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Solar eclipse

Photo taken during the French 1999 eclipse

A solar eclipse occurs when the Moon passes in front of the Sun and obscures it totally or partially. This configuration can only occur at New Moon, when the Sun and Moon are in conjunction, as seen from Earth. A total solar eclipse is considered by many to be the most spectacular natural phenomenon that one can observe.

Types of solar eclipses

There are four types of solar eclipses:

  • A total eclipse occurs when the Sun is completely obscured by the Moon. The intensely bright disk of the Sun is replaced by the dark outline of the Moon, and the much fainter corona is visible (see image right). During any one eclipse, a total eclipse is visible only from a fairly narrow track on the surface of the Earth.
  • An annular eclipse occurs when the Sun and Moon are exactly in line, but the apparent size of the Moon is smaller than that of the Sun. Hence the Sun appears as a very bright ring surrounding the outline of the Moon.
  • A hybrid eclipse is intermediate between a total and annular eclipse. At some points on the Earth it is visible as a total eclipse; whereas at others it is annular. The generic term for a total, annular or hybrid eclipse is a central eclipse.
  • A partial eclipse occurs when the Sun and Moon are not exactly in line, and the Moon only partially obscures the Sun. This phenomenon can usually be seen from a large part of the Earth outside of the track of a central eclipse. However, some eclipses can only be seen as a partial eclipse, because the central line never intersects the Earth's surface.

The reason why some solar eclipses are total and others are annular has to do with the elliptical nature of the Moon's orbit around Earth. One of the most remarkable co-incidences in nature is that (i) the Sun lies about 400 times as far from Earth as does the Moon, and (ii) the Sun is also about 400 times the diameter of the Moon. As seen from Earth, therefore, the Sun and the Moon appear to be about the same size in the sky - about 1/2 of a degree in angular measure. Because the Moon's orbit around Earth is an ellipse rather than a circle, however, at some times during the month the Moon is further away, and at other times it is closer to Earth, than average. The furthest point in the orbit is referred to as apogee, and the closest point is called perigee.

When a solar eclipse occurs when the Moon is at or near perigee, it appears large enough to cover the bright disk, or photosphere, of the Sun completely, and a total eclipse occurs. When a solar eclipse occurs when the Moon is at or near apogee, however, it appears smaller, and it cannot cover the Sun completely. In that case, at the time of greatest eclipse there remains a thin annulus (or ring) of brilliant Sun left uncovered. Hence the term annular eclipse. Slightly more annular eclipses than total eclipses occur, because on average the Moon lies too far away from Earth to cover the Sun completely.

Terminology

The term eclipse is actually a misnomer: The phenomenon of the Moon passing in front of the Sun is actually an occultation. Properly speaking, an eclipse occurs when one object passes into the shadow cast by another object. When the Moon disappears at Full Moon by passing into Earth's shadow, the event is properly called an eclipse, but when the Moon passes in front of the Sun, we see an occultation of the Sun by the Moon.

Photo taken by Wikipedia editor Luc Viatour (Lviatour) during the French 1999 eclipse Photo taken during the Spanish 2005 annular eclipse Photo taken in Valladolid (Spain) during the October 3, 2005 annular eclipse People observing a Solar eclipse in Iceland 2002

Observing a solar eclipse

Looking directly at the photosphere of the Sun (the bright disk of the Sun itself), even for just a few seconds, can cause permanent damage to the retina of the eye, because of the intense visible and invisible radiation that the photosphere emits. This damage can result in permanent impairment of vision, up to and including blindness. The retina has no sensitivity to pain, and the effects of retinal damage may not appear for hours, so there is no warning that injury is occurring.

Under normal conditions, the Sun is so bright that it's difficult to stare at it directly, so there is no tendency to look at it in a way that might damage the eye. However, during an eclipse, with so much of the Sun covered, it is easier and more tempting to stare at it. Unfortunately, looking at the Sun during an eclipse is just as dangerous as looking at it outside an eclipse, except during the brief period of totality, when the Sun's disk is completely covered (totality occurs only during a total eclipse and only very briefly—it does not occur during a partial or annular eclipse). Viewing the Sun's disk through any kind of optical aid (binoculars, a telescope, or even an optical camera viewfinder) is even more hazardous, although just viewing it with the naked eye can easily cause damage.

Viewing partial and annular eclipses

Viewing the Sun during partial and annular eclipses (and during total eclipses outside the brief period of totality) requires special eye protection, or indirect viewing methods.

The Sun's disk can be viewed using appropriate filtration to block the harmful part of the Sun's radiation. Sunglasses are not safe, since they do not block the harmful and invisible infrared radiation which causes retinal damage. Only properly designed and certified solar filters should ever be used for direct viewing of the Sun's disk.

The safest way to view the Sun's disk is by indirect projection. This can be done by projecting an image of the disk onto a white piece of paper or card using a pair of binoculars (with one of the lenses covered), a telescope, or another piece of cardboard with a small hole in it (about 1 mm diameter), often called a pinhole camera. The projected image of the Sun can then be safely viewed; this technique can be used to observe sunspots, as well as eclipses. However, care must be taken to ensure that no one looks through the projector (telescope, pinhole, etc.) directly.

Viewing the Sun's disk on a video display screen (provided by a video camera or digital camera) is safe, although the camera itself may be damaged by direct exposure to the Sun. The optical viewfinders provided with some video and digital cameras are not safe.

