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The Spectroscope
The Spectroscope

... the composition of objects made up of hot incandescent gases (like stars) and cool gases (like planetary atmospheres).  Spectrometers are used to analyze the amounts and types of spectral light that comes from objects in space. ...
TELESCOPE IN THE POCKET Abstract
TELESCOPE IN THE POCKET Abstract

... telescope?’ It is natural to continue the pondering of this idea by asking ‘how far you can see with your naked eye?’ Answering to these questions is not so easy. An eye as an observation tool has several limitations. The lens, called the pupil, is small, so it collects light only from a small area. ...
Homework 2
Homework 2

... to the Sun would be (a) twice as strong. (b) half as strong. (c) one quarter as strong. The force of gravity can be calculated using We begin with the equation Fg = G ...
Aging nearby spiral galaxies using H
Aging nearby spiral galaxies using H

... loss, spectral output, plasma/gas dynamics &c. » Different options to cover most types of conditions: ...
Volcanoes and Igneous Activity Earth
Volcanoes and Igneous Activity Earth

...  Uses a lens (called the objective) to bend (refract) the light to produce an image  Light converges at an area called the focus  The eyepiece is a second lens used to examine the image ...
Slide 1
Slide 1

... 3. To the stars and beyond, use the ___________________. 300 million Light travels at a speed of ______________meters per second The distance that light travels in a year is called a 6 trillion light year. 1 light year = _____________________ miles. Sun 8 light minutes ...
Final Exam Practice Part I
Final Exam Practice Part I

... 7. What is Nuclear Fusion? 8. How does nuclear fusion produce energy? 9. Nuclear fusion can only occur in the center of the solar system. Why is that? 10. What would happen to the orbit of a planet if it suddenly started orbiting faster? 11. As a new star is born, what type of atoms first begin to f ...
Specific Word Instruction Possible Sentences
Specific Word Instruction Possible Sentences

... stronomy is the study of the planets, stars, and galaxies. People have been watching the movement of the sun, moon, planets, and stars since ancient times. So astronomy is a very, very old science. From early times, people tried to make models of the universe. For many years, no one wanted to believ ...
Bruno Maffei/C. OʼSullivan, Lens vs mirror telescope - B-Pol
Bruno Maffei/C. OʼSullivan, Lens vs mirror telescope - B-Pol

... • Size limited by filter diameter not by aberrations • Flat Focal Plane • Edge pixel eccentricity ~ 0.02 ...
Reminiscing about Mt. Wilson 60
Reminiscing about Mt. Wilson 60

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L3.a Spiral Review

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Characteristics of Stars Stars Analyzing Starlight Star Characteristics

... Analyzing Starlight ...
Isaac Newton
Isaac Newton

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Lecture L24 ASTB21

... radiation pressure of a star and g is the attractive force due to the star's gravitation. If p > g, a microbe that has drifted into space will move away from the star; if p < g, the microbe will fall toward the star. For a microbe to escape into interstellar space from the vicinity of a star like th ...
Angular size and resolution - RIT Center for Imaging Science
Angular size and resolution - RIT Center for Imaging Science

... • Angular degree (º) is too large to be a useful angular measure of astronomical objects ...
Astronomy – Phys 181 – Midterm Examination
Astronomy – Phys 181 – Midterm Examination

... d) The region above the earth’s atmosphere ...
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Where to Put the Telescope

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Conjunctions an Oppositions
Conjunctions an Oppositions

... Planets without a telescope look just like stars Except, they move relative to the stars ...
Conjunctions an Oppositions
Conjunctions an Oppositions

... Planets without a telescope look just like stars Except, they move relative to the stars ...
Measuring the Solar Diameter with a Michelson Radio
Measuring the Solar Diameter with a Michelson Radio

Press release - ASTRONOMY GROUP – University of St Andrews
Press release - ASTRONOMY GROUP – University of St Andrews

... An astronomer at the University of St Andrews will use a powerful planet-hunting telescope to find out the true size of the Universe. Researcher Dr Alan Penny will use the brightness of half a dozen stars to refine estimates of how big the Universe actually is. Dr Penny hopes to solve the problem us ...
Word version with live links
Word version with live links

... is changing our view on that, as it is on the Moon which I have not mentioned here much because it is a satellite orbiting a planet even though it is not far off the size of Pluto which for some inexplicable reason has recently been downgraded from planet to object. Were the Plutonians advised of th ...
E1 a-d
E1 a-d

...  The Hubble is not hindered by the Earth’s ____________________. Rotation and Revolution  The Earth rotates or spins on an __________ once every 24 hours (1 day).  An __________ is an imaginary line through the center of an object.  Because of the Earth’s rotation we have a _____________ of day ...
Then another Big Bang will occur and the
Then another Big Bang will occur and the

...  As objects move away from the Earth they emit a Red Light called the Red Shift.  This was seen using the Hubble Telescope. ...
The Life Cycle of the Stars
The Life Cycle of the Stars

... different stages in their lives. They are born, they mature and, eventually, they die. However, 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 de ...
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International Ultraviolet Explorer



The International Ultraviolet Explorer (IUE) was an astronomical observatory satellite primarily designed to take ultraviolet spectra. The satellite was a collaborative project between NASA, the UK Science Research Council and the European Space Agency (ESA). The mission was first proposed in early 1964, by a group of scientists in the United Kingdom, and was launched on January 26, 1978 aboard a NASA Delta rocket. The mission lifetime was initially set for 3 years, but in the end it lasted almost 18 years, with the satellite being shut down in 1996. The switch-off occurred for financial reasons, while the telescope was still functioning at near original efficiency.It was the first space observatory to be operated in real time by astronomers who visited the groundstations in the United States and Europe. Astronomers made over 104,000 observations using the IUE, of objects ranging from solar system bodies to distant quasars. Among the significant scientific results from IUE data were the first large scale studies of stellar winds, accurate measurements of the way interstellar dust absorbs light, and measurements of the supernova SN1987A which showed that it defied stellar evolution theories as they then stood. When the mission ended, it was considered the most successful astronomical satellite ever.
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