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765833

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Charisse Marie Verallo

The document discusses the formation of the solar system and planetary systems. It explains that the solar system formed from a collapsing gas cloud about 4.6 billion years ago. As the cloud collapsed, a protostar and protoplanetary disk formed at the center. Over time, planets formed from accretion of matter in the disk. The document also discusses the properties of planets in our solar system as well as evidence that other stars have planets orbiting them.

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CHAPTER 5:CHAPTER 5: Formation of the Solar System and Other Planetary Systems
WHAT DO YOU THINK? How many stars are there in the solar system? Was the solar system created as a direct result of the formation of the universe? How long has the Earth existed? Is Pluto always the farthest planet from the Sun? What typical shapes do moons have? Have any Earth-like planets been discovered orbiting Sun-like stars?
You will discover…You will discover… •how the solar system formedhow the solar system formed •why the environment of the early solar system waswhy the environment of the early solar system was much more violent than it is todaymuch more violent than it is today •how the planets are groupedhow the planets are grouped •how astronomers characterize each planet’show astronomers characterize each planet’s “personality”“personality” •how the moons throughout the solar system formedhow the moons throughout the solar system formed •what the debris of the solar system is made ofwhat the debris of the solar system is made of •that planets have been observed around a growingthat planets have been observed around a growing number of starsnumber of stars •that newly forming star and planet systems are beingthat newly forming star and planet systems are being observedobserved
The lightest and simplest elements, hydrogen and helium, are abundant in the universe. Heavier elements, such as iron and silicon, are created by thermonuclear reactions in the interiors of stars, and then ejected into space by those stars. Ejection of Matter from StarsEjection of Matter from Stars FORMATION OF PLANETARY NEBULA SUPERNOVA EXPLOSIONS
Great clouds of gas and dust ejected from old stars are gathered into regions from which new stars can be made. This region in the constellation of Orion shows new stars still surrounded by the nebula from which they were formed.
Solar System FormationSolar System Formation Thanks to Mary Oshana
The Formation of a Solar SystemThe Formation of a Solar System A solar system begins as a gas cloud that collapses toward the center under the influence of gravity. A condensation forms at the center, which is called a protostar. A flattened disk of matter surrounds the protostar, which begins to shine.
The Formation of a Solar SystemThe Formation of a Solar System The rising temperature from the sun removes the gas from the inner regions, leaving dust and larger debris. The planets establish dominance in their regions of the solar system. After almost all of the remaining gas, dust, and small debris has been collected by the larger objects, the solar system takes on the form we recognize today.
Other Star Systems FormingOther Star Systems Forming We can look at young star systems developing today. The planets orbiting these stars are formed from the surrounding disks of gas and dust, called protoplanetary disks or proplyds.
PLANET FORMATIONPLANET FORMATION Within the disk that surrounds the protosun, solid grains collide and clump together into planetesimals. The terrestrial planets are built up by collisions and the accretion of planetesimals by gravitational attraction. The jovian planets are formed by gas accretion.
