Chapter 15
... 4. Uranus’s tilted axis may be the result of a glancing collision. 5. Miranda may have been almost destroyed in a collision. 6. Interactions between jovian protoplanets and planetesimals could be responsible for irregular moons. 7. Binary Kuiper belt objects (including the Pluto-Charon system) could ...
... 4. Uranus’s tilted axis may be the result of a glancing collision. 5. Miranda may have been almost destroyed in a collision. 6. Interactions between jovian protoplanets and planetesimals could be responsible for irregular moons. 7. Binary Kuiper belt objects (including the Pluto-Charon system) could ...
2 choices
... Classifying the Solar System – Key A 1. Earth B 2. Jupiter A 3. Mars A 4. Mercury B 5. Neptune B 6. Saturn B 7. Uranus A 8. Venus A 9. Earth B 10. Jupiter A 11. Mars A 12. Mercury B 13. Neptune B 14. Saturn B 15. Uranus A 16. Venus A 17. Jupiter A 18. Mars 15 | P a g e ...
... Classifying the Solar System – Key A 1. Earth B 2. Jupiter A 3. Mars A 4. Mercury B 5. Neptune B 6. Saturn B 7. Uranus A 8. Venus A 9. Earth B 10. Jupiter A 11. Mars A 12. Mercury B 13. Neptune B 14. Saturn B 15. Uranus A 16. Venus A 17. Jupiter A 18. Mars 15 | P a g e ...
Space – Align the Stars - VUTechieTeacher
... Space – Align the Stars 1. The sun, together with all the planets, asteroids, comets, and meteors that orbit around it, collectively make up our _____________. ...
... Space – Align the Stars 1. The sun, together with all the planets, asteroids, comets, and meteors that orbit around it, collectively make up our _____________. ...
Lecture14
... The Orbits of Comets • Newton recognized that the orbits of comets were highly eccentric • Edmund Halley published calculations in 1705 for the orbits of 24 comets and predicted that a particular comet would return in 1758 ...
... The Orbits of Comets • Newton recognized that the orbits of comets were highly eccentric • Edmund Halley published calculations in 1705 for the orbits of 24 comets and predicted that a particular comet would return in 1758 ...
46. Elliptical Orbits
... Place one pin in f0 and place a string loop around the pin. Place a pencil inside the string loop and pull the loop tight with one hand, while securing the pin with the other hand. Tilt the pencil slightly and move the pencil around 360o, keeping the string tight. This will draw a circle. Label the ...
... Place one pin in f0 and place a string loop around the pin. Place a pencil inside the string loop and pull the loop tight with one hand, while securing the pin with the other hand. Tilt the pencil slightly and move the pencil around 360o, keeping the string tight. This will draw a circle. Label the ...
PlanetaryScience
... “In 1965, a conference was held on the nature of the lunar surface. The basic conclusion of this conference was that both from the optical properties of the scattering of sunlight observed from the Earth, and from the early Ranger photographs, there was no evidence for an ...
... “In 1965, a conference was held on the nature of the lunar surface. The basic conclusion of this conference was that both from the optical properties of the scattering of sunlight observed from the Earth, and from the early Ranger photographs, there was no evidence for an ...
1 4th Nine Weeks 8th Grade SCIENCE EXAM
... collapses. The gravity from this mass is so strong that nothing can escape from it, not even light. Stars take different lengths of time to go through their life cycle. The length of a star’s life depends on its mass. The most massive stars live the shortest lives because they use up their fuel more ...
... collapses. The gravity from this mass is so strong that nothing can escape from it, not even light. Stars take different lengths of time to go through their life cycle. The length of a star’s life depends on its mass. The most massive stars live the shortest lives because they use up their fuel more ...
Module 6 Revision Guide Part One
... probably erupted from a volcano. If the crystals are larger and easily visible, the magma from which the rock was formed cooled more slowly, probably within the Earth’s crust. Metamorphic rocks are associated with present-day and ancient mountain belts. They are evidence of the high temperatures and ...
... probably erupted from a volcano. If the crystals are larger and easily visible, the magma from which the rock was formed cooled more slowly, probably within the Earth’s crust. Metamorphic rocks are associated with present-day and ancient mountain belts. They are evidence of the high temperatures and ...
History of Astronomy
... Moon revolves around Earth Earth rotates on axis causing apparent daily motion of the heavens Earth revolves around sun causing sun's annual movements Retrograde motion of planets is due to relative planetary motions Planetary orbits are perfect circles Copernicus was the first to accurately determi ...
... Moon revolves around Earth Earth rotates on axis causing apparent daily motion of the heavens Earth revolves around sun causing sun's annual movements Retrograde motion of planets is due to relative planetary motions Planetary orbits are perfect circles Copernicus was the first to accurately determi ...
Planetary Atmospheres
... • these temperature variations (determined by light interactions) define the major atmospheric layers ...
... • these temperature variations (determined by light interactions) define the major atmospheric layers ...
Chapter 8
... Three Kepler’s laws • 1. The law of orbits: All planets move in elliptical orbits, with the Sun at one focus • 2. The law of areas: A line that connects the planet to the Sun sweeps out equal areas in the plane of the planet’s orbit in equal time intervals • 3. The law of periods: The square of the ...
... Three Kepler’s laws • 1. The law of orbits: All planets move in elliptical orbits, with the Sun at one focus • 2. The law of areas: A line that connects the planet to the Sun sweeps out equal areas in the plane of the planet’s orbit in equal time intervals • 3. The law of periods: The square of the ...
Frostburg State Planetarium presents
... • Even the nearest planets appear as * (points) as we see them with our eyes; for even these objects very far away (if moon dist.=1, Venus dist.= 100) • To tell a planet from a star, all night stars twinkle and planets usually shine steady. • Also satellites (especially Space Station) shine steadily ...
