Lecture #33: Solar System Origin I The Main Point What is a
... All of the planets orbit the Sun in roughly the same plane (the ecliptic), which is very close to the Sun's equatorial plane. The orbits of the major planets are nearly circular. Planets, asteroids, and most comets circle the Sun counter-clockwise as viewed from “above” (exceptions: some comets). Th ...
... All of the planets orbit the Sun in roughly the same plane (the ecliptic), which is very close to the Sun's equatorial plane. The orbits of the major planets are nearly circular. Planets, asteroids, and most comets circle the Sun counter-clockwise as viewed from “above” (exceptions: some comets). Th ...
a 03 Scale and Comparing Planets to Stars ppt
... • This Means that the light we see from Andromeda Galaxy left there 2.2 million years ago. • It is therefore very possible that some of the stars in Andromeda have exploded as a supernova or gone out long ago. The message of these star finishing events just has not gotten to us yet! ...
... • This Means that the light we see from Andromeda Galaxy left there 2.2 million years ago. • It is therefore very possible that some of the stars in Andromeda have exploded as a supernova or gone out long ago. The message of these star finishing events just has not gotten to us yet! ...
gravity and keplers laws
... supporter Galileo was interviewed by the Inquisition and put under house arrest for the rest of his life and forbidden to publish. He got off lightly. But despite the best efforts of the church, astronomers could observe the motions of the planets, and soon it became known that the planets did indee ...
... supporter Galileo was interviewed by the Inquisition and put under house arrest for the rest of his life and forbidden to publish. He got off lightly. But despite the best efforts of the church, astronomers could observe the motions of the planets, and soon it became known that the planets did indee ...
File
... Planets (Inner Planets), are located close to the Sun, and are closely spaced. Jupiter, Saturn, Uranus, and Neptune, the Jovian Planets (Outer Planets), are located far from the Sun, and are spaced far ...
... Planets (Inner Planets), are located close to the Sun, and are closely spaced. Jupiter, Saturn, Uranus, and Neptune, the Jovian Planets (Outer Planets), are located far from the Sun, and are spaced far ...
9/29/16 pacing planet distance
... Objectives: Through completing this lesson the child will: 1) Gain an appreciation of the vastness of distances between the planets; 2) Compare these distances to the greatest distances that humans have ever traveled. ...
... Objectives: Through completing this lesson the child will: 1) Gain an appreciation of the vastness of distances between the planets; 2) Compare these distances to the greatest distances that humans have ever traveled. ...
Chapter 17 Tour: Formation of the Solar System
... 4. Why does the composition of giant gas planets differ from that of the rocky inner planets? THE OUTER GAS GIANTS ARE MADE OF GAS BECAUSE THEY WERE LOCATED FAR AWAY FROM THE SUN AND COULD COLLECT LOTS OF GAS & DUST. THE INNER PLANETS THAT ARE CLOSER TO THE SUN ARE MADE OF JUST ROCK BECAUSE THE GAS ...
... 4. Why does the composition of giant gas planets differ from that of the rocky inner planets? THE OUTER GAS GIANTS ARE MADE OF GAS BECAUSE THEY WERE LOCATED FAR AWAY FROM THE SUN AND COULD COLLECT LOTS OF GAS & DUST. THE INNER PLANETS THAT ARE CLOSER TO THE SUN ARE MADE OF JUST ROCK BECAUSE THE GAS ...
The Solar System
... They believe that this dust and gas began to collapse under the weight of its own gravity. As it did so, the matter contained within this could begin moving in a giant circle. At the center of this spinning cloud, a small star began to form. This star grew larger and larger as it collected more and ...
... They believe that this dust and gas began to collapse under the weight of its own gravity. As it did so, the matter contained within this could begin moving in a giant circle. At the center of this spinning cloud, a small star began to form. This star grew larger and larger as it collected more and ...
Planets - AState.edu
... system mainly made of? Planets, the asteroid belt, stars, sun, good class. Can someone name the planets in our solar system?” Give students a chance to answer. “Our terrestrial planets are: Mercury, Venus, Earth, and Mars. Our outer planets are: Jupiter, Saturn, Uranus, and Neptune. Today we are goi ...