Thanks to Tim Worley
COMPUTER SIMULATION OF THECOMPUTER SIMULATION OF THE FORMATION OF THE SOLAR SYSTEMFORMATION OF THE SOLAR SYSTEM
Common Properties ofCommon Properties of Planet Orbits in OurPlanet Orbits in Our Solar SystemSolar System As viewed from above, all of the planets orbit the Sun in a counter-clockwise direction. The planets orbit in nearly the same plane. All planets except Pluto have an orbital inclination of less than 7°.
Planets and moons which have no appreciable atmosphere will show scars from impacts with planetary debris, called craters. Our Moon still has numerous craters, providing evidence of many impacts in its history.
Debris in Our Solar System TodayDebris in Our Solar System Today Asteroids—rocky bodies several kilometers across which orbit the sun—are found mainly in the asteroid belt located between the orbits of Mars and Jupiter. Even smaller rocky objects, called meteoroids, are scattered throughout the solar system. Billions of chunks of rock and ice called comets are located beyond the orbit of Neptune. Occasionally, one of these will be pulled toward the inner solar system and form the familiar “tails” as it orbits close to the Sun.
Comparative PlanetologyComparative Planetology ORBITS •The planets nearest to the Sun (Mercury, Venus, Earth, and Mars) are relatively close together, while those farther away (Jupiter, Saturn, Uranus, Neptune, and Pluto) are more spread out. •Most of the planets are in nearly circular orbits.
•SIZE=the physical volume of the planet •MASS=the amount of matter in an object •DENSITY=the amount of mass per unit volume Density depends on the composition of an object and not just the size. The objects shown here all have the same mass but different densities.
Two Basic Groups of PlanetsTwo Basic Groups of Planets TERRESTRIALTERRESTRIAL Small sizeSmall size Low MassLow Mass Higher densityHigher density Mostly rockMostly rock Mercury, Venus, Earth,Mercury, Venus, Earth, MarsMars JOVIANJOVIAN Large sizeLarge size MassiveMassive Low densityLow density Mostly gasMostly gas Jupiter, Saturn,Jupiter, Saturn, Uranus, NeptuneUranus, Neptune
Evidence of Planets Orbiting Other StarsEvidence of Planets Orbiting Other Stars
Extrasolar planets are either too dim or too close to the stars they orbit to observe directly. However, we can detect the effect they have on the spectra from their star to confirm their existence.
The gravitational fields of a star and its planet will cause passing light to change direction. The focusing of light by gravity is called microlensing.
Separation between Extrasolar Planets and Their StarsSeparation between Extrasolar Planets and Their Stars
AN EXTRASOLARAN EXTRASOLAR SYSTEMSYSTEM Unlike our solar system, the Upsilon Andromedea System has large planets orbiting close to the star. The orbits of the inner planets in our solar system compared to those of the Upsilon Andromedea System
WHAT DID YOU KNOW? How many stars are there in the solar system? Only one star, the Sun. Was the solar system created as a direct result of the formation of the universe? No. All matter and energy were created by the Big Bang, but the solar system formed billions of years after the Big Bang. How long has the Earth existed? 4.6 billion years.
WHAT DID YOU KNOW?  Is Pluto always the farthest planet from the Sun?  No. Pluto’s orbit is highly eccentric, bringing the planet inside Neptune’s orbit for about 20 years every 250 years.  What typical shapes do moons have?  Most look roughly like potatoes.  Have any Earth-like planets been discovered orbiting Sun-like stars?  No. Nearly all the planets orbiting Sun-like stars are Jupiter-like gas giants.

