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Opakování z minulého cvičení
Opakování z minulého cvičení

... What is the optical astronomy? Astronomy based on observations made using visible light, essentially the same part of the electromagnetic spectrum that our eyes are sensitive to. Star catalogues: Is an astronomical catalogue that lists stars. There are many of star catalogues. The first catalogue is ...
IS AN ALTERNATE COSMOLOGY BECOMING NECESSARY?
IS AN ALTERNATE COSMOLOGY BECOMING NECESSARY?

... could be possible but it is likely to take trillions of years for two galaxies to complete the merger. This amount of time cannot be accepted so they are modeled to happen quickly. Galaxy collisions do occur infrequently and for the most part appear very destructive; there are very powerful tidal ef ...
Star Facts - Dr. Noha MH Elnagdi
Star Facts - Dr. Noha MH Elnagdi

... look more yellow (like the Sun), and some look blue or blue-white (like Sirius) ...
Night Sky
Night Sky

... Watching a time-lapsed movie of the stars, we clearly how the stars all seem to rotate around the North Celestial Pole (but really the Earth is rotating). ...
Nov13Guide - East-View
Nov13Guide - East-View

... Just below Andromeda lies the small constellation of Triangulum. Between the Andromeda Galaxy and Triangulum is another fairly large and local spiral galaxy, Messier 33 or the Pinwheel Galaxy. This galaxy is about three million light years distant but only contains about 40 billion stars. It is a di ...
THE HR DIAGRAM
THE HR DIAGRAM

... 3. HR DIAGRAM DETAIL  Figure 3 illustrates the full scale of an HR diagram. The x‐axis at the top utilizes both spectral  class and temperature while at the bottom, the x‐axis uses the B‐V color index. The y‐axis on  the left uses luminosity in solar units while absolute magnitudes are at right.   T ...
June, 2011. - University of Michigan
June, 2011. - University of Michigan

... These equations are used to relate measured zenith angles ZA to latitude, longitude and other parameters. There will be one such equation for each star measurement. Multiple star measurements provide a system of equations that is overdetermined when the number of measurements is greater than two. In ...
Chapter 11
Chapter 11

... 12. According to Figure 11-5, the Protosun was cooler yet much more luminous than the Sun is now. How can this be true? a. The Protosun had more mass. b. The Protosun was much larger. c. The rate of nuclear fusion was higher inside the Protosun. d. Both a and c above. e. Both b and c above. ...
1-1 H. Color Index: A color index is the difference of two color
1-1 H. Color Index: A color index is the difference of two color

Stellar Census
Stellar Census

... the stars are exaggerated Sirius A is considerably larger than the Sun, while Sirius B is about the size of the Earth 22 March 2005 ...
Publications 2003 - Département d`Astrophysique, Géophysique et
Publications 2003 - Département d`Astrophysique, Géophysique et

... description of the eigenfunctions in the star atmosphere. Numerous theoretical models have been computed in order to select the best model fitting the observed frequency values as well as the mode identifications. The derived mass is 9.62 solar masses with an age of 15.7 million years. ...
Study Guide 4 Part A Outline
Study Guide 4 Part A Outline

... o Most of the mass of the Milky Way is dark matter. The existence of the dark matter is inferred from the effect that its gravity has on stars in the outer part of the Galaxy. Those stars are orbiting faster than they would be expected to be moving if there were no dark matter. Nobody knows what the ...
The Sun and Stars The Sun is a typical star with a mass of about 2
The Sun and Stars The Sun is a typical star with a mass of about 2

... I is measured in Watt/m2 . So, a star that is 10 times farther away appears 100 time less bright. The brightness is sometimes expressed not in Watt/m2 but in magnitudes. The magnitude of Sirius (the brightest star in our sky) is -1.46, of Canopus -0.72, of Vega 0.04, of Deneb 1.26,. . . more or less ...
Introduction to Celestial Spheres (Professor Powerpoint)
Introduction to Celestial Spheres (Professor Powerpoint)

Astronomy.Practice.Quiz3
Astronomy.Practice.Quiz3

... 10. A Hertzsprung-Russell (H-R) diagram shows the relationship between ____. a. absolute magnitude and apparent magnitude b. temperature and absolute magnitude c. parallax and temperature d. apparent magnitude and parallax 11. The source of the Sun’s energy is ____. a. chemical burning b. nuclear fu ...
Satellities - stoweschools.com
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... Velocity of the Geostationary Satellite with respect to the sun ...
ch 2 the sky
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... Angular distance – a measure of the separation between two objects in the sky  Angular diameter – a measure of the size of an object in the sky  Scientific model – an intellectual concept designed to help us think about a natural process without necessarily being a conjecture of truth  South cir ...
Stellar Activity
Stellar Activity

... – Young stars show changes in mean brightness of several % from changes in surface markings, both bright and dark, but brightness varies inversely with chromospheric activity – Hyades show year-to-year brightness changes of order 0.04 mag over times of several years – For older stars, long term brig ...
Compact stars
Compact stars

Star Formation: Interstellar Gas and Dust
Star Formation: Interstellar Gas and Dust

... • Still denser state of matter than electron degeneracy. • Sun: 1,000,000 km diameter • White dwarf: 10,000 km (~ same diameter as Earth) • Neutron star: 20 km • Degenerate pressure of neutrons can support stars up to 3M ...
Fulltext PDF
Fulltext PDF

... star clusters are widely used as ideal samples to study stellar evolution as all other parameters are fixed, and the mass of stars defines it’s evolution. In the present times, they are also very useful in understanding star and planet formation as these are very closely linked processes, planet for ...
Chapter 19. Mapping the Universe from Herschel to Sloan
Chapter 19. Mapping the Universe from Herschel to Sloan

... slow process because you need to get many images of a galaxy spread out over more than a year and discover all the Cepheids, measure their brightnesses as a function of time, etc. Fortunately, a second discovery by Hubble has made this process much easier. While studying the velocities of galaxies ( ...
Stars part 2
Stars part 2

... Stellar Formation and Life Cycle Stars are theorized to evolve through six stages of development… 1. Protostar Stage – the gravitational collapse of a gaseous cloud mass. • The collapse may be triggered by the passing of, the eruption of, or the explosion of a near-by star. • Energy production is d ...
Lecture 3
Lecture 3

Galileo, Shakespeare, van Gogh - McMaster Physics and Astronomy
Galileo, Shakespeare, van Gogh - McMaster Physics and Astronomy

... And he will make the face of heaven so fine That all the world will be in love with Night And pay no worship to the garish Sun. ...
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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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