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Penentuan Azimut Kiblat Masjid Kampus UIN Sultanah Nahrasiyah Lhokseumawe Menggunakan Rumus Segitiga Bola Berbasis Python Ravik Walhidayah; Ismail Ismail
Astroislamica: Journal of Islamic Astronomy Vol. 4 No. 2 (2025): Astroislamica: Journal of Islamic Astronomy (Desember)
Publisher : Islamic Astronomy Department, Sharia and Law Faculty

Show Abstract | Download Original | Original Source | Check in Google Scholar | DOI: 10.47766/astroislamica.v4i2.6012

Abstract

Prayer time is a compulsory act of worship for Muslims, the validity of which depends on the fulfillment of specific conditions, one of which is facing the qibla, the direction of the Kaaba in the Masjid al-Haram, Makkah. Therefore, accurate determination of the qibla direction is a crucial aspect of performing prayer. Various methods have been used to determine the qibla direction, such as the annual Rashdul Qiblah phenomenon and calculations based on spherical trigonometry. The Rashdul Qiblah method is simple and accurate; however, its application is limited to specific times. In contrast, spherical trigonometry can be applied at any time and offers high precision, but the calculation process is relatively complex and prone to human error. This study aims to implement spherical trigonometry using the Python programming language to simplify the process of qibla direction determination and to evaluate its accuracy. The research employs a library research method with a computational simulation approach. The qibla direction is calculated by inputting the latitude and longitude coordinates of the location and the Kaaba into a Python program, and the results are then compared with field measurement data obtained using a theodolite. The results show that the Python-based qibla direction calculation produces an azimuth value with a difference of 32.62 arcseconds compared to the theodolite measurements. This difference is considered very small and does not practically affect the accuracy of the qibla direction. Therefore, the proposed method is proven to be accurate, efficient, and suitable as a modern alternative for determining the qibla direction.
An Analysis of the Effectiveness of the Apexel Lens as a Non-Conventional Optical Device for Hilal Observation Muhammad Khalil Mubarraq; Ravik Walhidayah; Ismail
AL - AFAQ : Jurnal Ilmu Falak dan Astronomi Vol. 8 No. 1 (2026): Juni 2026
Publisher : Universitas Islam Negeri Mataram

Show Abstract | Download Original | Original Source | Check in Google Scholar

Abstract

Crescent moon (Hilal) is a primary indicator to determine the onset of a new month in Hijri calendar, but access limitation to the conventional optical instrument such as telescope and theodolite remains a significant constaint across various strategic observation sites. This study aims to analyze the feasilibity of the Apexel telephoto lens as a non-conventional optical instrument for hilal observation, while also evaluating its potential as a screening tool to assessing the suitability of rukyat (crescent sighting) sites. The research employed a field-experimental approach, by comparing the optical performance of the Apexel lens mounted on a Google Pixel 5 with a standard astronomical telescope F70060 Telescope during Hilal observation conducted between November 21–24, 2025 at the Malikussaleh Observatory. The result demonstrate that Hilal image was successfully documented on November 23, 2025 with an altitude of 6° above the horizon. This outcome was significantly supported by favorable atmospheric conditions, characterized by cloud cover below 10%, which enabled the camera sensor to compensate for the Apexel lens's aperture limitations in capturing the low-contrast luminosity of the thin crescent. Conversely, detection attempts on other days failed due to adverse atmospheric conditions, wherein dense cloud cover attenuated hilal luminosity beyond the instrument's sensitivity threshold. From economic standpoint, this device represents a viable alternative for grassroots rukyat communities in remote areas, given its affordability and accessibility. Accordingly, Apexel telephoto lens has a potential to be a supplementary instrument for Hilal observation in the context of site exploration and public education, with the caveat that its performance is highly depends on sky clearance and astronomical parameters that meets the minimum visibility criteria.