The Path of the Moon, the Rising Points of the Sun, and the Oblique Great Circle on the Celestial Sphere

Centaurus ◽  
2003 ◽  
Vol 45 (1-4) ◽  
pp. 16-31 ◽  
Author(s):  
Lis Brack-Bernsen
1998 ◽  
Vol 162 ◽  
pp. 32-34
Author(s):  
J. V. Narlikar ◽  
N.C. Rana

A summary of work related to astronomy education carried out during the last three years in India is presented here. Since India is a huge country and many educational efforts are made by individuals alone, this report cannot be regarded as complete, but a specific sampling.India has more than 200 Universities, 8000 colleges, and about 100,000 schools, 33 planetaria, more than 100 museums and about 60 well known amateur astronomers’ clubs. Scores of dedicated astronomy oriented school teachers, act as nuclei of astronomy education for the general public and school children .The astronomical almanac, used in a typical household is in some way related to the stars in the sky and the movements of the Sun, the Moon and the planets. Traditionally, a rudimentary knowledge of the celestial sphere is common. The recent developments in space technology have brought a fascination and glamour to modern astronomy for all age groups, and this is noticeably reflected in the number of media coverages of astronomy.


2009 ◽  
Vol 5 (S260) ◽  
pp. 135-148 ◽  
Author(s):  
Xenophon Moussas

AbstractIn this review the oldest known advanced astronomical instrument and dedicated analogue computer is presented, in context. The Antikythera Mechanism a mysterious device, assumed to be ahead of its time, probably made around 150 to 100 BCE, has been found in a 1st century BCE shipwreck near the island of Antikythera in a huge ship full of Greek treasures that were on their way to Rome. The Antikythera Mechanism is a clock-like device made of bronze gears, which looks much more advanced than its contemporary technological achievements. It is based on mathematics attributed to the Hipparchus and possibly carries knowledge and tradition that goes back to Archimedes, who according to ancient texts constructed several automata, including astronomical devices, a mechanical planetarium and a celestial sphere. The Antikythera Mechanism probably had a beautiful and expensive box; looking possibly like a very elaborate miniature Greek Temple, perhaps decorated with golden ornaments, of an elegant Hellenistic style, even perhaps with automatic statuettes, ‘daemons’, functioning as pointers that performed some of its operations. Made out of appropriately tailored trains of gears that enable to perform specialised calculations, the mechanism carries concentric scales and pointers, in one side showing the position of the Sun in the ecliptic and the sky, possibly giving the time, hour of the day or night, like a clock. The position of the Moon and its phase is also shown during the month. On the other side of the Mechanism, having probably the size of a box (main part 32×20×6 cm), are two large spiral scales with two pointers showing the time in two different very long calendars, the first one concerning the eclipses, and lasting 18 years 11 days and 8 hours, the Saros period, repeating the solar and lunar eclipses, and enabling their prediction, and the 19 year cycle of Meton, that is the period the Moon reappears in the same place of the sky, with the same phase. An additional four-year dial shows the year of all Greek Festivities, the so-called ‘games’ (Olympic, Pythian, Isthmian etc). Two additional dials give the Exeligmos, the 54 year and 34 day cycle, which provides a more accurate prediction of eclipses. It is possible that the Mechanism was also equipped with a planetary show display, as three of the planets and their motion (stationary points) are mentioned many times in the manual of the instrument, so it was also a planetarium. From the manual we have hints that the mechanism was probably also an observational instrument, as having instructions concerning a viewfinder and possibly how to orient the viewfinder to pass a sunbeam through it, probably measuring the altitude of the Sun. There are fragmented sentences that probably give instructions on how to move the pointers to set the position of the Sun, the Moon and the planets in their initial places in the ecliptic, on a specific day, or how to measure angular distances between two celestial bodies or their coordinates. This mechanism is definitely not the first one of its kind. The fact that it is accompanied with instructions means that the constructor had in its mind to be used by somebody else and one posits that he made at least another similar instrument.


1976 ◽  
Vol 31 ◽  
pp. 58-62
Author(s):  
Anny-Chantal Levasseur ◽  
Jacques Blamont

From observations made with a photometer placed on board D2A-Tournesol from April 1971 to June 1973 at ε = ± 90° for all ecliptic latitudes, we had deduced that the intensity of the zodiacal light is not constant, but shows fluctuations, some of which we correlated with cometary debris. The measurements were carried out by scanning the celestial sphere in a plane orthogonal to the Sun-Earth direction with a one minute period (LEVASSEUR et BLAMONT, 1973). BURNETT, SPARROW and NEY (1974) have pointed out that our data could have been contaminated by stray moonlight; we have therefore refined our data analysis and conclude that indeed fluctuations of the intensity of the zodiacal light do exist, even when the Moon is much below the horizon.