... system mainly made of? Planets, the asteroid belt, stars, sun, good class. Can someone name the planets in our solar system?” Give students a chance to answer. “Our terrestrial planets are: Mercury, Venus, Earth, and Mars. Our outer planets are: Jupiter, Saturn, Uranus, and Neptune. Today we are goi ...
Name
... 20 kg satellite has a circular orbit with a period of 2.4 hr and a radius of 8.0 × 106 m around a planet of unknown mass. If the magnitude of the gravitational acceleration on the surface of the planet is 8.0 m!s 2, what is the radius of the planet? ...
... 20 kg satellite has a circular orbit with a period of 2.4 hr and a radius of 8.0 × 106 m around a planet of unknown mass. If the magnitude of the gravitational acceleration on the surface of the planet is 8.0 m!s 2, what is the radius of the planet? ...
Integrative Studies 410 Our Place in the Universe
... Where Stars come from: the Interstellar Medium • Gas – Single atoms and molecules – Mostly hydrogen (90%), 9% helium; deficient in heavier elements ...
... Where Stars come from: the Interstellar Medium • Gas – Single atoms and molecules – Mostly hydrogen (90%), 9% helium; deficient in heavier elements ...
jupiter interpretive sign - Town of Cumberland, Indiana
... JUPITER The image above illustrates the size of each planet in relation to each other. It does not give the relative distance between each planet in the solar system. Refer to map below for the distances between each planet. ...
... JUPITER The image above illustrates the size of each planet in relation to each other. It does not give the relative distance between each planet in the solar system. Refer to map below for the distances between each planet. ...
Our solar System
... • Atmospheric composition: 89.8% Hydrogen, 10.2% helium • Rotation: 99.6 hours (fast due to massive gravity) • Revolution: 11.86 earth years ...
... • Atmospheric composition: 89.8% Hydrogen, 10.2% helium • Rotation: 99.6 hours (fast due to massive gravity) • Revolution: 11.86 earth years ...
Word doc - UC
... neighborhood of the Milky Way galaxy, then “Earth-size planets are common around nearby Sun-like stars,” conclude Erik A. Petigura and Geoffrey W. Marcy from the University of California, Berkeley and Andrew W. Howard from the University of Hawaii. They were led to that conclusion by a monumental st ...
... neighborhood of the Milky Way galaxy, then “Earth-size planets are common around nearby Sun-like stars,” conclude Erik A. Petigura and Geoffrey W. Marcy from the University of California, Berkeley and Andrew W. Howard from the University of Hawaii. They were led to that conclusion by a monumental st ...
Extra-Solar Planets
... A planet needs the right star! Constraints on star systems: 1) Old enough to allow time for evolution (rules out high-mass stars - 1%) 2) Need to have stable orbits (might rule out binary/multiple star systems - 50%) 3) Size of “habitable zone”: region in which a planet of the right size could have ...
... A planet needs the right star! Constraints on star systems: 1) Old enough to allow time for evolution (rules out high-mass stars - 1%) 2) Need to have stable orbits (might rule out binary/multiple star systems - 50%) 3) Size of “habitable zone”: region in which a planet of the right size could have ...
Astronomy
... 8. Which two factors cause the Moon to have wide swings in temperature, so it gets both much hotter and much colder than the Earth? A) Lack of atmosphere, and its eccentric orbit B) Lack of atmosphere, and slow rotation C) Lack of atmosphere, and no magnetic field D) Eccentric orbit, and slow rotati ...
... 8. Which two factors cause the Moon to have wide swings in temperature, so it gets both much hotter and much colder than the Earth? A) Lack of atmosphere, and its eccentric orbit B) Lack of atmosphere, and slow rotation C) Lack of atmosphere, and no magnetic field D) Eccentric orbit, and slow rotati ...
Dynamics of the Earth
... Aberration of starlight Telescope moving at speed v must be tilted so that light reaches bottom. Lsinθ Lcosθ v ∆t = ...
