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Jan 2011 Regents
Jan 2011 Regents

... **W and Y are high tides because it is the moon’s gravitational pull that causes tidal changes. X and Y will experience low tides until those locations rotate into the appropriate positions.(approx 6 hours later)** ...
PDF Format
PDF Format

Phys 1533 Descriptive Astronomy
Phys 1533 Descriptive Astronomy

... • Equinoxes - two points where the ecliptic intersects the celestial equator. The day and night are of equal length at these two points. • Autumnal equinox - on September 21. • Vernal equinox - on or near March 21. • One tropical year - the interval of time from one vernal equinox to the next (365.2 ...
Voyage Grade 5-8 Education Unit
Voyage Grade 5-8 Education Unit

... Trans-neptunian (or Kuiper Belt Objects)—follow elliptical orbits around the Sun. Students first explore the geometric nature of ellipses, and the circle as a special case. These newly developed mathematical skills are then used to plot an accurate model of the outer Solar System, which contains the ...
teacher resource - Michigan Science Center
teacher resource - Michigan Science Center

... today. One of those planets is Earth. Earth is in the habitable zone in the solar system. This means that it is not too close or too far away from the sun. It is in a position that allows for life as we know it to exist. Life can exist here because of the sun’s interaction with the Earth and its atm ...
The Milky Way Galaxy
The Milky Way Galaxy

... When William Herschel (late 1700s) tried to measure the shape and size of the Galaxy and the sun’s position. He measured the direction and “distances” to visible stars. He came up with this… ...
Timeline, Topics, and Resources for iMovie Projects
Timeline, Topics, and Resources for iMovie Projects

... elegance, felt certain that the sun, moon and planets, being made of ether, would have a natural circular motion, since that is the simplest uniform motion that repeats itself endlessly, as their motion did. However, although the "fixed stars" did in fact move in simple circles about the North star, ...
3.6 spectral classes
3.6 spectral classes

... position is measured again. Nearby stars appear to shift back and forth relative to more distant stars as Earth revolves around the Sun. The apparent change in a star’s position observed when the star is sighted from opposite sides of Earth’s orbit is called stellar parallax ...
Conceptual Physics - Southwest High School
Conceptual Physics - Southwest High School

... fired horizontally from a very high mountain In a region devoid of air resistance. In the Absence of gravity, the cannonball would travel in a straight-line, tangential path. Yet in the presence of gravity, the cannonball would drop below this straight-line path and eventually fall to Earth (as in p ...
Chapter 2 - El Camino College
Chapter 2 - El Camino College

... Orbit of the Moon  Eclipses do not occur every month because the Moon’s orbit is tilted about 5 degrees with respect to Earth’s orbit around the Sun (the ecliptic). ...
37) What is the largest planet in the solar system?
37) What is the largest planet in the solar system?

... A) Mars, Mercury, Venus, Earth, Jupiter, Saturn, Uranus, Neptune B) Mercury, Venus, Earth, Mars, Jupiter, Saturn, Neptune, Uranus C) Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune D) Mars, Venus, Earth, Mercury, Saturn, Jupiter, Uranus, Neptune E) Venus, Mercury, Earth, Mars, Saturn, ...
Review of "Man`s Place in Nature" by Alfred Russel Wallace
Review of "Man`s Place in Nature" by Alfred Russel Wallace

... hardly any stars are visible, and those seen are projected on an intensely dark background, continue to present to some features in telescope of the highest to same features in telescopes of the highest powers as they do in those of moderate size. This could not possibly happen if the stars were inf ...
Final Study Guide
Final Study Guide

So, our cosmic address is
So, our cosmic address is

... •Our galaxy (the Milky Way) is about 100,000 light years in diameter. •The nearest star is 4.3 light years away. •The distance to the most distant object seen in the universe is about 14 billion light years (14 x 109 light years). •Looking at light that reaches us from many light years away is also ...
Stars, Galaxies and the Universe FORM A
Stars, Galaxies and the Universe FORM A

Sun - Astronomy Outreach
Sun - Astronomy Outreach

Sun - International Year of Astronomy 2009
Sun - International Year of Astronomy 2009

... reasoned that is was a large flaming ball, very far from the Earth. Medieval Arabs calculated the Earth-Sun distance, the Sun’s circumference, and proved that moonlight is reflected sunlight. The figures they calculated are very close to what we accept to be true today. A Persian (Iranian) astrolabe ...
Handy Pinhole Camera (Latin Camera Obscura) - (EU
Handy Pinhole Camera (Latin Camera Obscura) - (EU

Grzegorz F - (EU
Grzegorz F - (EU

... phenomena: eclipses, appearances of large sunspots and solar flair fields, or passing of the inner planets (Venus and Mercury) between the Sun and Earth. In the morning of June 6, 2012 we will be able to observe the passage of Venus against the solar disk. Transits of Venus are quite rare (we will h ...
File
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... inner planets, the only one known to have current geological activity, and the only place where life is known to exist. Its liquid hydrosphere is unique among the terrestrial planets, and it is also the only planet where plate tectonics has been observed. Earth's atmosphere is radically different fr ...
Chapter 13 Problems
Chapter 13 Problems

... rotates about a star (Fig. P13.51). The tangential speed of the ring is 1.25  106 m/s, and its radius is 1.53  1011 m. (a) Show that the centripetal acceleration of the inhabitants is 10.2 m/s2. (b) The inhabitants of this ring world live on the starlit inner surface of the ring. Each person exper ...
AST 443/PHY 517 Homework 1 Solutions
AST 443/PHY 517 Homework 1 Solutions

... 4. Which of these 5 stars is closest to the moon? What is the angular distance? Sirius, at about 44.3 degrees 5. The sidereal time at midnight advances by 3m 56s each day. What are the best days to observe these targets? See column (3) above. 6. What is the minimum zenith distance for each star? Se ...
ppt - Earth and Space Sciences at the University of Washington
ppt - Earth and Space Sciences at the University of Washington

... Oort cloud - extends out 50,000 AU (1000 x Pluto’s orbit) (nearly a light year, 25% of distance to nearest star) Voyager 1: 125AU, edge of heliosphere, 17km/s, 36 years, = 17 light-hours from Earth ...
Which month has larger and smaller day time?
Which month has larger and smaller day time?

August 2013 - Joliet Junior College
August 2013 - Joliet Junior College

... We are halfway through astronomical summer. The Celtic cross quarter day of Lughnasadh is on August 1st although August 6th is halfway between the first day of summer and the first day of fall. So, as to be expected, the summer sky is directly overhead at mid-evening during August. Directly above ar ...
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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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