STANDARD SET 4. Earth Sciences
... Planets move in elliptical but nearly circular orbits around the Sun just as the Moon moves in a nearly circular orbit around Earth. Each object in the solar system would move in a straight line if it were not pulled or pushed by a force. Gravity causes a pull, or attraction, between the mass (matte ...
... Planets move in elliptical but nearly circular orbits around the Sun just as the Moon moves in a nearly circular orbit around Earth. Each object in the solar system would move in a straight line if it were not pulled or pushed by a force. Gravity causes a pull, or attraction, between the mass (matte ...
Pocket Solar System Activity
... huge size differences involved. This is a simple little model to give you an overview of the distances between the orbits of the planets and other objects in our solar system. (It is also a good tool for reviewing fractions.) Materials needed: At least 1 meter of paper tape per person, such as add ...
... huge size differences involved. This is a simple little model to give you an overview of the distances between the orbits of the planets and other objects in our solar system. (It is also a good tool for reviewing fractions.) Materials needed: At least 1 meter of paper tape per person, such as add ...
The Nine Planets
... Not! Summer 2006, the International Astronomical Union (IAU) decided that Pluto is a dwarf planet. They made this decision for two reasons: 1. Size: Pluto is TINY & made out of rock & ice - definitely not like the other outer planets 2. Orbit: Pluto has a very weird orbit - its highly elliptical orb ...
... Not! Summer 2006, the International Astronomical Union (IAU) decided that Pluto is a dwarf planet. They made this decision for two reasons: 1. Size: Pluto is TINY & made out of rock & ice - definitely not like the other outer planets 2. Orbit: Pluto has a very weird orbit - its highly elliptical orb ...
File1 - School of Astronomy, IPM
... (1) What is the initial condition for the pre-inflationary area to have a suitable condition for a Habitable Universe (formation of planets and … life) (2) There is a Asymmetry between the matter and antimatter ( i.e. Baryons and Anti-Baryons, leptons and Anti-leptons). How big this asymmetry should ...
... (1) What is the initial condition for the pre-inflationary area to have a suitable condition for a Habitable Universe (formation of planets and … life) (2) There is a Asymmetry between the matter and antimatter ( i.e. Baryons and Anti-Baryons, leptons and Anti-leptons). How big this asymmetry should ...
Characteristics of the Sun
... However, compared with other stars, the Sun is rather ordinary. It is about in the middle of the ranges for star size and brightness. Many of the stars that you can see in the night sky are actually bigger and brighter than the Sun—they only appear smaller because they are much farther away. Howeve ...
... However, compared with other stars, the Sun is rather ordinary. It is about in the middle of the ranges for star size and brightness. Many of the stars that you can see in the night sky are actually bigger and brighter than the Sun—they only appear smaller because they are much farther away. Howeve ...
Working with the Illinois Learning Standards: A Constructivist
... • view (using appropriate safety precautions) a solar eclipse • “view” the different “faces” on the moon • note the changing position of the moon among the stars and in the sky at the same time each night. • measure the diameter of the sun from results of pinhole projection. discuss the greenhouse e ...
... • view (using appropriate safety precautions) a solar eclipse • “view” the different “faces” on the moon • note the changing position of the moon among the stars and in the sky at the same time each night. • measure the diameter of the sun from results of pinhole projection. discuss the greenhouse e ...
Our Solar System
... are also made of rock and have few or no moons. The outer planets—Jupiter, Saturn, Uranus, and Neptune—are huge, mostly gaseous, and have rings. The outer planets also have many moons. In general, the farther a planet is from the sun, the colder it is. Between Mars and Jupiter is the asteroid belt, ...
... are also made of rock and have few or no moons. The outer planets—Jupiter, Saturn, Uranus, and Neptune—are huge, mostly gaseous, and have rings. The outer planets also have many moons. In general, the farther a planet is from the sun, the colder it is. Between Mars and Jupiter is the asteroid belt, ...
Ice Giant Neptune Frontlines Potentially Hazardous Asteroid
... Discovered in February 2002 by the Lincoln NearEarth Asteroid Research (LINEAR), Asteroid CU11 orbits the Sun in 492 days, and will pass within 13.5 lunar distances (about 3.2 million miles distance) this time around. In August of 2080, Asteroid 2002 CU11 will flyby Earth at less than two lunar ...
... Discovered in February 2002 by the Lincoln NearEarth Asteroid Research (LINEAR), Asteroid CU11 orbits the Sun in 492 days, and will pass within 13.5 lunar distances (about 3.2 million miles distance) this time around. In August of 2080, Asteroid 2002 CU11 will flyby Earth at less than two lunar ...
Name - MIT
... are slowly rotating neutron stars. are white dwarfs that have finally ceased all nuclear reactions. are white dwarfs that have cooled and no longer produce visible light. are the end products of stars like the sun. are a name given to matter so compressed that even light can't escape. ...
