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Definition - SchoolNotes
Definition - SchoolNotes

... for thousands of years humans believed that the planets and stars revolved around the Earth. – Claudius Ptolemy, the great Romanian mathematician, geographer, and astronomer, who lived almost 2,000 years ago, was the first scientist to formulate this idea. In the Ptolemaic system, or geocentric view ...
Lecture (Powerpoint)
Lecture (Powerpoint)

... Either we are very special and everything is moving away from us, or Universe as a whole is expanding But if universe is steadily increasing in size, implies that at some time in the past, Universe was a single point. `Start of the Universe’ ...
X-RAY OBSERVATIONS OF SEYFERT GALAXIES The dawn of a …
X-RAY OBSERVATIONS OF SEYFERT GALAXIES The dawn of a …

... One important aspect of Copernicus’ work - he took his heliocentric model, went further and made a model for the cosmos by saying, lets assume several things, then use observations to test whether this is a good model Cosmological principles are the assumptions which allow us to deduce the whole of ...
Satellite stuff - Ms. Gamm
Satellite stuff - Ms. Gamm

... 3,000 teens start smoking every day in the United States. The average person spends two weeks of their life kissing. Scientists in Australia's Parkes Observatory thought they had positive proof of alien life, when they began picking up radio-waves from space. However, after investigation, the radio ...
Issue 122 - Aug 2014
Issue 122 - Aug 2014

... When you think about gravitation here on Earth, you very likely think about how constant it is, at 9.8 m/s2 (32 ft/s2). Only, that's not quite right. Depending on how thick the Earth's crust is, whether you're slightly closer to or farther from the Earth's center, or what the density of the material ...
02-02Stars_Part_One
02-02Stars_Part_One

... star delivers 100 times more W/m2 than a magnitude 6 star. ...
pdf format
pdf format

... – If Earth moved about the Sun, then one should observe stellar parallax, yet this was not observed. ...
Introduction to the Celestial Sphere
Introduction to the Celestial Sphere

... If you watch the skies for a few hours, you will note the apparent motion of this fictitious celestial sphere and all things on it. This apparent motion is caused by the spinning motion (rotation) of the Earth on its axis. ...
slides - Insight Cruises
slides - Insight Cruises

Stellar Evolution 1 Star Formation 2 Nebulae
Stellar Evolution 1 Star Formation 2 Nebulae

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Stellar Evolution

... the surface of the WD  Very hot, dense layer of nonfusing hydrogen on the WD surface  Explosive onset of H fusion Nova Cygni 1975 ...
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... 32) What is a CCD (which stands for charge-coupled device) used for? A) It is the world's largest operating telescope. B) It is an electronic detector that can be used in place of photographic film for taking images of the sky. C) It refers to any kind of instrument that can be hooked up to a telesc ...
December 2007 Clear Skies Newsletter PDF
December 2007 Clear Skies Newsletter PDF

the May 2017 Newsletter!
the May 2017 Newsletter!

... Porrima (Gamma Viriginis, magnitude 2.8) with the naked eye, but this time were able to see it, and, for example, we could see Delta Virginis at magnitude 3.4. Jupiter was the only planet visible, quite high up in the east. All four Galilean moons were visible early on, with Io close in to the west ...
Exercise 7
Exercise 7

... 9. So is model consistent with the Handbook? Suggest a reason that this 1700s value might be off. Hint: what might not have been as visible in the 1700s? ...
Measuring Stellar Distances
Measuring Stellar Distances

... error in intrinsic stellar luminosity since stellar luminosity depends upon the square of the distance. To date, ground based observations have made parallax measurements of approximately 8000 stars out to distances of 20 parsecs, but many of these are of relatively low quality. Furthermore, the vol ...
The Resounding Universe
The Resounding Universe

... sound itself. However, the sound of the planets is present since our birth and this explains why we cannot recognise it, not having the notion of its counterpart. Later, Aristotle retracts this enthralling theory affirming that if such a sound would exist, it would be so loud as to destroy life on E ...
November 2007
November 2007

