跳到主要內容

Ramadan 2024


P. ROCHER, INSTITUT DE MECANIQUE CELESTE ET DE CALCUL DES EPHEMERIDES OBSERVATOIRE DE PARIS


Calculation of the start and end of the month Ramadan for the Gregorian year 2024


The month of Ramadan in 2024 (year 1445 AH) begins at the visibility of the crescent Moon following the new moon of the second part of the month of March 2024. It ends at the visibility of the first crescent Moon following the new moon in the second part of the month of April 2024. 

In March 2024, the geocentric new moon falls on March 10 at 9h 0m 26s UTC (at 10h 0m 26s in legal time French).

In April 2024, the geocentric new moon falls on April 8 at 6:20:52 p.m. UTC (at 8:20:52 p.m. in French legal time). 

Please note, in mainland France, we switch to summer time on Sunday March 31.

The true lunation between the two new Moons lasts 29.3891811 days, or 29 days 9h 20m 25.255.

Between two new Moons, the following astronomical events will occur one after the other:

on 03/10/2024 at 09:00:26 UTC New moon.

on 03/11/2024 at 04:37:47 UTC the Moon has zero and increasing declination, right ascension 11.9m. Oh

on 03/12/2024 at 01:17:22 UTC the Moon passes through the ascending node of its orbit, mean longitude: +15° 42,2

03/17/2024 at 04:10:43 UTC First quarter moon.

on 03/17/2024 at 2:38:28 p.m. UTC the declination of the Moon is at its maximum, declination +28 32.3. 03/23/2024 at 3:44:59 p.m. UTC The Moon at apogee, distance from Earth 406,294.218 km, diameter

apparent: 29.49, mean longitude: 165.79°. on 03/25/2024 at 02h 08m 24s UTC the Moon has zero and decreasing declination, right ascension - 12h 11.9m.

03/25/2024 at 07:00:20 UTC: Full moon.

on 03/26/2024 at 04:07:29 UTC: the Moon passes through the descending node of its orbit, mean longitude:+195" 34.5.

on 04/01/2024 at 08:51:40 UTC the declination of the Moon is at its minimum, declination-28 34.3. 04/02/2024 at 03:14:44 UTC: Last quarter moon. on 04/07/2024 at 3:45:56 p.m. UTC the Moon has zero and increasing declination, right ascension Oh 11.9m.

on 04/07/2024 at 5:51:20 p.m. UTC The Moon at perigee, distance from Earth 358,849.734 km, apparent diameter: 33.38, mean longitude: 4.05.

on 04/08/2024 at 12:18:51 p.m. UTC: the Moon passes through the ascending node of its orbit, mean longitude: +15° 37.7

04/08/2024 at 6:20:52 p.m. UTC: New moon.


For the year 2024, the difference between TT-UTC is taken equal to 69.184s


Reminder of the criterion that we use at IMCCE for the naked eye visibility of the first crescent Moon: the crescent Moon is observable with the naked eye at sunset, if the center of the Moon is at minus 5º above the horizon and if its angular distance from the Sun (elongation) is at least 8". The minimum elongation of 8 corresponds to the slightly overestimated Danjon criterion (this criterion is more of the order of 7.5 °), the height difference of 5º corresponds to an arcus visionis of 5".

IMCCE

9 Apr Eid moon sighting live 

Hamariweb

Islamicfinder

Iuhk


留言

這個網誌中的熱門文章

CMOS sensor trends and astrophotography, from amateur astronomers perspective

Nowadays, even in low light conditions, digital camera can quality pictures with higher ISO, noise and hot pixels have been gradually reduced. Sony has introduced back illumination process for consumer market. Sony BSI sensors evolved  from Exmor to now Exmor RS( stacked) technology. This stacked technology allows further chip size reduction, which has strong demands in smartphone camera market. Digital astrophotography is also benefited from such advances, utilising Back Side Illumination technology Exmor: Within the CMOS sensor, it outputs low-noise digital signals by "on-chip column AD conversion" and "dual noise reduction" to suppress noise in the first half of the process In low light conditions, when a wide aperture is desirable to collect as much light as possible. At apertures wider than f/2.0, back-illuminated Exmor R sensors are significantly more efficient at collecting light than conventional, front-illuminated sensor...

ultrafast rendezvous to ISS

    14 Oct 2020,  being the first to use a new “ultrafast” rendezvous” scheme with the ISS. Following a flawless ascent to the correct orbit, Soyuz 2 .1a , Soyuz MS-17 caught up with the orbiting laboratory in only two orbits (three hours), halving the time it takes for crew to get to the Station.   The three space travelers of the Soyuz MS-17 mission launched on a six-month mission the International Space Station.  previous 3/4 orbit rendezvous: Soyuz MS-16 4 orbit rendezvous A three-orbit profile was deemed possible without major flight design changes after inauguration of the Soyuz 2-1A rocket that provides a much higher orbit injection accuracy than its predecessors and would allow the two correction maneuvers on Orbit #2 to be eliminated while the Automated Rendezvous Phase would still remain untouched. The deletion of the Orbit #2 maneuvers was expected to slightly tighten the already restrictive phase angle window from and upper limit of 30-35° to 25-28°...

Scythians 斯泰基 塞種 西古提人

900 BC - 200 AD British museum   Tomb of scythe prince, Buktarma valley, 1200 masl, Google map Herodotus   絲路上的帝國 Biblegeography   哥羅西書 3:11  在此並不分希利尼人、猶太人、受割禮的、未受割禮的、化外人、 西古提人 、為奴的、自主的.惟有基督是包括一切、又住在各人之內。 塞種 塞迦  saka 史記漢書 西域傳: 塞種  ctext 昔匈奴破大月氏,大月氏西君大夏,而塞王南君罽賓。塞種分散,往往為數國。自疏勒以西北,休循、捐毒之屬,皆故 塞種 也。 匈奴列傳 Ctext :塞王 《史記》在《大宛列傳》與《匈奴列傳》中, 詳細 記錄了中亞至天山一帶的塞種(塞王、塞地)狀況。例如,文中記載了月氏西破走塞王,導致塞人南遷越過懸度(今帕米爾高原及克什米爾一帶) Baike Genetic history   Genetics  Nih griffin  ? Scytho-Siberian  world 塞迦 saka  wiki Disappeared? Sarmatians ( 薩爾馬泰 , 奄蔡 史記 ,  Aorsi )and goths YouTube