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Spectroscope Lab
Spectroscope Lab

... object or the observer moves, the wavelength will change. The relationship between motion and observed wavelength is called the Doppler effect. ...
Some interesting geometric facts about eclipsing binaries (see if you
Some interesting geometric facts about eclipsing binaries (see if you

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March 2011 - Sunderland Astronomical Society
March 2011 - Sunderland Astronomical Society

... so close the stars are gravitationally distorted. They are actually elongated toward each other. They also interact tidally, keeping just one face toward the other, as the Moon does toward Earth. Such a close binary is “a built-in time bomb,” Drake declares. The continuous loss of mass from the two ...
WORD - UWL faculty websites
WORD - UWL faculty websites

... green dot represents the Earth. This diagram is NOT TO SCALE.  The bottom panel shows the combined absorption-line spectrum of the stars (with the lines from each star labeled “A” and “B”). A thin "stationary" absorption line appearing between the two lines shows the un-shifted location of each lin ...
Activity: Doppler Effect
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... green dot represents the Earth. This diagram is NOT TO SCALE. • The bottom panel shows the combined absorption-line spectrum of the stars (with the lines from each star labeled “A” and “B”). A thin "stationary" absorption line appearing between the two lines shows the un-shifted location of each lin ...
Mirrored Image Sep06.pub - High Desert Astronomical Society
Mirrored Image Sep06.pub - High Desert Astronomical Society

... On August 26th we finally got a very good night for a star party! Twenty eight people (plus Mike and Tony’s 2 dogs, whose names escape me) came out to the Landfill South observing site to enjoy the night sky. While Harold and Gloria Johnson were working on their Constellations about 8:45, Harold not ...
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Introduction to Basic Stargazing Part I - Naples Free-Net
Introduction to Basic Stargazing Part I - Naples Free-Net

... This brings up an important point. Wherever spot you choose to star gaze needs to be dark, as dark a place as you can find. Not just on the ground like inside the shadow of a building, but the sky needs to be dark too. So dark, that a passing cloud looks like a black hole in the sky. Those places a ...
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... 27. According to the H–R diagram, which type of stars have the highest surface temperature? ______________________________ 28. According to the H–R diagram, which type of stars are in spectral class B and have low luminosity? ______________________________ 29. According to the H–R diagram, which typ ...
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... finding planets of smaller sizes. With the launch of Kepler in 2009, astronomers hope to begin finding Earth-like planets, a quest that will continue with several more satellite telescopes within the next ten years. ...
seven winter constellations
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... his right hand. In his left arm he carries a small goat, marked by one bright star known as “the Mother Goat.” Just below “the Mother Goat” is a triangle of three smaller stars called “the Baby Goats.” ...
The Sun - GeoScience
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... 14. Diagram and label the positions of the Sun, Earth, and Moon during a Solar Eclipse. 15. When does a Total Solar Eclipse occur during the Moon’s phase cycle? Click on “Recent and Future Eclipses” under Related Links 16. What is the date of the next Eclipse that will be able to be seen from the W ...
Prime Focus - Tri-City Astronomy Club
Prime Focus - Tri-City Astronomy Club

... Without conclusively identifying and characterizing the foreground star, however, astronomers have had a difficult time determining the properties of the accompanying planet. Using Hubble and the Keck Observatory, two teams of astronomers have now found that the system consists of a Uranus-sized pl ...
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... ² We have thus been led to the following view of stellar evolution. 1. Stars form by collapse of interstellar gas clouds under the in°uence of gravity. As they shrink, they release gravitational energy. Once a protostar has become su±ciently dense to be opaque, this energy cannot be freely radiated ...
Edexcel GCSE - physicsinfo.co.uk
Edexcel GCSE - physicsinfo.co.uk

... All candidates are to answer questions 17 – 24. Before the test begins: Check that the answer sheet is for the correct test and that it contains your candidate details. How to answer the test: For each question, choose the right answer, A, B, C or D and mark it in HB pencil on the answer sheet. For ...
main characteristics of the emission from elliptical galaxies
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... Elliptical galaxies are one of the most characteristic objects we can nd in the sky. In order to unveil their properties, such as their structure or chemical composition, one must study their spectral emission. In fact they seem to behave rather dierently when observed with dierent eyes. This is ...
Astronomical Observations (Fall 2004) Final Exam
Astronomical Observations (Fall 2004) Final Exam

... The telescope we have used during our trip to Lulin Observatory has a primary mirror diameter of 1 m and the Cassegrain optical system has a focal ratio of f/8. (a) The PI VersArray 1300B CCD camera used to take images has effectively 1300 times 1300 pixels with 20 micron pixels. Calculate the field ...
stargazing - davis.k12.ut.us
stargazing - davis.k12.ut.us

... those ancient times, people have continued to make up stories, develop religious practices and grow crops based on groups of stars. Groups of stars are called constellations, patterns of stars in the sky that have been identified and named. Some constellations can be seen all year. These are stars t ...
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R136a1



RMC 136a1 (usually abbreviated to R136a1) is a Wolf-Rayet star located at the center of R136, the central condensation of stars of the large NGC 2070 open cluster in the Tarantula Nebula. It lies at a distance of about 50 kiloparsecs (163,000 light-years) in the Large Magellanic Cloud. It has the highest mass and luminosity of any known star, at 265 M☉ and 8.7 million L☉, and also one of the hottest at over 50,000 K.
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