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Sacred Fire – Our Sun - University of Louisville
Sacred Fire – Our Sun - University of Louisville

... ● Other than the hydrogen and helium formed at the time of the Big Bang, nuclear fusion within stars produces all atomic nuclei lighter than and including iron, and the process releases electromagnetic energy. Heavier elements are produced when certain massive stars achieve a supernova stage and exp ...
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... The two images below illustrate how light moves away from a source (S). Each example shows a specific portion of an expanding sphere or bubble of light as it moves outward. The original light spreads out over a wider and taller surface area as distance increases. For example, the left hand picture ...
Poster - University of North Dakota
Poster - University of North Dakota

... The motivation for finding new asteroids is to increase the database of known asteroids and therefore increase the knowledge about the structure of our solar system. In addition, observations of known asteroids are used to update orbital data. Asteroids play an important role in understanding the cr ...
The Future Sun
The Future Sun

... In what ways are HR diagrams of H+χ Perseus, Pleiades, Hyades, & NGC188 different? Q Which is false a. Perseus has hotter stars than Pleiades. b. Most stars are one the main sequence. c. Perseus has small range of luminosity d. Some clusters have giants. ...
Death of Stars
Death of Stars

... Birth Place of Stars: Dark and cold inter-stellar clouds These clouds are made of more hydrogen than helium. These clouds have very small amount of heavier elements. ...
How Hubble Space Telescope failed
How Hubble Space Telescope failed

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Lecture 5
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... • Binary stars, in which two stars are held in orbit • around each other by their mutual gravitational attraction, are surprisingly common • Those that can be resolved into two distinct star images by an Earth-based telescope are called visual binaries • Each of the two stars in a binary system move ...
Jan 2017 - Bays Mountain Park
Jan 2017 - Bays Mountain Park

... propagate through the solar plasma. By looking at how the Corona’s composition changes, researchers can determine which mechanism is more important, says Tom Woods, a solar scientist at the University of Colorado at Boulder and principal investigator of MinXSS: “It’s helping address this very long-t ...
Constants and Equations
Constants and Equations

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Astrophysics notes - School

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Chapter 18 Notes - Valdosta State University
Chapter 18 Notes - Valdosta State University

... expansion of space towards the red end of the spectrum. He concluded that the universe must be expanding. Hubble's Law states the recessional velocity of a galaxy depends directly on the distance from us to the galaxy. The equation is: ...
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INTL JOURNAL OF ELECTRONICS AND TELECOMMUNICATIONS

... science, precision engineering and much more. One of the most important fields of astronomical science is observational astronomy, which takes observation of celestial objects as the most important source of information about the universe and its structure. Astronomical observations can be performed ...
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... within a molecular cloud caused by nearby supernovas or other forces.  Most stars spend about 90% of their life-times as main sequence stars. During this time hydrogen is turned into helium by nuclear fusion at the star’s core. As the main sequence stage continues the luminosity, temperature and he ...
Eratosthenes (250 B.C) Ptolemy`s Geocentric Model
Eratosthenes (250 B.C) Ptolemy`s Geocentric Model

... Kepler’s third law 1. The cube of a planets semisemimajor axis is proportional to the square of its orbital period a3 = T2 2. a = semisemi-major axis –also average distance from planet to sun (also written as d or r). Units are AU’ AU’s. 3. T = orbital period (also written as P). Units are years. 4. ...
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... The star, Procyon A, is 11.4 light years away from Earth. If there is intelligent life on a planet in that solar system, which is looking at Earth with a special telescope, what are they able to see? A ...
TAP 702- 6: Binary stars - Teaching Advanced Physics
TAP 702- 6: Binary stars - Teaching Advanced Physics

... both will have their 589.0 nm spectral line red shifted by 0.13 nm, as both will have the same velocity relative to the Earth (question 4). When they move towards A and B, however, their velocities relative to Earth increase and decrease respectively, causing the spectral line to be red shifted by d ...
Why does Sirius twinkle?
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Star Formation - University of Redlands
Star Formation - University of Redlands

... Interstellar Gas • In Lab 2 we talked about spectral lines and how they apply to hot and cool gases. ...
High School Science Essential Curriculum - Astronomy
High School Science Essential Curriculum - Astronomy

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Astrophysics by Daniel Yang
Astrophysics by Daniel Yang

... 1. Our understanding of celestial objects depends upon observations made from Earth or from space near the Earth - Discuss Galileo’s use of the telescope to identify features of the Moon Galileo was not the inventor of the telescope, but he built his own that was clear enough to observe the moon. He ...
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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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