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Distance, Size, and Temperature of a Star
Distance, Size, and Temperature of a Star

... brighter than an entire galaxy, and can be seen from very far away. Because blue giant stars only live a short time, scientists use them to find places in outer space where new stars are forming. Remember when we talked about sun-sized stars? We said that at the end of their lives these stars expand ...
The HR Diagram (PowerPoint version)
The HR Diagram (PowerPoint version)

... Note that there are stars of all spectral types, from OB (hot) to M (cool) There are only a few quite bright stars (near the top) but lots of faint ones. (The bottom, magnitude 6, is the limit of the human eye.) There is no particular pattern: there are bright and faint hot stars, and bright and fai ...
Word Document - University of Iowa Astrophysics
Word Document - University of Iowa Astrophysics

... This lab exercise does not require a formal writeup. Data taking, drawings, and calculations are to be entered on this form and handed to the teaching assistant. However, you need to preserve your results for later in the semester when you will measure angular sizes of other objects, then use known ...
The Scale of the Cosmos
The Scale of the Cosmos

... • Lunar eclipses always occur at full moon but not at every full moon. • The Moon's orbit is tipped about 5 degrees to the ecliptic. • So, most full moons cross the sky north or south of Earth’s shadow and there is no lunar eclipse that month. • For the same reason, solar eclipses always occur at ne ...
PDF format - Princeton University Press
PDF format - Princeton University Press

... underworld. The vault of heaven remains forever fixed; the sun, the moon, and the stars move round under it, rising from Oceanus in the east and plunging into it again in the west. We are not told what happens to the heavenly bodies between their setting and rising. They cannot pass under the earth, ...
The Sun - Our Star
The Sun - Our Star

... Dark spots on the Sun were first reported by the Chinese in the 5th century B.C. Galileo and Thomas Harriott were the first Europeans to report these sunspots in the early 17th century. In 1851, Schwabe discovered the sunspot cycle, which lasts about 11 years. This periodic cycle, however, is not al ...
Celestial Navigation
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... Instances where electronic failure due lighting strikes, flooding and other disasters are often documented. Even battery-powered handheld equipment can fail when the batteries run out. Hence it’s advantageous to have some knowledge of celestial navigation for back up purposes. Furthermore celestial ...
Lesson #4: The Moon and its Phases
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PERMANENTLY SHADOWED AREAS AT THE LUNAR POLES
PERMANENTLY SHADOWED AREAS AT THE LUNAR POLES

... According to our estimates the permanently shaded areas in these craters is about 50 km2. The most enhanced hydrogen near North Pole is overlain the heavily cratered region near the crater Rozhdestvensky. There are many small craters, which could contain water ice deposits. Hydrogen is enhanced in s ...
Blocking Starlight Much Closer to Home 2: This Year`s
Blocking Starlight Much Closer to Home 2: This Year`s

... magnitude star than to find a ring around Pluto or to discover a moon. Anyway, we have the light curve of an occultation by that 15th magnitude star, which was the typical brightness of our occultation stars that we were observing anyway. We are about to submit a paper to the Astronomical Journal a ...
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... linked to distance from the Sun, ask how seasons differ between the two hemispheres. They should then see for themselves that it can’t be distance from the Sun, or seasons would be the same globally rather than opposite in the two hemispheres. • As a follow-up on the above note: Some students get co ...
October 2012 - astronomy for beginners
October 2012 - astronomy for beginners

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... constellations and asterisms on the sky in a coordinate framework, provided for general reference. Figure B.1 is bisected by the celestial equator into northern and southern halves. The chart is a Mercator projection4 of a variant of the equatorial system, one way of viewing the celestial sphere ind ...
Principal Features of the Sky
Principal Features of the Sky

Lecture 1a: Class overview and Early Observations 8/27
Lecture 1a: Class overview and Early Observations 8/27

... Length of Day and Month are changing •  Friction between the Earth and the Moon (seen daily in tides) •  Day becomes .002 seconds longer each century •  Moon receding from the Earth by 4 cm each year 500,000,000 years ago there were 22 hours in a day 400 days in a year Billions of years in the futu ...
Astronomy 114 - Department of Astronomy
Astronomy 114 - Department of Astronomy

June 2015 - Bristol Astronomical Society
June 2015 - Bristol Astronomical Society

... month in Cancer but moves into Leo on the 9th of June in its eastwards progress towards the star Regulus. Our best views of the planet are now past but, with a small telescope one may be able to see the equatorial bands in the atmosphere and up to four of the Gallilean moons as they weave their way ...
chapter 7
chapter 7

I Cloudy with a Chance of Making a star is no easy thing
I Cloudy with a Chance of Making a star is no easy thing

... located in the constellation Aquila. Its density structure is just what would be expected if the cloud’s thermal pressure were nearly in equilibrium with external pressure. An infrared source in the center may be an early-stage protostar, suggesting that the balance recently tilted in favor of colla ...
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Laws of planets motion

... words over and over again: "Let me not seem to have lived in vain." ...
DSLR photometry - British Astronomical Association
DSLR photometry - British Astronomical Association

Fulltext PDF - Indian Academy of Sciences
Fulltext PDF - Indian Academy of Sciences

... does not return to the same point after its daily cycle for instance, (unlike typical star-rises) the Sun rises at different spots on successive days. We give. a concrete example to illustrate the Sun's resultant path. Suppose that, at some instant, the Sun is at the point of intersection of the cel ...
Observing Jupiter and Saturn with a Vixen 80mm Fluorite Refractor
Observing Jupiter and Saturn with a Vixen 80mm Fluorite Refractor

... It sounds like an impossible task: Take a star a hundred times larger in diameter and millions of times more luminous than the Sun and hide it in our own galaxy where the most powerful optical telescopes on Earth cannot find it. But it is not impossible. In fact, there could be dozens to hundreds of ...
Chapter 17
Chapter 17

... By stage 5 Planetary formation around the star has likely begun, but the protostar itself is still not in equilibrium – ...
Glossary Topics - Home - DMNS Galaxy Guide Portal
Glossary Topics - Home - DMNS Galaxy Guide Portal

... mass), helium (~28%), and other elements and dust particles. 2. In denser parts of molecular clouds, gravity causes gas and dust to collapse into small, dense objects called cloud cores. These cores collapse until the center starts to heat up, forming a protostar. Magnetic fields erupt from the form ...
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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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