04.03.2018 Views

Seadet-i Ebediyye - Endless Bliss Fifth Fascicle

Various aspects of Hanafi Fiqh are explained, e.g., zakat, ramadan, hajj, sadaqa-i fitr, Qurban(sacrifice), Iyd(Eid), nikah(marriage), death, janaza, burial, visiting graves, condolence, isqat and knowledge of faraid.

Various aspects of Hanafi Fiqh are explained, e.g., zakat, ramadan, hajj, sadaqa-i fitr, Qurban(sacrifice), Iyd(Eid), nikah(marriage), death, janaza, burial, visiting graves, condolence, isqat and knowledge of faraid.

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

monthly tables showing the variations in its length. Since the earth<br />

revolves about the Sun, too, the duration of time between two<br />

conjunctions is 29 days and 13 hours. At the time of conjunction,<br />

the Sun and the moon pass the meridian at the same time. The<br />

moon can by no means be seen anywhere before the angle between<br />

the Sun and the moon as seen from the earth, which is termed<br />

Beynûnet (elongation), has become eight degrees [approximately<br />

fourteen hours after the moment of conjunction]. When the angle<br />

becomes eighteen (18) degrees maximum, the moon comes out of<br />

the state of invisibility and the new moon appears on the western<br />

horizon within the forty-five minutes during sunset. However, due<br />

to the fifty-seven minute lunar parallax [1] , when it reaches a<br />

position five degrees above the horizon, it can no longer be seen.<br />

After the moon comes out of the state of invisibility, the new moon<br />

can be observed in places situated on the same longitude as the<br />

location where the sunset is taking place. As for later hours, or, at<br />

night it can be observed after sunset in countries west of these<br />

places. For instance, close to the beginning of the month of Rajab,<br />

the time of conjunction was fifteen (15) hundred hours according<br />

to Turkish meantime [Izmit’s local time], on 14 May, Wednesday,<br />

1980. The new moon cannot be observed before 5 a.m. the<br />

following day, i.e. Thursday. When this angle is, as was accepted by<br />

the Ottoman scholars, eighteen (18) degrees, which means a<br />

duration of one and a half days, the first appearing of the new<br />

moon will be at 3 a.m. on 15 May, Friday. Since the time of sunset<br />

as of (that) Friday in Istanbul is 19.20 hours, it will be possible to<br />

observe the new moon during sunset on Friday [the night previous<br />

to Saturday] in the city of Chicago, America, where the sunset is<br />

16 hours earlier, that is, they are 240 degrees east of Istanbul and<br />

270 degrees east of London. It cannot be observed on this same<br />

night in places east of the two hundred and seventieth meridian.<br />

Their nights begin at the time of sunset and the mornings following<br />

these nights begin at midnight. The purpose for these calculations<br />

is not to determine the time when the lunar month begins, but to<br />

determine the (beginning of the) month when the new moon can<br />

be seen. Those who say that it began before Friday night should<br />

not be believed. Imâm-i-Subkî [2] also said so. We should not believe<br />

[1] Angle subtended at the moon by the earth’s equatorial radius.<br />

[2] Abû Hasan-i-Subkî ‘rahmatullâhi ta’âlâ ’alaih’ (683 [1284 A.D.], Subk,<br />

Egypt – 756 [1355], Cairo.)<br />

– 137 –

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!