Eclipses Have Advanced Our Knowledge of the Sciences in More Ways Than One
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I. ASYMMETRY of ECLIPSES. CALENDAR CYCLES Igor Taganov & Ville-V.E
I. ASYMMETRY OF ECLIPSES. CALENDAR CYCLES Igor Taganov & Ville-V.E. Saari 1.1 Metaphysics of solar eclipses p. 12 1.2 Calendar cycles of solar eclipses p. 20 Literature p. 26 To describe the two main types of solar eclipses in modern astronomy the old Latin terms – umbra, antumbra and penumbra are still used (Fig. 1.1). A “partial eclipse” (c. 35 %) occurs when the Sun and Moon are not exactly in line and the Moon only partially obscures the Sun. The term “central eclipse” (c. 65 %) is often used as a generic term for eclipses when the Sun and Moon are exactly in line. The strict definition of a central eclipse is an eclipse, during which the central line of the Moon’s umbra touches the Earth’s surface. However, extremely rare the part of the Moon’s umbra intersects with Earth, producing an annular or total eclipse, but not its central line. Such event is called a “non-central” total or annular eclipse [2]. Fig. 1.1. Main types of solar eclipses The central solar eclipses are subdivided into three main groups: a “total eclipse” (c. 27 %) occurs when the dark silhouette of the Moon completely obscures the Sun; an “annular eclipse” (c. 33 %) occurs when the Sun and Moon are exactly in line, but the apparent size of the Moon is smaller than that of the Sun; a “hybrid eclipse” or annular/total eclipse (c. 5 %) at certain sites on the Earth’s surface appears as a total eclipse, whereas at other sites it looks as annular. -
Roll 5, Side A
doi: 10.1038/nature07130 SUPPLEMENTARY INFORMATION Correction notice Calendars with Olympiad display and eclipse prediction on the Antikythera Mechanism Tony Freeth, Alexander Jones, John M. Steele & Yanis Bitsakis Nature 454, 614–617 (2008) In the version of the Supplementary Information originally posted online, there were minor errors in Supplementary Figs 20 and 25. In Supplementary Fig. 20, some glyphs were accidently omitted between months 26 and 67; in Supplementary Fig. 25, seven glyphs in the left-hand semicircle were inscribed one month too early. These have been corrected in the new version of the Supplementary Information; see Supplementary Information Table of Contents for details. doi: 10.1038/nature07130 SUPPLEMENTARY INFORMATION Calendars with Olympiad display and eclipse prediction on the Antikythera Mechanism SUPPLEMENTARY NOTES Tony Freeth1,2, Alexander Jones3, John M. Steele4 & Yanis Bitsakis1,5 1 Antikythera Mechanism Research Project, 3 Tyrwhitt Crescent, Roath Park, Cardiff CF23 5QP, UK. 2 Images First Ltd, 10 Hereford Road, South Ealing, London W5 4SE, UK. 3 Institute for the Study of the Ancient World, 15 East 84th Street, New York, NY 10028, USA. 4 Department of Physics, University of Durham, Rochester Building, South Road, Durham DH1 3LE, UK. 5 Centre for History and Palaeography, 3, P. Skouze str., GR-10560 Athens, Greece www.nature.com/nature doi: 10.1038/nature07130 SUPPLEMENTARY INFORMATION Calendars with Olympiad display and eclipse prediction on the Antikythera Mechanism Supplementary Notes Table of Contents TABLE OF CONTENTS 1. OVERVIEW OF THE ANTIKYTHERA MECHANISM 1 1.1 The Fragments 1 1.2 The Architecture of the Mechanism 1 2. DATA ACQUISITION & ANALYSIS 4 2.1 Data Acquisition 4 2.2 Data Analysis 5 3. -
Geminos and Babylonian Astronomy
