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Star Chart_May-June_2016
Star Chart_May-June_2016

34_alone
34_alone

... • A 10 km rock strikes earth about once every 100 million years. • Does this place an upper limit on civilization lifetime of around 100 million years? • Impact did not kill all life. Indeed it “helped” mammals evolve. • Perhaps we can now deflect/ destroy such a rock and, very likely, will be able ...
THE SOLAR SYSTEM
THE SOLAR SYSTEM

... a star and shines with light reflected from the star. We know of eight planets that orbit the sun in our solar system. Since 1992, astronomers have also discovered many planets orbiting other stars. World book ...
Our Solar System Study Guide 4 grade standard to be tested: S4E2
Our Solar System Study Guide 4 grade standard to be tested: S4E2

... Orbit: to move in a path around an object ...
Ancient astronomy Part 8
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... Many ancient North American tribes were hunter-gatherers who developed their astronomy in a context which differed from the mostly settled agricultural civilisations in Europe. They also commonly believe in a oneness with all life, all living things, including celestial objects, being inter-related. ...
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Chapter 2 Assignment GEarthOL

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... Earth than any other star. Ths Sun appears to be the largest star because it gives off the most light. 4) The light of Proxima Centauri takes about 4.22 years to reach Earth suggesting that its distance from Earth is A) 4.22 parsecs. C) 4.22 million miles. B) The Sun looks larger because of the Eart ...
Chapter 8, Lesson 1, pdf
Chapter 8, Lesson 1, pdf

Winter solstice, 2016 - NRC Publications Archive
Winter solstice, 2016 - NRC Publications Archive

... has caused the Zodiac to slip. The first sign was once Aries. It has slipped back one sign and it now starts with Pisces. In astronomy, we describe the positions of stars using analogues of the Earth’s latitude and longitude system, referred to the Earth because in space there are no usable referenc ...
Lesson 1, The Earth
Lesson 1, The Earth

... North Pole to the South Pole.  One complete spin on the axis is called a rotation.  Earth makes one rotation every 24 hours.  During each rotation all locations on Earth receives a certain amount of sunlight and a certain amount of darkness, depending on the time of year. ...
Earth`s Motions
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... axis of rotation of a largely axially symmetric object • happens because of tidal forces that cause the precession of the equinoxes to vary over time so that the speed of precession is not constant • principal sources of tidal force are the Sun and Moon, which continuously change location relative t ...
The Sun and planets
The Sun and planets

... Sun occupies one of the two foci (Kepler’s First Law). In particular, planets move along orbits that are slightly eccentric, i.e. slightly squashed, and almost all on the same plane because of the mechanism with which they were created during the formation of our planetary system. Dwarf planets and ...
Habitats Jr. 04
Habitats Jr. 04

... If you walked from a point on one side of the Moon straight through the center to the other side you would have traveled 2,160 miles (the Moon’s diameter). The distance from the Earth to the ...
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... contain instruments to collect data and travel out of earth’s orbit to explore places that would be too dangerous for astronomers; the instruments that a probe contains depends upon the space mission ...
Astronomical Numbers
Astronomical Numbers

... Constellations appear to travel in counterclockwise circles around Polaris (the North Star). ...
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... Telescope – is an optical (sense of sight) device that uses lenses to gather and focus light to provide a magnified view. The satellites orbiting through space are large telescopes. ______________________________________________________________ Kepler – published his 3 laws of planetary motion. Knew ...
SkyMatters Jan-2017 - CIT Blackrock Castle Observatory
SkyMatters Jan-2017 - CIT Blackrock Castle Observatory

... distance is constantly changing as we whizz around our parent star at an average of 107,000 km/h. When we are farthest from the Sun we reach a point called “aphelion” and when we are nearest the Sun the term is “perihelion”. The difference between the energy we receive from the Sun at aphelion and p ...
Lecture 1 Review Sheet
Lecture 1 Review Sheet

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Review 3 - Physics and Astronomy

... •Physical Properties of Stars •Structure of Milky Way, other galaxies and the Universe ...
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Slide 1 - Henrico

... Our Sun makes its energy from this reaction: ...
The Sun PPT
The Sun PPT

Environmental Science/Physics 141: Astronomy
Environmental Science/Physics 141: Astronomy

... nature of light itself – This sets an absolute limit on magnification (rule of thumb: 20 x diameter in cm) – If we want detailed images of the planets, we have to go out there physically and get them 7. How Telescopes Work ...
Dark Skies Above Downeast Maine
Dark Skies Above Downeast Maine

Angular size and resolution - RIT Center for Imaging Science
Angular size and resolution - RIT Center for Imaging Science

... – with binoculars, can easily see shapes/shading on Moon’s surface (angular sizes of 10's of arcseconds) • To see further detail you can use small telescope w/ magnification of 100-300 – can distinguish large craters w/ small telescope – angular sizes of a few arcseconds ...
June 2016 - Flint River Astronomy Club
June 2016 - Flint River Astronomy Club

... parallax, measures one arc-second when viewed from one side of Earth’s orbit and then the other side. One parsec equals 3.26 light-years, but all stars except the Sun are farther away than that. The nearest star, Proxima Centauri, is 1.3 parsecs away; that translates into 4.24 light-years. Astronome ...
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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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