These precautions apply to viewing the Sun at any time except during the totality phase of a total solar eclipse (see below).

Viewing totality during total eclipses

Contrary to popular belief, it is safe to observe the total phase of a total solar eclipse directly with the unaided eye, binoculars or a telescope, when the Sun's photosphere is completely covered by the Moon; indeed, this is a very spectacular and beautiful sight, and it is too dim to be seen through filters. The Sun's faint corona will be visible, and even the chromosphere, solar prominences, and possibly even a solar flare may be seen. However, it is important to stop directly viewing the Sun promptly at the end of totality. The exact time and duration of totality for the location from which the eclipse is being observed should be determined from a reliable source (local astronomers, etc.). Note that it is never safe to look at an annular or partial eclipse directly, because the Sun's disk is never completely covered during this type of eclipse.

Additional information

For more information on safe eclipse viewing, see:

  • Eye Safety During Solar Eclipses, Fred Espenak, NASA Goddard Space Flight Center
  • How to Watch a Partial Solar Eclipse Safely, Alan M. MacRobert, Sky & Telescope magazine

Eclipse Predictions

Geometry of an Eclipse

Diagram of solar eclipse (not to scale)

The diagram to the right shows the alignment of the Sun, Moon and Earth at a solar eclipse. The dark gray region to the right of the moon is the umbra, where the Sun is completely obscured by the Moon. The small area where the umbra touches the Earth's surface is where a total eclipse will be seen. The larger light gray area is the penumbra, in which a partial eclipse will be seen.

Motion of the Moon and Earth

The Moon's orbit around the Earth is inclined at an angle of just over 5 degrees to the plane of the Earth's orbit around the Sun (the ecliptic). Because of this, at the time of a New Moon, the Moon will usually pass above or below the Sun. A solar eclipse can occur only when the New Moon occurs close to one of the points (known as nodes) where the Moon's orbit crosses the ecliptic – hence the name.

The Moon's orbit is also elliptical, which means that the distance of the Moon from the Earth can vary by about 6% from its average value. This means that the apparent size of the Moon is sometimes larger or smaller than average, and it is this effect that leads to the difference between total and annular eclipses (the distance of the Earth from the Sun also varies during the year, but this is a smaller effect). On average, the Moon appears to be slightly smaller than the Sun, so the majority (about 60%) of central eclipses are annular. It is only when the Moon is closer to the Earth than average (near its perigee) that a total eclipse occurs.

The Moon orbits the Earth in approximately 27.3 days, relative to a fixed frame of reference. This is known as the sidereal month. However, during one sidereal month, the Earth has moved on in its orbit around the Sun. This means that the average time between one New Moon and the next is longer, and is approximately 29.6 days. This is known as the synodic month, and corresponds to what is commonly called the lunar month.

The Moon crosses from south to north of the ecliptic at its ascending node. However, the nodes of the Moon's orbit are gradually moving in a retrograde motion, due the the action of the Sun's gravity on the Moon's motion, and they make a complete circuit every 18.5 years. This means that the time between each passage of the Moon through the ascending node is slightly shorter than the sidereal month. This period is called the draconitic month.

Finally, the Moon's perigee is moving forwards in its orbit, and makes a complete circuit in about 9 years. The time between one perigee and the next is known as the anomalistic month.

Frequency of Solar Eclipses

The Moon's orbit intersects with the ecliptic at the two nodes that are 180 degrees apart. Therefore, the New Moon occurs close to the nodes at two periods of the year approximately six months apart, and there will always be at least one solar eclipse during these periods. Sometimes the New Moon occurs close enough to a node during two consecutive months. This means that in any given year, there will always be at least two solar eclipses, and there can be as many as five. However, some are visible only as partial eclipses, because the umbra passes either above or below the earth, and others are central only in remote regions of the arctic or antarctic.

Path of an Eclipse

During a central eclipse, the Moon's umbra (or antumbra, in the case of an annular eclipse) moves rapidly from west to east across the Earth. The Earth is also rotating from west to east, but the umbra always moves faster than any given point on the Earth's surface, so it almost always appears to move in a roughly west-east direction across a map of the Earth (there are some rare exceptions to this which can occur during an eclipse of the midnight sun in arctic or antarctic regions).

The width of the track of a central eclipse varies according to the relative apparent diameters of the Sun and Moon. In the most favourable circumstances, when a total eclipse occurs very close to perigee, the track can be over 250 km wide and the duration of totality may be over 7 minutes. Outside of the central track, a partial eclipse can usually be seen over a much larger area of the Earth.

Occurrence of Eclipses at a given place

Total Solar Eclipse Paths: 1001-2000. This image was merged from 50 separated images from http://sunearth.gsfc.nasa.gov/eclipse/

Total solar eclipses are rare events. Although they occur somewhere on Earth approximately every 18 months, it has been estimated that they recur at any given place only once every 370 years, on average (Stephenson, p.54). Then, after waiting so long, the total eclipse only lasts for a few minutes, as the Moon's umbra moves eastward at over 1700 km/h. Totality can never last more than 7 min 40 s, and is usually much shorter. During each millennium there are typically fewer than 10 total solar eclipses exceeding 7 minutes. The last time this happened was June 30, 1973. Observers aboard a Concorde aircraft were able to stretch totality to about 74 minutes by flying along the path of the Moon's umbra. The next eclipse of comparable duration will not occur until June 25, 2150. The longest total solar eclipse during the 8,000-year period from 3000 BC to 5000 AD will occur on July 16, 2186, when totality will last 7 min 29 s. (eclipse predictions by Fred Espenak, NASA/GSFC.)

