![]() ![]() Five Millennium Catalog of Hybrid Solar Eclipses: -1999 to +3000.Five Millennium Catalog of Solar Eclipses: -1999 to +3000.Catalog of Central Solar Eclipses: 1991-2030 (with links to Global Maps and Path Coordinates).NASA Technical Publication - Five Millennium Canon of Solar Eclipses: -1999 to +3000.World Map of Annular Solar Eclipses: 2001-2025 - ( Medium.World Map of Total Solar Eclipses: 2001-2025 - ( Medium.Maps of North American Eclipses: 1851-2100 - Web Page.World Maps of Solar Eclipses: -1999 - +3000 - World Atlas of Solar Eclipse Paths.Twenty Year Solar Eclipse Path Tables (w/Google Maps)Įach link in the following table displays a page containing 10 years of eclipses.Įvery eclipse has links of global maps, interactive Google maps, animations, path coordinate tables, and saros tables. ![]() Twenty Year Solar Eclipse Path Tables (w/Google Maps)Įach of the following links displays a table containing 20 years of total, annular and hybrid eclipses.Įach eclipse offers links to a global map, shadow animation, interactive Google map, path coordinates table, and saros table. This is the instant when the axis of the Moon's shadow passes closest to Earth's center. Central Duration is the duration of a total or annular eclipse at greatest eclipse. Eclipse magnitude is the fraction of the Sun's diameter obscured by the Moon.įor annular eclipses, the eclipse magnitude is always less than 1.įor total eclipses, the eclipse magnitude is always greater than orįor both annular and total eclipses, the value listed is actually the ratio of diameters between the Moon and the Sun. Such an eclipse is both total and annular along different sections of its umbral Hybrid eclipses are also known as annular/total eclipses. Is the instant when the distance between the Moon's shadow axis and Earth's center reaches a minimum. N = no northern limit, S = no southern limit, AT = annular-total hybrid, TA = total-annular hybrid The Key to Solar Eclipse Path Tables contains a more detailed description of each item in the table.įor more data on solar eclipses during this period, seeĬentral Eclipse Class abbreviations (used above): ![]() The Central Duration (column 9) gives the length of the eclipse as seen from the central line at greatest eclipse. The Path Width (column 8) gives the width of the central eclipse path (in kilometers) at the instant of greatest eclipse. The Eclipse Magnitude (column 7) gives the fraction of the Sun's diameter obscured at the instant of greatest eclipse. The link opens a table containing the Besselian elements for the eclipse. The parameter Gamma (column 6) is the perpendicular distance of the Moon's shadow axis and Earth's center at greatest eclipse. The Saros series that an eclipse belongs to is found in column 5.Īll eclipses in a particular Saros series can be viewed in a table via the Saros number link. The link opens a table containing the central path coordinates.Įclipses recur over the Saros cycle, a period of approximately 18 years 11 days. The parameters N and S identify paths that have no northern or southern limit, respectively. The Central Eclipse Class (column 4) indicates whether an eclipse is central or non-central. The link opens a window with the central eclipse path plotted on an interactive Google Map. The Eclipse Type (column 3) is either Total, Annular or Hybrid. The second column TD of Greatest Eclipse is the Terrestrial Dynamical Time when the axis of the Moon's shadow passes closest to Earth's center.Īnimations of the Moon's penumbral and umbral shadows across Earth are accessed by clicking the this link.Įach animated GIF file is from 40 KB to 175 KB in size. These figures are described in greater detail in the Key to Solar Eclipse Maps.Įach figure is stored as a gif of approximately 60 kilobytes. The track of the umbral/antumbral shadow (blue/red) defines the path of total or annular eclipse. The path of the Moon's penumbral shadow (cyan and magenta) covers the region of partial eclipse. This links to an orthographic projection map of Earth showing the region of visibility for an eclipse. The first column in the table gives the Calendar Date of the instant of greatest eclipse. When you click on a position, the eclipse times and circumstances at that location are calculated and displayed. You can zoom into the map and turn the satellite view on or off. The yellow lines plotted across the path indicate the position of maximum eclipse at 10-minute intervals. The northern and southern limits of each eclipse path are plotted in blue while the central line is red. These interactive maps utilize NASA eclipse path predictions and the plotting capabilities of Google Maps. In particular, the Eclipse Type (third column) links to dynamic maps showing the central path of eclipses across Earth's surface. The links in the table provide additional information and graphics for each eclipse. The table below is a concise summary of all
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