... • Even the nearest planets appear as * (points) as we see them with our eyes; for even these objects very far away (if moon dist.=1, Venus dist.= 100) • To tell a planet from a star, all night stars twinkle and planets usually shine steady. • Also satellites (especially Space Station) shine steadily ...
Outer Planets Lab
... Although mainly composed of gas, the outer planets also have other ingredients. Somewhere at the center is what scientist refer to as a rocky core, although it is actually composed of liquid heavy metals. While the inner planets have few or no moons, the outer planets have dozens each. The inner and ...
... Although mainly composed of gas, the outer planets also have other ingredients. Somewhere at the center is what scientist refer to as a rocky core, although it is actually composed of liquid heavy metals. While the inner planets have few or no moons, the outer planets have dozens each. The inner and ...
How the Solar System Formed: The Nebular
... all revolve in the same direction. All debris (matter) orbits the sun (except moons). The most dense materials are closest to the Sun. All the planets and most of the moons and asteroids are about the same age. The same materials (but in different proportions) make up all the objects in the solar sy ...
... all revolve in the same direction. All debris (matter) orbits the sun (except moons). The most dense materials are closest to the Sun. All the planets and most of the moons and asteroids are about the same age. The same materials (but in different proportions) make up all the objects in the solar sy ...
The Solar System
... • This tidal force varies from weaker to stronger as Io goes from closer to farther from Jupiter in its slightly elliptical orbit. This rhythmic squeezing and stretching of the moon heats the interior – tidal friction • It’s surprisingly effective. The volcanoes have vent temperatures of 2000F, melt ...
... • This tidal force varies from weaker to stronger as Io goes from closer to farther from Jupiter in its slightly elliptical orbit. This rhythmic squeezing and stretching of the moon heats the interior – tidal friction • It’s surprisingly effective. The volcanoes have vent temperatures of 2000F, melt ...
sample text - Highereducationresources
... Jupiter has 16 moons, the largest of which are Europa, Ganymede, Io, Callisto. Each of these major moons has surface characteristics distinctly different from the others. When Jupiter is nearest the Earth, the moons can be seen clearly through field glasses as they move around the giant planet. Satu ...
... Jupiter has 16 moons, the largest of which are Europa, Ganymede, Io, Callisto. Each of these major moons has surface characteristics distinctly different from the others. When Jupiter is nearest the Earth, the moons can be seen clearly through field glasses as they move around the giant planet. Satu ...
m15a02
... The Huygen’s Probe, supplied by the European Space Agency, is planned to be released from Cassini in December 2004. It will study the clouds, atmosphere, and surface of Saturn’s satellite Titan. The probe will enter and brake in Titan’s atmosphere and parachute a fully instrumented robotic laborator ...
... The Huygen’s Probe, supplied by the European Space Agency, is planned to be released from Cassini in December 2004. It will study the clouds, atmosphere, and surface of Saturn’s satellite Titan. The probe will enter and brake in Titan’s atmosphere and parachute a fully instrumented robotic laborator ...
PPT
... – Solar nebula spun faster as it contracted because of conservation of angular momentum. – Collisions between gas particles then caused the nebula to flatten into a disk. • Why are there two major types of planets? – Only rock and metals condensed inside the frost ...
... – Solar nebula spun faster as it contracted because of conservation of angular momentum. – Collisions between gas particles then caused the nebula to flatten into a disk. • Why are there two major types of planets? – Only rock and metals condensed inside the frost ...
Module 17 Asteroids - Kapitolyo High School
... a. a meteor is about to get married b. the earth passes through the asteroid belt c. the head of a comet hits the earth’s atmosphere d. the earth passes through a swarm of dust particles in space, the remnants of a comet, once a year 3. A meteorite is a. a rock from space that strikes the ground b. ...
... a. a meteor is about to get married b. the earth passes through the asteroid belt c. the head of a comet hits the earth’s atmosphere d. the earth passes through a swarm of dust particles in space, the remnants of a comet, once a year 3. A meteorite is a. a rock from space that strikes the ground b. ...
Saturn lecture
... – A 2:1 resonance between the B ring and Mimas forms the Cassini division – A 7:6 resonance between the A ring and Janus forms the outer edge of the A ring – The F ring is “herded” by two small satellites, Prometheus and Pandora (“Shepard moons”) – The gravitational influence from Pandora and Promet ...
... – A 2:1 resonance between the B ring and Mimas forms the Cassini division – A 7:6 resonance between the A ring and Janus forms the outer edge of the A ring – The F ring is “herded” by two small satellites, Prometheus and Pandora (“Shepard moons”) – The gravitational influence from Pandora and Promet ...
Asteroids The Asteroid Belt Composition and Classification
... that develops an atmosphere as it approaches the Sun • Comets can develop tails • Comets move with respect to the background stars but are much more unpredictable than planets • Comets are the best preserved, most primitive material available in the solar system Q ...
... that develops an atmosphere as it approaches the Sun • Comets can develop tails • Comets move with respect to the background stars but are much more unpredictable than planets • Comets are the best preserved, most primitive material available in the solar system Q ...
The Solar System - Thomas County Schools
... around the sun in elliptical (oval) orbits. http://lasp.colorado.edu/education/outerplanet s/orbit_simulator/ http://www.solarsystemscope.com/ The planets in our solar system differ in size, composition (rock or gas), surface and atmospheric conditions, and distance from the sun. ...
... around the sun in elliptical (oval) orbits. http://lasp.colorado.edu/education/outerplanet s/orbit_simulator/ http://www.solarsystemscope.com/ The planets in our solar system differ in size, composition (rock or gas), surface and atmospheric conditions, and distance from the sun. ...
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.