Prayer Times in Yevdokimovskiy
7 августа 2026 / 24 сафара 1448 г. х.
Monthly schedule
Yevdokimovskiy prayer times overview
The Yevdokimovskiy page shows prayer times calculated taking into account local time and geographic location. This is especially important for Fajr, Maghrib and Isha.
Yevdokimovskiy prayer times are tied to the local time zone, which is 5 часов ahead of Moscow time. For this reason, the prayer schedule here cannot be directly compared with Moscow time.
Yevdokimovskiy geographic location is 54.2365°N, 100.6671°E. These coordinates are important for calculating prayer times, since prayers are tied to the movement of the sun. In this latitude zone, the day length changes noticeably throughout the year, but without sharp polar phenomena.
Even if two cities are in the same time zone, prayer times may differ due to latitude and longitude. In the mid-latitude zone, the seasonal shifts of Fajr and Maghrib are especially noticeable.
Today in Yevdokimovskiy 15 часов 26 минут passes from sunrise to Maghrib: the sun rises at 05:40, while the evening prayer begins at 21:06. Right now the day is long, so Maghrib begins later, while the night interval shortens.
The night interval in Yevdokimovskiy begins after Maghrib at 21:06 and lasts until Fajr at 03:23. Its duration is 6 часов 17 минут. The night interval is relatively short, so it is convenient to plan Isha and suhur in advance.
In summer in Yevdokimovskiy the daylight length increases: this is especially noticeable for the early Fajr and late Maghrib.
When preparing for prayer in Yevdokimovskiy, it is convenient to check Fajr (03:23), Maghrib (21:06) and Isha (23:14) in advance. These times are often used as references for the start of the day, iftar and the night prayer.
The SAM RF method is applied when calculating the schedule for Yevdokimovskiy, while the Asr time is determined according to the Hanafi madhhab. This allows the schedule to be used as a daily reference for the obligatory prayers.
Today's key reference points
- Fajr — 03:23: the start of the morning prayer time and an important reference for ending suhur.
- Sunrise — 05:40: after sunrise the Fajr time ends.
- Dhuhr — 13:23: the time of the midday prayer.
- Asr — 18:38: the afternoon prayer calculated according to the Hanafi madhhab.
- Maghrib — 21:06: the evening prayer, and also a reference for iftar during Ramadan.
- Isha — 23:14: the night prayer.
Questions about prayer times in Yevdokimovskiy
Prayer times are determined by the sun's altitude above the horizon, which is unique for every geographic point. The calculation is affected by latitude, longitude and the established time zone. For this reason, even cities located in the same region have different values for Fajr, Sunrise, Dhuhr, Asr, Maghrib and Isha. The more a city is shifted to the north or south, the more the daylight length, and with it the prayer moments, differ.
Prayer times in Yevdokimovskiy are updated daily. This is related to the constant shifting of the sunrise and sunset moments following the Earth's orbit around the sun. The changes are especially noticeable during the transitional seasons — spring and autumn — when the day length changes fastest, sometimes by several minutes per day. For the schedule to remain accurate, it should be checked daily, not once a week.
Of course. To end suhur, use the Fajr time (03:23) as a reference — the pre-dawn meal must be completed before it begins. The start of iftar coincides with the Maghrib time (21:06): the fast can be broken as soon as the sun sets below the horizon. Since prayer times shift daily during Ramadan, we recommend checking the schedule daily so as not to be off even by a minute.
It is not recommended. The prayer schedule is sensitive to geography: even a difference of tens of kilometres leads to a discrepancy in the Fajr, Maghrib and Isha times. The sun rises and sets at its own moment above each locality, so the data of a neighbouring city is only approximate. To perform the prayer on time, it is advisable to use the schedule calculated for Yevdokimovskiy according to its coordinates specifically, not the nearest centre's.