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HERE
HERE

... Inclination of the Axis • Obliquity- Earth’s axis changes its tilt from more straight up and down to more tilted. • the Earth’s axis is currently tilted 23.5o from the ecliptic. • changes 22.2 to 24.5 through a 41,000 year period. • Tilt of the Earth is the cause of the Seasons. If you change the t ...
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... a ring of dust and comets around the star in very wide orbits. In the Vega system the outer edge of the ring is about 140 AU from the star. Any planets would be found in orbits nearer the star such as the Neptune-like planet in orbit around Vega. Orbit of Neptune-like planet around the star Vega: 65 ...
Astronomy 360 - indstate.edu
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... 19) Suppose you see two stars: a blue star and a red star. Which of the following can you conclude about the two stars? Assume that no Doppler shifts are involved. A) The red star is more massive than the blue star. B) The blue star is more massive than the red star. C) The blue star has a hotter su ...
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... 300 years ago it was discovered that stars move relative to each other and the constellations slowly change their shapes. The images to the left show Barnard's star, which has the largest proper motion of all stars. It moves by 10.4 arcseconds per year and its parallax amounts to 0.55 arcseconds. Ca ...
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... A. Venus, whose average distance from the Sun is the most similar to Earth's. B. Mars, whose axis is tilted almost the same amount as Earth's C. Mercury, whose distance to the Sun varies by nearly 50% during one orbit around the Sun. nd ...
The student will understand the hierarchical relationships of objects
The student will understand the hierarchical relationships of objects

... Recognize that there are enormous distances between objects in space. Explain how the speed of light is used to measure distance in space. Explain how astronomical bodies close to Earth are measured in AU units (distance between the Sun and Earth). Recognize that the universe contains many billions ...
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EGU06-A-00602 - Copernicus Meetings

3/3 What Are Planets?
3/3 What Are Planets?

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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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