cover
Contact Name
Ahmad Izzuddin
Contact Email
alhilal@walisongo.ac.id
Phone
+6285201241033
Journal Mail Official
alhilal@walisongo.ac.id
Editorial Address
Gedung Dekanat Fakultas Syariah dan Hukum, UIN Walisongo Semarang Jl. Prof. Dr. Hamka, Tambakaji, Kec. Ngaliyan, Kota Semarang, Jawa Tengah 50185
Location
Kota semarang,
Jawa tengah
INDONESIA
Al-Hilal: Journal of Islamic Astronomy
ISSN : 27751236     EISSN : 27752119     DOI : https://doi.org/10.21580/al-hilal
Al-Hilal Journal is a scientific journal published in April and October per year by the Islamic Astronomy at the Faculty of Sharia and Law, Universitas Islam Negeri (UIN) Walisongo, Semarang colaboration with Asosisasi Dosen Falak Indonesia (ADFI). Articles published in this journal are the results of empirical research in Islamic Astronomy (such as qibla, salat times, Islamic Calendar, Eclipse and others), and its approaching on other area studies (mathematics, physics, astrophysics, social, politics, anthropology, ethnography and others). This journal has specifications as a medium of publication and communication of Islamic Astronomy ideas derived from theoretical and analytical studies, as well as research results in the field of both natural and social science. The editor hopes that writers, researchers and legal experts will contribute in this journal.
Articles 114 Documents
UTILIZATION OF RADIO TELESCOPES IN DETERMINING THE BEGINNING OF THE ISLAMIC CALENDAR Anaam, Khairul
Al-Hilal: Journal of Islamic Astronomy Vol 6, No 2, 2024
Publisher : Fakultas Syari'ah dan Hukum UIN Walisongo

Show Abstract | Download Original | Original Source | Check in Google Scholar | DOI: 10.21580/al-hilal.2024.6.2.23416

Abstract

This study analyzes the use of radio telescopes in rukyat al-hilāl observations from the perspective of science and fiqh. In modern astronomy, radio telescopes have become essential for observing celestial objects emitting radio signals, including planets, stars, and other cosmic phenomena. However, its use in observing the Hilāl as a marker of the beginning of the Islamic month is still debated, especially from the perspective of Islamic law (fiqh). This study uses a literature study method with a qualitative descriptive approach. The study's results indicate that this technology is not scientifically suitable for detecting the hilāl and determining the beginning of the Hijri month. Meanwhile, from a fiqh perspective, radio telescopes cannot be considered valid for observing the hilāl in determining the beginning of the Hijri month. Observing the hilāl in determining the beginning of the Hijri month requires a visual vision of the crescent moon object visible after sunset as a sign of the start of the new month in the Hijri calendar.
INTERPRETATION OF FAJR ṢĀDIQ AND FAJR KĀDHIB IN Al-SHĀFI’Ī SCHOOL’S TEXTS: A HADITH AND ASTRONOMICAL PERSPECTIVES Qulub, Siti Tatmainul; Nadhifah, Nurul Asiya; Ahmad Munif; Mokhamad Ali Ridlo
Al-Hilal: Journal of Islamic Astronomy Vol 6, No 2, 2024
Publisher : Fakultas Syari'ah dan Hukum UIN Walisongo

Show Abstract | Download Original | Original Source | Check in Google Scholar | DOI: 10.21580/al-hilal.2024.6.2.23868

Abstract

This study explores the interpretation of false dawn (fajr kādhib) and true dawn (fajr ṣādiq) in al-Shāfi’ī fiqh texts through the lenses of hadith and astronomy. It compares classical definitions by al-Rāfi'ī and al-Nawawī with contemporary scientific and hadith-based perspectives. Using documentation and descriptive-critical analysis, the research finds that fajr kādhib is described as vertical light (mustathil) resembling a wolf's tail, appearing briefly and vanishing. In contrast, fajr ṣādiq is horizontal light (mustaṭīr) spreading across the horizon, gradually brightening. From a hadith perspective, this aligns with al-mu'taridh (true dawn) and al-mustathil (false dawn). Astronomically, fajr kādhib matches zodiacal light, which doesn’t disappear, and fajr ṣādiq corresponds to sunlight scattering. Thus, the disappearance of fajr kādhib, as described in classical texts, lacks modern scientific support.
Dynamics of the Neo-MABIMS Criteria in Determining the Beginning of the Hijri Month in Indonesia (1443–1446 H) Wahyuningsih, Yuniar; Firdiansyah, Ahmad Roihan
Al-Hilal: Journal of Islamic Astronomy Vol. 7 No. 2 (2025)
Publisher : Fakultas Syari'ah dan Hukum UIN Walisongo

Show Abstract | Download Original | Original Source | Check in Google Scholar | DOI: 10.21580/al-hilal.2025.7.2.28379

Abstract

This study explores the ongoing variations in determining the beginning of the Hijri month in Indonesia, despite the official adoption of the Neo-MABIMS criteria by the Ministry of Religious Affairs of the Republic of Indonesia. Employing a descriptive qualitative approach, the research outlines and deductively analyzes data related to formulating and implementing these criteria. The findings reveal two key points: first, discrepancies persist in determining the beginning of the Hijri month. Since implementing the Neo-MABIMS criteria up to Jumada al-Awwal 1446 H, two months, Jumada al-Akhirah 1445 H, and Muharram 1446 H, have produced different outcomes. Second, even when identical criteria are applied, differences in methodological approaches may lead to either divergent or convergent results. This study recommends future research involving expert interviews to strengthen analytical depth and include updated observational data on Hijri month determination to enhance the comprehensiveness and accuracy of the findings.
Critical Analysis and Reformulation of the Qibla Deviation Formula in the Book of Mekanika Benda Langit Luthfi, Muhammad; Fajri, M. Nur Iskandar; Reza, Izam Bahtiar; Aziz, M Abdul
Al-Hilal: Journal of Islamic Astronomy Vol. 7 No. 2 (2025)
Publisher : Fakultas Syari'ah dan Hukum UIN Walisongo

Show Abstract | Download Original | Original Source | Check in Google Scholar | DOI: 10.21580/al-hilal.2025.7.2.28219

Abstract

The calculation of Qibla deviation using the formula presented in the Mekanika Benda Langit book has become widely adopted and frequently cited in academic studies. However, this method still produces noticeable inaccuracies. This research aims to identify the causes of error in the Qibla deviation formula described in the Mekanika Benda Langit book and to reformulate a more accurate method for determining the Qibla direction. The study employed a literature-based qualitative design, with data obtained through documentation and interviews. Data analysis was conducted using descriptive statistical methods within a multidisciplinary approach. The findings reveal that the inaccuracy arises from the formula's reliance on the ratio between an arc and a flat circle, making it valid only for short distances (up to 2,000 km). A reformulation using spherical trigonometry provides higher precision and consistency across all distances and longitudinal variations. This new formulation significantly improves the accuracy of Qibla deviation calculations compared to the original method in Mekanika Benda Langit book.

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