The Earliest Visible Phase of the Moon

1920 ◽  
Vol 14 (3-4) ◽  
pp. 172-172
Author(s):  
T. Rice Holmes

I AM glad that Dr. Fotheringham in the interesting paper which appeared in the Classical Quarterly (April, 1920, pp. 97–8) adhered to the view that ‘Caesar calculated the new moon for January 1 [45 B.C]…and that this calculation determined the inaugural day of the Julian calendar.’ As the object of my brief note, on which he commented, was merely to show that Groebe had failed to prove that the day in question was January 2, I have only a few questions to ask. But first, in justice to Judeich, I ought to say that his calculations, which Dr. Fotheringham notices, were made with the help of the assistant-astronomer attached to the observatory of the University of Strassburg. While Dr. Fotheringham admits that I was right in maintaining that the new moon of January 2, 45 B.C. (1.26 a.m.) was not visible on the evening of that day, he holds that Groebe was ‘fairly entitled to say’ that the new moon of March 24, 58 B.C. (4.40 p.m.), was visible on March 25. Dr. Fotheringham may be justified in saying that it ought ‘in normal [or abnormally fine ?] weather to have been visible that evening’; but, as I observed in my note, Groebe affirmed that in calculating the time of visibility of the crescent we should accept the mean of the Babylonian estimates, 36 hours—less, I should have added, in the early spring and the winter, more in the summer and autumn. Was he entitled to deduct 9 hours from the mean for an observation made not in the clear atmosphere of the East, but in Switzerland? Dr. Fotheringham tells us that ‘the shortest interval between a new moon and the observation of the moon by Schmidt's naked eye comes’ not, as Groebe said, to 29, but ‘to 25.7 hours.’ But forty-eight of Schmidt's forty-nine observations were made at Athens, where the atmosphere is clearer than in Switzerland. The great difference in visibility which a clear atmosphere makes must strike everyone who goes from this country or from Switzerland to the East or to Northern Africa. I realized it for the first time when I was exploring in Tunisia before the war. Has Dr. Fotheringham or any other trustworthy observer ever seen with the naked eye in an atmosphere no clearer than that of Geneva a moon not more than 27 hours old? If so, is it not remarkable that, as Dr. Fotheringham has said, ‘Hitherto it has been the practice to assume that [in the early spring or the winter and in favourable weather ?] the moon becomes visible on the first evening when she is more than 30 hours old at sunset’?

1884 ◽  
Vol 12 ◽  
pp. 187-189
Author(s):  
John Aitken

When residing in the south of France lately, I happened to look at the new moon one evening through the clear air of the “Mistral,” which was blowing at the time, and not being able to see the dark body of the moon, it all at once struck me that something more was necessary than a clear atmosphere in order to enable us to see the dark side of the moon, and that the dark side would be best seen when the earth was to a great extent covered with clouds.


1989 ◽  
Vol 19 (1) ◽  
pp. 11-14 ◽  
Author(s):  
S A Bwala

The case records of 53 consecutive Nigerian inpatients with stroke in the University of Maiduguri Teaching Hospital, Maiduguri were retrospectively reviewed. The mean age at presentation was 55 years and the male to female ratio was 2.5: 1. The mean duration of symptoms before presentation was 11.1 weeks and the average duration of stay in hospital was 3 weeks. Thirty-three (63%) of the lesions were infarctive and 19 (37%) were haemorrhagic. Only 3 (6%) patients gave a history of prior transient ischaemic attacks (TIAs). Forty-two (79%) patients were hypertensive at presentation out of which 27 (64%) had the hypertension diagnosed for the first time. Four (8%) patients were non-insulin dependent diabetics. There were 11 hospital deaths (21%). Thus hypertension, more than half undiagnosed at admission, was the most common risk factor for stroke in the hospital population studied.


2012 ◽  
Vol 5 (12) ◽  
pp. 2993-3006 ◽  
Author(s):  
P. E. Sheese ◽  
K. Strong ◽  
E. J. Llewellyn ◽  
R. L. Gattinger ◽  
J. M. Russell ◽  
...  

Abstract. The Optical Spectrograph and InfraRed Imaging System (OSIRIS) on the Odin satellite is currently in its 12th year of observing the Earth's limb. For the first time, continuous temperature profiles extending from the stratopause to the upper mesosphere have been derived from OSIRIS measurements of Rayleigh-scattered sunlight. Through most of the mesosphere, OSIRIS temperatures are in good agreement with coincident temperature profiles derived from other satellite and ground-based measurements. In the altitude region of 55–80 km, OSIRIS temperatures are typically within 4–5 K of those from the SABER, ACE-FTS, and SOFIE instruments on the TIMED, SciSat-I, and AIM satellites, respectively. The mean differences between individual OSIRIS profiles and those of the other satellite instruments are typically within the combined uncertainties and previously reported biases. OSIRIS temperatures are typically within 2 K of those from the University of Western Ontario's Purple Crow Lidar in the altitude region of 52–79 km, where the mean differences are within combined uncertainties. Near 84 km, OSIRIS temperatures exhibit a cold bias of 10–15 K, which is due to a cold bias in OSIRIS O2 A-band temperatures at 85 km, the upper boundary of the Rayleigh-scatter derived temperatures; and near 48 km OSIRIS temperatures exhibit a cold bias of 5–15 K, which is likely due to multiple-scatter effects that are not taken into account in the retrieval.


