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Engineering the Heavens
Engineering the Heavens

... and allowed for are as good as nonexistent. In December in The North American Review, 1838, after only a year of final visual observations, Bessel showed the power of this error-quantification approach: When the astronomer undertakes to measure he announced that he had determined the parallax of 61 ...
Stars - CBSD.org
Stars - CBSD.org

... • The stars began to be ranked by letters, with A-D being white stars, E-L yellow, and M-N red. • However, it soon became clear that the colors didn’t really connect to the elements in the stars. – So you’d get weird pairings like A stars that have strong hydrogen lines and B stars that have weak on ...
H-R Diagrams
H-R Diagrams

... 3 The y-axis - luminosity: the values are actually multiples of some value L - the luminosity of our Sun. So they are all relative values. ...
Nucleus hydrogen helium Relative Mass 1.007825 4.0037 Helium
Nucleus hydrogen helium Relative Mass 1.007825 4.0037 Helium

... star may eventually form a black hole. To gain full marks in this question you should write your ideas in good English. Put them into a sensible order and use the correct scientific words. ...
MASS – LUMINOSITY RELATION FOR MASSIVE STARS
MASS – LUMINOSITY RELATION FOR MASSIVE STARS

Star Birth: The Formation of Stars Jonathan Rowles
Star Birth: The Formation of Stars Jonathan Rowles

... fusion of hydrogen to form helium. They range in size from 0.08 times the mass of the Sun to up to 120 Solar masses. They can have lifetimes ranging from a few million years to the age of the universe. ...
The Stellar Cycle
The Stellar Cycle

... While the exterior layers expand, the helium core continues to contract, while growing in mass, and eventually becomes hot enough (100 million Kelvin) for helium to begin to fuse into carbon Carbon ash is deposited in core and eventually a helium-burning shell develops. This shell is itself surround ...
Today`s Powerpoint
Today`s Powerpoint

... temperature from spectrum (black-body curve or spectral lines), then find surface area, then find radius (sphere surface area is 4 p R2) ...
Lab 4
Lab 4

... Photometry is the determination and use of the color spectrum of astronomical objects to determine the objects’ properties. Two properties you will investigate later are distance and age. The objects you will use are stars in various clusters in the Milky Way galaxy and beyond. This is known as the ...
Apr 2017 - Astronomical Society of Northern New England
Apr 2017 - Astronomical Society of Northern New England

... had when Galileo first looked up with his little telescope and discovered things we had never dreamed of, but are now completely taken for granted as obvious science. April 28. The moon passes near Mars this evening. Jan Oort was born on this day in 1900. The Oort’s cloud, the source of all of our c ...
Manual - Test Equipment Depot
Manual - Test Equipment Depot

... the Stars”. Thousands of years ago astrology was used to determine when to plant and harvest crops. At a later date this developed into the idea that you may be able to tell the future by the position of the stars and planets in relation to the sun. Astrologers maintain that everyone is born under a ...
Document
Document

... When astronomers look through their telescopes, they see billions of stars. What can they learn fromThe goal of this problem set is for you to understand that astronomers classify stars on the basis of two different criteria: (1) the intensity of one of the H absorption lines (called H), and (2) on ...
Module code: AA1
Module code: AA1

... The hypothetical question how the night sky would appear if all stars would possess the same luminosity as the sun or Barnard’s star was analysed with Excel diagrams leading to the conclusion that in case of the sun the night sky would have less bright stars and in case of Barnard’s star with the na ...
THE CELESTIAL SPHERE
THE CELESTIAL SPHERE

... imagine the stars to remain fixed on a sphere of very large radius with the earth at its centre. We call this sphere the celestial sphere. At any point of time we can only see the upper half of the celestial sphere. The point on this dome right above our head is known as zenith. The lower boundary o ...
Astronomy Assignment #1
Astronomy Assignment #1

... with a diameter of 1.23 solar diameters. Alpha Centauri B is (60/85) = 0.706 times smaller than Alpha Centauri A. based on the ratio of their angular sizes (and the fact that they are at the same distance). So Alpha Centauri B is slightly smaller than the Sun with a diameter of 0.867 solar diameters ...
Comet Pan-Starrs 12 March 2013
Comet Pan-Starrs 12 March 2013

Stars
Stars

... toward each other by gravity • Many stars orbit each other • More than 50% of stars occur in pairs or multiples. • Binary stars are used to determine the star property most difficult to calculate – It’s mass ...
Photometry of star clusters with SalsaJ - Eu-Hou
Photometry of star clusters with SalsaJ - Eu-Hou

... Photometry is generally used to generate light curves of objects such as variable stars and supernovae, where the interest is the variation of total light energy output by the system over time. It can also be used to discover exoplanets, by measuring the intensity of a stars light over a period of t ...
Black Body Radiation and Wien`s Law File
Black Body Radiation and Wien`s Law File

Chapter 10. Stellar Spectra
Chapter 10. Stellar Spectra

... One pneumonic device for remembering the odd order of the letters (not including L and T) is: Oh Be A Fine Guy (or Girl) Kiss Me. Since stellar spectra depend not only on the temperature of the stellar atmosphere but also on its pressure, there is a second parameter that is needed to classify them. ...
Stars and Their Characteristics
Stars and Their Characteristics

... though it is not nearly as hot.  When a temperature of about 27,000,000°F is reached, nuclear fusion begins. This is the nuclear reaction in which hydrogen atoms are converted to helium atoms plus energy. This energy (radiation) production prevents further contraction of the star.  The protostar i ...
The Bigger Picture
The Bigger Picture

... nearest star) is small. The atmosphere blurs stellar images to about 1 arcsecond so `astrometrists’ are trying to measure a tiny motion of the centroid as it moves back and forth every six months. The lack of parallax apparent to the unaided eye was used as a proof that the Earth did not revolve aro ...
Siriusposter
Siriusposter

... The maximum mass for a white dwarf progenitor Theoretically, the maximum mass of a white dwarf-forming star is about 8 solar masses. Stars more massive than that explode as supernovae, creating neutron stars. However, this theoretical limit has never been backed up by observational evidence. One of ...
mars, antares, the sting and more
mars, antares, the sting and more

... JAMES: NOW THAT WEVE INVESTIGATED THE HEART OF THE SCORPION, HOW ABOUT HIS TAIL? AT THE END OF THE FISHHOOK SHAPE, LOOK FOR TWO STARS THAT ARE VERY CLOSE TOGETHER. THESE ARE THE STARS SHAULA AND LESATH AND TOGETHER THEY ARE KNOWN AS, THE STING. DEAN: MAKES SENSE. ALTHOUGH THESE TWO STARS LOOK CLOSE ...
IOSR Journal of Applied Physics (IOSR-JAP)
IOSR Journal of Applied Physics (IOSR-JAP)

... The planets are moving around the stars by staying in a particular angle with their axis. Now the question is why they are moving on their axis in a particular angle? Like earth is moving in its axis with 23.50 angle. For the experiment I took a big plastic ball (a very light weight plastic ball) an ...
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Perseus (constellation)



Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.
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