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COMETS
COMETS

... with diameters less than 2 km are faint and hard to detect at these distances. A few have been discovered simply because they came very close to the Earth. Several more have been discovered near the Sun by the coronagraphs on orbiting spacecraft. Finally the Hubble Space Telescope is starting to ide ...
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... grains in one particular interstellar cloud were caught up in the developing solar nebula. Some of the grains survived formation of the Sun and avoided destruction by geological activity on the planets by being accreted into relatively small asteroid-size bodies. Fragments of asteroids that fall to ...
Bright versus Nearby Stars
Bright versus Nearby Stars

... A Comparison of the Nearest and Brightest Stars • The nearest stars to the Sun are thought to represent the true distribution of stars in the disk of the Milky Way Galaxy. • To truly understand the Galaxy, these stars must be studied. ...
Starry Night Companion - Starry Night Education
Starry Night Companion - Starry Night Education

... somewhere else. To make things worse, the co-ordinates change constantly over time as the sky rotates. For these reasons, stars and other objects in the sky are more commonly identified using the equatorial co-ordinate system. This system gives one unique set of co-ordinates for an object, which is ...
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I. ASYMMETRY OF ECLIPSES. CALENDAR CYCLES

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ISS Sighting Opportunities

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... Though this stream of particles shed by Comet Halley and left in orbit about the Sun is better observed from the southern hemisphere, we do see a fair amount of activity here. And this year astronomers believe we may see a dramatic increase in the number of meteors during the peak time. They’ve noti ...
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... The newly discovered objects are much smaller than Charon. Charon is about half Pluto’s size. The two new objects are about twice as far away from Pluto as Charon, but still close to the planet. A second image of Pluto taken three days later showed the objects in the same area. Scientists thought th ...
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2016 - 2017 Earth and Space Science R egular and H onors

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Coordinate Systems - AST 114, Astronomy Lab II for Spring 2017!

... Because RA and Dec are coordinates fixed to the sky, stars and other distant objects will keep their location in right ascension and declination throughout the year (just like we stay at the same latitude and longitude here in Tempe). Take, for example, the star Betelgeuse, in the Orion constellatio ...
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A S T R O N O M Y 1 1 0 - the Home Page for Voyager2.DVC.edu.

... Internet reference if you want to be able to show that the answer is correct. Part of what we are learning is how to convert units and how to use a logarithmic plot. So don’t spend a lot of time searching for the exact units (e.g. finding meters vs Earth radii). Converting Units: We compare the size ...
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Chapter 15 The Formation of Planetary Systems

... 7. Interactions between jovian protoplanets and planetesimals could be responsible for irregular moons. ...
Chapter 15 The Formation of Planetary Systems
Chapter 15 The Formation of Planetary Systems

... 7. Interactions between jovian protoplanets and planetesimals could be responsible for irregular moons. ...
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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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