Geminos and Babylonian astronomy J. M. Steele Introduction Geminos’ Introduction to the Phenomena is one of several introductions to astronomy written by Greek and Latin authors during the last couple of centuries bc and the first few centuries ad.1 Geminos’ work is unusual, however, in including some fairly detailed—and accurate—technical information about Babylonian astronomy, some of which is explicitly attributed to the “Chal- deans.” Indeed, before the rediscovery of cuneiform sources in the nineteenth century, Gem- inos provided the most detailed information on Babylonian astronomy available, aside from the reports of several eclipse and planetary observations quoted by Ptolemy in the Almagest. Early-modern histories of astronomy, those that did not simply quote fantastical accounts of pre-Greek astronomy based upon the Bible and Josephus, relied heavily upon Geminos for their discussion of Babylonian (or “Chaldean”) astronomy.2 What can be learnt of Babylonian astron- omy from Geminos is, of course, extremely limited and restricted to those topics which have a place in an introduction to astronomy as this discipline was understood in the Greek world. Thus, aspects of Babylonian astronomy which relate to the celestial sphere (e.g. the zodiac and the ris- ing times of the ecliptic), the luni-solar calendar (e.g. intercalation and the 19-year (“Metonic”) cycle), and lunar motion, are included, but Geminos tells us nothing about Babylonian planetary theory (the planets are only touched upon briefly by Geminos), predictive astronomy that uses planetary and lunar periods, observational astronomy, or the problem of lunar visibility, which formed major parts of Babylonian astronomical practice. -
The Moon and Eclipses
The Moon and Eclipses ASTR 101 September 14, 2018 • Phases of the moon • Lunar month • Solar eclipses • Lunar eclipses • Eclipse seasons 1 Moon in the Sky An image of the Earth and the Moon taken from 1 million miles away. Diameter of Moon is about ¼ of the Earth. www.nasa.gov/feature/goddard/from-a-million-miles-away-nasa-camera-shows-moon-crossing-face-of-earth • Moonlight is reflected sunlight from the lunar surface. Moon reflects about 12% of the sunlight falling on it (ie. Moon’s albedo is 12%). • Dark features visible on the Moon are plains of old lava flows, formed by ancient volcanic eruptions – When Galileo looked at the Moon through his telescope, he thought those were Oceans, so he named them as Marias. – There is no water (or atmosphere) on the Moon, but still they are known as Maria – Through a telescope large number of craters, mountains and other geological features visible. 2 Moon Phases Sunlight Sunlight full moon New moon Sunlight Sunlight Quarter moon Crescent moon • Depending on relative positions of the Earth, the Sun and the Moon we see different amount of the illuminated surface of Moon. 3 Moon Phases first quarter waxing waxing gibbous crescent Orbit of the Moon Sunlight full moon new moon position on the orbit View from the Earth waning waning gibbous last crescent quarter 4 Sun Earthshine Moon light reflected from the Earth Earth in lunar sky is about 50 times brighter than the moon from Earth. “old moon" in the new moon's arms • Night (shadowed) side of the Moon is not completely dark. -
Lecture 2: Our Place in Space Copernican Principle Multiwavelength Astronomy
Lecture 2: Our Place in Space •It is now clear that Earth is not central or special in its general properties (mass, distance from central star, etc.) •The Sun is an average star •The Milky Way is a typical spiral galaxy •This leads to the “principle of mediocrity” or “Copernican principle” Copernican Principle •The “principle of mediocrity” or “Copernican principle” states that physical laws are the same throughout the Universe •This principle can be tested using the scientific method! •So far, it seems to agree with observations perfectly •One of the key ideas is that we can use light from distant objects to understand conditions there, using the work of Isaac Newton Multiwavelength Astronomy •The color and energy of light are related to the Wavelength… •Different wavelengths of radiation tell us about objects with different temperatures… 1 Multiwavelength Astronomy Multiwavelength Astronomy •Using Newton’s techniques, combined with our knowledge of atomic structure, we can use light to study distant objects… X-ray optical composition of matter temperature of matter Scientific Method and Observation •Transformed the search for meaning into a quest for objective truth •We can deduce the properties of distant objects using observations •The scientific method originated in the renaissance, and is still used today: hypo thesi n s io tti iic d e r y p y p r r o o e o truth e truth h b h t s t e rr v a tt ii o n test 2 Copernican Principle •The validity of the “Copernican principle” is great news for science, because it means that we can -