... are slowly rotating neutron stars. are white dwarfs that have finally ceased all nuclear reactions. are white dwarfs that have cooled and no longer produce visible light. are the end products of stars like the sun. are a name given to matter so compressed that even light can't escape. ...
Obliquity and precession of the equinoxes The angle ε between the
... The month and the Moon’s motions The Moon orbits the Earth. It is new when it is in conjunction, that is, when it has the same ecliptic longitude as the Sun. In this geometry, the light of the Sun falls on the side of the Moon facing away from the observer. This also means that the Moon must be near ...
... The month and the Moon’s motions The Moon orbits the Earth. It is new when it is in conjunction, that is, when it has the same ecliptic longitude as the Sun. In this geometry, the light of the Sun falls on the side of the Moon facing away from the observer. This also means that the Moon must be near ...
Earth`s Moon
... The inner planets (between the Sun and the asteroid belt) include Mercury, Venus, Earth, and Mars. The outer planets (beyond the asteroid belt) include Jupiter, Saturn, Uranus, Neptune, and Pluto. An astronomical unit or AU is the distance that the Earth is from the Sun and is equal to about 9 ...
... The inner planets (between the Sun and the asteroid belt) include Mercury, Venus, Earth, and Mars. The outer planets (beyond the asteroid belt) include Jupiter, Saturn, Uranus, Neptune, and Pluto. An astronomical unit or AU is the distance that the Earth is from the Sun and is equal to about 9 ...
Document
... the possibility that its surface could sustain liquid water, or even life. It is 50 percent bigger and 5 times more massive than Earth. ...
... the possibility that its surface could sustain liquid water, or even life. It is 50 percent bigger and 5 times more massive than Earth. ...
Document
... ❶ In front of the class, explain the steps for assembling the solar system flip book: • Glue the photocopies of the planetary orbit sheets (Appendix 1) onto thick paper. • On each of the illustrations numbered 1 to 24, colour the Sun and four planets (Sun = yellow; Mercury = green; Venus = brown; Ea ...
... ❶ In front of the class, explain the steps for assembling the solar system flip book: • Glue the photocopies of the planetary orbit sheets (Appendix 1) onto thick paper. • On each of the illustrations numbered 1 to 24, colour the Sun and four planets (Sun = yellow; Mercury = green; Venus = brown; Ea ...
Your Birthday on Another Planet
... ❶ In front of the class, explain the steps for assembling the solar system flip book: • Glue the photocopies of the planetary orbit sheets (Appendix 1) onto thick paper. • On each of the illustrations numbered 1 to 24, colour the Sun and four planets (Sun = yellow; Mercury = green; Venus = brown; Ea ...
... ❶ In front of the class, explain the steps for assembling the solar system flip book: • Glue the photocopies of the planetary orbit sheets (Appendix 1) onto thick paper. • On each of the illustrations numbered 1 to 24, colour the Sun and four planets (Sun = yellow; Mercury = green; Venus = brown; Ea ...
Earth, moon, and sun
... Earth’s shadow, or when Earth is directly between the moon and sun. During a lunar eclipse, Earth blocks sunlight from reaching the ...
... Earth’s shadow, or when Earth is directly between the moon and sun. During a lunar eclipse, Earth blocks sunlight from reaching the ...
+ RA(*)
... Azimuth. A measurement of angle increasing from north through east. Altitude (astronomical). A measurement of angular distance from the true horizon upwards. Ecliptic. The great circle in the sky along which the Sun appears to move because of Earth’s orbit about it. Right Ascension. A celestial co-o ...
... Azimuth. A measurement of angle increasing from north through east. Altitude (astronomical). A measurement of angular distance from the true horizon upwards. Ecliptic. The great circle in the sky along which the Sun appears to move because of Earth’s orbit about it. Right Ascension. A celestial co-o ...
EARTH IN THE UNIVERSE TOPIC 3 2011-2012
... miles from Earth’s orbit, only a little more than the distance to the Moon…. Hermes approaches Earth’s orbit twice every 777 days. Usually our planet is far away when the orbit crossing happens, but in 1937, 1942, 1954, 1974 and 1986, Hermes came harrowingly [dangerously] close to Earth itself. We k ...
... miles from Earth’s orbit, only a little more than the distance to the Moon…. Hermes approaches Earth’s orbit twice every 777 days. Usually our planet is far away when the orbit crossing happens, but in 1937, 1942, 1954, 1974 and 1986, Hermes came harrowingly [dangerously] close to Earth itself. We k ...
Benchmark lesson
... sky. They used the predictable movements to track time. Over the years, people began to make tools to help them study the planets and stars. As technology got better, the tools people used to study astronomy got better too. One of the most important tools invented to study the sky was the telescope. ...
