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An Introduction To Parallax
An Introduction To Parallax

Drawing Constellations
Drawing Constellations

... her chair, spending half the year upside down. As for Cepheus, Poseidon gave him a number of medium sized stars that go to make his square face with a pointed crown. ...
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... a. along the ecliptic. b. along the celestial equator. c. near the south celestial pole. d. at mid and northern celestial latitudes. e. uniformly around the celestial sphere 2. Which statement below most accurately describes modern constellations? a. They are 88 well defined regions on the celestial ...
30-1 - Fremont Peak Observatory Association
30-1 - Fremont Peak Observatory Association

... more successful than the 2012 season. The season starts on the first Saturday in April and continues with up to 20 programs on the most suitable Saturday evenings through the last week of October. In addition there are 8 monthly solar viewing programs on New Moon Saturday afternoons from March to Oc ...
LARRY MARSCHALL CLEA
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Astronomical Motions I: The Night Sky

... difficult to convince yourself that the altitude of the pole star is equal to the latitude of the observer. Notice that in each diagram the observer’s horizon is shown; it is represented by a tangent plane to Earth’s surface at the point where the observer is standing. Objects below the observer’s h ...
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iStage2_EN_iSky smart measurements of the heaven

Astronomy Scope and Sequence 1st Quarter 1) Scientific processes
Astronomy Scope and Sequence 1st Quarter 1) Scientific processes

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... infrared data: Small clouds appear to decompose into only two or three fragments, each of which may be some two or three times as massive as the sun. At the other extreme, there are huge clouds— cosmic overcasts—which disintegrate into a dozen pieces or more. Some of the pieces are the equivalent of ...
The Sky Tonight - Northern Stars Planetarium
The Sky Tonight - Northern Stars Planetarium

... Constellations: Imaginary, dot-to-dot pictures drawn using the stars as the dots. These are used to map the night-time sky. There are 88 constellations all together. Forty-eight are of Greek origin the rest are a collection from various cultures worldwide. Light Year: A light year is the distance th ...
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... Tiamat (number 11) is between Mars (number 4) and Saturn (number 10). That is precisely the positioning of Tiamat before it exploded. Furthermore, Luna (number 2) is depicted next to Terra (number 6). That is precisely the current positioning of Luna. Before Tiamat exploded and became the current as ...
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... modest telescope.[19] The name of the star Aldebaran most likely comes from the fact that it follows the Pleiades during the nightly motion of the celestial sphere across the sky. Astronomers estimate that the cluster has approximately 500-1,000 stars, all of which are around 100 million years old. ...
End of the line for a star like ours
End of the line for a star like ours

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THE CONSTELLATION OCTANS, THE OCTANT

... Sigma Octantis is currently the southern pole star, and is sometimes known by the name Polaris Australis. It is the counterpart to Polaris in Ursa Minor, the northern pole star. Sigma Octantis is 25 times fainter than the North Star, which makes it too dim to be used for navigation, so it is the Sou ...
Warm-Up Monday, July 23, 2012
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... – Next brightest beta and so on ...
MS PowerPoint - National Schools` Observatory
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Latitude and Longitude in the Northern Hemisphere worksheet
Latitude and Longitude in the Northern Hemisphere worksheet

... of London where, on top of a hill at the old Royal Observatory you will find the line that divides the hemispheres. This is the position from which Greenwich Mean Time is derived. The line splitting the two hemispheres is invisible, by the way. But in the forecourt of the observatory in front of one ...
Volume 19 Issue 1 – January/February 2017 Edition
Volume 19 Issue 1 – January/February 2017 Edition

... result wads that Kepler determined that Mars orbited the Sun in an ellip cal orbit. And, it was  from this star ng point that Kepler subsequently concluded that all the planets revolve  around the Sun in some kind of oval or ellip cal paths. This discovery and his related laws of  planetary mo on is ...
Bolton-Stanley Cosmic Noise Expedition to New Zealand
Bolton-Stanley Cosmic Noise Expedition to New Zealand

... • The parameters of the exhibition (location, time of year, horizon etc ) determined by Cygnus A – only reached 15 deg above the horizon in the north – above the horizon for only 7 hours per day. The other radio objects were almost an after thought • The fact that it is far north from Australia and ...
After School Guide to Ology Astronomy
After School Guide to Ology Astronomy

Distance Between Stars - cK-12
Distance Between Stars - cK-12

second grade - Math/Science Nucleus
second grade - Math/Science Nucleus

Cataclysmic Variable Stars
Cataclysmic Variable Stars

... from ~ 5000 K at its outer edge to ~ few x 10^4 K at its inner edge, it radiates over a broad energy range from the optical through the far ultraviolet. Because of the small size and high luminosity of the boundary layer, its temperature is significantly higher than that of the accretion disk. When ...
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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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