
4 x What Powers the Sun? • Need to provide
... Magnetic field lines short out Î Huge burst of charged particles Due to “winding up” of Sun’s magnetic ...
... Magnetic field lines short out Î Huge burst of charged particles Due to “winding up” of Sun’s magnetic ...
Earth`s magnetic field – what is it good for?
... How does this work? When either or both magnetic fields is weak (as when the Sun sported fewer sunspots during the Maunder Minimum), more cosmic rays reach our atmosphere, creating muons (heavy electrons) that produce the condensation nuclei for cloud formation. An increase in cloudiness results in ...
... How does this work? When either or both magnetic fields is weak (as when the Sun sported fewer sunspots during the Maunder Minimum), more cosmic rays reach our atmosphere, creating muons (heavy electrons) that produce the condensation nuclei for cloud formation. An increase in cloudiness results in ...
Simon P. Balm Astronomy 5, Test #1, Sample Questions
... combined mass is slightly greater than the original nucleus B) a heavy nucleus breaks apart into a number of smaller nuclei whose combined mass are less than the original nucleus C) two or more nuclei fuse or stick together to form a heavier nucleus whose combined mass is slightly less than the orig ...
... combined mass is slightly greater than the original nucleus B) a heavy nucleus breaks apart into a number of smaller nuclei whose combined mass are less than the original nucleus C) two or more nuclei fuse or stick together to form a heavier nucleus whose combined mass is slightly less than the orig ...
Elements from Stardust
... With the high pressure and hot temperature in the sun, nuclei of atoms are squeezed together and they collide. Nuclear fusion combines smaller nuclei into larger nuclei—making bigger and heavier atoms. ...
... With the high pressure and hot temperature in the sun, nuclei of atoms are squeezed together and they collide. Nuclear fusion combines smaller nuclei into larger nuclei—making bigger and heavier atoms. ...
SNC1P - MsKhan
... -a star is a massive collection of gases and is luminous (it gives off its own light) -the Sun is the closest star to the Earth, which is why it appears so LARGE -planets = large, round, celestial objects that orbit around ________________ -there are 8 planets orbiting around our Sun -planets are no ...
... -a star is a massive collection of gases and is luminous (it gives off its own light) -the Sun is the closest star to the Earth, which is why it appears so LARGE -planets = large, round, celestial objects that orbit around ________________ -there are 8 planets orbiting around our Sun -planets are no ...
How is the universe both predictable and unpredictable at the same
... next closest star to us is ______________ light years away. - The light you see from some stars was really given off millions of years ago. B. Astronomical Units - Measures distance between objects in the solar system. - Is the average distance between Earth and the Sun…. about 150 million kilometer ...
... next closest star to us is ______________ light years away. - The light you see from some stars was really given off millions of years ago. B. Astronomical Units - Measures distance between objects in the solar system. - Is the average distance between Earth and the Sun…. about 150 million kilometer ...
Distances in Space
... 1 AU = average distance between Earth and Sun Earth is 150 000 000 km, or 1 AU away from the Sun. Mars is 230 000 000 km, from the sun, or approximately 1.5 a.u. from the Sun. So Mars is 1.5 times as far from the sun as Earth is from the sun. ...
... 1 AU = average distance between Earth and Sun Earth is 150 000 000 km, or 1 AU away from the Sun. Mars is 230 000 000 km, from the sun, or approximately 1.5 a.u. from the Sun. So Mars is 1.5 times as far from the sun as Earth is from the sun. ...
PPT - ILWS
... geomagnetic storms; seasonal and diurnal effect on these variations; recovery of the thermosphere and ionosphere after storms • Global electric field distributions during geomagnetic storms, their temporal and spatial variations, and their changes with ionospheric conductivity • The generation, prop ...
... geomagnetic storms; seasonal and diurnal effect on these variations; recovery of the thermosphere and ionosphere after storms • Global electric field distributions during geomagnetic storms, their temporal and spatial variations, and their changes with ionospheric conductivity • The generation, prop ...
PHYS 200 - Understanding the Universe
... • Report on: what makes up the solar system, what is the physical difference between planets and stars, whether stars live forever, and what makes up our Milky Way Galaxy. • Comprehend that cosmic bodies are always in motion relative to each other. That for example the relative motion of the Earth, ...
... • Report on: what makes up the solar system, what is the physical difference between planets and stars, whether stars live forever, and what makes up our Milky Way Galaxy. • Comprehend that cosmic bodies are always in motion relative to each other. That for example the relative motion of the Earth, ...
