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Sample Midterm - IUPUI Physics
Sample Midterm - IUPUI Physics

... d) you will not get a spectrum from the night side of this object 2. You discover a planet orbiting another star. The surface of the planet is 300 K but for some strange and unknown reason the atmosphere is 330 K. What type of spectrum do we expect to get from the light emitted from the surface of t ...
MAGIC
MAGIC

Larger, high-res file, best for printing
Larger, high-res file, best for printing

... same distance from us. In 1913 Ejnar Hertzsprung realized that this could provide a tool for finding distances, and he determined the zero-point for the period-luminosity relation. Then if one found a Cepheid, one had only to determine its period, and one would know its absolute magnitude; comparing ...
JMAPS
JMAPS

... The OTA consists of a plane-parallel entrance aperture window, made of fused silica. This window provides both a red band cutoff at about 920 nm as well as mechanical support for M2, with minimal stray light effects. There are three powered elements and six fold flats that are used to contain the 3 ...
No. 68 OBSERVATIONS OF COMET IKEYA
No. 68 OBSERVATIONS OF COMET IKEYA

... During the period in which the writer was taking plates with the astrograph, Milon observed from a point southeast of Tucson away from the city lights. Milon made observations with 7 X 35 mm binocu lars and used a portable 6-in. reflector to search for a tail. The tail was first seen, 20' long, on S ...
PowerPoint
PowerPoint

... 2. A change in the apparent color of an object because of a change in position of the observer or observing point. 3. A change in the apparent brightness of an object because of a change in position of the observer or observing point. ...
Universe 19
Universe 19

... 2. What evidence do astronomers have that the Sun is a typical star? 3. What is meant by a “first-magnitude” or “second-magnitude” star? 4. Why are some stars red and others blue? 5. What are the stars made of? 6. As stars go, is our Sun especially large or small? 7. What are giant, main-sequence, a ...
January 2016 - Newbury Astronomical Society
January 2016 - Newbury Astronomical Society

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Chapter 2 - personal.kent.edu
Chapter 2 - personal.kent.edu

... • Predicted the order of the planets – Mercury, Venus, Earth, Mars, Jupiter, Saturn – The only six visible with the naked eye – The Th telescope l had h d not yet been b invented i d ...
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Topic 3: The Spectroscope - Danielle`s science9 weebly

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Biosignatures of Kepler 62 e And Kepler f

... go even further and search for life in moons like Europa and Titan, what at one point was only found in science fiction and comic books. While sending a spacecraft to venture out and explore these exo-planets and return with little green men within a reasonable amount of time is not within current t ...
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... cloud collapses gravitationally into a star … is still a challenging theoretical problem… Astronomers have yet to find an interstellar cloud in the actual process of collapse.” ...
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Selected Physical and Astronomical Constants Conversion Factors

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Lecture9
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... What does any theory of the formation and evolution of the solar System have to account for, i.e., what are the “observed facts”? ...
Science 3rd prep. 1st term unit 3 lesson 2 The Solar System Millions
Science 3rd prep. 1st term unit 3 lesson 2 The Solar System Millions

... - it collects photos since millions of years .These photos allow astronomers an opportunity to study the evolution of the universe after the Big Bang. - Astronauts on a space shuttle regularly maintain this telescope in space. ...
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... • Simpler definition - A “large” object that orbits a star and shines primarily by reflecting light from its star. ...
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Week 9 Concept Summary - UC Berkeley Astronomy w

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Astronomy_Syllabus

... important, as it dealt with the question of the relationship between the Earth and all the heavenly bodies, including the Sun and Moon. Ancient cultures used their knowledge of the heavenly movements to regulate agricultural cycles, establish calendars, predict eclipses, and perform religious ritual ...
Chapter 27 Quasars, Active Galaxies, and Gamma
Chapter 27 Quasars, Active Galaxies, and Gamma

... • Early radio telescopes found radio emission from stars, nebulae, and some galaxies. • There were also point-like, or star-like, radio sources which varied rapidly these are the `quasi-stellar’ radio sources or quasars. • In visible light quasars appear as points, like stars. ...
Planet X - The 2017 Arrival
Planet X - The 2017 Arrival

... the darkness of outer space and it comes back into our inner solar system every 3,630 years! Because it is so large, Planet X also has an electromagnetic field surrounding it that is second only to that of the Sun in the solar system. In other words, it acts as a powerful magnet in space, pushing al ...
OUTSIDE THE SOLAR SYSTEM
OUTSIDE THE SOLAR SYSTEM

... that stars come in many colors. However, the unaided human eye tends to combine these colors into white light. Q: Should I be worried about the Sun dying? Will I need a warmer coat? A: As scientists have observed in other stars, the Sun goes through life cycle stages. Eventually it will die. But bef ...
Exploring the Solar System - Rourke Publishing eBook Delivery
Exploring the Solar System - Rourke Publishing eBook Delivery

... launched Sputnik 2. This time, a dog named Laika was aboard the satellite. ...
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Stars Study Guide KEY

... Originally, the universe was tiny, hot, and dense. (Everything was compressed together into a small ball.) Then, an enormous explosion threw matter in all directions. (The matter eventually formed everything that we now see.) 18. What evidence is used to support the theory? (Tell two) Galaxies are s ...
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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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