Astronomy Study Guide Key Vocabulary: Planet Jovian Moon
... Know why the moon rises and sets later each day over the course of a ~28 day period. Know why the moon appears to go through phases (different parts of the moon lit by the Sun) over the course of a ~28 day period. One half of the moon is always facing the Sun One half of the moon is always lit Kno ...
... Know why the moon rises and sets later each day over the course of a ~28 day period. Know why the moon appears to go through phases (different parts of the moon lit by the Sun) over the course of a ~28 day period. One half of the moon is always facing the Sun One half of the moon is always lit Kno ...
Section 5 — Earth Sciences (The Solar System) Student Edition
... More observations through time, and further questions that were investigated (and continue to be investigated) showed that Earth is not the center of the universe after all. In the 1500’s a Polish scientist named, Copernicus, used mathematics and his observations of the sky (without a telescope, whi ...
... More observations through time, and further questions that were investigated (and continue to be investigated) showed that Earth is not the center of the universe after all. In the 1500’s a Polish scientist named, Copernicus, used mathematics and his observations of the sky (without a telescope, whi ...
Historical View
... • Galileo Galilei discovered the existence of satellites around the Jupiter (miniature Solar System). • Around that term, there was a symbolic astronomical event. A bright comet appeared in 1577. Tycho Brahe (1546-1601) could successfully obtain a parallax. He found that the comet existed at least ...
... • Galileo Galilei discovered the existence of satellites around the Jupiter (miniature Solar System). • Around that term, there was a symbolic astronomical event. A bright comet appeared in 1577. Tycho Brahe (1546-1601) could successfully obtain a parallax. He found that the comet existed at least ...
solar system notes
... the MATLAB command line, which will perform Fourier transforms of each sun-planet distance versus time and plot them out. Exercise: Using the zoom function to find the time period that corresponds to the peak in power and write them down for each of the planets. How do these values compare to the or ...
... the MATLAB command line, which will perform Fourier transforms of each sun-planet distance versus time and plot them out. Exercise: Using the zoom function to find the time period that corresponds to the peak in power and write them down for each of the planets. How do these values compare to the or ...
Earth, Moon, and Beyond
... Saturn Best known for its rings, made of ice, dust, boulders, and frozen gas. Its rings stretch about 84,650 miles from the center of the planet. Has dozens of moons. ...
... Saturn Best known for its rings, made of ice, dust, boulders, and frozen gas. Its rings stretch about 84,650 miles from the center of the planet. Has dozens of moons. ...
![ASTRONOMY 101 SAMPLE FIRST EXAM [1] Kepler`s Law relating](http://s1.studyres.com/store/data/017742958_1-c5c5f19bce1080c6ad7c1fc92906a06f-300x300.png)
ASTRONOMY 101 SAMPLE FIRST EXAM [1] Kepler`s Law relating
... Kepler’s third law states that a planet in an elliptical orbit moves with a velocity such that (a) the planet moves slower as it approaches nearer the sun. (b) the line between the Sun and the planet sweeps out equal areas in equal times. (c) it won’t need to stop for the comets going by. __________ ...
... Kepler’s third law states that a planet in an elliptical orbit moves with a velocity such that (a) the planet moves slower as it approaches nearer the sun. (b) the line between the Sun and the planet sweeps out equal areas in equal times. (c) it won’t need to stop for the comets going by. __________ ...
Jun - Wadhurst Astronomical Society
... the results we find a sequence of distances that fairly accurately coincide with the distance of the orbits of the planets. Planet ...
... the results we find a sequence of distances that fairly accurately coincide with the distance of the orbits of the planets. Planet ...
SCI 103
... The planet takes one year to circle the star because it is 1 AU from it. The planet takes longer than one year to circle the star because it is so massive. The planet takes less than one year to circle the star because it is so massive. The planet takes longer than one year to circle the star becaus ...
... The planet takes one year to circle the star because it is 1 AU from it. The planet takes longer than one year to circle the star because it is so massive. The planet takes less than one year to circle the star because it is so massive. The planet takes longer than one year to circle the star becaus ...