For astronomers, a total solar eclipse forms a rare opportunity to observe the corona (the outer layer of the Sun's atmosphere). Normally this is not visible because the photosphere is much brighter than the corona.

Eclipse Cycles

If the date and time of a solar eclipse is known, it is possible to predict other eclipses using eclipse cycles. Two such cycles are the Saros and the Inex. The Saros cycle is probably the most well known, and one of the best, eclipse cycles. The Inex cycle is itself a poor cycle, but it is very convenient in the classification of eclipse cycles. After a Saros cycle finishes, a new Saros cycle begins 1 Inex later (hence its name: in-ex).

Historical solar eclipses

A solar eclipse of 15 June 763 BC mentioned in an Assyrian text is important for the Chronology of the Ancient Orient. This is the earliest solar eclipse that can be exactly dated. There have been other claims to date earlier eclipses, in Babylon and also in China, but these are highly disputed and rely on much supposition. For a discussion, see the text by Stephenson.

Herodotus wrote that Thales of Milete predicted an eclipse which occurred during a war between the Medians and the Lydians. Soldiers on both sides put down their weapons and declared peace as a result of the eclipse. Exactly which eclipse was involved has remained uncertain, although the issue has been studied by hundreds of ancient and modern authorities. One likely candidate took place on May 28, 585 BC, probably near the Halys river in the middle of modern Turkey.

An annular eclipse of the Sun occurred at Sardis on February 17, 478 BC, while Xerxes was departing for his expedition against Greece, as Herodotus, VII, 37 recorded ([Hind and Chambers, 1889: 323] considered this absolute date more than a century ago). Herodotus (book IX, 10, book VIII, 131, and book IX, 1) reports that another solar eclipse was observed in Sparta during the next year, on August 1, 477 BC. The sky suddenly darkened in the middle of the sky, well after the battles of Thermopylae and Salamis, after the departure of Mardonius to Thessaly at the beginning of the spring of (477 BC) and his second attack on Athens, after the return of Cleombrotus to Sparta. Note that the modern conventional dates are different by a year or two, and that these two eclipse records have been ignored so far.

Other Observations

During a solar eclipse special observations can be done with the unaided eye. Normally the spots of light which fall through the small openings between the leaves of a tree, have a circular shape. These are images of the sun. During a partial eclipse, the light spots will show the partial shape of the sun, as seen on the picture.

Images of the sun during a partial eclipse through the leaves of a tree

Special observation campaigns

  • May 30, 1965: Launch of rockets at Charlestown, USA
  • May 20, 1966: Launch of rockets at Karystos, Greece to watch the solar eclipse
  • November 12, 1966: Launch of two Titus-rockets fom Las Palmas, Argentina
  • February 26, 1979: Launch of rockets from Red Lake, Canada
  • February 16, 1980: Launch of rockets from San Marco platform

Solar eclipse before sunrise or after sunset

It is possible for a solar eclipse to attain totality (or in the event of a partial eclipse, near totality) before sunrise or after sunset from a particular location. When this occurs shortly before the former or after the latter, the sky will appear much darker than it would otherwise be immediately before sunrise or after sunset. On these occasions, an object — especially a planet (often Mercury) — may be visible near the sunrise or sunset point of the horizon when it could not have been seen without the eclipse.

Simultaneous occurrence of solar eclipse and transit of a planet

In principle, the simultaneous occurrence of a Solar eclipse and a transit of a planet is possible. But these events are extremely rare because of their short durations. The next anticipated simultaneous occurrence of a Solar eclipse and a transit of Mercury will be on July 5, 6757, and of a Solar eclipse and a transit of Venus is expected on April 5, 15232.

Only 5 hours after the transit of Venus on June 4, 1769 there was a total solar eclipse, which was visible in Northern America, Europe and Northern Asia as partial solar eclipse. This was the lowest time difference between a transit of a planet and a solar eclipse in the historical past.

More common — but still quite rare — is a conjunction of any planet (not confined exclusively to Mercury or Venus) at the time a total solar eclipse, in 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 — including Albert Einstein — hypothesized that there may have been a planet even closer to the Sun than Mercury; the only way to confirm its existence would have been to observe it during a total solar eclipse. When no such planet was found during such an eclipse, the possibility of its existence was ruled out.

Solar eclipses by artificial satellites

Artificial satellites can also get in the line between Earth and Sun. But none are large enough to cause an eclipse. At the altitude of the International Space Station, for example, an object would need to be about 3.35 km across to blot the Sun out entirely. This means the best you can get is a satellite transit, but these events are difficult to watch, because the zone of visibility is very small. The satellite passes over the face of the Sun in about a second, typically. Like a transit of a planet it will not get dark. [1]

Past and future eclipses

Although there is a total eclipse visible somewhere on Earth most years, some are more conveniently observed than others. Eclipses where the path of totality crosses major population centres generate the most interest in the general public.

Selected past and upcoming eclipses are:

(*) Duration of central eclipse.


