Salah times explained

Salat times are prayer times when Muslims perform salat. The term is primarily used for the five daily prayers including the Friday prayer, which takes the place of the Dhuhr prayer and must be performed in a group of aibadat. Muslims believe the salah times were revealed by Allah to Muhammad.

Prayer times are standard for Muslims in the world, especially the fard prayer times. They depend on the condition of the Sun and geography. There are varying opinions regarding the exact salah times, the schools of Islamic thought differing in minor details. All schools of thought agree that any given prayer cannot be performed before its stipulated time.

Most Muslims pray five times a day, with their prayers being known as Fajr (before dawn), Dhuhr (noon), Asr (late afternoon), Maghrib (at sunset), and Isha (nighttime), always facing towards the Kaaba.[1] Some Muslims pray three times a day.[2] [3] [4] The direction of prayer is called the qibla; the early Muslims initially prayed in the direction of Jerusalem before this was changed to Mecca in 624 CE, about a year after Muhammad's migration to Medina.[5]

The timing of the five prayers are fixed intervals defined by daily astronomical phenomena. For example, the Maghrib prayer can be performed at any time after sunset and before the disappearance of the red twilight from the west. In a mosque, the muezzin broadcasts the call to prayer at the beginning of each interval. Because the start and end times for prayers are related to the solar diurnal motion, they vary throughout the year and depend on the local latitude and longitude when expressed in local time.[6] In modern times, various religious or scientific agencies in Muslim countries produce annual prayer timetables for each locality, and electronic clocks capable of calculating local prayer times have been created. In the past, some mosques employed astronomers called the muwaqqits who were responsible for regulating the prayer time using mathematical astronomy.[6] You can also find accurate daily salah times for your geographical location with the help of online prayer times services.

The five intervals were defined by Muslim authorities in the decades after the death of Muhammad in 632, based on the hadith (the reported sayings and actions) of the Islamic prophet.

Daily prayers

The daily prayers are considered obligatory by many and they are performed at times determined essentially by the position of the Sun in the sky. Hence, salat times vary at different locations on the Earth. Wudu is needed for all of the prayers.

Some Muslims pray three times a day.[7] [8] [9]

Overview of prayer times considered obligatory by most[10]
Compulsory (fard) prayerPrescribed timeThe prescribed times of the prayers depicted in place of the position of the sun in the sky, relative to the worshipper.
FajrBegins at dawn, may be performed up to sunrise after Fajr nafl prayer
ZuhrFrom when the sun has passed the zenith, may be performed up to the time of Asr.
AsrFrom when the shadow cast by an object is once or twice its length, may be performed up to the time of Maghrib.
MaghribBegins at sunset, may be performed up to the end of dusk.
IshaBegins with the night, may be delayed up to dawn although disliked

Fajr (dawn)

See main article: Fajr prayer.

See also: Fajr nafl prayer and Qunut. Fajr begins at —true dawn or the beginning of twilight, when the morning light appears across the full width of the sky—and ends at sunrise.

Dhuhr (midday)

See main article: Zuhr prayer.

The time interval for offering the Zuhr or Dhuhr salah or namaz timing starts after the sun passes its zenith and lasts until call for the Asr prayer is given. This prayer needs to be given in the middle of the work-day, and people normally make their prayers during their lunch break.

Asr (afternoon)

See main article: Asr prayer.

Asr salat is the third of the obligatory prayers that Muslims offer daily.[11] It is also known as “middle prayer." The Asr prayer starts when the shadow of an object is the same length as the object itself (or, according to Hanafi school, twice its length) plus the shadow length at Dhuhr, and lasts till the start of sunset. Asr can be split into two sections; the preferred time is before the sun starts to turn orange, while the time of necessity is from when the sun turns orange until 15 minutes before Maghrib.

Maghrib (sunset)

See main article: Maghrib prayer.

The Maghrib prayer begins, when the sun sets, and lasts until the red light has left the sky in the west.

Isha (nights)

See main article: Isha prayer.

See also: Chafa'a and Witr. The Isha'a or Isha prayer starts when the red twilight disappears from the west, and lasts until the middle of the night, which is the middle point between Maghrib Salat and Fajr salat (others say it’s third of the night, or until fajr time)

Time calculation

To calculate prayer times two astronomical measures are necessary, the declination of the sun and the difference between clock time and sundial clock. This difference being the result of the eccentricity of the Earth's orbit and the inclination of its axis, it is called the equation of time. The declination of the sun is the angle between sun's rays and the equator plan.[12]

In addition to the above measures, to calculate prayer times for a specific location we need its spherical coordinates.[13]

In the following;

Z

is the time zone.

