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8th Grade Science
8th Grade Science

... This test covers the material in chapter 14, sections 1-5 1. Know the following scientists: who they were and what they contributed to our understanding of the solar system. a. Ptolemy d. Tycho Brahe b. Copernicus e. Kepler c. Galileo f. Newton 2. What was the ancient Greek’s knowledge of the solar ...
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... helium. They have the greatest gravitational forces allowing them to attract more objects such as moons. The gas giants are further away from the sun than the terrestrial planets. Jupiter is the largest planet in the solar system with the highest surface gravity. It also has the most moons of all th ...
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Solar System Formation
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Study Notes for Chapters 27: Planets of the Solar System Directions
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Observational Astronomy - Lecture 7 Solar System II
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Review Questions - Dublin City Schools

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webquest – solar system - Teach

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Earth in the Universe

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Solar System

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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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