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(*) Duration of central eclipse.. It was inspired by and featured Cindy Sheehan as a speaker at many rallies. Selected past and upcoming eclipses are:. It was a rolling anti-war protest against the Iraq War, beginning in Crawford, Texas, travelling three routes across the country (with rallies along the way) and culminating in a rally in Washington, DC in September 2005. Eclipses where the path of totality crosses major population centres generate the most interest in the general public. In September, the Bring Them Home Now Tour was organized by Gold Star Families for Peace, Iraq Veterans Against the War, Military Families Speak Out, and Veterans For Peace. Although there is a total eclipse visible somewhere on Earth most years, some are more conveniently observed than others. The following day, President Bush ended his five-week vacation early to focus on relief efforts in the wake of Hurricane Katrina.

[1]. Hurricane Katrina, a Category 4 storm, made landfall in southeastern Louisiana on 29 August. Like a transit of a planet it will not get dark. She also announced the Bring Them Home Now Tour, to depart on September 1 and arrive in Washington, D.C., on September 24 for three days of demonstrations. The satellite passes over the face of the Sun in about a second, typically. In late August, Sheehan stated that she would continue her campaign against the Iraq war even if granted a second meeting with the President. This means the best you can get is a satellite transit, but these events are difficult to watch, because the zone of visibility is very small. On 16 August, Sheehan moved her camp closer to the Bush ranch after being offered the use of a piece of land owned by a supporter, Fred Mattlage, who also happens to be a third cousin of Larry Mattlage, a rancher who had fired a shotgun on his property near the demonstration site several days earlier.[33][34].

At the altitude of the International Space Station, for example, an object would need to be about 3.35 km across to blot the Sun out entirely. Gold Star Families for Peace, of which Sheehan is a founding member, released a TV commercial featuring Sheehan, broadcast on Crawford and Waco cable channels near Bush's ranch.[31] The group conducted a walk to a police station just outside President Bush's Crawford ranch and delivered a bundle of oversized letters written by them to First Lady Laura Bush, appealing to her as a mother for support towards their movement.[32]. But none are large enough to cause an eclipse. On some days as many as 1500 supporters visited Camp Casey[30], including members of Congress, as well as several notable actors, singers, and civil rights activists. Artificial satellites can also get in the line between Earth and Sun. She spent the next four weeks in Crawford (except for 5 days spent in California to see her elderly mother, who had suffered a stroke[29]). When no such planet was found during such an eclipse, the possibility of its existence was ruled out. A few days later, the media began referring to Sheehan's camp as "Camp Casey."[28].

At one time, some scientists — including Albert Einstein — hypothesized that there may have been a planet even closer to the Sun than Mercury; the only way to confirm its existence would have been to observe it during a total solar eclipse. Bush's Prairie Chapel Ranch near Crawford, Texas and announced her intention to stay (sleeping in a pup tent at night) until she is granted a second face-to-face meeting with the President.[27] Sheehan started her protest the day the President started a planned five-week vacation. More common — but still quite rare — is a conjunction of any planet (not confined exclusively to Mercury or Venus) at the time a total solar eclipse, in 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. On 6 August, 2005, Sheehan created a makeshift camp in a ditch by the side of the road about 3 miles from George W. This was the lowest time difference between a transit of a planet and a solar eclipse in the historical past. [26]. Only 5 hours after the transit of Venus on June 4, 1769 there was a total solar eclipse, which was visible in Northern America, Europe and Northern Asia as partial solar eclipse. At least sixteen Democratic members of Congress signed a letter on August 9, 2005, asking that Bush meet with Sheehan and the other relatives of fallen soldiers, as well as calling on Bush to ensure that no one will be arrested for having a peaceful demonstration.

The next anticipated simultaneous occurrence of a Solar eclipse and a transit of Mercury will be on July 5, 6757, and of a Solar eclipse and a transit of Venus is expected on April 5, 15232. Prior to going on a bicycle ride on his Texas ranch on August 13, 2005 Bush gave journalists and aides a defense of his not meeting with Sheehan stating, as reported by Ken Herman of Cox Enterprises. But these events are extremely rare because of their short durations. Bush did speak to reporters at his ranch, saying:. In principle, the simultaneous occurrence of a Solar eclipse and a transit of a planet is possible. President George W. On these occasions, an object — especially a planet (often Mercury) — may be visible near the sunrise or sunset point of the horizon when it could not have been seen without the eclipse. Sheehan told the two officials she appreciated their meeting with her.

When this occurs shortly before the former or after the latter, the sky will appear much darker than it would otherwise be immediately before sunrise or after sunset. The Times also reported that Ms. It is possible for a solar eclipse to attain totality (or in the event of a partial eclipse, near totality) before sunrise or after sunset from a particular location. According to The New York Times (August 6, 2005) the meeting lasted 45 minutes. During a partial eclipse, the light spots will show the partial shape of the sun, as seen on the picture. On August 6, 2005, Sheehan met with two high-level Bush administration officials, National Security Adviser Stephen Hadley and Deputy White House Chief of Staff Joe Hagin. These are images of the sun. Some critics have likened her dissent to an act of treason [22] [23].

