all partial eclipses that took place that year. It was part of solar saros 150. The next eclipse was on April 16, 1874 in the same hemisphere,

neg: Solar eclipse of January 5, 1935 Solar eclipse of January 5, 1935 A partial solar eclipse occurred on January 5, 1935 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. It was one of five eclipses that took place that year, the next one was in the Northern Hemisphere on February 3 and covered much of North America. It was the last eclipse

neg: Solar eclipse of March 30, 2052 Solar eclipse of March 30, 2052 A total solar eclipse will occur on March 30, 2052. 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 will cross central Mexico and the

neg: Solar eclipse of March 25, 1857 the Pacific ocean, and ended near sunset across Mexico on March 25. Solar eclipse of March 25, 1857 A total solar eclipse occurred on March 25, 1857. 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

neg: Solar eclipse of March 13, 1812 Solar eclipse of March 13, 1812 A partial solar eclipse occurred on March 13, 1812. 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 one of four partial eclipses that took place that year, each two in two months, the last one was on February 12 and covered a part of the Northern Hemisphere. The next eclipse

neg: Eclipse the resulting shadow will sweep through a region of space, only passing through any particular location in the region for a fixed interval of time. As viewed from such a location, this shadowing event is known as an eclipse. Typically the cross-section of the objects involved in an astronomical eclipse are roughly disk shaped. The region of an object's shadow during an eclipse is divided into three parts: A total eclipse occurs when the observer is within the umbra, an annular eclipse when the observer is within the antumbra, and a partial eclipse when the observer is within the penumbra.

neg: Eclipse crosses the line of sight to the Sun at two points along Saturn's orbit. As the orbital period of Saturn is 29.7 years, an eclipse is only possible about every 15 years. The timing of the Jovian satellite eclipses was also used to calculate an observer's longitude upon the Earth. By knowing the expected time when an eclipse would be observed at a standard longitude (such as Greenwich), the time difference could be computed by accurately observing the local time of the eclipse. The time difference gives the longitude of the observer because every hour of difference corresponded to 15°

neg: Solar eclipse of January 22, 1841 the Northern Hemisphere. It was the last two of solar saros 109, the last one was on February 3, 1859. The eclipse was visible in the a part of northern Antarctica which had a 24-hour daylight that time and a part of the southwesternmost portion of the Indian Ocean and a very tiny part of the Atlantic. The edge of the eclipse included the area dividing the Indian and the Atlantic oceans. It showed about up to nearly 10% obscurity in Antarctica. The greatest eclipse was nearly about 30% of the way between Antarctica and the southernmost of Africa at

neg: Solar eclipse of July 9, 1888 Solar eclipse of July 9, 1888 A partial solar eclipse occurred on July 9, 1888 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. It was the second of three partial eclipses that took place that year, the last was on February 11 and the next was on August 7 in the Northern Hemisphere It was the

neg: Eclipse cycle of the two nodes of its orbit on the ecliptic at the time of the syzygy. Of course, to produce an eclipse, the Sun must also be near a node at that time: the same node for a solar eclipse, or the opposite node for a lunar eclipse. Up to three eclipses may occur during an eclipse season, a one- or two-month period that happens twice a year, around the time when the Sun is near the nodes of the Moon's orbit. An eclipse does not occur every month, because one month after an eclipse the relative geometry of the

neg: Ibrahim ibn Muhammad a solar eclipse (probably the annular eclipse which occurred in the early morning of 27 January 632, equivalent with the last or the penultimate day of Shawwal, 10 AH), Ibrahim died at the age of 16, 18 or 21 months. This may have been at the time of another solar eclipse, which occurred on the afternoon of 3 August 631 (29 Rabi'Akhir 10 AH). However, according to modern astronomical calculations this eclipse was not visible from Mecca or Medina. Tabari says Ibrahim died at the age of 21 months. If Ibrahim was born in the last month of 8 AH,

neg: Solar eclipse of April 3, 1848 Solar eclipse of April 3, 1848 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

