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Grade 11 Earth Science Lesson 1
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Fact Sheet in Earth Science
Lesson 1: The Universe and the Solar System
MOTIVATION: The Universe is said to be at least 13. billion of years old and the Earth/ Solar System at least 4.5-4.6 billion of years old. But how large exactly is a billion? How long will it take you to spend 1 billion pesos if you spend 1 peso per second?
Beyond our planet earth, we find it is but a small part of a larger entity, the solar system. It consists of the sun, nine planets and minor components such as satellites of planets, asteroids, comets, meteor and meteorites. The sun takes up more than 99% of the mass of the whole system.
The sun is but one of the billion stars forming the assembly called the Milky Way Galaxy. Outside the Milky Way at great distance are other galaxies, each containing 10 9 to 10 11 stars.
This galaxy is a cluster of billions of stars from superclusters. Because the galaxies are so far away, they look like tiny faint clouds in the night sky. Scattered throughout the system of stars are great clouds of gas and dust known as nebulae.
A galaxy is a cluster of billions of stars and clusters of galaxies form superclusters. In between the clusters is practically an empty space. This organization of matter in the universe. suggests that it is indeed clumpy at a certain
The sun is but one of the billion stars forming the assembly called the Milky Way Galaxy. Outside the Milky Way at great distance are other galaxies, each containing 10^9 to 10 11 stars.
This galaxy is a cluster of billions of stars from superclusters. Because the galaxies are so far away, they look like tiny faint clouds in the night sky. Scattered throughout the system of stars are great clouds of gas and dust known as nebulae.
All these celestial bodies and the vast space between them constitute the physical Universe. Because of its seemingly orderly arrangement, it is sometimes called the cosmos.
Cosmology is the study of the nature of the universe as a whole. It is the scientific inquiry into the origin, evolution, and the fate of the universe. By making assumptions that are not at odds with the observable universe, cosmologists create models, or theories that attempt to describe the universe, its origin, and its future.
Structure, Composition, and Age The universe is made of:
comprises atoms, planets, stars, galaxies, and other bodies. Example:
“While dark energy repels, dark matter attracts…”
Hydrogen Helium are the three most abundant elements. lithium
*Inside every new born star are hydrogen atoms fused together to make Helium. This process is called Fusion or “nuclear burning” (nucleosynthesis) and it creates the energy that powers every star (i.e. a natural hydrogen bomb).
Stars - the building block of galaxies born out of clouds of gas and dust in galaxies. Instabilities within the clouds eventually results into gravitational collapse, rotation, heating up, and transformation to a protostar.
Protostar - is a baby star, an area of material that hasn't yet formed into a full-fledged star.
Stellar interiors - are like furnaces where elements are synthesized or combined/fused together. main sequence star - stars that fuse hydrogen atoms to form helium atoms in their cores;
Steady State Model
Big Bang Theory
The Steady State Model and the Big Bang Theory are both models of how the universe began.
Expanding Universe
Edwin Hubble - in 1992, he announced his significant discovery of the “redshift” and its interpretation that galaxies are moving away from each other, hence as evidence for an expanding universe, just as predicted by Einstein’s Theory of General Relativity.
Red Shift – a change in frequency of the position of the lines.
***** You may have noticed that when an ambulance or police car goes past, its siren is high-pitched as it comes towards you, then becomes low-pitched as it goes away. This effect, where there is change in frequency and wavelength, is called the Doppler Effect. It happens with any wave source that moves relative to an observer.
This happens with light too. Our sun contains helium. We know this because there are black lines in the spectrum of the light from the sun, where helium has absorbed light. These lines form the absorption spectrum for helium.
When we look at the spectrum of a distant star, the absorption spectrum is there, but the pattern of lines has moved towards the red end of the spectrum, as you can see below.
The main differences between the two theories: