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Earths History Presentation
Earths History Presentation

... • The rate of radioactive decay is measured in terms of half-life. – Half-life is the amount of time it takes for half the atoms of a substance to decay into another element. – Different substances have different half-life’s • Examples are Uranium 238 and Carbon 14. ...
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... • Every so often the magnetic field will reverse. • When it does, so will the minerals in the igneous rocks that form at the time.  Stacked lava flows (layers)  Rocks at places where new crust is forming (Sea floor spreading = stripes) ...
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137 Amazing Facts of Earth Science

... 69. Sedimentary subclasses include clastic, organic, and chemical. 70. Limestone is formed both chemically and organically. 71. Clastic rocks are made of fragments- Conglomerate, sandstone, and shale. 72. Virginia resources include limestone, coal, and gravel. 73. Renewable resources can be replaced ...
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PART 1: DETERMINING RELATIVE AGE OF ROCKS Think about

... • the ratio of U-235 to Pb-207 in the pegmatite is 1:1 (50% uranium, 50% lead) • the ratio of U-235 to Pb-207 in the granite is 1:3. • the ratio of U-235 to Pb-207 in the the volcanic ash in the siltstone has a ratio of U-235:Pb-207 of 47:3 (94% of the original U-235 remains) • the ratio in the basa ...
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Age of the Earth



The age of the Earth is 4.54 ± 0.05 billion years (4.54 × 109 years ± 1%). This age is based on evidence from radiometric age dating of meteorite material and is consistent with the radiometric ages of the oldest-known terrestrial and lunar samples.Following the development of radiometric age dating in the early 20th century, measurements of lead in uranium-rich minerals showed that some were in excess of a billion years old.The oldest such minerals analyzed to date—small crystals of zircon from the Jack Hills of Western Australia—are at least 4.404 billion years old. Comparing the mass and luminosity of the Sun to those of other stars, it appears that the Solar System cannot be much older than those rocks. Calcium-aluminium-rich inclusions – the oldest known solid constituents within meteorites that are formed within the Solar System – are 4.567 billion years old, giving an age for the solar system and an upper limit for the age of Earth.It is hypothesised that the accretion of Earth began soon after the formation of the calcium-aluminium-rich inclusions and the meteorites. Because the exact amount of time this accretion process took is not yet known, and the predictions from different accretion models range from a few millions up to about 100 million years, the exact age of Earth is difficult to determine. It is also difficult to determine the exact age of the oldest rocks on Earth, exposed at the surface, as they are aggregates of minerals of possibly different ages.
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