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A Brief guide to the night Skies for those who know nothing
A Brief guide to the night Skies for those who know nothing

... Our planet - the Earth - is one of nine bodies travelling around our local star, which we call the Sun. The word "planet" comes from a Greek word which means, "wandering star". A PLANET is a relatively small body which revolves round a star and which does not emit light produced by internal nuclear ...
Vast Spaces Of The Universe
Vast Spaces Of The Universe

... worldly-minded politicians and money- The common snail,. Helix aspersa, lays merchants look mean and feeble. from forty to a hundred, inlittlenests at His text was " Seek ye first the King- the roots of grass. dom of God and His righteousness," and How does a Snipe Bleat? The bleating, or drumming, ...
The Night Sky This Month - Usk Astronomical Society
The Night Sky This Month - Usk Astronomical Society

... The Moon is at perigee (nearest Earth) on the 22nd and at apogee (most distant from Earth) on the 10th. * The names of moons were, at one time, associated with the names of the lunisolar months. The Romans, with the Julian calendar, helped to decouple that tradition. It is only in recent times that ...
1 WHY DO THE STARS IN ORION LOOK SO DIFFERENT FROM
1 WHY DO THE STARS IN ORION LOOK SO DIFFERENT FROM

... Luminosity shows the relationship of stars’ radii and surface temperature. Each of the stars in Table 1 is many times more luminous than our sun, and emits enormous amounts of energy. Luminosity is related to a stars surface area and temperature. Two stars having the same temperature and size will b ...
Sky & Astronomy - Wayne State University Physics and Astronomy
Sky & Astronomy - Wayne State University Physics and Astronomy

... the approximate length of the year The Mayans of Central America developed a calendar based on the planet Venus In the British Isles, one finds spectacular monuments (such as Stonehenge) that, one now believes, were used to track the motion of the Sun and the Moon Pythagoras already suggested (2500 ...
K - College of San Mateo
K - College of San Mateo

... SBIG Self Guiding Spectrograph (SGS) ___________________________________________________ ...
Session 2 - Early Autum Sky
Session 2 - Early Autum Sky

... When astronomers measure positions on the night sky, they use a coordinate system just like you find on maps of the earth which use latitude and longitude. Most of us use miles (or kilometers) to measure the separation between places on earth, but this won't work for the sky. Instead, we must use an ...
H-R Diagram - SFA Physics
H-R Diagram - SFA Physics

... Now plot all the stars from Table 7 onto Figure 3. Table 7 is a list of the 30 stars nearest the sun and the majority of these stars are considered to be the most common types of stars in the galaxy. Transfer the main sequence curve from Figure 1 to Figure 3. ...
Clear Skies - Cowichan Valley Starfinders Society
Clear Skies - Cowichan Valley Starfinders Society

... I have a little more information regarding the Cowichan 2008 North American Indigenous Games to be held in Duncan. A proposal has been sent to the Games Committee to hold the event at the Centre of the Universe/DAO. We are awaiting a response from the games committee. I think that this is a great op ...
Life Cycle of Stars
Life Cycle of Stars

... If the remaining mass of the star is more than about three times that of the Sun, it will collapse so completely that it will literally disappear from the universe. What is left behind is an intense region of gravity called a black hole ...
good - Cosmos
good - Cosmos

... to Mars is deduced, it is fitting that we accept with grateful minds this gift from God, and both acknowledge and build upon it. Hence, let us work upon it so as to at last track down the real form of celestial ...
1. dia - uri=members.iif
1. dia - uri=members.iif

... of the Sun, the Moon, and the planets. His measurements were more accurate, than the earlier data.  The result was, that neither Ptolemy’s Earthcentred theory nor Copernicus’s Sun-centered theory agreed with Brahe`s data. ...
It is evident from our observations of impact craters on planets and
It is evident from our observations of impact craters on planets and

... Stellar (heliocentric) parallax was used for determining distances to stars in Lab # 6. But the heliocentric parallax method breaks down beyond 100 parsecs (300 LY). In space, telescopes have increased our ability to use the stellar parallax method out to nearly 1000 parsecs. The presence of spectra ...
Lecture18
Lecture18

... and is now used by every country in the world EXCEPT the US The basic unit of length was defined at the meter and was based on a bar of platinum-iridium metal In 1960, the definition of the meter was changed to be 1,650,763.73 wavelengths of an atomic transition in krypton-86 In 1983, the meter was ...
Astronomy and Space Science
Astronomy and Space Science