λ

and

\phi

are the longitude and the latitude of the considered point, respectively.

\Deltat

and

\delta

denotes the equation of time term and the declination of the Sun for a given date, respectively.

We first give the midday (Dhuhr) time. The midday time is simply when the local true solar time reaches noon:

T_ = 12 + \Delta t + (Z - \lambda/15)

The first term is the 12 o'clock noon, the second term accounts for the difference between true and mean solar times, and the third term accounts for the difference between the local mean solar time and the timezone.

The other times require converting the Sun's altitude to time. We use a variant of the generalized sunrise equation:

T(\alpha) = \frac \arccos \left(\frac \right)

This gives, in hours, the difference between Dhuhr time and when the sun is at altitude

\alpha

. Now we calculate three of the other prayer times:

T(-0.833\circ)

. (The astronomical sunset/sunrise that occurs at

\alpha=0

, but atmospheric refraction makes the sun appear 50 arcminutes higher.) So

TShuruq=TDhuhr-T(0.833\circ)

and

TMaghrib=TDhuhr+T(0.833\circ)

.

0.0347\circ x \sqrt{h}

to 0.833°, where h is the elevation in meters (see).

\alpha

exist. It is of 17 and 18 degrees respectively for Fajr and Isha prayers according to the Muslim World League. As a result, we have

TFajr=TDhuhr-T(18\circ)

and

TIsha=TDhuhr+T(17\circ)

.

n

be the required length of the object shadow relative to its own length. We first find the Sun's altitude as

A(n)=\arccot(n+\left|\tan(\phi-\delta)\right|).

The Asr time is then given as

TShuruq=TDhuhr+T(A(n)),

where the ratio n is 1 or 2 depending on jurisprudence.

Muslims use readily available apps on their phone to find daily prayer times in their locality. Technological advances have allowed for products such as software-enhanced azan clocks that use a combination of GPS and microchips to calculate these formulas. This allows Muslims to live further away from mosques than previously possible, as they no longer need to rely solely on a muezzin in order to keep an accurate prayer schedule.[14]

See also

External links

Notes and References

  1. Book: Samovar . Larry A. . Porter . Richard E. . McDaniel . Edwin R. . Intercultural Communication: A Reader: A Reader . 2008 . . 978-0-495-55418-9 . 165 . en.
  2. Book: Islam and the Secular State . 9780674033764 . Na . Abdullahi Ahmed An-Na'im . Naʻīm . ʻabd Allāh Aḥmad . 30 June 2009 . .
  3. Book: Muslims in America: A Short History . 978-0-19-974567-8 . Curtis Iv . Edward E. . October 2009 . .
  4. Jafarli, Durdana. "The historical conditions for the emergence of the Quranist movement in Egypt in the 19th-20th centuries." МОВА І КУЛЬТУРА (2017): 91.
  5. Book: Heinz . Justin Paul . The Origins of Muslim Prayer: Sixth and Seventh Century Religious Influences on the Salat Ritual . 2008 . . en. 115, 123, 125, 133, 141–142 .
  6. Encyclopedia: On the role of the muezzin and the muwaqqit in medieval Islamic society. David A.. King. Tradition, Transmission, Transformation. E. Jamil Ragep . Sally P. Ragep. E.J. Brill. 285–345. 1996. 90-04-10119-5.
  7. Book: Islam and the Secular State . 9780674033764 . Na . Abdullahi Ahmed An-Na'im . Naʻīm . ʻabd Allāh Aḥmad . 30 June 2009 . .
  8. Book: Curtis Iv . Edward E. . Muslims in America: A Short History . October 2009 . . 978-0-19-974567-8.
  9. Jafarli, Durdana. "The historical conditions for the emergence of the Quranist movement in Egypt in the 19th-20th centuries." МОВА І КУЛЬТУРА (2017): 91.
  10. Web site: A Shi'ite Encyclopedia. 12 November 2013. Ahlul Bayt Digital Islamic Library Project.
  11. Web site: Afzal . Rabia . Prayer time Toronto . prayertimetoronto . rabia . 28 January 2024.
  12. http://aa.usno.navy.mil/faq/docs/SunApprox.php Approximate Solar Coordinates
  13. http://praytimes.org/calculation/#Calculating_Prayer_Times Calculating Prayer Times
  14. Gorman. Carma R.. 2009. Religion on Demand: Faith-based Design. Design and Culture. 1. 1. 9–22. 10.2752/175470709787375715. 143513427.