Antiquity ◽  
1966 ◽  
Vol 40 (159) ◽  
pp. 212-216 ◽  
Author(s):  
R. J. C. Atkinson

The astronomical significance of Stone- henge has been the subject of intermittent debate and speculation ever since 1740, when Stukeley [I] first observed that the axis of the sarsen structure and of the Avenue pointed at least approximately to the sunrise at the summer solstice. Apart from Sir Norman Lockyer [z], however, few professional astronomers concerned themselves with this question, until the appearance in,Nature of the two articles by Gerald S. Hawkins, Professor of Astronomy at Boston University, in 1963 and 1964 [3]. The first of these claimed the discovery of a number of additional alignments of astronomical significance, marked by pairs of stones and other features of the site; and the second suggested that the Aubrey Holes had been used as a neolithic 'computer' for the prediction of movements of the moon and of eclipses. Subsequently these theories received much wider publicity, in Britain as well as in the United States, through a CBS television programme, The Mystery of Stonehenge, which provided a superb example of partiality and tendentiousness in the presentation of an academic controversy.Professor Hawkins has now elaborated his ideas in a book whose title, Stonehenge Decoded, leaves no doubt of his confidence in the rightness of his conclusions-a confidence explicity echoed in his text. 'There can be no doubt that Stonehenge was an observatory; the impartial mathematics of probability and the celestial sphere are on my side' (p. vii). 'I think I have demonstrated beyond reasonable doubt that the monument was deliberately, accurately, skilfully oriented to the sun and the moon' (pp. 146-7). 'I think I have put forward the best theory to account for the otherwise unexplained holes' (p. 147). 'I think there is little else in these areas that can be discovered at Stonehenge'(p. 147).


Author(s):  
Brian Rogers ◽  
Stuart Anstis

When the sun is near the horizon and the moon is visible and higher in the sky, there is a compelling illusion that the sun is not in a direction perpendicular to the boundary between the lit and dark sides of the moon. This New Moon illusion has been observed and discussed previously but without a complete explanation. This chapter argues that both perceptual and cognitive factors contribute to the illusion and that it arises from the fact that the straight line joining the sun and the moon describes a great circle over the flattened dome of the sky. The New Moon illusion also raises the question of how we are able to judge the straightness of extended straight and parallel lines.


1962 ◽  
Vol 55 (4) ◽  
pp. 286-290
Author(s):  
E. S. Kennedy ◽  
Haydar Sharkas

The sun, in its daily trip overhead from the eastern horizon to the west, seems to travel along the arc of a circle on the celestial sphere. On the first day of spring, when the lengths of day and night are equal, the sun's path is a great circle, the celestial equator (Fig. 1). As the season advances, the sun moves slowly northward along the ecliptic, and its daily path is then, very nearly, one of the small circles which are parallel to the equator.


2018 ◽  
Vol 3 (2) ◽  
pp. 207-216 ◽  
Author(s):  
David Fisher ◽  
Lionel Sims

Claims first made over half a century ago that certain prehistoric monuments utilised high-precision alignments on the horizon risings and settings of the Sun and the Moon have recently resurfaced. While archaeoastronomy early on retreated from these claims, as a way to preserve the discipline in an academic boundary dispute, it did so without a rigorous examination of Thom’s concept of a “lunar standstill”. Gough’s uncritical resurrection of Thom’s usage of the term provides a long-overdue opportunity for the discipline to correct this slippage. Gough (2013), in keeping with Thom (1971), claims that certain standing stones and short stone rows point to distant horizon features which allow high-precision alignments on the risings and settings of the Sun and the Moon dating from about 1700 BC. To assist archaeoastronomy in breaking out of its interpretive rut and from “going round in circles” (Ruggles 2011), this paper evaluates the validity of this claim. Through computer modelling, the celestial mechanics of horizon alignments are here explored in their landscape context with a view to testing the very possibility of high-precision alignments to the lunar extremes. It is found that, due to the motion of the Moon on the horizon, only low-precision alignments are feasible, which would seem to indicate that the properties of lunar standstills could not have included high-precision markers for prehistoric megalith builders.


1967 ◽  
Vol 71 (2) ◽  
pp. 215
Author(s):  
Earle R. Caley ◽  
Andre Emmerich
Keyword(s):  
The Sun ◽  

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