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Final Exam Prep
Final Exam Prep

... 4. Ch 27 Planets of the Solar Systems pp685-708 Review the Nebular Hypothesis (Section 1- How did the Solar System Form) Review your big super summary sheet that lists the characteristics of the Inner and Outer Planets. Terms: solar nebula, planetessimal, terrestrial planet, gas giant planet 5. Ch 2 ...
Unit 3
Unit 3

...  Mercury can be seen from Earth just before sunrise or just after sunset. Why? Mercury always appears near the Sun when viewed from Earth.  Mercury has a very thin atmosphere. Humans would not be able to live there.  The surface of Mercury has holes in it where objects such as meteorites (i.e., a ...
Week 9
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... How did jovian planets form? • Ice crystals forms small particles outside the frost line. • Larger planetesimals and planets form by sweeping out larger area of orbit. • Metal particles form cores of gas giants • Gravity of these larger planets was able to draw in surrounding H and He gases. ...
The most important questions to study for the exam
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... • by the ancient Greeks as they observed the stars and the "wandering stars," which they called the planets ...
day_and_night - Primary Resources
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... Why do we have day and night? ...
Planets and Moons
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... What are moons?  Moons are like little planets that encircle the real planets.  Usually, they are much smaller than planets.  Planets can have no moons (like Mercury and Venus), one moon (like Earth) or up to a very large number of moons (e.g. 63 for Jupiter). ...
Asteroids PP - MR D`S ICT CORNER
Asteroids PP - MR D`S ICT CORNER

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Benchmark One Study Guide: Science Benchmark Wed
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... The universe began as a tiny ball of matter called a singularity that exploded and sent the entire universe flying out in space, or expanding. The theory was originated by George Llamatre and supported by Edwin Hubble. 13. What is nebula? A cloud of gas and dust that forms stars and planets. 14. Wha ...
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... from each other, but they appear grouped together when viewed from Earth • One of the 88 sectors into which astronomers divide the sphere of the skynamed after a traditional constellation in that sector • Patterns of constellations are dynamic; therefore, the constellations of 100,000 years ago are ...
day 1 lesson plan - University of Chicago
day 1 lesson plan - University of Chicago

... Opener (5 min): Name all of the planets in our solar system. We know that on the moon we would have a different weight than we do here on earth. Would you have different weights on the other planets? If so, on which planet do you think you weigh the least? the most? Go over opener (5min) Introduce t ...
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... will complete one circle ‘cycle’ and point back at the same point. This is known as? 24.The Earth’s axis of tilt can vary from its current 23.5 degree tilt (T/F) 26. In another 13,000 years, Earth's axial tilt will point in the opposite direction it does now. Assuming the other astronomical influenc ...
Introduction Notes - Sunflower Astronomy
Introduction Notes - Sunflower Astronomy

... - involves huge numbers for distances, mass, and time. - involves small numbers for describing phenomena at the atomic level. Overview of the Universe Solar System: Eight (or Nine) planets, Sun, minor planets, moons, comets, meteoroids, and dust. Terrestrial Planets: Mercury, Venus, Earth, and Mars ...
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AN INTRODUCTION TO ASTRONOMY Dr. Uri Griv Department of Physics, Ben-Gurion University

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... • If the sun makes up 99.8% of the solar system and the more massive an object is the more gravity it has, why aren’t Mercury and Venus pulled into the sun? • The Law of Universal Gravitation states that all objects in the universe have a gravitational attraction towards each other. Therefore, the o ...
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space - Kidblog

... mass of all the other planets of the solar system put together! It is a gas giant, rather than a terrestrial planet, and is made largely of hydrogen and helium. Jupiter was first visited by Pioneer 10 in 1973 and later by Pioneer 11, Voyager 1, Voyager 2 and Ulysses. The unmanned spacecraft Galileo ...
Planets and Moons - Fraser Heights Chess Club
Planets and Moons - Fraser Heights Chess Club

...  The planets are kept in their orbits due to the pulling force of the Sun’s gravity.  The time a planet makes one trip around the Sun is called a Year.  Each planet spins around itself and around the Sun. The face of the planet towards the Sun, receives the light, the other is in the dark The pla ...
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Study Guide: Solar System

... b. Copernicus: Proposed that the Sun was the center (heliocentric model) of the  solar systems orbiting in perfect circles  c. Kepler: Supported the heliocentric model but discovered that the orbits of the  planets were not circular but elliptical.  d. Galileo: Worked with the refracting telescopes  ...
4th-grade-science-lesson-plan
4th-grade-science-lesson-plan

... out the introduction cards. If not, the teacher will read this aloud so each group can hear) 4. The group will see who has the first planet, read it, and then the entire group will proceed to do the activity. 5. This will continue until all cards are used and the students reach Neptune COOL DOWN  G ...
Terrestrial planet formation In the inner Solar System, think dust (no
Terrestrial planet formation In the inner Solar System, think dust (no

... called planetary embryos (Moon to Mercury size) Slower assembly of 50-100 embryos into final terrestrial planets. 10 - 100 million years. ...
Astro 1010 Planetary Astronomy Sample Questions for Exam 3
Astro 1010 Planetary Astronomy Sample Questions for Exam 3

... c) meteorites and meteoroids. d) moons and stars. ...
8.1_Formation of the Universe
8.1_Formation of the Universe

... Our Galaxy- Milky Way ...
Glossary from “The Wizard from Space”
Glossary from “The Wizard from Space”

... star to Earth. The other stars are so far away from us that they appear to be points of light in the night sky. Some stars are smaller than the sun while others are much larger. Cooler stars have a surface temperature of a few thousand degrees, the sun has a surface temperature of 6000 degrees, whil ...
Our Solar System
Our Solar System

... planet, temperatures get as low as –235 degrees C. • It is the only planet not visited by any space craft. • It is 3,666 million miles from the sun. • Not much is know about Pluto. ...
the major characteristics of each planet
the major characteristics of each planet

... SURFACE FEATURES OF THE PLANETS MERCURY Rocky, with many lunar-like craters up to 200 km across. 2 km-4 km high cliffs, hundreds of kilometres long, caused by the planet cooling and shrinking. Darkest surface of all the planets. VENUS ...
Sept2 - University of Arizona
Sept2 - University of Arizona

... by the Congregation of the Index "until corrected." It stayed on this list of prohibited books and teachings until 1822. Martin Luther (1483-1546): [Copernicus] “is a fool who wishes to reverse the entire scheme of astronomy; but sacred scripture tells us that Joshua commanded the Earth to stand sti ...
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History of Solar System formation and evolution hypotheses



Ideas concerning the origin and fate of the world date from the earliest known writings; however, for almost all of that time, there was no attempt to link such theories to the existence of a ""Solar System"", simply because almost no one knew or believed that the Solar System, in the sense we now understand it, existed. The first step towards a theory of Solar System formation was the general acceptance of heliocentrism, the model which placed the Sun at the centre of the system and the Earth in orbit around it. This conception had been gestating for thousands of years, but was only widely accepted by the end of the 17th century. The first recorded use of the term ""Solar System"" dates from 1704.
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