6.2 Measuring the Planets
... This work is protected by U.S. copyright laws and is provided solely for the use of instructors in teaching their courses and assessing student learning. Dissemination or sale of any part of this work (including on the World Wide Web) will destroy the integrity of the work and is not permitted. The ...
... This work is protected by U.S. copyright laws and is provided solely for the use of instructors in teaching their courses and assessing student learning. Dissemination or sale of any part of this work (including on the World Wide Web) will destroy the integrity of the work and is not permitted. The ...
Mission to Planet X - The Education Fund
... planets. Since the mobile we make in this unit has planets that are to scale but not distances to scale, this video is perfect for teaching that aspect. Students will be amazed at the vast distance between the outlying planets Kids Astronomy: The Solar System This interactive site gives users a chan ...
... planets. Since the mobile we make in this unit has planets that are to scale but not distances to scale, this video is perfect for teaching that aspect. Students will be amazed at the vast distance between the outlying planets Kids Astronomy: The Solar System This interactive site gives users a chan ...
Celestial Mechanics
... Celestial Mechanics The Heliocentric Model of Copernicus Sun at the center and planets (including Earth) orbiting along circles. inferior planets - planets closer to Sun than Earth - Mercury, Venus superior planets - planets farther from Sun than Earth - all other planets elongation - the angle seen ...
... Celestial Mechanics The Heliocentric Model of Copernicus Sun at the center and planets (including Earth) orbiting along circles. inferior planets - planets closer to Sun than Earth - Mercury, Venus superior planets - planets farther from Sun than Earth - all other planets elongation - the angle seen ...
The Origin of the Solar System
... Asteroids are small, generally rocky bodies that orbit Sun Most asteroids (thousands) lie in the asteroid belt, a region between the orbits of Mars and Jupiter The combined mass of all the asteroids is probably less than 1/1000 the mass of the Earth ...
... Asteroids are small, generally rocky bodies that orbit Sun Most asteroids (thousands) lie in the asteroid belt, a region between the orbits of Mars and Jupiter The combined mass of all the asteroids is probably less than 1/1000 the mass of the Earth ...
DO NOT WRITE ON THIS PAPER Standard 1 Objective 1 Study
... 19.According to the nebular theory the solar system formed as a cloud of spinning dust and gas condensed into the sun and planets. 20.Meteorites that fall to Earth support the nebular theory because the meteorites are the same age and composition as Earth. 21.A rotating cloud of gas and dust from wh ...
... 19.According to the nebular theory the solar system formed as a cloud of spinning dust and gas condensed into the sun and planets. 20.Meteorites that fall to Earth support the nebular theory because the meteorites are the same age and composition as Earth. 21.A rotating cloud of gas and dust from wh ...
Getting to Know: Rotation, Orbits, and the Seasons
... is spread over a larger area, resulting in cooler temperatures. This is why there is little seasonal variation at locations near the equator. The Sun shines more directly onto equatorial regions throughout the year. Keep exploring this concept to learn more about the seasons and how Earth’s rotation ...
... is spread over a larger area, resulting in cooler temperatures. This is why there is little seasonal variation at locations near the equator. The Sun shines more directly onto equatorial regions throughout the year. Keep exploring this concept to learn more about the seasons and how Earth’s rotation ...
Lecture 4 - Twin Cities - University of Minnesota
... • Jovian planets got big enough that their gravity was great enough to capture hydrogen and helium gas ...
... • Jovian planets got big enough that their gravity was great enough to capture hydrogen and helium gas ...
Terrestrial Planets
... dust & rocks), outflow has stopped, the star is visible. Theory: Gas disperses, “planetesimals” form (up to 100 km diameter rocks), collide & stick together due to gravity forming protoplanets). Protoplanets interact with dust disks: tidal torques cause planets to migrate inward toward their host st ...
