A grahan is an eclipse. The word means a seizing, and the traditional account of it is the story of Rahu, the head of the demon Svarbhanu, who tasted the nectar of immortality and was cut in two by Vishnu’s discus. The head, Rahu, and the tail, Ketu, still pursue the Sun and the Moon and now and then swallow them for a while. The astronomical account is quieter and just as old. An eclipse happens when the Sun, the Earth and the Moon line up, and it can only happen at a new moon or a full moon that falls close to the points where the Moon’s path crosses the Sun’s, the very points the tradition names Rahu and Ketu. You can read more about those two on the page about Rahu and Ketu and the past-life blueprint.
This section gives you every eclipse of 2026 and 2027, what each one looks like, who can see it, and the local times for 49 cities in India and abroad. It also gives the sutak time, the period of caution that many households keep before an eclipse. Nothing here is a prediction of events. It is a calendar, with the astronomy worked out carefully, and it leaves the question of what to do with it to your family and your temple.
Solar and lunar eclipses
At a solar eclipse, or Surya Grahan, the Moon passes in front of the Sun at the new moon, which Hindu calendars call Amavasya (see the page on Amavasya). The Moon’s shadow is small, so the full eclipse is seen only along a narrow track across the Earth. On either side of it a partial eclipse is seen, and far from it nothing is seen at all. A total eclipse hides the whole Sun for a few minutes, and an annular one leaves a bright ring because the Moon is a little too far away to cover it.
At a lunar eclipse, or Chandra Grahan, the Moon passes into the Earth’s shadow at the full moon, the day of Purnima. Because the Earth’s shadow is large, everyone on the night side of the Earth can see it, whatever their city, as long as the Moon is above the horizon. A total lunar eclipse turns the Moon a dim copper red. A partial one takes a dark bite out of it. A penumbral eclipse only dims it slightly, so slightly that many people never notice it.
The traditional rules in brief
Sutak is counted from twelve hours before a solar eclipse and nine hours before a lunar eclipse. It is kept only at places where the eclipse is visible, and it ends when the eclipse ends. The common practices are to close temples, to avoid cooking and eating during the period, to chant mantras and bathe after the eclipse. Penumbral eclipses are generally not counted as a grahan and have no sutak. These are traditions, and families vary in how they keep them, so what we give is the time and not a ruling. Pregnant women, children, the elderly and the unwell are widely excused.
For the Sun, the first rule of watching is a safety rule, not a tradition: never look at it directly. Each solar eclipse page carries the details.
How the pages were made
The time of every eclipse and the shape of the shadows come from NASA’s published data, which is in the public domain. For each of the 49 cities the page works out the local circumstances with the standard method, then checks that the Sun or the Moon is above the horizon. The results were compared with timeanddate.com for several cities for every eclipse, and the first and last contacts agreed to within a minute, and moonrise, moonset and sunset to within two minutes. The same code runs in the eclipse visibility calculator for any town. Day by day panchang timings for your city are in the panchang section.
Yes means the whole eclipse can be seen, Part means the Sun or the Moon is up for only part of it, and No means it is not seen or, for a lunar eclipse, shows no visible change. Open an eclipse page for the exact local times.
How the solar eclipse times are worked out
The shadow of the Moon is described by a small set of numbers, the Besselian elements, that NASA publishes for every eclipse (Fred Espenak, eclipse.gsfc.nasa.gov, public domain). For each city this site finds where the Moon's shadow axis passes in relation to the place and when the edge of the shadow reaches it, which gives first contact, the moment of greatest eclipse and last contact, and the share of the Sun's diameter covered, called the magnitude. The share of the Sun's disc that is hidden is the obscuration. The Sun's height above the horizon decides what can be seen, so where the Sun rises or sets during the eclipse the table says so and shows the first or last moment you can see it.
Times are the local clock time of the city, with daylight saving where it applies, cut to the whole minute. Magnitude and obscuration are for the moment shown in the Maximum column.
Sutak. By Hindu tradition the period of caution before a solar eclipse, sutak, begins twelve hours before first contact and ends when the eclipse ends. It is kept only at places where the eclipse can be seen. Temples close, cooking and eating are avoided in many households, and a bath and fresh food follow the eclipse. Some families go by a sutak of a different length, and some regions keep it more loosely, so follow your own family or temple. Children, the elderly and the unwell are generally excused from fasting.
How the lunar eclipse times are worked out
The time of greatest eclipse, the magnitude and the lengths of the penumbral, partial and total phases are taken from NASA's catalogue of lunar eclipses (Fred Espenak, eclipse.gsfc.nasa.gov, public domain). A lunar eclipse starts and ends at the same instant for everybody on the night side of the Earth, so what changes between cities is the clock time and whether the Moon is above the horizon. This site works out the Moon's height for each city at each stage, and the table gives the first and last moment you can see the eclipse.
Times are the local clock time of the city, with daylight saving where it applies, cut to the whole minute. For eclipses with a dark umbral stage the table lists that stage, when the Moon enters the dark core of the Earth's shadow, because the traditional rules count it. The faint penumbral stage is the one listed only for eclipses that have no umbral stage.
Sutak. By Hindu tradition the period of caution before a lunar eclipse, sutak, begins nine hours before the eclipse and ends when it ends. This page counts it from the first umbral contact, and only for a city where the eclipse can be seen. A penumbral eclipse is not counted as a grahan in most almanacs and has no sutak. Families follow their own rules for what is avoided during sutak, so follow your own family or temple. Children, the elderly and the unwell are generally excused from fasting.
Frequently asked questions
↳ How many eclipses are there in 2026 and 2027?
There are nine, four solar and five lunar. In 2026 there are two of each, and in 2027 there are two solar and three lunar. Of the nine, only three show anything from Indian cities: the lunar eclipse of 3 March 2026 at moonrise, the faint penumbral eclipse of 20 February 2027 and the partial solar eclipse of 2 August 2027, as the table above shows city by city.
↳ Is sutak kept for an eclipse that I cannot see?
By the usual rule, no. Sutak and the other grahan observances apply where the eclipse is visible. Where only a small part is seen, for example at moonrise, practice varies, and many families still keep the sutak that the almanac gives for their city. When in doubt, follow your family or your temple.
↳ Why do the times differ between cities?
A lunar eclipse begins at one moment for everybody who can see it, but the clock shows a different time in each city. A solar eclipse is different in a second way too, because the Moon's shadow reaches each place at a different moment and covers a different share of the Sun there.
↳ Can I use the tables for a town that is not listed?
Yes. The eclipse visibility calculator takes any town or city and gives the same figures for every eclipse in the section, using the same method as the tables.
↳ Are the 2026 eclipses on these pages still useful?
The four eclipses of 2026 have already taken place, and their pages are kept as a record, with the times that applied to each city. The five eclipses of 2027 are still ahead.