neg: Solar eclipse of August 18, 1830 Solar eclipse of August 18, 1830 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. It was one of four partial eclipses that took place that year, each two in two months, the last one was on March 30 in the same hemisphere, the next one was on

neg: Solar eclipse of August 7, 1812 Solar eclipse of August 7, 1812 A partial solar eclipse occurred on August 7, 1812 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. It was one of four partial eclipses that took place that year, each two in two months, the last one was on March 13 in the same hemisphere, the next one was on

neg: Eclipse Park third and last Eclipse Park was located at the corner of 7th and Kentucky streets in the Limerick neighborhood of Louisville. This ballpark was built by George "White Wings" Tebeau as the home for the American Association minor league Louisville Colonels who played there from 1902 through 1922. All three Eclipse Park locations were destroyed by fire. Eclipse Park Eclipse Park was the name of three successive baseball grounds in Louisville, Kentucky in the late 19th and early 20th centuries. They were the home of the Louisville baseball team first known as the Louisville Eclipse and later as the Louisville

neg: Solar eclipse of December 13, 1898 km above the area (66.8 S) south of the Antarctic Circle. Solar eclipse of December 13, 1898 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. It was the last of three solar eclipses that took place that year, the only one that was partial. It was the

neg: February 2009 lunar eclipse (a half saros). This lunar eclipse is related to two partial solar eclipses of Solar Saros 150. February 2009 lunar eclipse A penumbral lunar eclipse took place on February 9, 2009, the first of four lunar eclipses in 2009, and being the deepest of three penumbral eclipses. It also happened on the Lantern Festival, the first since February 20, 1989. The eclipse was not visible in the East coast of the United States, South America and southernmost Mexico, Western Africa and western Europe. Best visibility was expected over most of Asia, the Western US, Mexico and throughout the Pacific region.

neg: February 2009 lunar eclipse February 2009 lunar eclipse A penumbral lunar eclipse took place on February 9, 2009, the first of four lunar eclipses in 2009, and being the deepest of three penumbral eclipses. It also happened on the Lantern Festival, the first since February 20, 1989. The eclipse was not visible in the East coast of the United States, South America and southernmost Mexico, Western Africa and western Europe. Best visibility was expected over most of Asia, the Western US, Mexico and throughout the Pacific region. A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days

neg: Solar eclipse of March 7, 1970 was visible across southern Mexico and the Gulf of Mexico, the southeast Atlantic coast of the United States, northeast to the Maritimes of eastern Canada, and northern Miquelon-Langlade in the French overseas collectivity of Saint Pierre and Miquelon. Greatest eclipse occurred over Mexico at 11:38 am CST, with totality lasting 3 minutes and 28 seconds. Totality over the U.S. lasted up to 3 minutes and 10 seconds. The media declared Perry as the first municipality in Florida to be in the eclipse direct path. Inclement weather obstructed the viewing from that location and most of the eclipse path through the

neg: Solar eclipse of March 29, 2006 Zealand pay TV company, failed the day after this eclipse at around 1900 local time. While SKY didn't directly attribute the failure to the eclipse, they said in a media release that it took longer to resolve the issue because of it, but this claim was refuted by astronomers. The main reason for the failure was because of an aging and increasingly faulty satellite. This solar eclipse was preceded by the penumbral lunar eclipse on March 14, 2006. Photos: Solar eclipse of March 29, 2006 A total solar eclipse occurred on March 28–29, 2006. A solar eclipse occurs when the

neg: December 2009 lunar eclipse December 2009 lunar eclipse A partial lunar eclipse was visible on New Year's Eve, December 31, 2009. It was the last and largest of four minor lunar eclipses in 2009. This lunar eclipse is also notable, because it occurred during a blue moon (a second full moon in December). The next eclipse on New Year's Eve and blue moon will occur on December 31, 2028. Only a small portion of the Moon entered the Earth's umbral shadow, but there was a distinct darkening visible over the Moon's southern surface at greatest eclipse. It was visible from all of Africa, Europe,

