Big Bang Theory Scientific origin of the Universe
... How are distances in the universe measured? • Light-year – the distance that light travels in one year going at the speed of light • Speed of light – 300,000 km/second • Speed of light – 186, 000 miles/second • 9.5 trillion km in one year • Closest star (other that sun) is Proxima Centauri is 4.3 l ...
... How are distances in the universe measured? • Light-year – the distance that light travels in one year going at the speed of light • Speed of light – 300,000 km/second • Speed of light – 186, 000 miles/second • 9.5 trillion km in one year • Closest star (other that sun) is Proxima Centauri is 4.3 l ...
DO PHYSICS ONLINE SPACE MOTION OF SATELLITES
... maximum acceleration of 8g. The container and contents have a mass of 50 kg. (c) Calculate the kinetic energy of the container as it traveling with the satellite. (d) The gravitational potential energy of the container relative to the surface of the Earth is the difference between the gravitational ...
... maximum acceleration of 8g. The container and contents have a mass of 50 kg. (c) Calculate the kinetic energy of the container as it traveling with the satellite. (d) The gravitational potential energy of the container relative to the surface of the Earth is the difference between the gravitational ...
Earth
... Our Sun is not unique in the universe. It is a common middle-sized yellow star which scientists have named Sol, after the ancient Roman name. This is why our system of planets is called the Solar System. There are trillions of other stars in the universe just like it. Many of these stars have their ...
... Our Sun is not unique in the universe. It is a common middle-sized yellow star which scientists have named Sol, after the ancient Roman name. This is why our system of planets is called the Solar System. There are trillions of other stars in the universe just like it. Many of these stars have their ...
Earth Science Curriculum Unit 1 Maps and Measurements
... Students will be able to: Explain how observed redshift in far away stars provides evidence for the expansion of the universe and the Big Bang. Explain the how uniform cosmic background radiation evidence for the Big Bang. Describe how our solar system was formed through accretion due to gravi ...
... Students will be able to: Explain how observed redshift in far away stars provides evidence for the expansion of the universe and the Big Bang. Explain the how uniform cosmic background radiation evidence for the Big Bang. Describe how our solar system was formed through accretion due to gravi ...
UNIVERSAL GRAVITATION
... In this case it is not a centripetal force being provided by gravity, but simply a deceleration force to slow the expansion. The observed mass density of the universe is only about 4% of the critical value shown above, so the universe appears to be open – ie it will go on expanding forever. There ar ...
... In this case it is not a centripetal force being provided by gravity, but simply a deceleration force to slow the expansion. The observed mass density of the universe is only about 4% of the critical value shown above, so the universe appears to be open – ie it will go on expanding forever. There ar ...
The basic premise of the Nebular Model or Theory is that planets var
... This may have been started by a shock wave from an exploding star. Like water going down a drain, it started to spin as it contracted into a disc shape. Eventually, the density and temperature at its center began nuclear fusion, and started the sun shining. The rest of the gas and dust, that did not ...
... This may have been started by a shock wave from an exploding star. Like water going down a drain, it started to spin as it contracted into a disc shape. Eventually, the density and temperature at its center began nuclear fusion, and started the sun shining. The rest of the gas and dust, that did not ...
Characteristics of Stars WS Questions 1-20
... Answer all of the following questions by rephrasing and using complete sentences. If you do not rephrase or use complete sentences, you will automatically lose half of the points available. 1. If you could travel at the speed of light, how long would it take you to travel from Earth to the sun? ...
... Answer all of the following questions by rephrasing and using complete sentences. If you do not rephrase or use complete sentences, you will automatically lose half of the points available. 1. If you could travel at the speed of light, how long would it take you to travel from Earth to the sun? ...
Mountain-Skies-2016-0718
... Saturn through a telescope recently, make an effort to do so. Its rings are fully “open” as we say meaning they are tilted the maximum towards the earth and present a beautiful picture through a telescope. They also contribute to Saturn’s brightness ma ...