Normally the spots of light which fall through the small openings between the leaves of a tree, have a circular shape. Lennox Yearwood, CEO of the Hip Hop Caucus, to describe her as "the Rosa Parks of the antiwar movement." [17] Later during the demonstration, Sheehan also gained the label of "Peace Mom" from the mainstream media [18] [19] [20] [21]. During a solar eclipse special observations can be done with the unaided eye. Sheehan's actions have led supporters such as Rev. Note that the modern conventional dates are different by a year or two, and that these two eclipse records have been ignored so far. Toward the end of her vigil, she said she was "very, very, very grateful" Bush did not grant her that meeting because it would have ended the momentum the peace movement gained from the popularity of her vigil [16]. The sky suddenly darkened in the middle of the sky, well after the battles of Thermopylae and Salamis, after the departure of Mardonius to Thessaly at the beginning of the spring of (477 BC) and his second attack on Athens, after the return of Cleombrotus to Sparta. She has also promised that, if she is not granted a second meeting, she will return to Crawford each time Bush visits there in the future [15].

Herodotus (book IX, 10, book VIII, 131, and book IX, 1) reports that another solar eclipse was observed in Sparta during the next year, on August 1, 477 BC. Demanding a second meeting with the President and an explanation of the "noble cause" for which her son died [13] [14], she created a peace camp called Camp Casey by pitching a tent by the side of the road and announced her intention to stay, day and night, for the full five weeks, or until such a meeting is granted. An annular eclipse of the Sun occurred at Sardis on February 17, 478 BC, while Xerxes was departing for his expedition against Greece, as Herodotus, VII, 37 recorded ([Hind and Chambers, 1889: 323] considered this absolute date more than a century ago). Although she had spoken publicly against the Iraq war and occupation since 2004, Sheehan gained national attention in early August 2005 when she traveled to President Bush's Prairie Chapel Ranch just outside Crawford, Texas, during his five-week vacation retreat there. One likely candidate took place on May 28, 585 BC, probably near the Halys river in the middle of modern Turkey. As of August 2005, at least 63 other relatives of fallen soldiers are listed as members. Exactly which eclipse was involved has remained uncertain, although the issue has been studied by hundreds of ancient and modern authorities. Sheehan is one of the nine founding members of Gold Star Families for Peace, an organization founded in January 2005 that seeks to end the occupation of Iraq and provide support for families of fallen soldiers.

Soldiers on both sides put down their weapons and declared peace as a result of the eclipse. "Behind these boots is one broken-hearted family," she stated as she donated her son Casey's boots to travel with Eyes Wide Open when it stopped in San Francisco later that month [12]. Herodotus wrote that Thales of Milete predicted an eclipse which occurred during a war between the Medians and the Lydians. She was also a featured speaker when the exhibition opened in San Diego in March, 2005 [11] and traveled with the exhibition other locations. For a discussion, see the text by Stephenson. Cindy wrote about the experience in a commentary article [10]. There have been other claims to date earlier eclipses, in Babylon and also in China, but these are highly disputed and rely on much supposition. There she met other families who lost loved ones in Iraq, and together they discussed the need to create an organization for similiar families.

This is the earliest solar eclipse that can be exactly dated. military casualty. A solar eclipse of 15 June 763 BC mentioned in an Assyrian text is important for the Chronology of the Ancient Orient. to speak at the opening of Eyes Wide Open: the Human Cost of War, a traveling exhibition created by the American Friends Service Committee that displays pairs of combat boots to represent every U.S. After a Saros cycle finishes, a new Saros cycle begins 1 Inex later (hence its name: in-ex). During the Presidential Inauguration in January, 2005, Cindy traveled to Washington D.C. The Inex cycle is itself a poor cycle, but it is very convenient in the classification of eclipse cycles. [9].

The Saros cycle is probably the most well known, and one of the best, eclipse cycles. She further stated that her son's death had compelled her to speak out against what she feels to be an unjust war, in order to help to bring the troops home and hold politicians accountable. Two such cycles are the Saros and the Inex. Sheehan gave another interview on October 4, 2004 stating that she did not understand the reasons for the Iraq invasion and never thought that Iraq posed an imminent threat to the United States. If the date and time of a solar eclipse is known, it is possible to predict other eclipses using eclipse cycles. [8]. Normally this is not visible because the photosphere is much brighter than the corona. And I know he's a man of faith." [7] On July 4, 2005 she was again interviewed by a local paper in Fort Lewis, Washington, regarding her meeting with President Bush, this time describing it as "one of the most disgusting experiences I ever had and it took me almost a year to even talk about it." She described President Bush as being "detached from humanity" and said that "his mouth kept moving, but there was nothing in his eyes or anything else about him that showed me he really cared or had any real compassion at all." She continued, "He didn’t even know our names," asking "Who we'all honorin' here today?" when he first entered the room, and then referring to her as "Ma" or "Mom".

For astronomers, a total solar eclipse forms a rare opportunity to observe the corona (the outer layer of the Sun's atmosphere). The president has changed his reasons for being over there every time a reason is proven false or an objective reached." It should be noted that she also stated that President Bush was "...sincere about wanting freedom for the Iraqis...I know he's sorry and feels some pain for our loss. (eclipse predictions by Fred Espenak, NASA/GSFC.). In a June 24, 2004 interview with the Vacaville Reporter published soon after the meeting, she stated, "We haven't been happy with the way the war has been handled. The longest total solar eclipse during the 8,000-year period from 3000 BC to 5000 AD will occur on July 16, 2186, when totality will last 7 min 29 s. Bush in June 2004 at Fort Lewis, near Tacoma, Washington, nearly three months after her son's death. The next eclipse of comparable duration will not occur until June 25, 2150. Sheehan and other military families met with President George W.