... dust & rocks), outflow has stopped, the star is visible. Theory: Gas disperses, “planetesimals” form (up to 100 km diameter rocks), collide & stick together due to gravity forming protoplanets). Protoplanets interact with dust disks: tidal torques cause planets to migrate inward toward their host st ...
Neptune - ClassZone
... can form high enough in the atmosphere of Neptune to look white. Storm systems can appear in darker shades of blue than the rest of the planet. One storm, seen during the flyby of the Voyager 2 spacecraft in 1989, was named the Great Dark Spot. Unlike the huge storm on Jupiter, the Great Dark Spot d ...
... can form high enough in the atmosphere of Neptune to look white. Storm systems can appear in darker shades of blue than the rest of the planet. One storm, seen during the flyby of the Voyager 2 spacecraft in 1989, was named the Great Dark Spot. Unlike the huge storm on Jupiter, the Great Dark Spot d ...
Jupiter, the fifth planet from the sun and the largest planet in our
... area as the Crab Nebula (right). Almost all elements heavier than hydrogen and helium are created in the fusion of stars or during their death as supernovae. Most of the material in your body was made inside a star! ...
... area as the Crab Nebula (right). Almost all elements heavier than hydrogen and helium are created in the fusion of stars or during their death as supernovae. Most of the material in your body was made inside a star! ...
Planets - burnsburdick11
... and beauty. Venus is the second brightest natural object in space, apart from the moon. Venus' diameter is about 7,520 miles! Its has a iron core, and a molten rocky mantle, like earth's interior. Venus is very dry, it is like a huge desert. This planet is the 6th largest in the solar system. Venus ...
... and beauty. Venus is the second brightest natural object in space, apart from the moon. Venus' diameter is about 7,520 miles! Its has a iron core, and a molten rocky mantle, like earth's interior. Venus is very dry, it is like a huge desert. This planet is the 6th largest in the solar system. Venus ...
Chapter 1 Questions
... asteroid came within 1/3 the distance of the Moon and was detected three days after it had passed the Earth. v. While none are expected to collide in the next century, calculations indicate that most Earth-crossing asteroids will eventually collide with Earth at the rate of about three each million ...
... asteroid came within 1/3 the distance of the Moon and was detected three days after it had passed the Earth. v. While none are expected to collide in the next century, calculations indicate that most Earth-crossing asteroids will eventually collide with Earth at the rate of about three each million ...
Montage of Jupiter and the Galilean satellites
... luminosity, in units of the SunΥsluminosity. The solid white lin es show where stars of different luminosity classes fall on the diagram; supergiants at the very top; giants just below them; and finally mainsequence stars. The relative sizes of the stars are shown correctly within each luminosity cl ...
... luminosity, in units of the SunΥsluminosity. The solid white lin es show where stars of different luminosity classes fall on the diagram; supergiants at the very top; giants just below them; and finally mainsequence stars. The relative sizes of the stars are shown correctly within each luminosity cl ...
Lecture #33: Solar System Origin I The Main Point What is a
... ordinary chondrite meteorites ALL have ages of approximately 4.6 billion years. • Tiny fractions of some very primitive meteorites and cosmic dust particles have ages even slightly older than this. • The oldest rocks from the lunar highlands are about 4.4 billion years old. Astro 102/104 ...
... ordinary chondrite meteorites ALL have ages of approximately 4.6 billion years. • Tiny fractions of some very primitive meteorites and cosmic dust particles have ages even slightly older than this. • The oldest rocks from the lunar highlands are about 4.4 billion years old. Astro 102/104 ...
Tides on Earth
... Callisto - that were discovered by by Galileo in 1610. In addition to the four large moons discovered by Galileo, scientists have observed dozens of smaller moons around Jupiter. ...
... Callisto - that were discovered by by Galileo in 1610. In addition to the four large moons discovered by Galileo, scientists have observed dozens of smaller moons around Jupiter. ...
Formation and evolution of the Solar System
The formation of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.This widely accepted model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as the Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution.In roughly 5 billion years, the Sun will cool and expand outward many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.