The Draconic Gearing of the Antikythera Mechanism: Assembling the Fragment D, Its Role and Operation
The Draconic gearing of the Antikythera Mechanism: Assembling the Fragment D, its role and operation A.Voulgaris1, C.Mouratidis2, A.Vossinakis3, G.Bokovos4 (Submitted 14 January 2020) 1Municipality of Thessaloniki, Directorate Culture and Tourism, Thessaloniki, GR-54625, Greece 2Hellenic Ministry of Education, Research and Religious Affairs, Kos, GR-85300, Greece 3Thessaloniki Astronomy Club, Thessaloniki, GR-54646, Greece 4Thessaloniki Science Center and Technology Museum-Planetarium, Thermi, GR-57001, Greece Abstract The unplaced Fragment D of the Antikythera Mechanism with an unknown operation was a mystery since the beginning of its discovery. The gear-r1, which was detected on the Fragment radiographies by C. Karakalos, is preserved in excellent condition, but this was not enough to correlate it to the existing gear trainings of the Mechanism. The suggestion that this gear could be a part of the hypothetical planet indication gearing is still a hypothesis since no mechanical evidence has been preserved. After the analysis of AMRP tomographies of Fragment D and its mechanical characteristics revealed that it could be part of the Draconic gearing. Although the Draconic cycle was well known during the Mechanism’s era as represents the fourth Lunar cycle, it seems that it is missing from the Antikythera Mechanism. The study of Fragment D was supported by the bronze reconstruction of the Draconic gearing by the authors. The adaptation of the Draconic gearing on the Antikythera Mechanism improves its functionality and gives answers on several questions. 1. Introduction. The Antikythera Mechanism, a geared machine based on the lunar cycles The Antikythera Mechanism a creation of an ingenious manufacturer of the Hellenistic era was a geared machine capable of performing complex astronomical calculations, mostly based on the lunar periodic cycles. -
Born During a Solar Eclipse Season
ECLIPSES July 2 Solar Eclipse @ 10 Cancer & July 16 Lunar Eclipse @ 25 Capricorn stepping back and looking at the geometry of Brady suggests interpreting the natal Born During a how eclipses occur, not on the individual level chart or life of someone born in an Eclipse but rather on the larger cyclic playing field Season, assuming that this particular indi- of life. For each seemingly isolated eclipse vidual connects more deeply to that Saros Solar Eclipse belongs to a larger pattern, each eclipse is a Series and its meaning. member of a family and each family has par- She gives us in her book Predictive ticular characteristics” (Brady, B: 2005:1) Astrology: The Eagle and the Lark, a detailed Season: The larger pattern mentioned above is list of Solar Saros series between 1900 and what we call a Saros Series. A Saros Series 2050, with the commencement date of that Salvador Allende alludes to a recurrence in which the Sun series and the planetary positions at that and the Moon return to approximately the moment, the tightest aspects also between by Alice Thomas same position in their orbits where eclipses planets and midpoints and offers a tenta- can happen. tive delineation. ny Eclipse occurs Saros, a name coined by Suidas, (10th Everyone born 18 and a half days before at times of syzygy century AD) means something to be a Solar Eclipse and 18 and a half days later during a plane- repeated. This recurring pattern or repeti- is born during Eclipse Season, and theo- A tion occurs approximately every 18 years retically could be connected to this Saros tary alignment between the Sun, the Moon, and and 11 days (or 223 lunations), but the Series pattern. -
