Nothing there is beyond hope, nothing can be sworn impossible, nothing wonderful,
since Zeus, father of the Olympians, made night from mid-day, hiding the light of
the shining sun, and sore fear came upon men."
— Archilochus, Greek poet, following the total solar eclipse of 648 BC
On April 8, 2024, a total solar eclipse will be visible to fortunate observers in the United States along a narrow band, approximately 115 miles (185 km) wide, that will cross fifteen states from Texas to Maine.
Calculate local circumstances
Major U.S. Cities in the path of totality: Austin, TX; Dallas, TX; Ft. Worth, TX; Little Rock, AR; Indianapolis, IN; Dayton, OH; Toledo, OH; Cleveland, OH; Buffalo, NY; Rochester, NY; Burlington, VT; Montpelier, VT; Waco, TX; Syracuse, NY.
Use the form below to calculate the local circumstances for cities or towns in the U.S. or its territories.
View global map and circumstances (USNO Eclipse Portal)
The USNO Eclipse Portal provides diagrams and animations showing the global circumstances and local circumstances at selected locations. The Portal is a joint effort with Her Majesty's Nautical Almanac Office (HMNAO), United Kingdom Hydrographic Office.
Times are given in UT; for help converting them to local time, see World Time Zone Map.
View global visibility map (The Astronomical Almanac)
For visibility maps of other eclipses, see Eclipses of the Sun and Moon.
View local circumstances at Torreon, Mexico (maximum duration of totality)
Local circumstance diagram for Torreon, Mexico (location of maximum duration of totality) from USNO Eclipse Portal.
General eclipse resources
- Eclipses of the Sun and Moon
Solar and lunar eclipse visibility maps for recent and upcoming events
- Solar Eclipse Computer
Computes local circumstances for selected solar eclipses at any given location
- Lunar Eclipse Computer
Computes circumstances for selected lunar eclipses at any given location
- USNO Eclipse Portal
Provides diagrams and animations of global and select local circumstances for solar and lunar eclipses, 1501–2100
- References on Eclipses
Provides a representative survey of the available literature
- the angular distance of a celestial body above or below the horizon, measured along the great circle passing through the body and the zenith. Altitude is 90° minus the zenith distance.
- the angular distance measured eastward along the horizon from a specified reference point (usually north). Azimuth is measured to the point where the great circle determining the altitude of an object meets the horizon.
- the difference between Terrestrial Time (TT) and Universal Time (UT): ΔT=TT − UT1.
- the obscuration of a celestial body caused by its passage through the shadow cast by another body.
- eclipse, solar:
- actually an occultation of the Sun by the Moon in which the Earth passes through the shadow cast by the Moon. It may be total (observer in the Moon's umbra), partial (observer in the Moon's penumbra), annular, or annular-total.
- magnitude of a solar eclipse:
- the fraction of the solar diameter obscured by the Moon at the greatest phase of a solar eclipse, measured along the common diameter.
- the obscuration of one celestial body by another of greater apparent diameter; especially the passage of the Moon in front of a star or planet, or the disappearance of a satellite behind the disk of its primary. If the primary source of illumination of a reflecting body is cut off by the occultation, the phenomenon is also called an eclipse. The occultation of the Sun by the Moon is a solar eclipse.
- 1. The portion of a shadow in which light from an extended source is partially but not completely cut off by an intervening body. 2. The area of partial shadow surrounding the umbra.
- the portion of a shadow cone in which none of the light from an extended light source (ignoring refraction) can be observed.