Observers aboard a Concorde aircraft were able to stretch totality to about 74 minutes by flying along the path of the Moon's umbra. Although Sheehan had "always been a Democrat," [5] and had initially questioned the urgency of the invasion of Iraq, she did not become active in the anti-war effort until after her son's death [6]. The last time this happened was June 30, 1973. [2] [3] Sheehan was posthumously awarded the Bronze Star Medal and the Purple Heart [4]. During each millennium there are typically fewer than 10 total solar eclipses exceeding 7 minutes. A few weeks later, on April 4, 2004 Sheehan was killed in action, along with several other soldiers, after volunteering as part of a Quick Reaction Force to rescue American troops. Totality can never last more than 7 min 40 s, and is usually much shorter. On March 19, 2004 Sheehan's company, Charlie Battery, arrived at FOB War Eagle in Sadr City as part of the post-invasion Iraq occupation.

Then, after waiting so long, the total eclipse only lasts for a few minutes, as the Moon's umbra moves eastward at over 1700 km/h. Sheehan re-enlisted, knowing that his unit would be sent to Iraq. Although they occur somewhere on Earth approximately every 18 months, it has been estimated that they recur at any given place only once every 370 years, on average (Stephenson, p.54). Near the end of his first tour of duty with the First Cavalry Division, the 2003 invasion of Iraq began. Total solar eclipses are rare events. The Army trained him as a mechanic instead. Outside of the central track, a partial eclipse can usually be seen over a much larger area of the Earth. In May 2000 Sheehan enlisted, hoping to become a chaplain's assistant.

In the most favourable circumstances, when a total eclipse occurs very close to perigee, the track can be over 250 km wide and the duration of totality may be over 7 minutes. Army. The width of the track of a central eclipse varies according to the relative apparent diameters of the Sun and Moon. Cindy Sheehan is the mother of Specialist Casey Sheehan, who served in the U.S. The Earth is also rotating from west to east, but the umbra always moves faster than any given point on the Earth's surface, so it almost always appears to move in a roughly west-east direction across a map of the Earth (there are some rare exceptions to this which can occur during an eclipse of the midnight sun in arctic or antarctic regions). . During a central eclipse, the Moon's umbra (or antumbra, in the case of an annular eclipse) moves rapidly from west to east across the Earth. [1].

However, some are visible only as partial eclipses, because the umbra passes either above or below the earth, and others are central only in remote regions of the arctic or antarctic. She is sometimes referred to by the media as the "Peace Mom". This means that in any given year, there will always be at least two solar eclipses, and there can be as many as five. Bush's Texas ranch. Sometimes the New Moon occurs close enough to a node during two consecutive months. Cindy Lee Miller Sheehan (born July 10, 1957 in Bellflower, California) is an American anti-Iraq War activist who attracted international attention in August 2005 for her extended demonstration at a peace camp outside President George W. Therefore, the New Moon occurs close to the nodes at two periods of the year approximately six months apart, and there will always be at least one solar eclipse during these periods.
.

The Moon's orbit intersects with the ecliptic at the two nodes that are 180 degrees apart. [59]. The time between one perigee and the next is known as the anomalistic month. [58]Sheehan also announces she intends to sue. Finally, the Moon's perigee is moving forwards in its orbit, and makes a complete circuit in about 9 years. "The officers made a good faith, but mistaken effort to enforce an old unwritten interpretation of the prohibitions about demonstrating in the Capitol," Chief Terrance Gainer says in a statement. This period is called the draconitic month. February 1, 2006: Capitol Police drop all charges against Sheehan and apologize for ejecting her and Young.

This means that the time between each passage of the Moon through the ascending node is slightly shorter than the sidereal month. [57]. However, the nodes of the Moon's orbit are gradually moving in a retrograde motion, due the the action of the Sun's gravity on the Moon's motion, and they make a complete circuit every 18.5 years. Bill Young (R-FL), is ordered to leave the gallery during Bush's speech because she is wearing a shirt with the words "Support the Troops Defending Our Freedom." [56] After complying with the officer's request to leave the gallery, Young says she argued loudly with officers and called one of them "an idiot." Unlike Sheehan, Young is not arrested, leaving on her own accord. The Moon crosses from south to north of the ecliptic at its ascending node. Code § 10-503.16(b)(7), implemented by Capitol Grounds Regulations Article XIX §158(a) which allow, "wearing Tee shirts, buttons, or other similar articles of apparel that convey a message." [54] Sheehan was released on her own recognizance after four hours in jail.[55] Beverly Young, the wife of Rep. This is known as the synodic month, and corresponds to what is commonly called the lunar month. [53] Sheehan was charged with unlawful conduct, a misdemeanor carrying a maximum penalty of six months in jail and/or a $500 fine — D.C.

This means that the average time between one New Moon and the next is longer, and is approximately 29.6 days. Sheehan states that she had not been asked to cover her shirt prior to her arrest; a Capitol Police spokeswoman states that Sheehan was warned first, but that she did not respond. However, during one sidereal month, the Earth has moved on in its orbit around the Sun. How many more?" Officer Mike Weight removes her from the gallery and handcuffs her before Bush arrives. This is known as the sidereal month. Lynn Woolsey (D-CA) to attend the event.[52] After being seated about fifteen minutes prior to the speech, Sheehan removes her jacket, uncovering the t-shirt she had worn to the earlier "People's State of the Union" press conference, bearing the message "2,245 dead. The Moon orbits the Earth in approximately 27.3 days, relative to a fixed frame of reference. Bush, Sheehan reluctantly accepts an invitation by Rep.