Different Types of Solar Eclipses
Solar Eclipse Background Information Different types of solar eclipses What is a solar eclipse? • A total eclipse occurs when the dark silhouette of the Moon A solar eclipse occurs when the moon passes in a direct line between completely obscures the intensely bright light of the Sun, the Earth and the sun. The moon's shadow travels over the Earth's allowing the much fainter solar corona to be visible. surface and blocks out the sun's light as seen from Earth. • An annular eclipse occurs when the Sun and Moon are exactly in line, but the apparent size of the Moon is smaller than that of Why isn’t there a solar eclipse every month? the Sun. Hence the Sun appears as a very bright ring Because the moon orbits the Earth at an angle, approximately 5 surrounding the dark disk of the Moon. degrees relative to the Earth-sun plane, the moon crosses the Earth's • A hybrid eclipse shifts between a total and annular eclipse. At orbital plane only twice a year. These times are called eclipse seasons, certain points on the surface of Earth it appears as a total because they are the only times when eclipses can occur. For an eclipse, whereas at other points it appears as annular. Hybrid eclipse to take place, the moon must be in the correct phase during an eclipses are comparatively rare. eclipse season; for a solar eclipse, it must be a new moon. This • A partial eclipse occurs when the Sun and Moon are not condition makes solar eclipses relatively rare. -
Eclipse Season Starts for NASA's SDO 13 February 2018
Eclipse season starts for NASA's SDO 13 February 2018 Most spacecraft observing the Sun from an orbit around Earth have to contend with such eclipses. SDO's orbit is designed to maximize the amount of data the spacecraft can send back to Earth, but twice a year Earth gets in the way of the spacecraft's view. The spring eclipse season began on Feb. 10 with a partial eclipse and concludes March 5, 2018. Provided by NASA's Goddard Space Flight Center On Sunday, Feb. 11, 2018, NASA's SDO saw a total solar eclipse in space. These images were taken in a wavelength of extreme ultraviolet light, a type of light that is typically invisible to our eyes, but is colorized here in purple. Credit: NASA's Goddard Space Flight Center/SDO/Joy Ng On Sunday, Feb. 11, 2018, NASA's Solar Dynamics Observatory, or SDO, saw a total solar eclipse in space when Earth crossed its view of the Sun. Also known as a transit, Earth's passage was brief, lasting from 2:10 a.m. to 2:41 a.m. EST and covering the entire face of the Sun. So marks the beginning of SDO's eclipse season—as well as the mission's eighth launch anniversary. SDO's eclipse season is a three-week period that comes twice a year near the equinoxes during which Earth blocks SDO's view of the Sun for a short while each day. The eclipses are fairly short near the beginning and end of the season but ramp up to 72 minutes in the middle. -
1. OVERVIEW of the ANTIKYTHERA MECHANISM 1 1.1 the Fragments 1 1.2 the Architecture of the Mechanism 1
doi: 10.1038/nature07130 SUPPLEMENTARY INFORMATION Calendars with Olympiad display and eclipse prediction on the Antikythera Mechanism SUPPLEMENTARY NOTES Tony Freeth1,2, Alexander Jones3, John M. Steele4 & Yanis Bitsakis1,5 1Antikythera Mechanism Research Project, 3 Tyrwhitt Crescent, Roath Park, Cardiff CF23 5QP, UK. 2Images First Ltd, 10 Hereford Road, South Ealing, London W5 4SE, UK. 3Institute for the Study of the Ancient World, 15 East 84th Street, New York, NY 10028, USA. 4Department of Physics, University of Durham, Rochester Building, South Road, Durham DH1 3LE, UK. 5Centre for History and Palaeography, 3, P. Skouze str., GR-10560 Athens, Greece www.nature.com/nature 1 doi: 10.1038/nature07130 SUPPLEMENTARY INFORMATION Calendars with Olympiad display and eclipse prediction on the Antikythera Mechanism Supplementary Notes Table of Contents TABLE OF CONTENTS 1. OVERVIEW OF THE ANTIKYTHERA MECHANISM 1 1.1 The