... sky. They used the predictable movements to track time. Over the years, people began to make tools to help them study the planets and stars. As technology got better, the tools people used to study astronomy got better too. One of the most important tools invented to study the sky was the telescope. ...
Astronomy Today
... planetary motions epicycle (used to explain planetary motions) = Ptomely’s theory © 2014 Pearson Education, Inc. ...
... planetary motions epicycle (used to explain planetary motions) = Ptomely’s theory © 2014 Pearson Education, Inc. ...
Professor Jonathan Fortney TA Kate Dallas Thursday, February 11
... 46) From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation? A) infrared, visible light, ultraviolet, X rays, gamma rays, radio B) radio, X rays, visible light, ultraviolet, infrared, gamma rays C) radio, infrared, visible l ...
... 46) From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation? A) infrared, visible light, ultraviolet, X rays, gamma rays, radio B) radio, X rays, visible light, ultraviolet, infrared, gamma rays C) radio, infrared, visible l ...
Venus Investigation
... right after further research. Venus was proved to be a barren and uninhabitable wasteland containing several times as many volcanoes as Earth that shaped the Venusian surface. As Earth’s “sister planet”, Venus has a similar size, and gravity. This has been important in making the planet of such inte ...
... right after further research. Venus was proved to be a barren and uninhabitable wasteland containing several times as many volcanoes as Earth that shaped the Venusian surface. As Earth’s “sister planet”, Venus has a similar size, and gravity. This has been important in making the planet of such inte ...
How is energy stored in atoms? Energy Level Transitions A Simple
... the Solar System LectureTutorial: Pg. 111-112 • Work with a partner or two • Read directions and answer all questions carefully. Take time to understand it now! • Come to a consensus answer you all agree on before moving on to the next question. ...
... the Solar System LectureTutorial: Pg. 111-112 • Work with a partner or two • Read directions and answer all questions carefully. Take time to understand it now! • Come to a consensus answer you all agree on before moving on to the next question. ...
Gravity Kepler`s Laws - historical remarks - UW
... • Kepler’s First Law: – All planets move in elliptical orbits with the sun at one focus ...
... • Kepler’s First Law: – All planets move in elliptical orbits with the sun at one focus ...
Slide 1
... the face of the Sun. They are typically about 2,000 degrees Kelvin cooler than the average temperature on the photosphere. This makes them appear to be dark in comparison to their very bright surroundings. Following long-lived sunspots through time allows one to determine the rotation rate of the Su ...
... the face of the Sun. They are typically about 2,000 degrees Kelvin cooler than the average temperature on the photosphere. This makes them appear to be dark in comparison to their very bright surroundings. Following long-lived sunspots through time allows one to determine the rotation rate of the Su ...
Geocentric model
In astronomy, the geocentric model (also known as geocentrism, or the Ptolemaic system) is a description of the cosmos where Earth is at the orbital center of all celestial bodies. This model served as the predominant cosmological system in many ancient civilizations such as ancient Greece including the noteworthy systems of Aristotle (see Aristotelian physics) and Ptolemy. As such, they believed that the Sun, Moon, stars, and naked eye planets circled Earth.Two commonly made observations supported the idea that Earth was the center of the Universe. The stars, the sun, and planets appear to revolve around Earth each day, making Earth the center of that system. The stars were thought to be on a celestial sphere, with the earth at its center, that rotated each day, using a line through the north and south pole as an axis. The stars closest to the equator appeared to rise and fall the greatest distance, but each star circled back to its rising point each day. The second observation supporting the geocentric model was that the Earth does not seem to move from the perspective of an Earth-bound observer, and that it is solid, stable, and unmoving.Ancient Roman and medieval philosophers usually combined the geocentric model with a spherical Earth. It is not the same as the older flat Earth model implied in some mythology, as was the case with the biblical and postbiblical Latin cosmology. The ancient Jewish Babylonian uranography pictured a flat Earth with a dome-shaped rigid canopy named firmament placed over it. (רקיע- rāqîa').However, the ancient Greeks believed that the motions of the planets were circular and not elliptical, a view that was not challenged in Western culture until the 17th century through the synthesis of theories by Copernicus and Kepler.The astronomical predictions of Ptolemy's geocentric model were used to prepare astrological and astronomical charts for over 1500 years. The geocentric model held sway into the early modern age, but from the late 16th century onward was gradually superseded by the heliocentric model of Copernicus, Galileo and Kepler. There was much resistance to the transition between these two theories. Christian theologians were reluctant to reject a theory that agreed with Bible passages (e.g. ""Sun, stand you still upon Gibeon"", Joshua 10:12 – King James 2000 Bible). Others felt a new, unknown theory could not subvert an accepted consensus for geocentrism.