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PowerPoint - Chandra X
PowerPoint - Chandra X

... solar system is shown in the image. The image is brighter to the upper right -- the side of the nebula nearest the Earth -- where there is less obscuring material to block the X-ray emission. NGC 7027 is the remains of a sun-like star that has ejected much of its mass to expose its hot core. The X-r ...
Section 11: GRAPHIC STIMULUS
Section 11: GRAPHIC STIMULUS

... A. It arose after a dying star called ‘red giant’ shed its outer layers B. It arose when an ancient star exploded C. It arose when a space cloud collapsed D. It was born as a new star ...
hw5
hw5

... At a time when the Earth’s atmosphere lacked ozone’s protection from ultraviolet light, the oceans provided a safe region that UV can’t penetrate. p. 458 RQ# 9 How does intelligence make a creature more likely to survive? A creature’s likelyhood of surviving changes in their environment over time de ...
Syllabus and Reading Assignments
Syllabus and Reading Assignments

... Course Description This one-semester course is a descriptive survey of and introduction to the conceptual aspects of astronomy. It presents the planets, satellites, asteroids, comets, meteors, Sun, stars, and galaxies. Emphasis of this course is on understanding how the scientific process was develo ...
Astronomy Study Guide #2
Astronomy Study Guide #2

... 05. What two parameters does the brightness of a star depend on? 06. What is the stellar spectral classification sequence? 07. What do studies of binary stars help us learn? 08. Solar granulation is evidence for what aspect of energy transport? 09. In traveling from the center of the sun to the top ...
Scattering (and the blue sky)
Scattering (and the blue sky)

... The dark dust clouds are very opaque in the visible, but we can see through them better and better, the longer the wavelength of light that is used. Looking through the galactic plane has the same effect; to see to the heart of the Galaxy you must use infrared or radio (or X-rays!). ...
Brichler-powerpoint
Brichler-powerpoint

... • Parallax – an apparent shift in the position of an object when viewed from different locations. • Using parallax and trigonometry, astronomers can find distances to stars. • Closer stars seem to move more than distant stars as the earth revolves around the sun. ...
Stars Jeopardy
Stars Jeopardy

... photosphere ...
Infinity Express-1
Infinity Express-1

... S G2: Nature of Science S G3: History of Science Infinity Express has content relating directly to these particular standards, including: • IE explicitly reviews the development of astronomical knowledge over time • Modern satellite technology has created a “data storm” from observations of Earth. T ...
Stars
Stars

... à=Ð/Ð8šThe Nearby Stars: A Tour of Our Neighborhood When we look up into the night sky, it is easy to imagine, as did the ancient Greeks, that all the stars are the same distance, stuck to some sort of Celestial Sphere that rotates through the heavens as the Earth stands still. This conclusion would ...
School Supplies - Rowan County Schools
School Supplies - Rowan County Schools

...  Our solar system is located on the ___________ Arm – 30,000 light years from the center.  Part of the __________ _________ of super clusters (Andromeda is also part of this group)  Astronomers use __________ and _____________ telescopes to “see” the center of the galaxy  We can’t actually “see” ...
the young astronomers newsletter
the young astronomers newsletter

... common stars in the universe) are prime targets in the ever found - a chunk of space rock about 65 miles in search for extraterrestrial life. But new research diameter beyond the orbit of Mars. It had been seen indicates some such planets may not be hosting life before but then lost. This was one of ...
ASTRO VOLUME 2 - Global Friendship Through Space Education
ASTRO VOLUME 2 - Global Friendship Through Space Education

What is a galaxy - University of Melbourne
What is a galaxy - University of Melbourne

... Why study galaxies across time ★ Cosmic origin theme: ★ Where are we coming from? ...
Hertzsprung-Russell (H-R) Diagram Hertzsprung-Russell Diagram March 16 −
Hertzsprung-Russell (H-R) Diagram Hertzsprung-Russell Diagram March 16 −

... Which is the hottest star? Which is the smallest star? Which is the biggest star? If stars A-D replaced the sun, would people be able to live in Michigan? a. b. c. d. e. ...
RFS_multiple_choice_Dec8_Key
RFS_multiple_choice_Dec8_Key

... C. Objects which lie within 5 degrees on either side of the ecliptic, and are hence occulted by the moon at some time or the other. D. All of them lie in the Milky Way band of the sky (the galactic equator) 3. On July 4, 1054, Chinese astronomers (and possibly Native Americans) recorded a supernova ...
Galaxies • Test 3 (New date) – Thurs, 9 April
Galaxies • Test 3 (New date) – Thurs, 9 April

... A gas cloud moves under influence of the gravity of the galaxy. The gas cloud moves once around the galaxy in a specified orbit. If the time is short, the mass of the galaxy is greater. Write an equivalent statement for the galaxy NGC 3672 Mass ...
File
File

... Q3.The diagram shows a teacher using a loudspeaker to demonstrate an important effect. The loudspeaker, which produces a note of constant frequency, is swung around in a ...
Article “What Astronomers Do” (appendix C) one per student
Article “What Astronomers Do” (appendix C) one per student

... century later that an appropriate explanation was given for the mysterious lines seen in the stars' spectra. In 1859, the German physicist Gustav Kirchoff (in collaboration with the German chemist Robert Bunsen) suggested that Fraunhofer's lines were due to the presence of specific chemical elements ...
Spectroscopic Investigation of Companion Stars in Herbig
Spectroscopic Investigation of Companion Stars in Herbig

... Stars were chosen to be the known binary companion to a Herbig star, with a binary separation greater than 0.8 arcseconds to avoid any contamination from the primary star. Data was collected using the Gemini South GNIRS instrument (PI Rodgers).Two types of spectral measurements were made, high resol ...
Stars and Galaxies – Notes
Stars and Galaxies – Notes

... Many stars are found in multiple-star systems. Alpha Centauri is in a multiple star system. It is made up of three stars called a triple star system. Over half of the stars in the sky have at least one companion star. Most of these stars are doublestar systems in which two stars revolve around each ...
Early Astronomy and Gravity
Early Astronomy and Gravity

... 2. A line between the Sun and a planet sweeps out equal areas in equal times 3. The square of a planet’s orbital period is proportional to the cube of its semimajor axis P2 ∝ R3 or ...
Note Taking Guide #2: Characteristics of Stars Welcome back! As
Note Taking Guide #2: Characteristics of Stars Welcome back! As

PPT
PPT

... There is an advantage in most solar system observations - we have a very good idea of what the general source characteristics are, including general expected flux densities and extent of emission. This can be used to great advantage in the imaging, deconvolution, and self-calibration stages of data ...
New Earthlike Planet Discovered
New Earthlike Planet Discovered

... liquid form, and in galactic terms is relatively nearby at 120 trillion miles away. But the star it closely orbits, known as a "red dwarf," is much smaller, dimmer and cooler than our sun. There's still a lot that is unknown about the new planet, which could be deemed inhospitable to life once more ...
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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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