Fragments 1 1.2 The Architecture of the Mechanism 1 2. DATA ACQUISITION & ANALYSIS 4 2.1 Data Acquisition 4 2.2 Data Analysis 5 3. METONIC, OLYMPIAD & CALLIPPIC DIALS 6 3.1 Fragments that witness the Back Dials 6 3.2 The Calendar of the Metonic spiral 7 3.3 Structure of the Calendar 12 3.4 The Calendar's Provenance 14 3.5 The Olympiad Dial 19 3.6 Gearing for the Olympiad Dial 22 3.7 The Callippic Dial 23 3.8 Reconstruction of the Upper Back Dials 23 4. SAROS & EXELIGMOS DIALS 24 4.1 The Saros Dial & the Glyphs 24 4.2 Matching the Glyphs with Observations 29 4.3 Babylonian Schemes for Eclipse Prediction 31 4.4 Alphabetical Index Letters 32 4.5 Models for generating the Antikythera Glyph Sequence 33 4.6 The Problem of the Glyph Times 37 4.7 The Four-Turn Saros Dial 39 4.8 The Exeligmos Dial 40 4.9 Reconstruction of the Lower Back Dials 41 5. -
W:09/19/18 Eclipses
PHYS 1411 Intro to Astronomy Extra Credit Homework Announcement Assigned on MindTap for Chapter 1, 2, 3 Due Monday December 3rd , 2018 @ 5:00 am Topics for Today’s Class Topics for Today’s Class • Chapter 3: Lunar Eclipse • Chapter 3: Solar eclipse – How to make a shadow or an eclipse? – What is a Solar eclipse? – Types of shadows – How to safely observe Solar eclipse – The importance of angular diameter in – Types of Solar eclipse eclipses – Some examples and dates – What is a Lunar eclipse? – Conditions for Solar and Lunar eclipses to – Types of Lunar eclipses occur – Why Pinkish Moon during Lunar eclipse? – Saros Cycle The Angular Diameters of the How to make a shadow? Sun & Moon • The shadow cast by a map tack can be used to understand how shadows produce eclipses – Umbra = The region of total shadow – Penumbra = The region of partial shadow – Penumbra = The region of partial shadow 1 Angular Size and Distance Two Types of Movements Increasing Distance from Eye Dime Quarter Partial Total Annular Not Visible Transit Occultation View from Eye View from Eye What is a Lunar Eclipse? Small Angle Formula Earth’s shadow consists of a zone of partial angular diameter linear diameter shadow, the Penumbra, 206,265 distance and a zone of full shadow, Example for Moon the Umbra. angular diameter 3476 km 206,26 5 384,000 km 1870 angular diameter 187 0 0.5 60 60 If the moon passes through Earth’s full shadow (Umbra), we see a lunar eclipse. If the entire surface of the moon enters Angular Diameter of Sun and Moon is important for Eclipses to occur the Umbra, the lunar eclipse is total. -
Five Millennium Canon of Lunar Eclipses: –1999 to +3000 (2000 BCE to 3000 CE)
NASA/TP–2009–214172 Five Millennium Canon of Lunar Eclipses: –1999 to +3000 (2000 BCE to 3000 CE) Fred Espenak and Jean Meeus January 2009 COVER CAPTION: Basic lunar eclipse geometry is illustrated in this figure from “New Astronomy” by David Todd (1906). The NASA STI Program Offi ce … in Profi le Since its founding, NASA has been ded i cated to the • CONFERENCE PUBLICATION. Collected ad vancement of aeronautics and space science. The pa pers from scientifi c and technical conferences, NASA Sci en tifi c and Technical Information (STI) symposia, sem i nars, or other meetings spon sored Pro gram Offi ce plays a key part in helping NASA or co spon sored by NASA. maintain this impor tant role. • SPECIAL PUBLICATION. Scientifi c, techni cal, The NASA STI Program Offi ce is operated by or historical information from NASA pro grams, Langley Research Center, the lead center for projects, and mission, often concerned with sub- NASA’s scientifi c and technical infor ma tion. The jects having substan tial public interest. NASA STI Program Offi ce pro vides ac cess to the NASA STI Database, the largest collec tion of • TECHNICAL TRANSLATION. En glish-language aero nau ti cal and space science STI in the world. trans la tions of foreign scien tifi c and techni cal ma- The Pro gram Offi ce is also NASA’s in sti tu tion al terial pertinent to NASA’s mis sion. mecha nism for dis sem i nat ing the results of its research and devel op ment activ i ties.