... C rises barely above the eastern horizon, moves along the southern horizon, and sets in the West D rises straight up in the East, passes directly overhead, and descends straight down in the West 13 Parallax can be used to measure a star’s— ...
Problem Set 1, due Sep 4
Problem Set 1, due Sep 4

Lab Writeup
Lab Writeup

... The procedure consists of estimating the angular sizes of objects viewed through the eyepiece of our refractor telescopes. At least two eyepieces will be used. The first will have a fairly large field of view. The second will have higher magnification, and has a scale which allows you to fairly accu ...
SR Stellar Properties
SR Stellar Properties

... Scientists began to learn about stars by observing properties of stars, including brightness and color. Astronomers tried to make sense of the star data by grouping together stars with similar properties. The Hertzsprung-Russell diagram provides a way to group similar stars. The H-R diagram is a gra ...
Chapter 4
Chapter 4

... of the sky the primary mirror is made with spherical curvature and an aspheric `corrector plate' is placed at the top end of the telescope tube. There are three large Schmidt telescopes in the world with fields about 6° across (the Moon's apparent diameter in the sky is half a degree). The oldest of ...
Harappan Astronomy
Harappan Astronomy

... Harappan culture evolved and merged and transformed over this period (Gangal et al., 2011), and it also went through a complex evolutionary pattern (Vahia and Yadav, 2011a). It was the most advanced preiron civilisation in the world. It is no surprise, therefore, that the Harappans had a vibrant int ...
Northern and Southern Hemisphere Star Chart
Northern and Southern Hemisphere Star Chart

... Stars come in different brightnesses, sizes and colours. Look out at the sky tonight and you will see how stars vary in brightness. Some are bright because they are relatively close to us, while others are bright because they are thousands of times brighter than our own nearby Sun. Find the easily-s ...
Summer Triangle (Winter in the south hemisphere) Lyra
Summer Triangle (Winter in the south hemisphere) Lyra

... The tale of the Lyre then passes to Orpheus. Apollo became entranced by the songs of the great musician Orpheus and gave him the instrument so that Orpheus could accompany his words. Orpheus is said to have been so grateful for the instrument that he would often seek a high mountain before sunrise, ...
Frostburg State Planetarium presents
Frostburg State Planetarium presents

... • Sun sets near direction West as we turn. • To find North, face where sun goes down and extend your right arm out, points North. ...
Charcteristic of Stars Powerpoint C
Charcteristic of Stars Powerpoint C

... • The brightness of a star depends on both its size and temperature. A larger star tends to be brighter than a smaller star. A hotter star tends to be brighter than a cooler star. • How bright a star appears depends on both its distance from Earth and how bright the star truly is. Because of these t ...
Celestial Equator
Celestial Equator

... • The arctic circle is the parallel of latitude located 23.5° from the north pole; i.e., 90° - 23.5° = 66.5°. • Within (north of) the arctic circle, the Sun becomes circumpolar around the time of the summer solstice. (“Land of the Midnight Sun”.) • Conversely, near the winter solstice, the Sun remai ...
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Chinese astronomy



Astronomy in China has a very long history, with historians indicating that the Chinese were the most persistent and accurate observers of celestial phenomena anywhere in the world before the Arabs. Star names later categorized in the twenty-eight mansions have been found on oracle bones unearthed at Anyang, dating back to the middle Shang Dynasty (Chinese Bronze Age), and the mansion (xiù:宿) system's nucleus seems to have taken shape by the time of the ruler Wu Ding (1339-1281 BC).Detailed records of astronomical observations began during the Warring States period (fourth century BC) and flourished from the Han period onward. Chinese astronomy was equatorial, centered as it was on close observation of circumpolar stars, and was based on different principles from those prevailing in traditional Western astronomy, where heliacal risings and settings of zodiac constellations formed the basic ecliptic framework.Some elements of Indian astronomy reached China with the expansion of Buddhism after the Eastern Han Dynasty (25–220 AD), but the most detailed incorporation of Indian astronomical thought occurred during the Tang Dynasty (618-907), when numerous Indian astronomers took up residence in the Chinese capital, and Chinese scholars, such as the great Tantric Buddhist monk and mathematician Yi Xing, mastered its system. Islamic astronomers collaborated closely with their Chinese colleagues during the Yuan Dynasty, and, after a period of relative decline during the Ming Dynasty, astronomy was revitalized under the stimulus of Western cosmology and technology after the Jesuits established their missions. The telescope was introduced in the seventeenth century. In 1669, the Peking observatory was completely redesigned and refitted under the direction of Ferdinand Verbiest. Today, China continues to be active in astronomy, with many observatories and its own space program.
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