2019 ◽  
Vol 6 (2) ◽  
pp. 197-207
Author(s):  
Nandi Pinto

The Problem of hisab and ru’yat on its development are not regardless of development Islamic thingking history who much be embellishment of ideology, mazhab or firqah, who present differentiation on opinion who related Islamic law framework especially in Indonesia. The result of understanding different about argumentation normative hisab-ru’yat were think out a differntiation and understanding on the Islamic member of a religious community. This thesis is field research, who has special understanding on construe of Hadis ru’yat al-hilal of Tarekat Syatariah. Interpretation this Hadith of Tarekat Syatariah have different understanding to understand the context of Hadis. Now focus of this research is to know understanding and implementation of Hadith ru’yat al-hilal according to Syatariah scholar Ulakan Padang Pariaman. The result of this research are, First, understanding of hadis ru’yat al-hilal according to Syatariah scolar Ulakan Padang Pariaman is both collaboration of that hadis, because of the first hadis be explanation of the second hadis that are when the moon can’t be seen with the naked eyes because closed of fog or cloud, than word of presuppositioning (faqdurulah) on the first hadis be exclamation of passages of Koran by supplying additional information by Syatariah scholar be completed Sya’ban moon to be 30 days. Second, understanding implementation of Hadis ru’yat al-hilal is with together see new moon (al-hilal) at place who be certained of scolar (Tuangku) from the last time , they are Ulakan beach Padang Pariaman and Koto Tuo Agam. They are see new moon naked eye, although use the modern tools to see it the last judgmen according to them how to see it with naked eye, if it can’t be seen so, the new moon was not visible, although with modern tools to see it, and that not have influenced on determination al-hilal was seem or not. Their jedgment is still on argument if the new moon can’t see with naked eyes, so, al-hilal be evidented not visible and Sya’ban moon be completed to 30 days.


ELFALAKY ◽  
2019 ◽  
Vol 3 (2) ◽  
Author(s):  
Heri Zulhadi

Abstract Hisab and rukyah are two methods of study used by Muslims to determine the start time of prayer, fasting, hajj and so forth. Periodesasi hisab rukyah, at a glance must have imagined what is meant by hisab rukyah. In the discourse about the Hijri calendar known by the term hisab and rukyah. Hisab is a calendar calculation system based on the average circulation of the moon that surrounds the earth and is conventionally defined. This reckoning system began since the establishment of Caliph Umar ibn Khattab ra (17H) as a reference for composing an enduring Islamic calendar. Another opinion says that this calendar system started in 16 H or 18 H, but the more popular is the year 17 H. While Rukyah is seeing the hilal directly with the naked eye or with the help of tools such as telescopes or other tools that support to see the new moon every end of Qamariyah month. The word rukyah is more famous as rukyatul hilalyaitu see moon. In this study, the author will describe a little about the history of hisab and rukyah in the period of prophets, companions, tabi'in, mid to modern period today. In this study, the scope of hisab rukya includes prayer times, Qibla direction, the beginning of Qamariyah month, eclipse and hijri calendar. Keyword: Hisab, Rukyah.


2019 ◽  
Vol 17 (2) ◽  
Author(s):  
Willy Vila Nova Pessoa ◽  
Jonas de Assis Almeida Ramos ◽  
Paulo Guilherme Vasconcelos de Oliveira

ABSTRACT The influence of the moon cycles on the ichthyofauna has been little studied in the surf zone. In this study, the number of species, density and biomass were evaluated as a function of the moon. A total of 49 species distributed in 24 families were captured in two areas of Miramar beach. The mean density was significant high in the weaning and low in the new moon, while density and biomass together showed differences for areas. The most abundant species were Anchoa tricolor and Trachinotus falcatus (new moon), and Anchovia clupeoides showed significant differences in the waning moon. The RDA indicates that turbidity influenced significantly the presence of two species group. The group I were represented by Stellifer brasiliensis, Trachinotus goodei, A. clupeoides, Chilomycterus spinosus and Conodon nobilis that occurred on the waning and new phases in both areas, while the group II were represented by Polydactylus virginicus and Haemulopsis corvinaeformis in the full moon. The surf zones may also be strongly governed by the lunar phases. Therefore, the results found in this study, showed that the biological interactions between the species with turbidity and moon might explain the density and biomass variations for some species in the surf zone.