... Saturn through a telescope recently, make an effort to do so. Its rings are fully “open” as we say meaning they are tilted the maximum towards the earth and present a beautiful picture through a telescope. They also contribute to Saturn’s brightness ma ...
Simulating Gravitational Attraction Activity
... a) How does this represent a planet’s motion and the forces that cause it? b) How can you make the planet (rubber stopper) go faster? Slower? c) Ho do radius and speed relate? d) Does this agree with the fact that Jupiter takes almost 12 times longer than the Earth to go once around the sun? e) In g ...
... a) How does this represent a planet’s motion and the forces that cause it? b) How can you make the planet (rubber stopper) go faster? Slower? c) Ho do radius and speed relate? d) Does this agree with the fact that Jupiter takes almost 12 times longer than the Earth to go once around the sun? e) In g ...
Teacher`s Show Guide
... size of the ball gets larger. It gets flatter! In fact, your palm is pretty flat when holding the beach ball. Then think about how much larger the Earth is than a beach ball! 5. If you have a sunny window, tape an "X" on the window so that it casts a shadow on the floor. What does the shadow do over ...
... size of the ball gets larger. It gets flatter! In fact, your palm is pretty flat when holding the beach ball. Then think about how much larger the Earth is than a beach ball! 5. If you have a sunny window, tape an "X" on the window so that it casts a shadow on the floor. What does the shadow do over ...
Our Solar System
... Consortium; page 8: courtesy of NASA/Johns Hopkins University Applied Physics Laboratory/Arizona State University/Carnegie Institution of Washington. Image reproduced courtesy of Science/AAAS; pages 9, 13: courtesy of NASA/JPL/ USGS; page 11: courtesy of NASA/GSFC/GOES/NOAA; pages 12, 17, 21: courte ...
... Consortium; page 8: courtesy of NASA/Johns Hopkins University Applied Physics Laboratory/Arizona State University/Carnegie Institution of Washington. Image reproduced courtesy of Science/AAAS; pages 9, 13: courtesy of NASA/JPL/ USGS; page 11: courtesy of NASA/GSFC/GOES/NOAA; pages 12, 17, 21: courte ...
Mountain Skies - Pisgah Astronomical Research Institute
... Saturn through a telescope recently, make an effort to do so. Its rings are fully “open” as we say meaning they are tilted the maximum towards the earth and present a beautiful picture through a telescope. They also contribute to Saturn’s brightness making this planet, while not as bright as Jupiter ...
... Saturn through a telescope recently, make an effort to do so. Its rings are fully “open” as we say meaning they are tilted the maximum towards the earth and present a beautiful picture through a telescope. They also contribute to Saturn’s brightness making this planet, while not as bright as Jupiter ...
Science 09 Space Review 1. Know what a light year is
... 2. Given the solar system data, you should be able to determine scale model distances for ANY planet in the solar system (or indeed, any celestial object). Example: If earth is at 10 m in a model, where is Jupiter in the model? Planets distance = planet's model distance earth's distance earth's mode ...
... 2. Given the solar system data, you should be able to determine scale model distances for ANY planet in the solar system (or indeed, any celestial object). Example: If earth is at 10 m in a model, where is Jupiter in the model? Planets distance = planet's model distance earth's distance earth's mode ...
Neptune and Beyond, Asteroids, Comets
... thought it was due to the gravitational pull of hitherto unknown plant causing the deviation of Uranus orbit. They independently predicted the position of such an object that would account for the deviations observed. Neptune was first observed by Johan Galle and Heinrich d'Arrest on 1846 Sept 23 ve ...
