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The Interstellar Medium (ISM) Part II: Interstellar Gas
The Interstellar Medium (ISM) Part II: Interstellar Gas

Stars Chapter 21
Stars Chapter 21

... • Light Year- Astronomers use light years to measure the distances between stars –A light year is the distance that light travels in one year • 9,460,730,472,580.8 km • 5,878,630,000,000 miles ...
Astronomy Club
Astronomy Club

... On the lines of VIBGYOR Spectral Classes of Stars Categorizing the stars, all different and huge in number had really been a challenging task for astronomers. In the classification of stars mentioned here, the stars are classified in various categories according to the strength of the Balmer lines ...
Witnesses to Local Cosmic History - Max-Planck
Witnesses to Local Cosmic History - Max-Planck

... folk in historiography, they were long neglected by astronomers. Unjustly so, because these small bodies can reveal a lot about why our solar system became what it is today. Astronomers from the Max Planck Institute for Solar System Research persuade them to reveal these secrets with telescopes, sim ...
Week 1B
Week 1B

... Stars seem to be on the inner surface of a sphere surrounding the Earth They aren’t, but can use twodimensional spherical coordinates (similar to latitude and longitude) to locate sky objects ...
New Astronomy With a Virtual Observatory S. G. Djorgovski (Caltech)
New Astronomy With a Virtual Observatory S. G. Djorgovski (Caltech)

... • A response of the astronomical community to the scientific and technological challenges posed by massive data sets • A Virtual Observatory (VO) would federate the existing and forthcoming large digital sky surveys and archives, and provide the tools for their scientific exploitation • A top recomm ...
- Fermi Gamma-ray Space Telescope
- Fermi Gamma-ray Space Telescope

... observations by FIRAS and longer wavelengths of DIRBE DMR and the shorter wavelengths of DIRBE ...
Skymax-180 Review by Sky At Night Magazine
Skymax-180 Review by Sky At Night Magazine

... I call the scope my ‘planet killer’! The best single upgrade I have made to the telescope was to add a Moonlite focuser. This has made a great telescope into an amazing one, as I take high-resolution lunar images and the focuser makes this a breeze to achieve, critical focus is important. After 30 y ...
SPACE  Section 8-STARS- OBSERVING CONSTELLATIONS
SPACE Section 8-STARS- OBSERVING CONSTELLATIONS

... day and pointing. Have them draw its constellation, learn to find it by the three bright stars in the belt, and look for Orion at night with their parents. [S, stars-season] 7. TELESCOPES [S, telescopes-magnify] Every day we learn more about space through telescopes. Ask students to describe what a ...
Lookback Time in Our Everyday Lives
Lookback Time in Our Everyday Lives

... time), your finger will appear to move back and forth relative to a more distant object. Each eye sees your finger at a slightly different angle. This is parallax, the same principle that allows us to use our eyes to estimate distances (and one of the reasons we have two eyes) or to watch 3D movies. ...
Unit 2 - Astronomy
Unit 2 - Astronomy

... Galaxies and Stars • Stars have a life cycle and undergo stellar evolution • Stars originate from a cloud of dust and gases • Gravity causes them to clump together and form larger balls of dust and gases ...
27.1: Characteristics of Stars
27.1: Characteristics of Stars

... About 3 billion can be seen through ground-based telescopes Over 1 trillion can be observed from the Hubble Space Telescope The visibility of a star depends on its brightness and its distance from the Earth. Astronomers use two scales to describe the brightness of a star: apparent magnitude and abso ...
Our galaxy, the Milky Way, has about 3 billion solar masses of HI
Our galaxy, the Milky Way, has about 3 billion solar masses of HI

Unit 1
Unit 1

... • Photons traveling away from a massive object will experience a gravitational redshift. – Their frequency will be shifted toward the red end of the ...
Life Cycle of Stars
Life Cycle of Stars

... Life span of a star depends on its size. – Very large, massive stars burn their fuel much faster than smaller stars – Their main sequence may last only a few hundred thousand years – Smaller stars will live on for billions of years because they burn their fuel much more slowly ...
1st Semester Earth Science Review 2014-15
1st Semester Earth Science Review 2014-15

Kentucky Monthly - Cold Spring Observatory
Kentucky Monthly - Cold Spring Observatory

... telescope. After writing letters to telescope makers and distributors, they obtained equipment that was a little more sophisticated. Now they have a club telescope that allows them to dive farther into the night sky. “The first few sessions start with a look at stars and planets and learn our way ar ...
ABC`s of the Sky - Northern Stars Planetarium
ABC`s of the Sky - Northern Stars Planetarium

... Hubble Space Telescope A special telescope that orbits Earth up in space. Because it does not have to look through the air, it can see further into space than any previous telescope. Io Io is a moon of Jupiter. It is about the same size as Earth’s moon, but it has many active volcanoes, which gives ...
What have we learned?
What have we learned?

... • How were neutron stars discovered? – Beams of radiation from a rotating neutron star sweep through space like lighthouse ...
Spokane Public Library The Spokane Astronomical
Spokane Public Library The Spokane Astronomical

... subjects to appear like the photographs you see in books and magazines; many will look like dim gray smudges. As you become more experienced and your observing skills get sharper, you will be able to ferret out more and more subtle details and structure. Deep-Sky Objects, also referred to as “dim-f ...
Bellringer - Madison County Schools
Bellringer - Madison County Schools

... • The brightness of a star depends on both its SIZE and TEMPERATURE. ...
Astronomy 242: Review Questions #1 Distributed: February 10
Astronomy 242: Review Questions #1 Distributed: February 10

... effective temperature T = 7350 K. (a) What is the distance d to Canopus? Include an estimate of the uncertainty in d. (b) How fast is Canopus moving with respect to the Sun? (c) What is the absolute bolometric magnitude Mbol of Canopus? (d) Given that the Sun has absolute bolometric magnitude Mbol,⊙ ...
Crux The Southern Cross
Crux The Southern Cross

... telescope appear as two dots. It is common for two stars to be locked together gravitationally to form a binary star system. Sometimes double stars may only appear close together from our vantage point on earth. If in reality they do not interact then we call this an optical double. It is possible, ...
Stargazer - Everett Astronomical Society
Stargazer - Everett Astronomical Society

... the group has been able to calculate the likelihood of any 'Earths' existing in the so-called habitable zone - the range of distances from each central star where life as we know it could survive. Popularly known as the "Goldilocks" zone, this region would be neither too hot for liquid water, nor to ...
The Spectrum & Doppler Shift
The Spectrum & Doppler Shift

... special part of the spectrum consists of waves that we can see. This is called the visible spectrum. We see different wavelengths as different colors ranging from red (long wavelengths) to blue/violet (short wavelengths). ...
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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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