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The Dimensions Program - Asnuntuck Community College
The Dimensions Program - Asnuntuck Community College

No. 54 - Institute for Astronomy
No. 54 - Institute for Astronomy

... They found the planets using measurements from the Automated Planet Finder (APF) Telescope at the University of California’s Lick Observatory, the W. M. Keck Observatory on Maunakea, and the Automatic Photometric Telescope (APT) at Tennessee State University’s Fairborn Observatory in Arizona. All th ...
SPECTRAL ANALYSIS OF A NEWLY DISCOVERED HgMn STAR
SPECTRAL ANALYSIS OF A NEWLY DISCOVERED HgMn STAR

... The HgMn stars rotate more slowly than normal stars having similar spectral class. An average rotational velocity of 29 km s-1 was derived by [5]. This velocity is large enough to affect the abundance anomalies in HgMn stars. Most of the HgMn stars belong to double or multiple star system [4]. In th ...
An Ancient Universe
An Ancient Universe

... the school science curriculum. The study of astronomy is deeply rooted in culture and philosophy. It harnesses our curiosity, imagination, and a sense of shared exploration and discovery, and it is also an area of great interest to people of all ages—especially children. With new and better telescop ...
Ch 3 PPT - Blountstown Middle School
Ch 3 PPT - Blountstown Middle School

... • Astronomers learn about the energy, distance, temperature, and composition of stars by studying their light. • Astronomers measure distances in space in astrological units and in light-years. They measure star brightness as apparent magnitude and as luminosity. ...
Oct 2012 - Bays Mountain Park
Oct 2012 - Bays Mountain Park

... telescope and crank up the power on the southwestern one. This is Uranus, and with about 100-150X, you should be able to spy the 6 arcsecond face of the planet. Uranus is currently about 1.77 billion miles from Earth. Jupiter rises around 10 p.m. in early October and is high enough for observing by ...
Course Description: This is an introductory course in Descriptive
Course Description: This is an introductory course in Descriptive

... a) Describing star brightness, the scales of apparent and absolute magnitude and the relation between luminosity, apparent magnitude and distance. b) Describing color index and the relation between star color and temperature. c) Defining the major spectral classes of stars, including the classificat ...
the text the talk here
the text the talk here

... remained in Athens for twenty years. Aristotle founded his own school, the Lyceum, which was more scientific than the Academy. In order to understand the physical universe, Aristotle looked for causes, which back then was a novel idea. The book that Raphael’s Aristotle is holding is the Nicomachean ...
Astronomy 114 - Department of Astronomy
Astronomy 114 - Department of Astronomy

Document
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... reach the earth, but light from the next nearest star takes a few years to arrive. The trip to that star would take the fastest rocket thousands of years.  Understand that some distant galaxies are so far away that their light takes several billion years to reach the earth. People o ...
Stellar Evolution: Evolution: Birth, Life, and Death of Stars
Stellar Evolution: Evolution: Birth, Life, and Death of Stars

... change their brightness with time Most of the stars are variable; can vary because they vibrate, shine brightly, erupt or explode, or are eclipsed by a companion star or planet Variable stars provide important information about the stellar nature and evolution ...
abstract - Maths, NUS
abstract - Maths, NUS

... As the motion of the moon is not steady, the duration of a Tithi may vary from 19.98 hours to 26.78 hours. This sometimes results in a Tithi period covering two successive sunrises, or falling between these, i.e. not covering any sunrise. When this happens there is a break in the counting of tithis ...
Standing in Awe - Auckland Astronomical Society
Standing in Awe - Auckland Astronomical Society

... Clarity, talks to the unit and is great for generating local displays and alarms. It can also provide a contact closure to, for instance, close the roof of an observatory if there is heavy cloud or rain. Perhaps you’re inside at Waharau waiting for the sky to clear at 1am, the beeper sounds, the sky ...
Chapter 9 “The Family of Stars “
Chapter 9 “The Family of Stars “

Oct 2011 - Bays Mountain Park
Oct 2011 - Bays Mountain Park

... focus of our attention these October evenings; it’s well up at dusk and visible 'til just before dawn. Ol' Jove is found between the constellations of Aries and the more elusive Cetus in the east as darkness falls. At magnitude -2.9 it is unmistakable to the naked eye in the fairly blank area betwee ...
MS Word version
MS Word version

... demonstrating the Eclipsing Binary Simulator in a classroom situation. We provide these suggestions with appropriate questions (shown in bold italics) to pose to the class as an aid in promoting interactivity. We encourage instructors to adapt these suggestions to their particular educational goals ...
PDF of story and photos
PDF of story and photos

Electronic version
Electronic version

... Edited in the Nara era, these contain solar and lunar eclipses as far back as the 6th century. During the Heian era, when Kyoto was the capital, many astronomical descriptions found their way into novels, essays, and diaries. The most famous of these may be the (Diary of the Full Moon) written in th ...
Apr/May 2003 - Madison Astronomical Society
Apr/May 2003 - Madison Astronomical Society

... orange, starlike object that wanders eastward among the stars. But about every 2 years, it begins to brighten, reverses its course and is prominent as a fiery orange-red star in the evening sky. At times it even exceeds mighty Jupiter in brightness. Then, after a month or two, it begins to fade and ...
A n   A n c i e n... How Astronomers Know the Vast Scale of Cosmic Time
A n A n c i e n... How Astronomers Know the Vast Scale of Cosmic Time

... the school science curriculum. The study of astronomy is deeply rooted in culture and philosophy. It harnesses our curiosity, imagination, and a sense of shared exploration and discovery, and it is also an area of great interest to people of all ages—especially children. With new and better telescop ...
W > 1 - The Open University
W > 1 - The Open University

... test for moderate apertures is the nebulosity around some of the other brighter stars of the group, especially Merope. Nebula/UHC filters will help. The Hyades oc is another naked eye star cluster although more spread out than the Pleiades. The first magnitude star Aldebaran (0.9) is not a member of ...
PHYS3380_111615_bw - The University of Texas at Dallas
PHYS3380_111615_bw - The University of Texas at Dallas

... - required some revisions to models of high mass stellar evolution, which had suggested that supernovae would result from red supergiants. Now believe star was chemically poor in elements heavier than He - contracted and heated up after phase as cool, red supergiant during which it lost much of its ...
PowerPoint Presentation - The Sun as a Power House
PowerPoint Presentation - The Sun as a Power House

... via the Carbon-Nitrogen-Oxygen chain. The more reactions there are, the more neutrinos are produced and the more that should be detected here on the Earth. February 7, 2006 ...
Night Sky III Planetary Motion Lunar Phases Astronomy 1 — Elementary Astronomy
Night Sky III Planetary Motion Lunar Phases Astronomy 1 — Elementary Astronomy

... Suppose it is early in the month and you are going on a cruise to view a total solar eclipse later the same month. The moon is currently full. If it only takes a day or so to get to the viewing location, about when might your cruise depart? ...
Interplanetary Vagabonds
Interplanetary Vagabonds

... details to constrain our models for comets. ...
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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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