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Our Solar System
Our Solar System

... massive loop of plasma lifting off the surface of the sun. Prominences can loop hundreds of thousands of miles into space. Prominences are held above the Sun's surface by strong magnetic fields and can last for many months. ...
8003
8003

... Earth–type planets were initially formed as giant planets, similarly to the planets of the group of Jupiter and simultaneously with the solar mass by the accumulation of aqueous–hydrogen planetesimals, which were similar by physical state to Pluto, Charon, and comets. Gravitational compression was a ...
Now - National Geographic Magazine, UK
Now - National Geographic Magazine, UK

... a time when planetary scientists were puzzled by several other features of the solar system. By the early 2000s they had long since realized that the birth pangs of the solar system had been violent. The planets had not condensed gently from the solar nebula; instead they had grown to full size by a ...
The Inner Solar System - Super Teacher Worksheets
The Inner Solar System - Super Teacher Worksheets

... caps at the poles are water, forever frozen because of the colder temperatures further from Second in line comes Venus, which is the Sun. The only place the temperature rises sometimes called Earth's twin. It's about the same above freezing is at the equator, or the middle of size as Earth, but that ...
The Inner Solar System - Super Teacher Worksheets
The Inner Solar System - Super Teacher Worksheets

... caps at the poles are water, forever frozen because of the colder temperatures further from Second in line comes Venus, which is the Sun. The only place the temperature rises sometimes called Earth's twin. It's about the same above freezing is at the equator, or the middle of size as Earth, but that ...
Our Solar System Planets Their Size and Distance
Our Solar System Planets Their Size and Distance

... • Included are moons for Earth, Saturn, Jupiter (4) and Pluto • The planets are exhibited as 3D models. • The 2 largest planetary models, Jupiter and Saturn, measure 4-5 feet across (1.22 - 1.52 m), and the 2 mid-sized planets Uranus and Neptune measure 21-22 inches (53 - 56 cm) http://pages.umpi.ed ...
GLY 1001 Answers to Chapter 21 Review Questions
GLY 1001 Answers to Chapter 21 Review Questions

... 8. No; however, he was the first to use it astronomically. 9. A rotating Earth is necessary in the Copernican system; however, it was believed that Earth would fly apart if it rotated. Hence, if the Sun could rotate and remain intact, so could Earth. 10. (Diagrams will vary) Venus will be full when ...
The Solar System - Belle Vernon Area School District
The Solar System - Belle Vernon Area School District

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Powerpoint - BU Imaging Science
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... • Asteroids are small, rocky bodies that orbit the Sun. Most are found in the asteroid belt between Mars and Jupiter. There are many asteroids. • Comets are small, icy bodies that orbit the Sun. Comets have very elliptical orbits, only becoming visible when they form tails in the inner solar system. ...
Our Planetary System (Chapter 7)
Our Planetary System (Chapter 7)

... • Asteroids are small, rocky bodies that orbit the Sun. Most are found in the asteroid belt between Mars and Jupiter. There are many asteroids. • Comets are small, icy bodies that orbit the Sun. Comets have very elliptical orbits, only becoming visible when they form tails in the inner solar system. ...
Nebula Theory
Nebula Theory

... • Farther out in the protoplanetary disk where the temperature of the gas is lower, the density of solids is enhanced with rocky and icy planetesimals. • Such an enhancement of the solid density may cause collisional accumulation of solids and results in runaway growth to a mass of approximately10 E ...
Solar System
Solar System

... • Giant Impact Theory – Mars-size planetesimal collides with Earth – Metal sinks to Earth’s core, volatiles lost, mantle material “splashed” into space – Mantle material coalesces into Moon – Moon spirals away from Earth over time ...
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Mercury Mercury is a dead planet and the