neg: Solar eclipse of November 25, 2011 of the Sun. This was the last of four partial solar eclipses in 2011, with the others occurring on January 4, 2011, June 1, 2011, and July 1, 2011. <BR>Animated path It proceeded the total lunar eclipse which occurred on December 10, 2011. Solar eclipse of November 25, 2011 A partial solar eclipse occurred on November 25, 2011. 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

neg: June 2011 lunar eclipse June 2011 lunar eclipse A total lunar eclipse took place on June 15, 2011. It was the first of two such eclipses in 2011. The second occurred on December 10, 2011. This was a relatively rare central lunar eclipse, in which the center point of Earth's shadow passes across the moon. The last time a lunar eclipse was closer to the center of the earth's shadow was on July 16, 2000. The next central total lunar eclipse was on July 27, 2018 over South America, western Africa, and Europe, and setting over eastern Asia. In western Asia, Australia, and the

neg: Solar eclipse of January 21, 1852 Solar eclipse of January 21, 1852 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. It was first of three partial eclipses that took place that year within the space of nearly six months, the last one was on June 1852 in the same hemisphere with a very

neg: Solar eclipse of October 19, 1819 Solar eclipse of October 19, 1819 A partial solar eclipse occurred on October 19, 1819 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 one of four partial eclipses that took place that year, each two in two months, the last one was on September 19 and covered a part of the Northern Hemisphere. The

neg: December 2009 lunar eclipse lunar eclipse is related to two partial solar eclipses of Solar Saros 122. December 2009 lunar eclipse A partial lunar eclipse was visible on New Year's Eve, December 31, 2009. It was the last and largest of four minor lunar eclipses in 2009. This lunar eclipse is also notable, because it occurred during a blue moon (a second full moon in December). The next eclipse on New Year's Eve and blue moon will occur on December 31, 2028. Only a small portion of the Moon entered the Earth's umbral shadow, but there was a distinct darkening visible over the Moon's

neg: Solar eclipse of August 28, 1848 occurred in a smaller part of the same area where the previous solar eclipse happened which was on April 3, the next one was on September 27 and covered a part of the Northern Hemisphere This minor eclipse was visible offshore from the peninsular Antarctica along with its islands and the Trans-Antarctic Mountains. It was the last eclipse of solar saros 113 with the moon's penumbra touching the earth for just about 30 minutes. The greatest eclipse was at 19:18:22 UTC (8:18:22 local time) just south of the 70th parallel. Solar eclipse of August 28, 1848 A very small partial

neg: American Eclipse (horse) Walter who lost. At this point, a match race was organized between American Eclipse and James J. Harrison’s noted horse Sir Charles. Sir Charles, with 20 wins to his credit, injured himself in a workout, and Harrison was required to forfeit the match, which American Eclipse won. A second match was arranged only a single heat, and this time Sir Charles raced but broke down, leaving American Eclipse an easy winner. When American Eclipse was nine years old, another challenge was issued with the intent to race five top horses against American Eclipse, who would represent the North. The race

neg: August 2008 lunar eclipse it when it is visible. The penumbral eclipse began at 18:23 UTC, with the partial eclipse beginning at 19:36. The time of greatest eclipse was 21:10. The partial eclipse ended at 22:44, and the penumbral eclipse will ended at 23:57. The planet Neptune was 2 days past opposition, visible in binoculars as an 8th magnitude "star" just two degrees west and slightly south of the moon. A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two total solar eclipses of Solar Saros 145.

neg: Solar eclipse of January 5, 2038 Solar eclipse of January 5, 2038 An annular solar eclipse will occur on January 5, 2038. 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. <BR>Animated path There are 7 eclipses in

neg: One Aviation their current locations: Albuquerque, New Mexico and Chicago, Illinois for the Eclipse, and Superior, Wisconsin and Brunswick, Maine for the Kestrel. The merger of Eclipse and Kestrel to form the new company was announced on 15 April 2015 at the AERO Friedrichshafen aviation trade show. In 2016, One Aviation announced that it was devoting its resources to developing an improved version of the Eclipse 550, the Eclipse 700. The company suspended the Kestrel K-350 project and in March 2017 announced that it would phase out Eclipse 550 production, to concentrate on the EA700. The first testbed for the aircraft's new

neg: Lunar eclipse of the first of the eclipses in this sequence on April 15, 2014. At least two lunar eclipses and as many as five occur every year, although total lunar eclipses are significantly less common. If the date and time of an eclipse is known, the occurrences of upcoming eclipses are predictable using an eclipse cycle, like the saros. Eclipses occur only during an eclipse season, when the Sun appears to pass near either node of the Moon's orbit. Lunar eclipse A lunar eclipse occurs when the Moon passes directly behind Earth and into its shadow. This can occur only when

neg: November 1947 lunar eclipse Last Central Lunar Eclipse: 2488 Oct 20 Last Total Lunar Eclipse: 2651 Jan 28 Last Partial Lunar Eclipse: 2867 Jun 08 Last Penumbral Lunar Eclipse: 3011 Sep 04 November 1947 lunar eclipse A penumbral lunar eclipse took place on November 28, 1947. It was completely visible over Asia, Australia, Pacific, Arctic, and the Americas. It was rising over Asia and Australia and setting over the Americas. Lunar Saros series 144, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 20 total lunar eclipses. First Penumbral Lunar Eclipse: 1749 Jul 29 First Partial Lunar

neg: Solar eclipse which event the planet will be visible very near the eclipsed Sun, when without the eclipse it would have been lost in the Sun's glare. At one time, some scientists hypothesized that there may be a planet (often given the name Vulcan) even closer to the Sun than Mercury; the only way to confirm its existence would have been to observe it in transit or during a total solar eclipse. No such planet was ever found, and general relativity has since explained the observations that led astronomers to suggest that Vulcan might exist. During a total solar eclipse, the Moon's

neg: Solar eclipse of September 16, 1792 ended at sunset in Borneo, Java and the coast of western Australia. The subsolar marking was in Abyssinia (now in Kenya). In parts of the world, the eclipse was not seen in some areas in areas that had monsoon rains mainly within the rim areas. Weather conditions in some areas during the eclipse was unknown. The weather conditions for a part of western Europe including France was mainly cloudy and rainy. At the time, France was experiencing the French Revolution. Solar eclipse of September 16, 1792 An annular solar eclipse occurred on September 16, 1792. A solar eclipse occurs when

neg: Solar eclipse of July 2, 2038 Solar eclipse of July 2, 2038 An annular solar eclipse will occur on July 2, 2038. 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. <BR>Animated path There are a 7 eclipses

neg: Solar eclipse of November 21, 1881 in the Antarctic Peninsula at 81.2 S, 114.5 W at 16:31 UTC (9:31 AM local time). Solar eclipse of November 21, 1881 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

neg: Rubén Espinosa Rubén Espinosa Rubén Manuel Espinosa Becerril (29 November 1983 – 31 July 2015) was a Mexican self-taught photographer and journalist. He worked for AVC News agency and "Proceso" and "Cuartoscuro" magazines. He covered daily news and social protests. He documented several protests where individuals were assaulted. Espinosa was killed in Narvate, Mexico City, Mexico along with four women. Espinosa was born in Mexico City, Mexico. For the majority of his career, Espinosa concentrated on social movements and protests. As a self-taught photographer and journalist, he began his career with Eclipse Photo in Mexico City, Mexico. While with Eclipse Photo, his

neg: Eclipse cycle is obtained by taking the integer part and adding 2. For instance, the eclipse in saros series zero and inex series zero was in the middle of 2884 BC. Eclipse cycle Eclipses may occur repeatedly, separated by certain intervals of time: these intervals are called eclipse cycles. The series of eclipses separated by a repeat of one of these intervals is called an eclipse series. Eclipses may occur when the Earth and the Moon are aligned with the Sun, and the shadow of one body cast by the Sun falls on the other. So at new moon, when the Moon

