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Stars - BrainBytes
Stars - BrainBytes

... Middle aged star  predicted to keep shining for 5 billion more years Diameter: 870,000 miles wide ...
Document
Document

... • They have a greater aperture so they collect more light. This enables you to see dimmer stars than with the naked eye. ...
Astronomy 2
Astronomy 2

... uses data from lots of stars, so there are lots of dots. The position of each dot on the diagram corresponds to the star's luminosity and its temperature  The vertical position represents the star's luminosity (absolute magnitude).  The horizontal position represents the star's surface temperature ...
Planet definition - International Year of Astronomy 2009
Planet definition - International Year of Astronomy 2009

... The featured programme “Global Star Party”, commencing at sunset on 4 April, is set to be an all-encompassing event of extraordinary scope. Amateur astronomers, clubs and other groups will be setting up telescopes in public places to allow as many people as possible to look at the heavens. Tradition ...
Life Cycle of a Star
Life Cycle of a Star

... Remnants can be seen for several weeks ...
What is it? - Carmenes - Calar Alto Observatory
What is it? - Carmenes - Calar Alto Observatory

... Our Solar System has eight planets. Four of them are “terrestrial” planets: Mercury (with its Moon-like surface), Venus (with its greenhouse atmosphere), the Earth (with its living creatures) and Mars (with its volcanoes and canyons), while the other four are “gas giant” planets: Jupiter (with its R ...
Solutions to test #1 taken on Tuesday
Solutions to test #1 taken on Tuesday

... ii. just those people within a narrow band passing through Redlands 4. (2) Vega and Altair are two of the stars that make up the Summer Triangle. What is the third? ______Deneb__________________ 5. (2) In the greenhouse effect, sunlight is absorbed by the earth’s surface and is reemitted in what par ...
3.3 e describe the method of heliocentric parallax
3.3 e describe the method of heliocentric parallax

... Click on the link below (Java needs to be on your computer to operate the model. This can be downloaded free of charge from the internet) When the screen shows the parallax model, left click on the area once Move the orange star to the left using the mouse Left click on ‘Show Bounds’ Left click on ‘ ...
SHELL H II REGIONS IN NGC 6334
SHELL H II REGIONS IN NGC 6334

... • Approach that takes advantage of old archival data that can be compared with more recent observations. • Addresses key parameters in astronomy such as mass, distance, and age. ...
SX TransPORT .(English)
SX TransPORT .(English)

... (UCLP) set up at 1GbE to the Joint Institution for VLBI in Europe (JIVE, NL) • The Physical path for the UCLP involved the use of CAnet4 (CA) from Pacific Wave to the ManLan (US) facility in New York; the Internet Educational Equal Access Foundation’s (IEEAF, US) trans-Atlantic capacity to the SURFn ...
physics_cosmic_engine - HSC Guru
physics_cosmic_engine - HSC Guru

... The early models were limited by the technology that was available at the time. For example, since the development of the telescope, more information about the universe has been collected. ...
Hubble space telescope. - Physics | Oregon State University
Hubble space telescope. - Physics | Oregon State University

... six sensors. This is done because many different ranges of light can be used to provide different information about the part of space being viewed. Each sensor has a different operating range and sensitivity level allowing each part of spaced being viewed at a time to be studied in multiple ways. Fi ...
The Telescope - Salt Lake Astronomical Society
The Telescope - Salt Lake Astronomical Society

... For as long as man has been capable of wondering, the night sky has provided subject material to wonder about. Trying to see more clearly and to find greater detail of the objects in the sky had been a desire of all the ancient astronomers. The true beginning of telescopes is somewhat foggy in histo ...
TELESCOPES: An Introduction to Your Galileoscope
TELESCOPES: An Introduction to Your Galileoscope

... – They have a much larger field – Most “spotting” telescopes are Keplerians with an additional “erecting” lens ...
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Document

... The main function of a telescope is to gather faint light from an astronomical source and to focus that light into an image The light gathering ability of a telescope is defined by its diameter or aperture Before the 20th century, astronomer looked through the telescope with their eyes Today the ima ...
Light and Telescopes
Light and Telescopes

... where visible light is completely absorbed). ...
Stars and Their Characteristics
Stars and Their Characteristics

... • absolute magnitudemeasure of how bright the star would be if all stars were at the same distance from Earth – The more negative the number, the brighter the star ...
Tue, April 1, 2003
Tue, April 1, 2003

... earth, so the moon has both day and night. But the moon’s rotation is slow; a lunar day lasts two weeks, followed by two weeks of night. As the moon orbits the earth, its rotation speed as it spins on its axis matches its revolution about the earth, so it rotates once for every orbit. This is called ...
A Red Giant - Cloudfront.net
A Red Giant - Cloudfront.net

... When the Sun like star starts to run out of helium its fusion slows and the core shrinks. This briefly speeds up fusion The Star expands… and cools Becoming a Red Supergiant for about 15 million years. In the cool outer layers flakes of Carbon and Silicon ...
MOPTOP
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... galactic nuclei, X-ray binaries and gamma ray bursts (GRBs) (see Jermak et al 2016 for an example of studying linear polarisation in blazars). As an example, use of polarimetry as a diagnostic tool in time domain programs has increased by a factor 5 on the Liverpool Telescope over the period 2012-20 ...
Siriusposter
Siriusposter

... white dwarfs. At these energies, white dwarfs are far brighter than most normal stars, and with ROSAT’s help we have been able to identify over 20 of these degenerate objects in binaries with bright, normal companions, just like the Sirius system. At optical wavelengths the white dwarfs are unresolv ...
As can be read from the textbook Fig. 8-9, or... transition has less energy and so a longer wavelength than... 4→3 3→2
As can be read from the textbook Fig. 8-9, or... transition has less energy and so a longer wavelength than... 4→3 3→2

... This is a perfectly reasonable separation for a binary star system. NOTE: A lot of people made the mistake of using their calculator to get the sine or tangent of an angle, but left the calculator in “degrees” instead of radians. You should remember that this is never necessary for problems like thi ...
9-Unit 1Chapter 11 Workbook
9-Unit 1Chapter 11 Workbook

The Universe: Big, weird and kind of scary!
The Universe: Big, weird and kind of scary!

... Modeling the motion of the Earth: 1. Draw a color diagram that shows the Earth’s motion around the sun. Place the earth’s axis correctly in its orbit, and show which part of the earth is in sunlight or darkness. Include the dates of the solstices and equinoxes. 2. Answer these questions about this m ...
No Slide Title
No Slide Title

... Solar absorption spectrum for the Sun (a typical “G” star) ...
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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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