our solar system i origins of the solar system astronomy 12

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Our Solar Our Solar System I System I Origins of the Solar System Astronomy 12

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Page 1: Our Solar System I Origins of the Solar System Astronomy 12

Our Solar System IOur Solar System I

Origins of the Solar System

Astronomy 12

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Learning Outcomes (Students will…)-Explain the theories for the origin of the solar system

-Distinguish between questions that can be answered by science and those that cannot, and between problems that can be solved by technology and those that cannot with regards to solar system formation.

-Estimate quantities of distances in parsec. Estimate the age of the solar system. -Describe and apply classification systems and nomenclature used in the sciences. Classify planets as terrestrial vs. Jovian, inner vs. outer, etc. Classify satellites. Classify meteoroid, asteroid, dwarf planet, planet. Classify comets as long period vs. short period. etc

-Formulate operational definitions of major variables. Given data such as diameter and density describe the properties that divide the planets and moons into groups.

-Tools and methods used to observe and measure the inner and the outer planets and the minor members of the solar system

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Our Solar SystemOur Solar System

Our solar system is made Our solar system is made up of:up of:

SunSunEight planets Eight planets Their moonsTheir moonsAsteroids & MeteroidsAsteroids & MeteroidsCometsComets

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Inner PlanetsInner Planets

The inner four rocky planets The inner four rocky planets at the center of the solar at the center of the solar system are:system are:

MercuryMercuryVenusVenusEarthEarthMarsMars

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MercuryMercury

Planet nearest the sunPlanet nearest the sunSecond smallest planetSecond smallest planetCovered with cratersCovered with cratersHas no moons or ringsHas no moons or ringsAbout size of Earth’s moonAbout size of Earth’s moon

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VenusVenus

Sister planet to EarthSister planet to EarthHas no moons or ringsHas no moons or ringsHot, thick atmosphereHot, thick atmosphereBrightest object in sky besides sun and Brightest object in sky besides sun and

moon (looks like bright star)moon (looks like bright star)Covered with craters, volcanoes, and Covered with craters, volcanoes, and

mountainsmountains

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EarthEarth

Third planet from sunThird planet from sunOnly planet known to have life and Only planet known to have life and

liquid waterliquid waterAtmosphere composed of Nitrogen Atmosphere composed of Nitrogen

(78%), Oxygen (21%), and other gases (78%), Oxygen (21%), and other gases (1%).(1%).

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MarsMars

Fourth planet from sunFourth planet from sunAppears as bright reddish color in the Appears as bright reddish color in the

night skynight skySurface features volcanoes and huge Surface features volcanoes and huge

dust stormsdust stormsHas 2 moons: Has 2 moons: Phobos and DeimosPhobos and Deimos

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Asteroid BeltAsteroid Belt

Separates the inner, terrestrial planets Separates the inner, terrestrial planets from the outer, Jovian planetsfrom the outer, Jovian planets

Contains ~100,000 asteroids.Contains ~100,000 asteroids.Largest known asteroid: 4 VestaLargest known asteroid: 4 VestaLargest object : Ceres (dwarf planet)Largest object : Ceres (dwarf planet)

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Outer PlanetsOuter Planets

The outer planets composed The outer planets composed of gas are :of gas are :

JupiterJupiterSaturnSaturnUranusUranusNeptuneNeptune

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JupiterJupiter

Largest planet in solar systemLargest planet in solar system Brightest planet in skyBrightest planet in sky At last count, 65 moons: 5 visible from EarthAt last count, 65 moons: 5 visible from Earth Strong magnetic fieldStrong magnetic field Giant red spotGiant red spot Rings have 3 parts: Halo Ring, Main Ring, Rings have 3 parts: Halo Ring, Main Ring,

Gossamer RingGossamer Ring

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SaturnSaturn 66thth planet from sun planet from sun Beautiful set of rings Beautiful set of rings 62 moons62 moons Largest moon, Titan, Largest moon, Titan, Easily visible in the night Easily visible in the night

skysky Voyager explored Saturn Voyager explored Saturn

and its rings.and its rings.

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UranusUranus 77thth planet from sun planet from sun Has a faint ring systemHas a faint ring system 27 known moons27 known moons Covered with cloudsCovered with clouds Uranus sits on its side with the north Uranus sits on its side with the north

and south poles sticking out the and south poles sticking out the sides.sides.

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NeptuneNeptune

88thth planet from sun planet from sunDiscovered through mathDiscovered through math12 known moons12 known moonsTriton largest moonTriton largest moonGreat Dark Spot thought to be a Great Dark Spot thought to be a

hole, similar to the hole in the hole, similar to the hole in the ozone layer on Earthozone layer on Earth

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A Dwarf PlanetA Dwarf Planet

Pluto is a small solid icy Pluto is a small solid icy planet is smaller than the planet is smaller than the Earth's Moon.Earth's Moon.

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PlutoPluto

Never visited by Never visited by spacecraftspacecraft

Orbits very slowlyOrbits very slowly

Charon, its moon, is Charon, its moon, is very close to Pluto very close to Pluto and about the same and about the same sizesize

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Two Types of Planets: Terrestrial and Jovian

Why?