... thought it was due to the gravitational pull of hitherto unknown plant causing the deviation of Uranus orbit. They independently predicted the position of such an object that would account for the deviations observed. Neptune was first observed by Johan Galle and Heinrich d'Arrest on 1846 Sept 23 ve ...
theory (casual usage of the word) vs. scientific theory
... – Sexual reproduction arises and SPEEDS up the evolutionary process! Leads to much more variation!! (pg. 428) – A few hundred million years after sexual repro. evolved we begin to see the fossil evidence of MULTICELLULAR life forms. ...
... – Sexual reproduction arises and SPEEDS up the evolutionary process! Leads to much more variation!! (pg. 428) – A few hundred million years after sexual repro. evolved we begin to see the fossil evidence of MULTICELLULAR life forms. ...
The solar system - Secondary Education
... asteroid in the main asteroid belt between Mars and Jupiter, was also declared a dwarf planet. The third and final (for now!) dwarf planet is Eris, an icy body on the edge of our Solar System that was discovered recently in 2005. Eris was temporarily labeled 2003 UB313 when it was first discovered, ...
... asteroid in the main asteroid belt between Mars and Jupiter, was also declared a dwarf planet. The third and final (for now!) dwarf planet is Eris, an icy body on the edge of our Solar System that was discovered recently in 2005. Eris was temporarily labeled 2003 UB313 when it was first discovered, ...
Space Revision Answers File
... 3. What is the difference between a solar eclipse and a lunar eclipse? A lunar eclipse occurs when the Earth passes between the Moon and the Sun, and the Earth's shadow obscures the moon or a portion of it. A solar eclipse occurs when the Moon passes between the Earth and the Sun, blocking all or a ...
... 3. What is the difference between a solar eclipse and a lunar eclipse? A lunar eclipse occurs when the Earth passes between the Moon and the Sun, and the Earth's shadow obscures the moon or a portion of it. A solar eclipse occurs when the Moon passes between the Earth and the Sun, blocking all or a ...
Angular Momentum
... Today we can understand the physical reasons for these laws … Let’s remind us first of the geometry of the ellipse and then discuss the three laws. ...
... Today we can understand the physical reasons for these laws … Let’s remind us first of the geometry of the ellipse and then discuss the three laws. ...
stars and planets
... gas in the interstellar medium while others are the result of the death throws of a massive star. • Hydrogen clumps together inside these clouds of gas growing ever larger and hotter until eventually the early stage of a star called a Protostar is formed. As gravity collapses the Protostar even more ...
... gas in the interstellar medium while others are the result of the death throws of a massive star. • Hydrogen clumps together inside these clouds of gas growing ever larger and hotter until eventually the early stage of a star called a Protostar is formed. As gravity collapses the Protostar even more ...
Sun - rmwright
... There are thick, colorful clouds of poisonous gases surrounding it Has a famous “red spot” Fifth planet from the Sun ...
... There are thick, colorful clouds of poisonous gases surrounding it Has a famous “red spot” Fifth planet from the Sun ...
Planet Formation Gas Giants
... The Inner Planets • Within 5 AU dust grains grow to ~1 m in ~1000 years and accrete into vast numbers of “planetesimals”. • The biggest planetesimals undergo “runaway growth” to form the terrestrial planet cores. Their exact chemical composition depends on their distance from the Sun. ...
... The Inner Planets • Within 5 AU dust grains grow to ~1 m in ~1000 years and accrete into vast numbers of “planetesimals”. • The biggest planetesimals undergo “runaway growth” to form the terrestrial planet cores. Their exact chemical composition depends on their distance from the Sun. ...
astro 001.101 summer 2002 exam 2
... passing a slower car on the highway: As you overtake the slower can, from your point of view it appears that the car is moving backwards. Thus it is for the slower planets that Earth overtakes from time to time. b) Arguments raised by the Greeks included: 1) Dropping an object, without giving it any ...
... passing a slower car on the highway: As you overtake the slower can, from your point of view it appears that the car is moving backwards. Thus it is for the slower planets that Earth overtakes from time to time. b) Arguments raised by the Greeks included: 1) Dropping an object, without giving it any ...
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.