It is only when the Moon is closer to the Earth than average (near its perigee) that a total eclipse occurs. January 31, 2006: Two hours prior to the State of the Union address by George W. On average, the Moon appears to be slightly smaller than the Sun, so the majority (about 60%) of central eclipses are annular. Dianne Feinstein (D-CA) in the June 2006 Democratic primary. This means that the apparent size of the Moon is sometimes larger or smaller than average, and it is this effect that leads to the difference between total and annular eclipses (the distance of the Earth from the Sun also varies during the year, but this is a smaller effect). January 31, 2006: Sheehan participates in the "People's State of the Union" press conference, where she tells reporters that she is still considering challenging Sen. The Moon's orbit is also elliptical, which means that the distance of the Moon from the Earth can vary by about 6% from its average value. participating in a public forum at the Bus Boys and Poets Bookstore, where she was one of a six person panel [51].

A solar eclipse can occur only when the New Moon occurs close to one of the points (known as nodes) where the Moon's orbit crosses the ecliptic – hence the name. January 30, 2006: Sheehan is back in Washington, D.C. Because of this, at the time of a New Moon, the Moon will usually pass above or below the Sun. Later that day, Feinstein announces that she will support the filibuster against Alito, but it is not clear if this announcement is prompted by Sheehan's statement [50]. The Moon's orbit around the Earth is inclined at an angle of just over 5 degrees to the plane of the Earth's orbit around the Sun (the ecliptic). January 27, 2006: While in Venezuela, Sheehan releases a statement that unless Senator Dianne Feinstein votes to fillibuster the confirmation of Samuel Alito, she will challenge Feinstein for Senate. The larger light gray area is the penumbra, in which a partial eclipse will be seen. January 24, 2006: In a trip funded by Venezuela's foreign ministry, Sheehan joins more than 10,000 anti-globalization activists in Venezuela for the Caracas World Social Forum with Venezuela's President Hugo Chavez [49] and states "I admire President Chavez for his strength to resist the United States.".

The small area where the umbra touches the Earth's surface is where a total eclipse will be seen. aircraft refueling at Shannon Airport, stating, "Your Government, even though they didn't send troops to Iraq, are complicit in the crimes by allowing the planes to land and refuel..."[48]. The dark gray region to the right of the moon is the umbra, where the Sun is completely obscured by the Moon. She voices her objection to U.S. The diagram to the right shows the alignment of the Sun, Moon and Earth at a solar eclipse. December 13, 2005 Sheehan travels to Ireland, where she meets Irish Foreign Affairs minister Dermot Ahern. For more information on safe eclipse viewing, see:. Later in the evening, she attends a play written by Dario Fo (Literature Nobel laureate) about her [47], in which the role of Sheehan was played by Frances de la Tour.

Note that it is never safe to look at an annular or partial eclipse directly, because the Sun's disk is never completely covered during this type of eclipse. Sheehan is received enthusiastically in Britain, where she is celebrated as an American heroine of the anti-war movement. The exact time and duration of totality for the location from which the eclipse is being observed should be determined from a reliable source (local astronomers, etc.). December 10, 2005: Sheehan addresses the International Peace Conference, organized by the Stop the War Coalition and held at The Royal Horticultural Halls. However, it is important to stop directly viewing the Sun promptly at the end of totality. She is interviewed by BBC Radio[45] and by The Guardian [46]. The Sun's faint corona will be visible, and even the chromosphere, solar prominences, and possibly even a solar flare may be seen. December 9, 2005: Sheehan brings her campaign to London, England.

Contrary to popular belief, it is safe to observe the total phase of a total solar eclipse directly with the unaided eye, binoculars or a telescope, when the Sun's photosphere is completely covered by the Moon; indeed, this is a very spectacular and beautiful sight, and it is too dim to be seen through filters. [44]. These precautions apply to viewing the Sun at any time except during the totality phase of a total solar eclipse (see below). The theme of the banquet was “Make 2006 a turning point year in the fight for peace and justice." The PWW is the newspaper of the Communist Party USA. The optical viewfinders provided with some video and digital cameras are not safe. December 4, 2005: Sheehan travels to Chicago to attend the annual People's Weekly World banquet. Viewing the Sun's disk on a video display screen (provided by a video camera or digital camera) is safe, although the camera itself may be damaged by direct exposure to the Sun. Bush plans to stay in Crawford through November 28, 2005.[43].

However, care must be taken to ensure that no one looks through the projector (telescope, pinhole, etc.) directly. November 25, 2005: Sheehan returns to Texas to protest Bush's vacation without bringing the soldiers home. The projected image of the Sun can then be safely viewed; this technique can be used to observe sunspots, as well as eclipses. She states that if she is arrested, she will return to the fence as soon as she gets out of jail. This can be done by projecting an image of the disk onto a white piece of paper or card using a pair of binoculars (with one of the lenses covered), a telescope, or another piece of cardboard with a small hole in it (about 1 mm diameter), often called a pinhole camera. October 24, 2005: During a media interview[42], Sheehan expresses plans to speak at the White House and then tie herself to the fence. The safest way to view the Sun's disk is by indirect projection. October 5, 2005: Sheehan returns home to Northern California.[40] [41] She states that she will continue her campaign against the war in Iraq until all the troops are brought back to the United States.