PEDIATRICS ◽  
1978 ◽  
Vol 61 (2) ◽  
pp. 300-300
Author(s):  
T. E. C.

The following statistics were obtained from women who appeared at the University College Hospital (in 1870) to be attended in their confinement. In 2,696 cases menstruation occurred for the first time- From these cases it would appear most common at 14 years of age, then 15, 16, 13, 17, 12, 18, 19, 20, 10. The mean age in these cases is 14.96 years nearly.


The table given in this paper contains the results of calculations relating to the objects specified in the title; cast into periods of six, seven, or eight days, so as to bring the day of the lunar phase belonging to it in the middle of the time. The observations were all made in the neighbourhood of London. It appears from them that in the period of the last quarter of the moon the barometer is highest, the temperature a little above the mean, and the depth of rain the smallest. In the period of the new moon, both the barometer and temperature are considerably depressed, and the rain increased in quantity. The influence of the first quarter shows itself by the further depression of the barometer; but the temperature rises almost to the point from which it had fallen, and the rain still increases, but not in an equal ratio. Lastly, the full moon again reduces the temperature; while the barometer attains its maximum mean height, and the quantity of rain is the greatest. Thus it appears, that during this lunar cycle, the approach of the last quarter is the signal for the clearing up of the air, and the return of sunshine.


1822 ◽  
Vol 112 ◽  
pp. 237-238 ◽  

Dear Sir, Cape Town, Cape of Good Hope, December 13,1821. I take the earliest opportunity of communicating to you a curious appearance which I lately observed upon the moon. My present means of making observations of this kind are indeed very limited, as the large telescopes, destined for the Cape Observatory, have not yet arrived. Still, however, it is right to have phenomena of this kind recorded, though the description may, from the want of proper instruments, be imperfect. About eight o’clock in the evening of the 28th of Novem­ber last, the sky being extremely clear, and the moon shin­ing with a brilliancy which I never observed in England, my attention was drawn to a whitish spot on the dark part of the moon’s limb, sufficiently luminous to be seen with the naked eye. Lest I might be mistaken, I requested Mr. Fayror, the assistant astronomer, to look at the moon attentively, and inform me whether he could observe any bright appearance upon the dark part of it. We both agreed in the identity of the spot, and remarked that now and then it seemed to flash with considerable lustre. Mr. Fayror having in his posses­sion a good achromatic telescope, which Mr. Troughton had given him previous to our departure from England, I requested the loan of it for a few nights, so that I might be able to exa­mine this appearance more minutely. Having directed the telescope to the moon, I immediately recognised the luminous spot, which seemed like a star of the sixth magnitude, and three others much smaller, but one of these more brilliant than the one we had seen with the naked eye. The largest spot was surrounded by a nebulous appearance. I could not per­ceive any thing of the kind about the small brilliant spot. The two others were similar to faint nebulae, increasing in intensity towards the middle, but without any defined lumi­nous point. As I am not yet in possession of a micrometer, by means of which the situation of these spots might be ascertained, you must rest satisfied with this imperfect de­scription. On the evening of the 29th, the sky being equally favourable for observation as on the former one, I found that the large spot was, at the least, as bright as before, two others were nearly invisible, and the small brilliant spot had disappeared. I was unable to make any farther observations, as a strong south-east wind began to blow with great violence on the goth, accompanied with rain, and which lasted several days. I wait with great anxiety for the next new moon, when, if the sky be clear, I shall not fail to examine it as carefully as my means at present will permit.


2010 ◽  
Vol 6 (S269) ◽  
pp. 3-6
Author(s):  
George V. Coyne

AbstractDuring the very last year of what he himself described “as the best [eighteen] years of his life” spent at the University of Padua, Galileo first observed the heavens with a telescope. In order to appreciate the marvel and the true significance of those observations we must appreciate both the intellectual climate in Europe and the critical intellectual period through which Galileo himself was passing at the time those observations were made. Through his studies on motion Galileo had come to have serious doubts about the Aristotelian concept of nature. What he sensed was lacking was a true physics. He was very acute, therefore, when he came to sense the significance of his observations of the moon, of the phases of Venus, of the moons of Jupiter and of the Milky Way. The preconceptions of the Aristotelians were crumbling before his eyes. He had remained silent long enough, over a three month period, in his contemplations of the heavens. It was time to organize his thoughts and tell what he had seen and what he thought it meant. It was time to publish! In so doing he would become one of the pioneers of modern science. For the first time in over 2,000 years new significant observational data had been put at the disposition of anyone who cared to think, not in abstract preconceptions but in obedience to what the universe had to say about itself.


Sign in / Sign up

Export Citation Format

Share Document