... Aberration of starlight Telescope moving at speed v must be tilted so that light reaches bottom. Lsinθ Lcosθ v ∆t = ...
Planetary Diversity - MIT Computer Science and Artificial
... ; (seefigure 2). Gas refers primarily to hydrogen and helium, the most abundant elements in the universe. stars by a gravitational instability ofthe gas disk, provided These elements also happen to comprise molecules that do it is sufficiently cold and dense. No one knows whether not condense as sol ...
... ; (seefigure 2). Gas refers primarily to hydrogen and helium, the most abundant elements in the universe. stars by a gravitational instability ofthe gas disk, provided These elements also happen to comprise molecules that do it is sufficiently cold and dense. No one knows whether not condense as sol ...
Chapter 29 Our Solar System
... 5. Interior: Solid core of __________, ___________, & ____________ Asteroid belt 1. Left over planetary debris from solar system formation, that never formed planets 2. Located between Mars & Jupiter 3. Separates terrestrial planets and gas giants ...
... 5. Interior: Solid core of __________, ___________, & ____________ Asteroid belt 1. Left over planetary debris from solar system formation, that never formed planets 2. Located between Mars & Jupiter 3. Separates terrestrial planets and gas giants ...
Chapter 8 Formation of the Solar System Agenda What properties of
... The nebular theory states that our solar system formed from the gravitational collapse of a giant interstellar gas cloud—the solar nebula ...
... The nebular theory states that our solar system formed from the gravitational collapse of a giant interstellar gas cloud—the solar nebula ...
Chapter-6 Lecture Spring Semester
... Nebular contraction is followed by condensation around dust grains (condensation nuclei), known to exist in interstellar clouds such as the one shown here. Accretion then leads to larger and larger clumps (planetesimals); finally gravitational attraction takes over and first protoplanets and then pl ...
... Nebular contraction is followed by condensation around dust grains (condensation nuclei), known to exist in interstellar clouds such as the one shown here. Accretion then leads to larger and larger clumps (planetesimals); finally gravitational attraction takes over and first protoplanets and then pl ...
Planets Chart: Planet Distance From Sun Size Rotation Orbit
... least dense, life on one moon? Rocky rings around equato r, on an ...
... least dense, life on one moon? Rocky rings around equato r, on an ...
Pocket Solar System - University of Virginia
... There are two reasons why no planet formed at the distance of the asteroid belt. First, even though there are many asteroids, most are very small. All of the asteroids added together have only 0.4% the mass of the Earth (or 4% the mass of the Moon)! Second, both Jupiter and Mars ...
... There are two reasons why no planet formed at the distance of the asteroid belt. First, even though there are many asteroids, most are very small. All of the asteroids added together have only 0.4% the mass of the Earth (or 4% the mass of the Moon)! Second, both Jupiter and Mars ...
Lecture1
... • Angular diameter of the Sun is 0.53 degrees • Knowing Earth’s diameter (13,000 km) you can find the extent of Earth’s shadow: 1.4 million km. • From observing the radius of curvature of the shadow we see the angular size of Earth’s shadow at the distance of the Moon is ...
... • Angular diameter of the Sun is 0.53 degrees • Knowing Earth’s diameter (13,000 km) you can find the extent of Earth’s shadow: 1.4 million km. • From observing the radius of curvature of the shadow we see the angular size of Earth’s shadow at the distance of the Moon is ...
History of Solar System formation and evolution hypotheses
Ideas concerning the origin and fate of the world date from the earliest known writings; however, for almost all of that time, there was no attempt to link such theories to the existence of a ""Solar System"", simply because almost no one knew or believed that the Solar System, in the sense we now understand it, existed. The first step towards a theory of Solar System formation was the general acceptance of heliocentrism, the model which placed the Sun at the centre of the system and the Earth in orbit around it. This conception had been gestating for thousands of years, but was only widely accepted by the end of the 17th century. The first recorded use of the term ""Solar System"" dates from 1704.