... Someday  humans  may  live  on  Mars,  but  it   won’t  be  easy.    The  carbon  dioxide   atmosphere  is  so  poisonous  and  cold  that   think  liquid  water  cannot  exist  on  the  surface.    But  if  you  like  pink   da ...
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... of a star surrounded by planets and other objects. In 1995, astronomers found a planet orbiting (going around) a distant star like our Sun. Since then, they have found other solar systems. Astronomers now think that there are many solar systems in the universe. They do not know whether there is life ...
The Earth and Other Planets
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... Explore First, students will be given a poster and small materials such as a quarter, grain of salt, pencil eraser, etc. As a group, students will predict which planet each object is similar to in size. Each group will share their predictions with the class. Then the class will have an introduction ...
2nd Leaflet: A Tour of the Human Orrery
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... Saturn is most famous for its distinctive ring system. For many years these rings seemed to be unique in the known solar system. However, faint rings were discovered around Uranus in 1977, and shortly thereafter also around Jupiter and Voyager 2 image of Saturn, July 1981 (NASA and Neptune. Saturn’s ...
Astronomy
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... of Jupiter (4) = Earth is not the center of all universal motion  Planets are circular disc = must be Earth-like  Venus has phases like the moon = orbits light source (sun)  Moon’s surface not smooth = validated others who named areas based on features (Sea of Tranquility)  Sun has dark regions ...
Satellites of Other Planets
Satellites of Other Planets

... lies beyond Neptune’s orbit Matter leftover from the formation of the solar system ...
planets finalized - Hewlett
planets finalized - Hewlett

... Heliocentric model A heliocentric system is one in which the planets revolve around a fixed sun. Thus Mercury, Venus, the Earth, Mars, Jupiter and Saturn all revolve around the sun ...
Smaller Bodies of the Solar System
Smaller Bodies of the Solar System

... _______ supposedly left over from the formation of the solar system proposed as source for long-period comets and a replenisher of the Oort Cloud.  beyond Neptune (extending from 30 AU out to around 100 AU).  occasionally disturbed by gravitational interactions these objects are sent hurtling into ...
Destination Antarctica Study Buddy
Destination Antarctica Study Buddy

... may happen as a result. Polar ice-caps are reducing in average size. The result is possible coastline flooding and weather changes. I can describe characteristics of each of the planets in our solar system. Mercury—smallest and closest to the sun Venus—the hottest, referred to as Earth’s twin Earth— ...
GEOL3025, Section 030 Lecture #11 31 August 2007
GEOL3025, Section 030 Lecture #11 31 August 2007

... AKA Jovian Planets (like Jupiter) Gas Giants: Jupiter & Saturn Ice Giants: Uranus & Neptune + Pluto (Rocky-Ice planet?) ...
Powerpoint Presentation (large file)
Powerpoint Presentation (large file)

... • The Jovian (Jupiter-like) planets are composed primarily of light elements such as hydrogen and helium, which gives these planets low ...
Comparative Planetology I: Our Solar System Chapter Seven
Comparative Planetology I: Our Solar System Chapter Seven

... • The Jovian (Jupiter-like) planets are composed primarily of light elements such as hydrogen and helium, which gives these planets low ...
Explore Our Solar System
Explore Our Solar System

... Jupiter is the largest planet. It is made of thick gases. If you tried to land a rocket ship, you would sink into the planet! Saturn is the second-largest planet. Like Jupiter, it is made mostly of gases. Its rings are made up of rock, ice, and dust. Uranus is cold and windy. It was the first planet ...
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Late Heavy Bombardment



The Late Heavy Bombardment (abbreviated LHB and also known as the lunar cataclysm) is a hypothetical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago, corresponding to the Neohadean and Eoarchean eras on Earth. During this interval, a disproportionately large number of asteroids apparently collided with the early terrestrial planets in the inner Solar System, including Mercury, Venus, Earth, and Mars. The LHB happened after the Earth and other rocky planets had formed and accreted most of their mass, but still quite early in Earth's history.Evidence for the LHB derives from lunar samples brought back by the Apollo astronauts. Isotopic dating of Moon rocks implies that most impact melts occurred in a rather narrow interval of time. Several hypotheses are now offered to explain the apparent spike in the flux of impactors (i.e. asteroids and comets) in the inner Solar System, but no consensus yet exists. The Nice model is popular among planetary scientists; it postulates that the gas giant planets underwent orbital migration and scattered objects in the asteroid and/or Kuiper belts into eccentric orbits, and thereby into the path of the terrestrial planets. Other researchers argue that the lunar sample data do not require a cataclysmic cratering event near 3.9 Ga, and that the apparent clustering of impact melt ages near this time is an artifact of sampling materials retrieved from a single large impact basin. They also note that the rate of impact cratering could be significantly different between the outer and inner zones of the Solar System.
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