... telescopes. (Note - the limiting visual magnitude for a 60mm scope is 11.4 with a Dawes limit of ~ 2” which puts this system well within the reach of the most modest armature equipment, always assuming that reasonably dark skies and good seeing conditions exist.) The brightest member, Keid A, is one ...
The Life Cycle of the Stars
The Life Cycle of the Stars

... unlike humans, the typical star may last for millions or billions of years. While we cannot witness the complete life cycle of any one star, the night sky does reveal stars in various stages of stellar development. In some ways we’ve got a time machine that enables us to look back and out into the f ...
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... within a molecular cloud caused by nearby supernovas or other forces.  Most stars spend about 90% of their life-times as main sequence stars. During this time hydrogen is turned into helium by nuclear fusion at the star’s core. As the main sequence stage continues the luminosity, temperature and he ...
2017 Sixth Grade Science and Honors Science Pacing Guide
2017 Sixth Grade Science and Honors Science Pacing Guide

... of the sun, Earth, moon system based on a one-meter diameter sun). LTF: Not so Lost in Space ALCOS 2 Pearson: 11.3, 12.1, 12.2, 12.6 Construct models and use simulations (e.g., diagrams of the relationship between Earth and man-made satellites, rocket launch, AMSTI Planetary Systems: Lesson 3, 5, 7, ...
chapter9
chapter9

... Stars produce energy by nuclear fusion of hydrogen into helium. ...
We Are Stardust: Synthesis of the Elements Essential for Life Aparna
We Are Stardust: Synthesis of the Elements Essential for Life Aparna

... (at about 2 million degrees) first revealed emission lines from an element unknown on Earth at the time. Helium is rare on Earth but is the second most simple and abundant chemical element in the universe. Finally, no stars or pockets of galactic gas have been found with helium abundances ranging ou ...
society journal - Auckland Astronomical Society
society journal - Auckland Astronomical Society

... ovember's Film Night featured a documentary showing how extreme solar activity could disrupt power supplies and threaten our electricity dependent civilisation. It explained how a solar flare sends charged particles and radiation out into space. The Earth’s atmosphere and magnetic fields are usually ...
powerpoints - Georgia Southern University Astrophysics
powerpoints - Georgia Southern University Astrophysics

... convectively mixed during the supernova event by calculating the density and temperature of the ionizing gas that generates the spectral lines. However, spectroscopy of supernova remnants is not clear cut and drawing conclusions is complicated; it is sometimes difficult to determine if a remnant is ...
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Theoretical astronomy

Theoretical astronomy is the use of the analytical models of physics and chemistry to describe astronomical objects and astronomical phenomena.Ptolemy's Almagest, although a brilliant treatise on theoretical astronomy combined with a practical handbook for computation, nevertheless includes many compromises to reconcile discordant observations. Theoretical astronomy is usually assumed to have begun with Johannes Kepler (1571–1630), and Kepler's laws. It is co-equal with observation. The general history of astronomy deals with the history of the descriptive and theoretical astronomy of the Solar System, from the late sixteenth century to the end of the nineteenth century. The major categories of works on the history of modern astronomy include general histories, national and institutional histories, instrumentation, descriptive astronomy, theoretical astronomy, positional astronomy, and astrophysics. Astronomy was early to adopt computational techniques to model stellar and galactic formation and celestial mechanics. From the point of view of theoretical astronomy, not only must the mathematical expression be reasonably accurate but it should preferably exist in a form which is amenable to further mathematical analysis when used in specific problems. Most of theoretical astronomy uses Newtonian theory of gravitation, considering that the effects of general relativity are weak for most celestial objects. The obvious fact is that theoretical astronomy cannot (and does not try) to predict the position, size and temperature of every star in the heavens. Theoretical astronomy by and large has concentrated upon analyzing the apparently complex but periodic motions of celestial objects.
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