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• Sun, a star, at the center

• Inner (rocky) Planets (Mercury, Venus, Earth, Mars) ~ 1 AU

• Asteroid Belt ~ 3 AU

• Outer (gaseous) Planets (Jupiter, Saturn, Neptune, Uranus) ~ 5-40 AU

• Kuiper Belt ~ 30 to 50 AU-includes Pluto

• Oort Cloud ~ 50,000 AU

What does the solar system look like from far away?

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Bode’s Law•A rough rule that predicts the spacing of the planets in the Solar System

•To find the mean distances of the planets, beginning with the following simple sequence of numbers:

0 3 6 12 24 48 96 192 384•With the exception of the first two, the others are simple twice the value of the preceding number.

•Add 4 to each number:4 7 10 16 28 52 100 196 388

•Then divide by 10:0.4 0.7 1.0 1.6 2.8 5.2 10.0 19.6 38.8

PlanetPlanet Actual Distance (AU)Actual Distance (AU) Bode’s LawBode’s Law

Mercury 0.39 0.4

Venus 0.72 0.7

Earth 1.00 1.0

Mars 1.52 1.6

Jupiter 5.20 5.2

Saturn 9.54 10.0

Uranus 19.2 19.6

Neptune 30.1 38.8

Works for

moons too!

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AsteroidsAsteroids Small bodies Small bodies Believed to be left over Believed to be left over

from the beginning of from the beginning of the solar system billions the solar system billions of years agoof years ago

100,000 asteroids lie in 100,000 asteroids lie in belt between Mars and belt between Mars and JupiterJupiter

Largest asteroids have Largest asteroids have been given namesbeen given names

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Most asteroids are located in two regions:

•Asteroid belt

•Orbit of Jupiter… the Hildas (the orange "triangle" just inside the orbit of Jupiter) and the Jovian Trojans (green). The group that leads Jupiter are called the "Greeks" and the trailing group are called the "Trojans"

Where are the asteroids?

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CometsComets

Small icy bodiesSmall icy bodiesTravel past the SunTravel past the SunGive off gas and dust as Give off gas and dust as

they pass bythey pass by

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Anatomy of a Comet

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Where are the comets?

Kuiper Belt A large body of small objects orbiting (the short period comets <200 years) the Sun in a radial zone extending outward from the orbit of Neptune (30 AU) to about 100 AU. Pluto maybe the biggest of the Kuiper Belt object.

Oort Cloud Long Period Comets (period > 200 years) seems to come mostly from a spherical region at about 50,000 AU from the Sun.

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Key Ideas

Properties of the Planets: All of the planets orbit the Sun in the same direction and in almost the same plane. Most of the planets have nearly circular orbits.

The four inner planets are called terrestrial planets. They are relatively small (with diameters of 5000 to 13,000 km), have high average densities (4000 to 5500 kg/m3), and are composed primarily of rocky materials.

The four giant outer planets are called Jovian planets. They have large diameters (50,000 to 143,000 km) and low average densities (700 to 1700 kg/m3) and are composed primarily of light elements such as hydrogen and helium.

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Key Ideas

Satellites and Small Bodies in the Solar System: Besides the planets, the solar system includes satellites of the planets, asteroids, comets, and trans-Neptunian objects.

Seven large planetary satellites (one of which is our Moon) are comparable in size to the planet Mercury. The remaining satellites of the solar system are much smaller.

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Key Ideas

Asteroids are small, rocky objects, while comets and trans-Neptunian objects are made of ice and rock. All are remnants left over from the formation of the planets.

Most asteroids are found in the asteroid belt between the orbits of Mars and Jupiter, and most trans-Neptunian objects lie in the Kuiper belt outside the orbit of Neptune. Pluto is one of the largest members of the Kuiper belt.

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Key Ideas

Spectroscopy and the Composition of the Planets: Spectroscopy, the study of spectra, provides information about the chemical composition of objects in the solar system.

The spectrum of a planet or satellite with an atmosphere reveals the atmosphere’s composition. If there is no atmosphere, the spectrum indicates the composition of the surface.

The substances that make up the planets can be classified as gases, ices, or rock, depending on the temperatures at which they solidify.

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Key Ideas

Impact Craters: When an asteroid, comet, or meteoroid collides with the surface of a terrestrial planet or satellite, the result is an impact crater.

Geologic activity renews the surface and erases craters, so a terrestrial world with extensive cratering has an old surface and little or no geologic activity.

Because geologic activity is powered by internal heat, and smaller worlds lose heat more rapidly, as a general rule smaller terrestrial worlds are more extensively cratered.

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Key Ideas

Magnetic Fields and Planetary Interiors: Planetary magnetic fields are produced by the motion of electrically conducting liquids inside the planet. This mechanism is called a dynamo. If a planet has no magnetic field, that is evidence that there is little such liquid material in the planet’s interior or that the liquid is not in a state of motion.

The magnetic fields of terrestrial planets are produced by metals such as iron in the liquid state. The stronger fields of the Jovian planets are generated by liquid metallic hydrogen or by water with ionized molecules dissolved in it.