• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Starlight & Stars - Wayne State University Physics and Astronomy
Starlight & Stars - Wayne State University Physics and Astronomy

... object being observed! The old magnitude-system was based on how bright a star appeared to the unaided eye Today’s magnitude system (based on more accurate measurements) goes beyond Hipparchus' original range of magnitudes 1 through 6 Very bright objects can have a magnitude of 0, or even a negative ...
The Dramatic Lives of Stars
The Dramatic Lives of Stars

Presentation - University of Idaho
Presentation - University of Idaho

... Period = 10 days Magnitude = 14 150,000 light years away ...
Phase Analysis of RV Tauri and Semi-regular Variables Abstract
Phase Analysis of RV Tauri and Semi-regular Variables Abstract

... RV Tauri variable stars, related classes of pulsating variable stars. The ultimate objective for our research is to determine whether the stars stellar properties such as temperature, radius, and luminosity correlate with their pulsation cycles. In order to determine this, we need to closely examine ...
BlackHoleintheCenter..
BlackHoleintheCenter..

... NASA's COBE satellite scanned the heavens at infrared wavelengths in 1990 and produced this premier view of the central region of our own Milky Way Galaxy. The Milky Way is a typical spiral galaxy with a central bulge and extended disk of stars. However, gas and dust within the disk obscure visible ...
Lecture 31: The Properties of Stars
Lecture 31: The Properties of Stars

... of stars. The color of a star depends on its temperature: cooler stars are redder, hotter stars are blue. Luminosity, the total energy output expressed in Watts or Solar Luminosities, depends on the radius and temperature. The absorption spectra of stars form a distinct sequence with stellar tempera ...
Part II: Ideas in Conflict.
Part II: Ideas in Conflict.

... luminous its redshift indicates it is 4 billion light years away!! ...
The infrared void in the Lupus dark clouds revisited: a
The infrared void in the Lupus dark clouds revisited: a

... 100 m IRAS emisison ...
Document
Document

...  Pluto first discovered in 1930 by Clyde W. Tombaugh  A full-fledged planet is an object that orbits the sun and is large enough to have become round due to the force of its own gravity. In addition, a planet has to dominate the neighborhood around its orbit.  Pluto has been demoted to be a “Dwar ...
Dec 2017 - What`s Out Tonight?
Dec 2017 - What`s Out Tonight?

... GEMINI is a favorite and Albireo in CYGNUS is Kepler Copernicus too faint to see with the eyes because it shines at well liked for its blue & gold colors. Ptolemaeus magnitude +11. The second closest star visible to Alphonsus the naked eye is Sirius at 8.6 ly followed by Epsilon Moon (e) Eridani at ...
Introduction - Arecibo Observatory
Introduction - Arecibo Observatory

... would provide unique databases in a number of ways. Firstly, they would yield full spatial frequency mapping at a number of previously unmapped wavelengths, with competitive resolution for such extended features as the Galactic background emission, HII complexes, and middle-aged and old SNRs. Compar ...
Characteristics of Stars
Characteristics of Stars

... nuclear fusion is happening at their cores… they create their own light • Have different characteristics which allow many different ‘varieties’ of stars to exist ...
Matariki-Maori New Year
Matariki-Maori New Year

... similar festival marking the event. ...
Document
Document

... used up their H fuel and are gone. • The position of the hottest, brightest star on a cluster’s main sequence is called the main sequence turnoff point. ...
Turbulence Layers - Facultad de Ciencias
Turbulence Layers - Facultad de Ciencias

...  Galactic astronomy  The Galactic Center  Nearby AGN  Quasars and high-z galaxies ...
softwares and past experience
softwares and past experience

... Field = 1.9x1.9°, sampling 3.3 arcsec/pix About 12 GRBs/year Variable stars Minor planets Follow up of ToO ...
Astronomy Webquest Part 1: Life of Stars: Go to http://www.odec.ca
Astronomy Webquest Part 1: Life of Stars: Go to http://www.odec.ca

... 6. What type of stars can become a white dwarf and eventually a black dwarf? __________________________________________ The Death of Massive Stars 7. For a massive star, it starts by burning ______________ & ______________. Helium atoms fuse to form _____________ & _____________. Carbon then fuses t ...
Southern cross Crux - The Southern Cross Crux, the Southern Cross
Southern cross Crux - The Southern Cross Crux, the Southern Cross

... 26 other stars, each of which represents a state; Acrux represents the State of Sao Paulo. Physical Properties ...
ppp
ppp

... two dimensions • The following slides depict a collision between two galaxies • The galaxy on the top of the screen is the more massive of the two • There are 10,000 stars per galaxy ...
the summary
the summary

... contracts a bit, this helium can further fuse to heavier elements such as carbon, nitrogen and oxygen. In the most massive stars this can continue until the core consists of iron. Around the core, there will be shells made from earlier fusion reactions, like the layers in an onion. The outermost she ...
Archaeology of the Universe
Archaeology of the Universe

... Galileo was the one to get the archaeology of the universe started, and for two reasons. First of all, Galileo was convinced that light takes time to propagate, that is, it has a finite speed, not infinite; and this is precisely where the possibility of looking at things in their past states comes f ...
Universe and Star Formation - White Plains Public Schools
Universe and Star Formation - White Plains Public Schools

... • Stars with masses similar to the sun evolve in essentially the same way as low-mass stars. • During their collapse from red giants to white dwarfs, medium-mass stars are thought to cast off their bloated outer layer, creating an expanding round cloud of gas called planetary nebula. ...
Stars, Constellations, and Quasars
Stars, Constellations, and Quasars

... Virtually every ancient civilization observed and studied the nighttime sky, and archaeological evidence such as Stonehenge points to these early studies of astronomy. Ancient cultures also developed elaborate mythologies around stars and constellations and gave them names, some of which are still i ...
The Development Of Astronomy
The Development Of Astronomy

... Kepler’s Laws of Planetary Motion – Kepler obtained Brahe’s data after his death despite the attempts by Brahe’s family to keep the data from him in the hope of monetary gain. There is some evidence that Kepler obtained the data by less than legal means; it is fortunate for the development of modern ...
The Universe - HMXEarthScience
The Universe - HMXEarthScience

... Which conclusion can be made by comparing the standard spectrum to the spectrum produced from this distant star? A) The star’s spectral lines have shifted toward the ultraviolet end of the spectrum and the star is moving toward Earth. B) The star’s spectral lines have shifted toward the ultraviolet ...
< 1 ... 224 225 226 227 228 229 230 231 232 ... 456 >

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.
  • studyres.com © 2026
  • DMCA
  • Privacy
  • Terms
  • Report