neg: Solar eclipse of December 25, 1935 the maximum possible. The next time this will occur is 2206. Solar eclipse of December 25, 1935 An annular solar eclipse occurred on December 25, 1935. 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

neg: HMS Eclipse (1807) her on 31 August 1831. "Lloyd's Register" for 1816 shows an "Eclipse", Dover-built, nine years old, and 391 tons (bm). This vessel continued in commercial service for a number of years. She appears to have traded with India until 1823 when William and Daniel Bennett purchased her for use as a whaler. From 1823 on "Eclipse" made seven voyages as a whaler, the last one ending in June 1846. On her first whaling voyage, "Eclipse", Duncan, master, left on 11 April 1823 bound for the Brazil Banks. She was reported to be whaling at San Blas on 6 August 1824.

neg: DayJet indicated that he was still attempting to raise capital to restart the company and that it would be a smaller, scaled back operation. He also stated at that time that there were a number of problems that caused the company to cease operations, but that the key issue was the credit crisis. In analyzing DayJet's situation Iacobucci said that problems with Eclipse had contributed, but that the Eclipse 500 was the best choice for DayJet when it was starting up due to its purchase price and projected maintenance costs. Using the Eclipse 500 also permitted DayJet to start with a

neg: Solar eclipse total, annular, or hybrid eclipse. This is, however, not completely correct: the definition of a central eclipse is an eclipse during which the central line of the umbra touches the Earth's surface. It is possible, though extremely rare, that part of the umbra intersects with the Earth (thus creating an annular or total eclipse), but not its central line. This is then called a non-central total or annular eclipse. The last (umbral yet) non-central solar eclipse was on April 29, 2014. This was an annular eclipse. The next non-central total solar eclipse will be on April 9, 2043. The phases

neg: Solar eclipse of May 6, 1883 no major landfall. Partiality was visible from far eastern Australia at sunrise, and New Zealand, as well as western South America and southern Mexico near sunset. This eclipse is a member of Solar Saros 136, and its maximum duration was 5 minutes and 58 seconds. An expedition of American astronomers traveled from Peru to Caroline Island aboard the to observe the total solar eclipse. A French expedition also observed the eclipse from Caroline, and the United States Navy mapped the atoll. Johann Palisa, a member of the expedition, discovered an asteroid later that year which he named Carolina "in remembrance

neg: Eclipse season every new moon, and all solar eclipses would be the same type. An eclipse season is the only time during which the Sun (from the perspective of the Earth) is close enough to one of the Moon's nodes to allow for an eclipse to occur. During the season, whenever there is a full moon a lunar eclipse will occur and whenever there is a new moon a solar eclipse will occur. If the Sun is close enough to a node, then a total eclipse will occur. Each season lasts from 31 to 37 days, recurring about every 6 months. At

neg: History of Eclipse Aviation understandably, distance themselves from." Eclipse Aviation Corporation was founded in 1998 by Microsoft employee #18 Vern Raburn. Due to Raburn's relationship with Microsoft, Bill Gates became a major stakeholder early in the Eclipse project. Raburn and his team initially based the company in Scottsdale, Arizona, formed a Board of Directors in 1999 and started design work on the first aircraft. Due to investments made by the State of New Mexico and incentives and concessions from the City of Albuquerque, the company decided to set up its production facilities in Albuquerque, and also moved its headquarters there in 2000. In addition

neg: History of Eclipse Aviation told that they would not be paid for the past two weeks' work. Billson informed the employees that the problem was in obtaining financing from Europe and that employees should go home and await further notice. Employees "expressed anger, frustration and uncertainty before speeding out of the facility's parking lot." State of New Mexico Economic Development Secretary Fred Mondragon said that there were indications that the banks had frozen the assets of Eclipse Aviation, saying "I understand the banks put a squeeze on the company, freezing their cash assets. The news is not good." The Eclipse service facility in Gainesville,

