How to Find Qibla Direction Without an App
You can find the Qibla direction without an app by observing the sun's path (east to west), using a standard compass with your city's specific bearing, or aligning with the Mihrab of local mosques. (updated )
Three Traditional Methods to Find Qibla
1. The Sun and Shadow Method
Since the sun rises in the east and sets in the west, you can establish basic cardinal directions. In addition, there are two days a year (May 27-28 and July 15-16) when the sun passes directly over the Kaaba in Mecca (called Rasad al-Qibla). At those precise moments, looking directly at the sun or aligning with the shadow of a vertical object points directly toward the Qibla.
2. Using a Standard Magnetic Compass
By lookup up your city's specific Qibla compass bearing (e.g., approximately 291° clockwise from North in New Delhi, India, or 294° in Jakarta, Indonesia), you can use any standard magnetic compass to locate the exact direction of Mecca.
3. Local Mosque Alignment
Mosques are built with their main prayer hall and Mihrab (the niche at the front of the hall) aligned precisely toward the Qibla. If you are near a mosque, checking the orientation of its structure is one of the most reliable ways to find the direction of Salah.
Need a Digital Tool?
If you want a precise visual compass and coordinates on your phone, you can also use our free Qibla Finder Tool to automatically calculate the direction based on your live GPS coordinates.
Frequently Asked Questions
- Can I find the Qibla using only the sun?
- Yes. By knowing that the sun rises in the East and sets in the West, you can establish your cardinal directions. Depending on where you are relative to Mecca (e.g., Mecca is West/North-West of India, and West/North-West of Indonesia), you can estimate the direction of Salah.
- What is the exact date the sun is directly above the Kaaba?
- The sun passes directly over the Kaaba twice a year: on May 27 or 28 at 9:18 AM UTC (12:18 PM Mecca time) and on July 15 or 16 at 9:27 AM UTC (12:27 PM Mecca time).