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... Black pixels: parameter space where detection is possible at 3-sigma level ...
Combining Practices with Core Ideas in the NGSS
Combining Practices with Core Ideas in the NGSS

... the distance to a star the baseline is the diameter of Earth’s orbit around the sun. To show the evidence that the sun and stars are made from the same elements, I could have the students use a diffraction grating to see that the spectrum of a light source is like a fingerprint, and share the ninete ...
Sirius Astronomer - Orange County Astronomers
Sirius Astronomer - Orange County Astronomers

review_one - MSU Solar Physics
review_one - MSU Solar Physics

... Go to the following rooms, based on team number: Teams 1-33: EPS 103 Teams 34-66: Leon Johnson 339 Teams 67-100: Roberts 101 Understand and be prepared to explain the following: Unit 1  The three components to measuring radiation  The difference between light gathering power and resolving power  ...
2007-8 Astronomy Outline
2007-8 Astronomy Outline

... **Night Sky Journal Entry 1 Example** Date: Time: (try to go out around the same time each night) Light Conditions: (here is where you state how dark it is; cloud cover; how much light is coming in from other houses aka light pollution) Location: where you are and the direction you are facing Observ ...
stars-notes
stars-notes

... • When a chemical element emits light, only some colors in the spectrum show up. The colors that appear are called emission lines. • Every element has a unique set of emission lines that act like a fingerprint for that element. ...
Astronomy 360 - indstate.edu
Astronomy 360 - indstate.edu

... football field is about 1 arc minute across. • Each minute of arc is divided into 60 seconds of arc • The ball in the tip of a ballpoint pen viewed from across the length of a football field is about 1 arc second across. • The Sun and Moon are both about 0.5 degrees. • Bowl of the Big Dipper is abou ...
THE LIFE CYCLES OF STARS (3)
THE LIFE CYCLES OF STARS (3)

... We can do the same with a prism or other devices. Illust Fraunhofer spectrum Fraunhofer found dark lines crossing the sun's spectrum. He was not the first to see them but was the first to catalogue them. He named them A,B,C,D,……. He did not know what caused them. These dark lines mean something. We ...
32Brightness
32Brightness

... source, where discrete colors are absorbed by atoms – From emission and absorption lines, get composition of objects and also their temperature ...
Astronomy news
Astronomy news

... XDIN, its X-ray flux doesn’t show any apparent contamination from non thermal magnetospheric emission, and a parallactic distance (117 12 pc) has been reported. It is an ideal target to derive information on the neutron star radius and thus constrain the equation of state of matter at super nuclear ...
Universe Now - Course Pages of Physics Department
Universe Now - Course Pages of Physics Department

... • Cataclysmic or explosive variable stars: – Stars that irregularly increase in brightness by a large factor. – Nova or dwarf nova: occurs in semidetached binaries where a white dwarf star is accreting matter from an ordinary companion star. When the accreted layer is about half a meter thick, the t ...
Measuring Distances
Measuring Distances

Calculating Radial Velocities of Low Mass Eclipsing Binaries
Calculating Radial Velocities of Low Mass Eclipsing Binaries

... between June 2009 and January 2011. Each EBLM target was typically observed about 8 times over this time period. The spectra were processed using standard astronomical software, and a cross-correlation method was used to measure the radial velocity of the target star at each observed epoch. Radial v ...
Galaxy Powerpoint
Galaxy Powerpoint

... a) Does not have a definite shape. b) Could be the result of two galaxies ...
Star Formation
Star Formation

... • This causes a pressure build-up which slows (or stops) the collapse. • Energy is radiated away. ...
Star formation jeopardy
Star formation jeopardy

... The stars are in old age (Red Giants) and there are hundreds of thousands to millions of stars in a cluster. ...
this PDF file - University of Leicester Open Journals
this PDF file - University of Leicester Open Journals

Physics-Y11-LP3 - All Saints` Catholic High School
Physics-Y11-LP3 - All Saints` Catholic High School

... with a period related to their luminosity • recall that and explain qualitatively how this relationship enables astronomers to estimate the distance to Cepheid variable stars • understand the role of observations of Cepheid variable stars in establishing the scale of the Universe and the nature of m ...
Print Activity - Let`s Talk Science
Print Activity - Let`s Talk Science

... 4. If you don’t have access to glow-in-the-dark stickers, you can cover the end of a flashlight with red cellophane and shine this on the image when you’re outside (this way you can look at the image and the night sky without losing your ‘night vision’). 5. Go outside to a dark area where you have a ...
Earth Science Library wk 2 (WP)
Earth Science Library wk 2 (WP)

... If the Earth moved,the nearer stars should appear to move amongst more distant stars Absolutely true, however, the stars are much further away than they supposed. First successful measurement of stellar parallax was in 1838. ...
PPT
PPT

... • Compiled the most accurate (one arcminute) naked eye measurements ever made of planetary positions. • He still could not detect stellar parallax, and thus still thought Earth must be at center of solar system (but recognized that other planets must go around the Sun) • Hired Johannes Kepler, who l ...
SigAssignment
SigAssignment

... 3) In the equation E=mc^2 mass and energy are related. The reason why is because they are both variables in this equation. If you change one of them, the other one is directly affected by the change in the other. 4) I would have to agree with the statement “if it is possible to change mass into ener ...
M = 5.5 - The Millstone
M = 5.5 - The Millstone

... On the left, the scale of Absolute Magnitude reflects the true luminousity of the star. In order to determine Absolute Magnitude, we must have a measure of the stellar distance (by other means). Absolute magnitude, M, expresses the brightness of a star as it would be if it were placed 10 parsecs awa ...
Big Bang and Life Cycle of Stars
Big Bang and Life Cycle of Stars

... and the core starts to shrink. - Core temperature heats up and fusion begins, the outer region of the star expands. - This star then cools to red, and is so named as a red giant - When the collapsing core gets hot enough to process helium fusion, this process leads to production of carbon, oxygen, e ...
UCAC4 is a compiled, all-sky star catalog covering mainly the 8 to
UCAC4 is a compiled, all-sky star catalog covering mainly the 8 to

... value: the one given in the catalog for sigma position. If the astrometric data for a star was substituted from an external catalog like Hipparcos, Tycho or High proper motion data, a mean error in position and proper motion depending on the catalog and magnitude of the star was adopted. For stars w ...
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Hipparcos



Hipparcos was a scientific satellite of the European Space Agency (ESA), launched in 1989 and operated until 1993. It was the first space experiment devoted to precision astrometry, the accurate measurement of the positions of celestial objects on the sky. This permitted the accurate determination of proper motions and parallaxes of stars, allowing a determination of their distance and tangential velocity. When combined with radial-velocity measurements from spectroscopy, this pinpointed all six quantities needed to determine the motion of stars. The resulting Hipparcos Catalogue, a high-precision catalogue of more than 118,200 stars, was published in 1997. The lower-precision Tycho Catalogue of more than a million stars was published at the same time, while the enhanced Tycho-2 Catalogue of 2.5 million stars was published in 2000. Hipparcos‍ '​ follow-up mission, Gaia, was launched in 2013.The word ""Hipparcos"" is an acronym for High precision parallax collecting satellite and also a reference to the ancient Greek astronomer Hipparchus of Nicaea, who is noted for applications of trigonometry to astronomy and his discovery of the precession of the equinoxes.
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