neg: June 1983 lunar eclipse June 1983 lunar eclipse A partial lunar eclipse took place on June 25, 1983. It was completely visible over Australia, Pacific and the Americas. Lunar Saros series 139, repeating every 18 years and 11 days, has a total of 79 lunar eclipse events including 27 total lunar eclipses. First Penumbral Lunar Eclipse: 1658 Dec 09 First Partial Lunar Eclipse: 1947 Jun 03 First Total Lunar Eclipse: 2073 Aug 17 First Central Lunar Eclipse: 2109 Sep 09 Greatest Eclipse of Lunar Saros 139: 2199 Nov 02 Last Central Lunar Eclipse: 2488 Apr 26 Last Total Lunar Eclipse: 2542 May 30 Last

neg: Solar eclipse of January 22, 1879 22 January 1879, approximately 1700 British soldiers were annihilated by Zulu warriors during the Zulu War in South Africa. At 2:29 PM there was a solar eclipse, and according to legend, this motivated the Zulus, who claimed that it was a sign that they would prevail. The conflict was named the Battle of Isandlwana, the Zulu name for the battle translates as "the day of the dead moon". Solar eclipse of January 22, 1879 An annular solar eclipse occurred on January 22, 1879. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly

neg: Eclipse 550 Eclipse 550 The Eclipse 550 is a very light jet initially built by Eclipse Aerospace and later One Aviation of Albuquerque, New Mexico, United States. The aircraft is a development version of the Eclipse 500, which was produced by predecessor Eclipse Aviation. Like the 500, the 550 is a low-wing, six seat, twin engine jet-powered aircraft. The Eclipse 550 is certified for single-pilot operation. The aircraft was announced at the National Business Aviation Association convention in Las Vegas, Nevada in October 2011. The first example was rolled out in March 2013 and the first customer delivery was on 22 October

neg: Eclipse Cassini probe observed in 2006. Lunar eclipses occur when the Moon passes through the Earth's shadow. This happens only during a full moon, when the Moon is on the far side of the Earth from the Sun. Unlike a solar eclipse, an eclipse of the Moon can be observed from nearly an entire hemisphere. For this reason it is much more common to observe a lunar eclipse from a given location. A lunar eclipse lasts longer, taking several hours to complete, with totality itself usually averaging anywhere from about 30 minutes to over an hour. There are three types of

neg: May 2023 lunar eclipse Total Lunar Eclipse: 2167 Aug 01 First Central Lunar Eclipse: 2221 Sep 02 Greatest Eclipse of the Lunar Saros 141: 2293 Oct 16 Last Central Lunar Eclipse: 2546 Mar 18 Last Total Lunar Eclipse: 2618 May 01 Last Partial Lunar Eclipse: 2744 Jul 16 Last Penumbral Lunar Eclipse: 2888 Oct 11 1901-2100 March 1915 lunar eclipse March 1933 lunar eclipse March 1951 lunar eclipse April 1969 lunar eclipse April 1987 lunar eclipse April 2005 lunar eclipse May 2023 lunar eclipse May 2041 lunar eclipse May 2059 lunar eclipse June 2077 lunar eclipse June 2095 lunar eclipse This eclipse is the

neg: April 2005 lunar eclipse Total Lunar Eclipse: 2167 Aug 01 First Central Lunar Eclipse: 2221 Sep 02 Greatest Eclipse of the Lunar Saros 141: 2293 Oct 16 Last Central Lunar Eclipse: 2546 Mar 18 Last Total Lunar Eclipse: 2618 May 01 Last Partial Lunar Eclipse: 2744 Jul 16 Last Penumbral Lunar Eclipse: 2888 Oct 11 1901-2100 March 1915 lunar eclipse March 1933 lunar eclipse March 1951 lunar eclipse April 1969 lunar eclipse April 1987 lunar eclipse April 2005 lunar eclipse May 2023 lunar eclipse May 2041 lunar eclipse May 2059 lunar eclipse June 2077 lunar eclipse June 2095 lunar eclipse This eclipse is the