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A Starscape in Red and Blue - Royal Astronomical Society of Canada
A Starscape in Red and Blue - Royal Astronomical Society of Canada

... of a historical, biographical, or educational nature of general interest to the astronomical community. All contributions are welcome, but the editors reserve the right to edit material prior to publication. Research papers are reviewed prior to publication, and professional astronomers with institu ...
The redshift of extragalactic nebulae
The redshift of extragalactic nebulae

... famous Einstein effect. It appeared, however, that it was not possible in this way to uncover rational relationships. E. HUBBLE then tried to correlate the redshift with the distance of different nebulae. This experiment has, as is well known, since then been crowned by great success. The nebulae wh ...
NASA-TV Highlights
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... Does night already seem to be falling about as early as it ever will? You're right! We're still a whole month away from the winter solstice — but the Sun sets its earliest around December 7th, and right now it already sets within only about 5 minutes of that time (if you're near latitude 40° north). ...
Chapter 26
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Comparative study of two solar eclipses in the 21st century
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Chapter 26 - Diploma Plus Net / Welcome
Chapter 26 - Diploma Plus Net / Welcome

Digital STARLAB Teachers Guide
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Galaxies - University of Iowa Astrophysics
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... Piazzi tried to predict Ceres’ orbit. Astronomers need this information so they could try to find it. He observed Ceres for six weeks. He did not have enough information to determine Ceres’ orbit. After that, others searched for Ceres in vain. Several astronomers tried to work out Ceres’ orbit from ...
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... the illuminated parts of Venus. Both size and phase are represented in accordance with my mathematical model. Sizes are to be compared with each other. The images do not reproduce the absolute dimensions that Galileo would have seen through his telescope, but simply dimensions relative to each other ...
a changing cosmos - Whittier Union High School District
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... this next step—the application of spectroscopy to stars, in the same way as Kirchhoff had done for the Sun—a natural one to undertake. The first person to embark on observing stellar spectra in the 1860s was Giovanni Donati (1826 –1873) in Florence. He used a single prism spectroscope on his 41-cm r ...
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Chapter 1 Telescopes 1.1 Lenses

... This is why many more stars are seen using a telescope than using the unaided eye. The greater the diameter of the objective of a telescope, the greater the number of stars that can be seen. Planets and other astronomical objects in the solar system are magnified using a telescope (unlike stars whic ...
MOON PRACTICE MULTIPLE CHOICE
MOON PRACTICE MULTIPLE CHOICE

... the starlight when it is between Ogle-Tr-3 and Earth. This observation allowed scientists to find not only the planet, but also to determine the planet’s mass and density The mass has been calculated to be approximately 159 times the mass of Earth. The planet is only 20% as dense as Jupiter. Scienti ...
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Astronomical unit

The astronomical unit (symbol au, AU or ua) is a unit of length, roughly the distance from the Earth to the Sun. However, that distance varies as the Earth orbits the Sun, from a maximum (aphelion) to a minimum (perihelion) and back again once a year. Originally conceived as the average of Earth's aphelion and perihelion, it is now defined as exactly 7011149597870700000♠149597870700 meters (about 150 million kilometers, or 93 million miles). The astronomical unit is used primarily as a convenient yardstick for measuring distances within the Solar System or around other stars. However, it is also a fundamental component in the definition of another unit of astronomical length, the parsec.
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