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765833

  • 1. CHAPTER 5:CHAPTER 5: Formation of the Solar System and Other Planetary Systems
  • 2. WHAT DO YOU THINK? How many stars are there in the solar system? Was the solar system created as a direct result of the formation of the universe? How long has the Earth existed? Is Pluto always the farthest planet from the Sun? What typical shapes do moons have? Have any Earth-like planets been discovered orbiting Sun-like stars?
  • 3. You will discover…You will discover… •how the solar system formedhow the solar system formed •why the environment of the early solar system waswhy the environment of the early solar system was much more violent than it is todaymuch more violent than it is today •how the planets are groupedhow the planets are grouped •how astronomers characterize each planet’show astronomers characterize each planet’s “personality”“personality” •how the moons throughout the solar system formedhow the moons throughout the solar system formed •what the debris of the solar system is made ofwhat the debris of the solar system is made of •that planets have been observed around a growingthat planets have been observed around a growing number of starsnumber of stars •that newly forming star and planet systems are beingthat newly forming star and planet systems are being observedobserved
  • 4. The lightest and simplest elements, hydrogen and helium, are abundant in the universe. Heavier elements, such as iron and silicon, are created by thermonuclear reactions in the interiors of stars, and then ejected into space by those stars. Ejection of Matter from StarsEjection of Matter from Stars FORMATION OF PLANETARY NEBULA SUPERNOVA EXPLOSIONS
  • 5. Great clouds of gas and dust ejected from old stars are gathered into regions from which new stars can be made. This region in the constellation of Orion shows new stars still surrounded by the nebula from which they were formed.
  • 6. Solar System FormationSolar System Formation Thanks to Mary Oshana
  • 7. The Formation of a Solar SystemThe Formation of a Solar System A solar system begins as a gas cloud that collapses toward the center under the influence of gravity. A condensation forms at the center, which is called a protostar. A flattened disk of matter surrounds the protostar, which begins to shine.
  • 8. The Formation of a Solar SystemThe Formation of a Solar System The rising temperature from the sun removes the gas from the inner regions, leaving dust and larger debris. The planets establish dominance in their regions of the solar system. After almost all of the remaining gas, dust, and small debris has been collected by the larger objects, the solar system takes on the form we recognize today.
  • 9. Other Star Systems FormingOther Star Systems Forming We can look at young star systems developing today. The planets orbiting these stars are formed from the surrounding disks of gas and dust, called protoplanetary disks or proplyds.
  • 10. PLANET FORMATIONPLANET FORMATION Within the disk that surrounds the protosun, solid grains collide and clump together into planetesimals. The terrestrial planets are built up by collisions and the accretion of planetesimals by gravitational attraction. The jovian planets are formed by gas accretion.
  • 12. COMPUTER SIMULATION OF THECOMPUTER SIMULATION OF THE FORMATION OF THE SOLAR SYSTEMFORMATION OF THE SOLAR SYSTEM
  • 13. Common Properties ofCommon Properties of Planet Orbits in OurPlanet Orbits in Our Solar SystemSolar System As viewed from above, all of the planets orbit the Sun in a counter-clockwise direction. The planets orbit in nearly the same plane. All planets except Pluto have an orbital inclination of less than 7°.
  • 14. Planets and moons which have no appreciable atmosphere will show scars from impacts with planetary debris, called craters. Our Moon still has numerous craters, providing evidence of many impacts in its history.
  • 15. Debris in Our Solar System TodayDebris in Our Solar System Today Asteroids—rocky bodies several kilometers across which orbit the sun—are found mainly in the asteroid belt located between the orbits of Mars and Jupiter. Even smaller rocky objects, called meteoroids, are scattered throughout the solar system. Billions of chunks of rock and ice called comets are located beyond the orbit of Neptune. Occasionally, one of these will be pulled toward the inner solar system and form the familiar “tails” as it orbits close to the Sun.
  • 16. Comparative PlanetologyComparative Planetology ORBITS •The planets nearest to the Sun (Mercury, Venus, Earth, and Mars) are relatively close together, while those farther away (Jupiter, Saturn, Uranus, Neptune, and Pluto) are more spread out. •Most of the planets are in nearly circular orbits.
  • 17. •SIZE=the physical volume of the planet •MASS=the amount of matter in an object •DENSITY=the amount of mass per unit volume Density depends on the composition of an object and not just the size. The objects shown here all have the same mass but different densities.
  • 18. Two Basic Groups of PlanetsTwo Basic Groups of Planets TERRESTRIALTERRESTRIAL Small sizeSmall size Low MassLow Mass Higher densityHigher density Mostly rockMostly rock Mercury, Venus, Earth,Mercury, Venus, Earth, MarsMars JOVIANJOVIAN Large sizeLarge size MassiveMassive Low densityLow density Mostly gasMostly gas Jupiter, Saturn,Jupiter, Saturn, Uranus, NeptuneUranus, Neptune
  • 19. Evidence of Planets Orbiting Other StarsEvidence of Planets Orbiting Other Stars
  • 20. Extrasolar planets are either too dim or too close to the stars they orbit to observe directly. However, we can detect the effect they have on the spectra from their star to confirm their existence.
  • 21. The gravitational fields of a star and its planet will cause passing light to change direction. The focusing of light by gravity is called microlensing.
  • 22. Separation between Extrasolar Planets and Their StarsSeparation between Extrasolar Planets and Their Stars
  • 23. AN EXTRASOLARAN EXTRASOLAR SYSTEMSYSTEM Unlike our solar system, the Upsilon Andromedea System has large planets orbiting close to the star. The orbits of the inner planets in our solar system compared to those of the Upsilon Andromedea System
  • 24. WHAT DID YOU KNOW? How many stars are there in the solar system? Only one star, the Sun. Was the solar system created as a direct result of the formation of the universe? No. All matter and energy were created by the Big Bang, but the solar system formed billions of years after the Big Bang. How long has the Earth existed? 4.6 billion years.
  • 25. WHAT DID YOU KNOW?  Is Pluto always the farthest planet from the Sun?  No. Pluto’s orbit is highly eccentric, bringing the planet inside Neptune’s orbit for about 20 years every 250 years.  What typical shapes do moons have?  Most look roughly like potatoes.  Have any Earth-like planets been discovered orbiting Sun-like stars?  No. Nearly all the planets orbiting Sun-like stars are Jupiter-like gas giants.

Editor's Notes

  1. The orbital inclination is the angle between a planet’s orbit and the ecliptic.