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Star Patterns - Lincoln-Sudbury Regional High School
Star Patterns - Lincoln-Sudbury Regional High School

The 2016 Transit of Mercury
The 2016 Transit of Mercury

... V ENUS TRANSITS (2004 AND 2012) New focus: refine techniques for finding planets around sun-like stars. Most widely observed transit to date! VT-2004 project had nearly 3,000 participants around the world. Many school children made timings of transit. The AU measured to within a fraction of the acc ...
Explaining Retrograde Motion of the Planets
Explaining Retrograde Motion of the Planets

... Ptolemy: Basic Model of Planetary Motion The simulation below shows the wide variety of motions that can be produced using the Ptolemy’s model. Thus Ptolemy was able to reproduce the location of the planets with very good accuracy. To improve the accuracy, Ptolemy created a more complicated model b ...
Chapter-by-Chapter Guide
Chapter-by-Chapter Guide

... Most of the atoms in our bodies (all the elements except for hydrogen, since our bodies generally do not contain helium) were made by stars well after the Big Bang. So most of the stuff in our bodies was once part of stars. Light travels at 300,000 kilometers per second. A light-year is the distance ...
Our Place in the Cosmos Elective Course Autumn 2006
Our Place in the Cosmos Elective Course Autumn 2006

... gravitational forces directly, but he was able to show that his law of gravity predicted that the planets should orbit the Sun just as Kepler’s empirical laws described • Newton was thus able to explain Kepler’s laws • Gravity is just one example of a physical law that was first tested by astronomic ...
the space shuttle - Literacy from Scratch
the space shuttle - Literacy from Scratch

... The shuttle flies in big S-shaped curves to slow down dramatically in the thicker air of the atmosphere 12 km from the runway and 3 km high, the shuttle deploys its flaps to slow from 682 km/h to 346 km/h A typical jet plane touches down at 260 km/h ...
lecture 2
lecture 2

... An Annular Solar Eclipse ...
PS119 maths review
PS119 maths review

... to make progress is usually quite modest. The mathematics you need for this program will be reviewed in the first half of this lab. The second part of the lab introduces you to the elements of mathematical reasoning. Enrico Fermi (who built the first nuclear reactor in the world at this university) ...
Chapter 2 PowerPoint
Chapter 2 PowerPoint

... • Circular motion of the axis projected into space – ~ 26,000 years for one complete ...
The Electromagnetic Spectrum
The Electromagnetic Spectrum

... • This differential rotation distorts the magnetic ...
Exploring the Solar System - Rourke Publishing eBook Delivery
Exploring the Solar System - Rourke Publishing eBook Delivery

12-3 Planets and Satellites Types of Orbits
12-3 Planets and Satellites Types of Orbits

... the use of instructors in teaching their courses and assessing student learning. Dissemination or sale of any part of this work (including on the World Wide Web) will destroy the integrity of the work and is not permitted. The work and materials from it should never be made available to students exc ...
Earth, Moon, Sun, and Stars
Earth, Moon, Sun, and Stars

... Key words: air, atmosphere, calendar, circle, crescent, dark, day, Earth, energy, full moon, gas, heat, light, month, Moon, neighbor, new moon, night, orbit, phases, planet, reflect, revolve, rock, rotate, sky, space, spin, star, Sun, water, year ...
The Orrery - Eli Whitney Museum
The Orrery - Eli Whitney Museum

... Earth. As those two planets travel around the Sun, the furthest they can appear away from the Sun is when their position in their orbit is perpendicular to Earth. In this position Venus has a maximum angle of 35 degrees from the Sun and Mercury has a maximum angle of 21 degrees. If the Sun was just ...
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Document

... • Can predict time and position of Sun during eclipse years in advance. • Measure the positions of stars SOHO spacecraft 6 months before when they are up at night. • During eclipse, measure their Result: Theory of Relativity confirmed! positions again. ...
Chap. 2: Known the Heavens
Chap. 2: Known the Heavens

... • The Earth is stationary and at the center of the sphere • Note that it is an imaginary object that has no basis in physical reality • However, it is a model that remains to be very useful for positional astronomy • It represents well the diurnal motion, by assuming the whole sphere rotates in a da ...
Space Study Guide
Space Study Guide

... we call it red shifting because the spectra appear redder. When objects are moving toward us, the spectral lines are shifted toward the blue end of the spectrum, and we call it blue shifting. Due to this red shifting of nearly every other galaxy, Hubble announced that the universe is expanding and t ...
Slide 1
Slide 1

... We are searching in a tiny portion of the Milky Way galaxy, and yet our galaxy is only one of more than 100 billion galaxies in the Universe! All but 4 specks in this “Hubble Deep Field” image are entire galaxies, each of them with 100 billion stars. ...
Branches of Astronomy
Branches of Astronomy

... Full moon - The phase of the moon when the side facing the earth is completely lit by sunlight. Geology - the study of the Earth. Giant planets - Jupiter, Saturn, Uranus, and Neptune. Gibbous moon - the phases between half moon and full moon. Great Red Spot - Thel large red storm going around like a ...
File - Zemali Salem
File - Zemali Salem

... The solar system consists of the sun and everything that orbits around it: the eight planets and their moons, comets, asteroids, and various other objects. The solar system itself is a relatively tiny part of the enormous Milky Way galaxy. It orbits around the center of the galaxy once every 225 mil ...
Orbit of Mercury
Orbit of Mercury

... – Causes apparent increases in brightness of stellar image ...
and Concept Self-test (1,2,3,5,6,7,8,9)
and Concept Self-test (1,2,3,5,6,7,8,9)

... ABSOLUTE MAGNITUDE – The apparent magnitude of all objects if they were all viewed at a distance of 10 parsecs (pc) from the observer. Absolute magnitude is equivalent to luminosity. Temperatures of Stars – Remember, using color (EM wavelength) we can determine temperature using ...
Satellite Communications - Institute of Electronics
Satellite Communications - Institute of Electronics

... parallels of latitude, meridians) shifts against geographical places? ...
Nicolaus Copernicus – 500 years of experimental science
Nicolaus Copernicus – 500 years of experimental science

The Sun
The Sun

... ANSWERS Exercise A: ...
< 1 ... 152 153 154 155 156 157 158 159 160 ... 369 >

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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