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Word - Sam Davyson
Word - Sam Davyson

... and the two viewing points in two lots of the parallax angle. So ab using the diagram parallax angle = . This method is only really usable over ...
Physics@Brock - Brock University
Physics@Brock - Brock University

... 1. During May the constellation Cancer is visible near the Western Horizon. However in June the Cancer is no longer visible in the night sky. The reason for that is that (a) the Earth is spinning about North-South axis. (b) the Earth is revolving around the Sun. (c) the Earth has rotational axis tip ...
Planetarium Key Points
Planetarium Key Points

... the ecliptic, they tend to pull the equatorial bullge of the Earth towards it and most of this “flattening torque” is caused by the Moon and the Sun. But the Earth is rotating and therefore the torque cannot change the inclination of the equator relative to ecliptic, the rotation axis turns in a dir ...
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8Oct_2014

proposed october viewing list
proposed october viewing list

... CS = Carbon Star, * = Video imaging optional, ** = Video imaging recommended ...
March
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... standard planetary nebula with a 16th magnitude central star. The unusual appearance is due to the angle of the nebular ring that is expanding outward from the white dwarf at about 42 K/sec. Most of the visible light is emitted in the OIII doubly ionized Oxygen band so the use of a nebula or OIII fi ...
Stars through the year
Stars through the year

... If you go out on a clear night and look at the sky for a while you will see that the stars seem to move across the sky during the night. This movement is not due to the stars themselves moving but to the Earth spinning on its axis. Now go out at the same time on different night during the year and y ...
Slide 1
Slide 1

... Galaxy, according to the best measurements with a speed of about v = 250 km/s at a distance from the Galaxy center of about r = 28,000 ly. The gravitational force between the mass of the galaxy M and the mass of our solar system m is actually centripetal force: ...
powerpoint version
powerpoint version

... • Measured velocity of up to 216 km per hour • Orbital period of candidate planet 4.2 days • Mass about half that of Jupiter • Just 0.05 AU from star (1/20th of Earth-Sun) • Surface temperature probably about 1300 K • Confirmed by Marcy and Butler Nothing like Mercury / the solar system. How did it ...
astronomy ch4 - Fort Thomas Independent Schools
astronomy ch4 - Fort Thomas Independent Schools

... How hot is a “red hot” object? Of all objects that glow from heat stored or generated inside them, those that glow red are the coolest. What color is the Sun? The Sun emits all wavelengths of electromagnetic radiation, with blue-green most intense. How can we determine the age of space debris found ...
Science 9: Unit E: Space Exploration
Science 9: Unit E: Space Exploration

Class 11 and 12 lecture slides (giant planets)
Class 11 and 12 lecture slides (giant planets)

I. Layers of the Sun
I. Layers of the Sun

Type Ia supernovae and the ESSENCE supernova survey
Type Ia supernovae and the ESSENCE supernova survey

... is not enough to show a deceleration of the universe. The SN points fall along a curve that is most easily interpreted as evidence for a positive cosmological ...
l rest
l rest

... are possible. The details are not crucial now As long as there is a strong interaction, matter and EMR can reach an equilibrium When matter and EMR are at equilibrium in a given body, absorption and emission balance each other, I.e. matter does not gain or loose energy, and keep its temperature the ...
The magnitude scale, parallax, the parsec, and Cepheid distances
The magnitude scale, parallax, the parsec, and Cepheid distances

... Filters  only  allow  light  from  a  specifice  wavelength  range  through   Examples  are  ugriz  or  BVRI  in  the  op;cal  or  YJHK  in  the  near-­‐IR   Use  filter  symbols  as  subscript,  i.e.,  mK  =  K-­‐band  magnitude   If ...
Kepler`s laws - FSU High Energy Physics
Kepler`s laws - FSU High Energy Physics

Lecture21
Lecture21

...  The most stable arrangement of nucleons is one where neutrons and protons are found in a lattice of increasingly neutron rich nuclei: ...
Big bang galaxies stars Name: Date: 1. The diagram below
Big bang galaxies stars Name: Date: 1. The diagram below

... of light from distant celestial objects appear closer to the red end of the spectrum than light from similar nearby celestial objects. The explanation for the red shift is that the universe is presently A. ...
the Sun - University of Redlands
the Sun - University of Redlands

Solutions
Solutions

... see quite a number of interacting galaxies; one example is on the title page of your textbook. We never see stars in the disk of our Galaxy run into each other, however. (We do see binary stars, but they are stars which have formed together, and have always been companions.) 2. Chapter 4, Question 1 ...
Stars Names - astrofoto.org
Stars Names - astrofoto.org

... Stars Names ...
Cosmic Distance Ladder
Cosmic Distance Ladder

... every 243 years, with pairs of transits eight years apart separated by long gaps of 121.5 years and 105.5 years. ...
Astro twopages
Astro twopages

... --------------------------------------------------------------------------------------Alternately try the "Galaxy Song" by Monty Python from the meaning of life (which can be downloaded in mp3 from http://www.mwscomp.com/sound.html): Just remember that you're standing on a planet that's evolving And ...
I. What is an Exoplanet?
I. What is an Exoplanet?

... when the gravitational field of one star acts like a lens and magnifies the light of a distant background star.  Such an effect occurs only when the two stars are almost exactly aligned.  If the lens star has a planet orbiting it, the gravitational field of the planet may cause small variations in ...
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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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