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The Earth`s Orbit and Season Demonstration
The Earth`s Orbit and Season Demonstration

... The Earth’s Orbit and Season Demonstration Goal of the activity: To demonstrate why we see different star patterns at different times of the year and way it’s warmer in the summer and cold in the winter. Materials Required: 1. 12 pieces of Bristol board 2. A globe with the tilted axis 3. A flashligh ...
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... The Earth is surrounded by a magnetosphere, a region of strong magnetic forces that extends upward from about 140 km in the upper atmosphere. In the magnetosphere, the magnetic field of the Earth traps rapidly moving charged particles, the majority of which appear to be emitted by the Sun during per ...
Mercury is the first planet from the sun. Named by
Mercury is the first planet from the sun. Named by

... Uranus is the seventh planet from the sun. It was discovered on March 13, 1781. Uranus is the third largest planet in the solar system by diameter. Uranus is named after the Greek god Ouranos, god of the sky. It takes Uranus approximately 30,707 days to complete its orbit around the sun. Uranus has ...
Eddie Sun - İngilizce
Eddie Sun - İngilizce

... • It takes one year to revolve around the sun • It is the only planet to support life ...
Science, 4th 9 weeks
Science, 4th 9 weeks

...  The cosmos is vast and explored well enough to know its basic structure and operational principles.  Everything in the Universe exerts a gravitational force on everything else; there is interplay between magnetic fields and electrical currents. ...
Pocket Planetarium 3C V9N4.W1T
Pocket Planetarium 3C V9N4.W1T

... Mars is impossible to miss, straddling the border between Aries and Taurus, close to the Hyades and Pleiades. It’s so bright that it outshines all the other stars, and its orange colour dispels any doubt about why it’s called the “Red Planet”. On the evening of October 29, the distance between Earth ...
The Solar Nebula Theory
The Solar Nebula Theory

... all of the other inhabitants of our SS should be roughly the same age, which evidence ...
Homework 1 – Exercise 1 1/9
Homework 1 – Exercise 1 1/9

... In 1672, an international effort was made to measure the parallax angle of Mars at the time of opposition, when it was closest to Earth. Consider two observers who are separated by a baseline equal to Earth’s diameter. If the difference in their measurements of Mars’s angular position is 33.6’’. Wha ...
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mike-ken_transit

... Transition Region and Coronal Explorer http://trace.lmsal.com/ Museum of the History of Science, University of Oxford Astronomical Society of the Pacific ...
Introduction to Space
Introduction to Space

... closest celestial body (any object beyond the Earth and visible in the sky) to the Earth ~From a dark site away from city lights, we can see nearly 3000 stars (compared to the only a few hundred from the city) ~Along with the Moon, a few planets are clearly visible in our sky. Because planets are fu ...
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... Umbra = kernschaduw, darkest part of a shadow Penumbra = halfschaduw, the less dark part of a shadow What are total eclipse, and annular eclipses? When the Moon is close enough to the Earth, it will cover the Sun completely; this is a total solar eclipse. When the moon is further away from the Earth ...
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Pythagoras Eudoxus of Cnidus Aristotle Eratosthenes Hipparchus

... would fall to the ground, but they had no idea why that happened. Newton explained that there was a force called gravity that pulled objects toward the center of the earth. Newton developed the theory of gravitational pull. Gravity is a force that pulls objects toward the center of an area. The Eart ...
Some space objects are visible to the human eye.
Some space objects are visible to the human eye.

... Earth and eight other major planets orbit the Sun. The Sun, the planets, and various smaller bodies make up the solar system. The Sun is about 100 times greater in diameter than Earth. You could fit more than 4000 bodies the size of the Sun between the Sun and the solar system’s outermost planet at ...
CT9b
CT9b

... Also, the work-energy theorem saysWnet = KE. The work must be positive, since by Kepler's second law, the planet moves faster (has higher KE) when it is nearer the Sun, so KE>0. ...
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... It’s densest atmosphere of the four terrestrial planets seems to be caused by a history of smoky volcanism which periodically resurfaces the entire planet. A high level of sulfuric acid which can rain out of Venus’ atmosphere suggests ongoing volcanic activity. Another heating factor is Venus’s slow ...
Heliocentric Model by Copernicus
Heliocentric Model by Copernicus

... • To explain why Venus is never seen very far from the Sun, the Ptolemaic model had to assume that the deferents of Venus and of the Sun move together in lockstep, with the epicycle of Venus centered on a straight line between the Earth and the Sun • In this model, Venus was never on the opposite si ...
Transcript - Cheap Astronomy
Transcript - Cheap Astronomy

... of the Sun and the planets represented a local system which operated quite independently from the background stars. Indian astronomers as far back as 800 BC had suggested this. Islamic astronomers, who were active around the time the Ptolemaic model was becoming embedded in European thought, were qu ...
Take-home midterm, due Fri 3/16
Take-home midterm, due Fri 3/16

... 3. Interstellar dust grains have typical masses of approximately 1x10-17 kg. Find the rms speed of a dust grain in an interstellar molecular cloud whose temprature is 10 K. Molecular clouds are composed mainly of H2 gas. 4. A comet that is 1 km in diameter strikes the surface of Titan, Saturn’s larg ...
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Meteors, Meteoroids, and Meteorites

... bowl-shaped dimples that measure up to about 25 kilometers in diameter. Scientists have found more than 140 impact craters on the Earth. One of the most famous, the Meteor Crater in Arizona, is about 1,275 meters across and 175 meters deep. It formed nearly 50,000 years ago when an iron meteorite we ...
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A) B) C) D) 1. Which diagram best represents the regions of Earth in

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June - astra
June - astra

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Earth-Moon-Sun Answer Key

... E.ST.04.11 There are many stars larger than our Sun. Why does the Sun appear to be larger than all the other stars? A. The sun is the hottest star. B. The sun is the brightest star. C. The sun is closer to Earth than other stars. D. The sun is the only star in the Milky Way Galaxy. E.ST.04.11 Why do ...
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Earth and Space Science - science

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PPT - FLYPARSONS.org

... New Stars – Discovered that his telescopes revealed far more stars than are accessible to the unaided eye. ...
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Comparative planetary science

Comparative planetary science or comparative planetology is a branch of space science and planetary science in which different natural processes and systems are studied by their effects and phenomena on and between multiple bodies. The planetary processes in question include geology, hydrology, atmospheric physics, and interactions such as impact cratering, space weathering, and magnetospheric physics in the solar wind, and possibly biology, via astrobiology.Comparison of multiple bodies assists the researcher, if for no other reason than the Earth is far more accessible than any other body. Those distant bodies may then be evaluated in the context of processes already characterized on Earth. Conversely, other bodies (including extrasolar ones) may provide additional examples, edge cases, and counterexamples to earthbound processes; without a greater context, studying these phenomena in relation to Earth alone may result in low sample sizes and observational biases.
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