
Chapter 3 Section 2 (pgs 68-73) the sun`s outer atmosphere – this is
... and the gases moving in our atmosphere ...
... and the gases moving in our atmosphere ...
Exploding carbon star blowing molecules (red gas) into space Focus
... Oka,Avery,Bronson,McLeod(NRC);Alexander,Kirby,Walton(Sussex) ...
... Oka,Avery,Bronson,McLeod(NRC);Alexander,Kirby,Walton(Sussex) ...
Big Bang
... Era of galaxies • Lasts from one billion years after Big Bang to present • Galaxies form • Gravitationally bound system of stars, gas, and dust ...
... Era of galaxies • Lasts from one billion years after Big Bang to present • Galaxies form • Gravitationally bound system of stars, gas, and dust ...
here - Next Wave
... system that’s not too hot nor too cold, but just right for life like us to exist. But even with all the atoms and molecules needed for living things to flourish, and the Earth’s perfect distance from the sun to ensure that water is found everywhere, it is still not enough. The sun is continually bom ...
... system that’s not too hot nor too cold, but just right for life like us to exist. But even with all the atoms and molecules needed for living things to flourish, and the Earth’s perfect distance from the sun to ensure that water is found everywhere, it is still not enough. The sun is continually bom ...
ch16 b - Manasquan Public Schools
... stable atmosphere, and moderate stable temperatures give Earth perfect conditions to support life as we know it. ...
... stable atmosphere, and moderate stable temperatures give Earth perfect conditions to support life as we know it. ...
The Milky Way
... • How do scientists know about nature? • Where are you in the universe? • How does human history fit on the time scale of the universe? ...
... • How do scientists know about nature? • Where are you in the universe? • How does human history fit on the time scale of the universe? ...
The Sun
... Very Old. G stars becoming giants. All the same age and composition Can actually see evolution off the MS ...
... Very Old. G stars becoming giants. All the same age and composition Can actually see evolution off the MS ...
January 23
... A globular cluster is a roughly spherical collection of up to millions of stars bound together by the force of gravity. Astronomers can measure the velocities of the stars (rotation curves) in the cluster to get an idea of the mass distribution (as shown Monday). Assuming the stars have roughly the ...
... A globular cluster is a roughly spherical collection of up to millions of stars bound together by the force of gravity. Astronomers can measure the velocities of the stars (rotation curves) in the cluster to get an idea of the mass distribution (as shown Monday). Assuming the stars have roughly the ...
Word version with live links
... science view eg Hardy and Bonestall – book are available for lone on these topics. Stars These have a life cycle from birth to death when they seem to either collapse in on themselves and then explode, or just explode. By all accounts, we are safe for a good while because our own sun is fairly insig ...
... science view eg Hardy and Bonestall – book are available for lone on these topics. Stars These have a life cycle from birth to death when they seem to either collapse in on themselves and then explode, or just explode. By all accounts, we are safe for a good while because our own sun is fairly insig ...
2015-16 Space Week 1 and 2 ppt
... 21. The Doppler Shift is used to tell the distance between objects in our vast Universe. Fill the blanks with the next 4 words from the Doppler Shift song. "When a star is approaching and it's heading our way, _____ _____ _____ _____." 22. What was the date that the first woman to pilot a Space Shut ...
... 21. The Doppler Shift is used to tell the distance between objects in our vast Universe. Fill the blanks with the next 4 words from the Doppler Shift song. "When a star is approaching and it's heading our way, _____ _____ _____ _____." 22. What was the date that the first woman to pilot a Space Shut ...
Planet Earth - ThinkChemistry
... • What is the difference between stars, planets and moons? • What is the difference between The Solar System, a galaxy and The Universe? ...
... • What is the difference between stars, planets and moons? • What is the difference between The Solar System, a galaxy and The Universe? ...
The Universe: “Beyond the Big Bang” Video Questions
... 48. Where did the sounds that Penzias and Wilson heard originate? everywhere 49. What was the “smoking gun” that Penzias and Wilson discovered? cosmic background ...
... 48. Where did the sounds that Penzias and Wilson heard originate? everywhere 49. What was the “smoking gun” that Penzias and Wilson discovered? cosmic background ...
Chapter105.ppt
... • The church hierarchy adopted this view as dogma because it confirmed their own view that the Earth was the most important place in the Universe and human beings the Universe’s most important creatures. (Also, at the time, most people believe the Earth was flat, not spherical, and that if you sail ...
... • The church hierarchy adopted this view as dogma because it confirmed their own view that the Earth was the most important place in the Universe and human beings the Universe’s most important creatures. (Also, at the time, most people believe the Earth was flat, not spherical, and that if you sail ...
It all began with a Big Bang!
... first stars to form. New stars were being born 10 times as fast as now. ...
... first stars to form. New stars were being born 10 times as fast as now. ...
light years - Physics and Astronomy
... Distances to nearby stars are measured by: A: bouncing radar signals off them B: using laser beams C: using geometry and parallax measurements D: measuring how long it took a spacecraft to get there and back and assuming a constant velocity. ...
... Distances to nearby stars are measured by: A: bouncing radar signals off them B: using laser beams C: using geometry and parallax measurements D: measuring how long it took a spacecraft to get there and back and assuming a constant velocity. ...
ExpandUniv
... There is a chain of links which get us out to the distances of galaxies. Errors in any one affect all the further ones. ...
... There is a chain of links which get us out to the distances of galaxies. Errors in any one affect all the further ones. ...
Lecture notes 4: The Sun as a Star i
... limb. If the temperature gradient dt/dr falls with height in the photosphere we therefore expect the observed effect of limb darkening since high temperature gas emits more vigorously than low temperature gas. Should we expect that the color of the light is different at the limb and at sun center? Th ...
... limb. If the temperature gradient dt/dr falls with height in the photosphere we therefore expect the observed effect of limb darkening since high temperature gas emits more vigorously than low temperature gas. Should we expect that the color of the light is different at the limb and at sun center? Th ...
Section 11: GRAPHIC STIMULUS
... In most large cities [6] like Singapore, we can only see a few of the large bright stars out in space. This is due to the increased pollution of earth [7] s atmosphere especially in the cities. The polluted skies obscure most of the other smaller stars [8] However [9] the stars are fascinating to so ...
... In most large cities [6] like Singapore, we can only see a few of the large bright stars out in space. This is due to the increased pollution of earth [7] s atmosphere especially in the cities. The polluted skies obscure most of the other smaller stars [8] However [9] the stars are fascinating to so ...
Section 11: GRAPHIC STIMULUS
... In most large cities [6] like Singapore, we can only see a few of the large bright stars out in space. This is due to the increased pollution of earth [7] s atmosphere especially in the cities. The polluted skies obscure most of the other smaller stars [8] However [9] the stars are fascinating to so ...
... In most large cities [6] like Singapore, we can only see a few of the large bright stars out in space. This is due to the increased pollution of earth [7] s atmosphere especially in the cities. The polluted skies obscure most of the other smaller stars [8] However [9] the stars are fascinating to so ...
Chapter 02 Earth in Space
... A. By measuring the age of the oldest known asteroids B. By measuring the relative motion of other galaxies C. By measuring speed of light from distant stars ...
... A. By measuring the age of the oldest known asteroids B. By measuring the relative motion of other galaxies C. By measuring speed of light from distant stars ...
22 October: The Formation of Stars
... • Now, how to stars form? What do they form from? Space seems to be empty. Where does the material come from? ...
... • Now, how to stars form? What do they form from? Space seems to be empty. Where does the material come from? ...
Sample Exam Questions
... d) neutral atoms moving in an electric field 35. A "cosmological redshift" results from the a) velocity of a distant object relative to Earth c) combined gravity of all the mass in the Universe 36. Quasars are thought to be a) very distant active galaxies c) enormous black holes ...
... d) neutral atoms moving in an electric field 35. A "cosmological redshift" results from the a) velocity of a distant object relative to Earth c) combined gravity of all the mass in the Universe 36. Quasars are thought to be a) very distant active galaxies c) enormous black holes ...
Cosmic Hierarchy 9.5, 9.6
... Random and then press Load Preset and then run. This provides a thousand random masses, with random motion that obey the laws of physics for gravity and circular motion. a) How well does it match the solar nebula theory? ...
... Random and then press Load Preset and then run. This provides a thousand random masses, with random motion that obey the laws of physics for gravity and circular motion. a) How well does it match the solar nebula theory? ...
Space revision notes
... This theory gives an explanation of how the Universe began around 14 billion years ago – ...
... This theory gives an explanation of how the Universe began around 14 billion years ago – ...
Outer space
Outer space, or just space, is the void that exists between celestial bodies, including the Earth. It is not completely empty, but consists of a hard vacuum containing a low density of particles, predominantly a plasma of hydrogen and helium as well as electromagnetic radiation, magnetic fields, neutrinos, dust and cosmic rays. The baseline temperature, as set by the background radiation from the Big Bang, is 2.7 kelvin (K). Plasma with a number density of less than one hydrogen atom per cubic metre and a temperature of millions of kelvin in the space between galaxies accounts for most of the baryonic (ordinary) matter in outer space; local concentrations have condensed into stars and galaxies. In most galaxies, observations provide evidence that 90% of the mass is in an unknown form, called dark matter, which interacts with other matter through gravitational but not electromagnetic forces. Data indicates that the majority of the mass-energy in the observable Universe is a poorly understood vacuum energy of space which astronomers label dark energy. Intergalactic space takes up most of the volume of the Universe, but even galaxies and star systems consist almost entirely of empty space.There is no firm boundary where space begins. However the Kármán line, at an altitude of 100 km (62 mi) above sea level, is conventionally used as the start of outer space in space treaties and for aerospace records keeping. The framework for international space law was established by the Outer Space Treaty, which was passed by the United Nations in 1967. This treaty precludes any claims of national sovereignty and permits all states to freely explore outer space. Despite the drafting of UN resolutions for the peaceful uses of outer space, anti-satellite weapons have been tested in Earth orbit.Humans began the physical exploration of space during the 20th century with the advent of high-altitude balloon flights, followed by manned rocket launches. Earth orbit was first achieved by Yuri Gagarin of the Soviet Union in 1961 and unmanned spacecraft have since reached all of the known planets in the Solar System. Due to the high cost of getting into space, manned spaceflight has been limited to low Earth orbit and the Moon.Outer space represents a challenging environment for human exploration because of the dual hazards of vacuum and radiation. Microgravity also has a negative effect on human physiology that causes both muscle atrophy and bone loss. In addition to these health and environmental issues, the economic cost of putting objects, including humans, into space is high.