Only properly designed and certified solar filters should ever be used for direct viewing of the Sun's disk. [38][39]. Sunglasses are not safe, since they do not block the harmful and invisible infrared radiation which causes retinal damage. October 3, 2005: Sheehan holds a rally in Phoenix, Arizona and urges Governor Janet Napolitano to withdraw the Arizona National Guard from Iraq. The Sun's disk can be viewed using appropriate filtration to block the harmful part of the Sun's radiation. [36][37]. Viewing the Sun during partial and annular eclipses (and during total eclipses outside the brief period of totality) requires special eye protection, or indirect viewing methods. October 1, 2005: Sheehan protests Hillary Clinton's soft stance on the war, stating that Clinton must either speak out against the war or risk losing her job.

Viewing the Sun's disk through any kind of optical aid (binoculars, a telescope, or even an optical camera viewfinder) is even more hazardous, although just viewing it with the naked eye can easily cause damage. September 27, 2005: Sheehan meets with Senator John McCain (a Vietnam veteran) and afterwards calls him a warmonger.[35]. Unfortunately, looking at the Sun during an eclipse is just as dangerous as looking at it outside an eclipse, except during the brief period of totality, when the Sun's disk is completely covered (totality occurs only during a total eclipse and only very briefly—it does not occur during a partial or annular eclipse). However, during an eclipse, with so much of the Sun covered, it is easier and more tempting to stare at it. Under normal conditions, the Sun is so bright that it's difficult to stare at it directly, so there is no tendency to look at it in a way that might damage the eye.

The retina has no sensitivity to pain, and the effects of retinal damage may not appear for hours, so there is no warning that injury is occurring. This damage can result in permanent impairment of vision, up to and including blindness. Looking directly at the photosphere of the Sun (the bright disk of the Sun itself), even for just a few seconds, can cause permanent damage to the retina of the eye, because of the intense visible and invisible radiation that the photosphere emits. When the Moon disappears at Full Moon by passing into Earth's shadow, the event is properly called an eclipse, but when the Moon passes in front of the Sun, we see an occultation of the Sun by the Moon.

Properly speaking, an eclipse occurs when one object passes into the shadow cast by another object. The term eclipse is actually a misnomer: The phenomenon of the Moon passing in front of the Sun is actually an occultation. Slightly more annular eclipses than total eclipses occur, because on average the Moon lies too far away from Earth to cover the Sun completely. Hence the term annular eclipse.

In that case, at the time of greatest eclipse there remains a thin annulus (or ring) of brilliant Sun left uncovered. When a solar eclipse occurs when the Moon is at or near apogee, however, it appears smaller, and it cannot cover the Sun completely. When a solar eclipse occurs when the Moon is at or near perigee, it appears large enough to cover the bright disk, or photosphere, of the Sun completely, and a total eclipse occurs. The furthest point in the orbit is referred to as apogee, and the closest point is called perigee.

Because the Moon's orbit around Earth is an ellipse rather than a circle, however, at some times during the month the Moon is further away, and at other times it is closer to Earth, than average. As seen from Earth, therefore, the Sun and the Moon appear to be about the same size in the sky - about 1/2 of a degree in angular measure. One of the most remarkable co-incidences in nature is that (i) the Sun lies about 400 times as far from Earth as does the Moon, and (ii) the Sun is also about 400 times the diameter of the Moon. The reason why some solar eclipses are total and others are annular has to do with the elliptical nature of the Moon's orbit around Earth.

There are four types of solar eclipses:. . A total solar eclipse is considered by many to be the most spectacular natural phenomenon that one can observe. This configuration can only occur at New Moon, when the Sun and Moon are in conjunction, as seen from Earth.

A solar eclipse occurs when the Moon passes in front of the Sun and obscures it totally or partially. February 16, 1980: Launch of rockets from San Marco platform. February 26, 1979: Launch of rockets from Red Lake, Canada. November 12, 1966: Launch of two Titus-rockets fom Las Palmas, Argentina.

May 20, 1966: Launch of rockets at Karystos, Greece to watch the solar eclipse. May 30, 1965: Launch of rockets at Charlestown, USA. MacRobert, Sky & Telescope magazine. How to Watch a Partial Solar Eclipse Safely, Alan M.

Eye Safety During Solar Eclipses, Fred Espenak, NASA Goddard Space Flight Center. However, some eclipses can only be seen as a partial eclipse, because the central line never intersects the Earth's surface. This phenomenon can usually be seen from a large part of the Earth outside of the track of a central eclipse. A partial eclipse occurs when the Sun and Moon are not exactly in line, and the Moon only partially obscures the Sun.

The generic term for a total, annular or hybrid eclipse is a central eclipse. At some points on the Earth it is visible as a total eclipse; whereas at others it is annular. A hybrid eclipse is intermediate between a total and annular eclipse. Hence the Sun appears as a very bright ring surrounding the outline of the Moon.

An annular eclipse occurs when the Sun and Moon are exactly in line, but the apparent size of the Moon is smaller than that of the Sun. During any one eclipse, a total eclipse is visible only from a fairly narrow track on the surface of the Earth. The intensely bright disk of the Sun is replaced by the dark outline of the Moon, and the much fainter corona is visible (see image right). A total eclipse occurs when the Sun is completely obscured by the Moon.