The Sun, the closest star - University of Iowa Astrophysics
... The Sun has a “heartbeat”; its properties change on a period of ...
... The Sun has a “heartbeat”; its properties change on a period of ...
Introduction to the Earth
... New Insights into the Big Bang Recent mapping of microwave and temperature variations suggest that the Universe may be flat – not spherical! Implications? ...
... New Insights into the Big Bang Recent mapping of microwave and temperature variations suggest that the Universe may be flat – not spherical! Implications? ...
Exam Name___________________________________
... 26) What will happen to the Sun in about 5 billion years? Describe the appearance of the Sun and the processes inside the Sun to cause any changes in appearance. 27) What is the helium flash and what causes it? 28) What are neutrinos? Describe the properties of neutrinos: mass, size, electrical char ...
... 26) What will happen to the Sun in about 5 billion years? Describe the appearance of the Sun and the processes inside the Sun to cause any changes in appearance. 27) What is the helium flash and what causes it? 28) What are neutrinos? Describe the properties of neutrinos: mass, size, electrical char ...
lecture 32 orbits
... even move backwards with respect to the surrounding stars (retrograde motion). During a planet’s retrograde motion, it appeared brighter than at other times. This suggested to the Greeks that the planet was closer to Earth during its retrograde motion. ...
... even move backwards with respect to the surrounding stars (retrograde motion). During a planet’s retrograde motion, it appeared brighter than at other times. This suggested to the Greeks that the planet was closer to Earth during its retrograde motion. ...
Accretion Friction Braking in Stellar Metamorphosis
... documentaries about big name astronomers and astrophysicists are all wrong when it comes to stars. The only thing cooking in a star is a planet. Matter synthesis happens in active galaxies or AGNs, events which actually have the energy required to fuse matter at high velocities, and in gargantuan qu ...
... documentaries about big name astronomers and astrophysicists are all wrong when it comes to stars. The only thing cooking in a star is a planet. Matter synthesis happens in active galaxies or AGNs, events which actually have the energy required to fuse matter at high velocities, and in gargantuan qu ...
The Universe and Big Bang Theory Review Sheet
... - gravity causes the gas and dust clouds to clump up, forming larger balls of gas and dust molecules. 9. A star is born how? (step 3 in Star Origin notes) -When the mass becomes slightly larger than Jupiter, the gravitational contraction causes enough high temp and high pressure to start Nuclear Fus ...
... - gravity causes the gas and dust clouds to clump up, forming larger balls of gas and dust molecules. 9. A star is born how? (step 3 in Star Origin notes) -When the mass becomes slightly larger than Jupiter, the gravitational contraction causes enough high temp and high pressure to start Nuclear Fus ...
Space Unit Test - grade 6 science
... 8. There is no way you could live on me, because I have very little oxygen due to no atmosphere. I am also red because of all the rust on me. I am _____________. 9. Hello, I move very slowly around the sun (165 years for one orbit). Oh yeah, I have the Great Dark Spot, but it vanished in 1994. I am ...
... 8. There is no way you could live on me, because I have very little oxygen due to no atmosphere. I am also red because of all the rust on me. I am _____________. 9. Hello, I move very slowly around the sun (165 years for one orbit). Oh yeah, I have the Great Dark Spot, but it vanished in 1994. I am ...
Topic 4: Sun, Earth, Moon and the Solar System
... Essential Questions: How does space exploration involve scientists from many different fields? How does classifying stars help scientists to understand the universe? Why is scientific argumentation necessary in scientific inquiry and what role does it play in the generation and validation of scienti ...
... Essential Questions: How does space exploration involve scientists from many different fields? How does classifying stars help scientists to understand the universe? Why is scientific argumentation necessary in scientific inquiry and what role does it play in the generation and validation of scienti ...
astronomy - sfox4science
... The universe is estimated to be over 10 billion years old. The universe is composed of galaxies, stars, planets, asteroids, comets, and meteors, each having different properties. Our solar system exists within the Milky Way galaxy. The known components of our solar system are the Sun, four terrestri ...
... The universe is estimated to be over 10 billion years old. The universe is composed of galaxies, stars, planets, asteroids, comets, and meteors, each having different properties. Our solar system exists within the Milky Way galaxy. The known components of our solar system are the Sun, four terrestri ...
GR Cosmology: The Robertson
... The 3-sphere, k 1 , is a very serious candidate for the geometry of space in our universe, and it would mean that the further away you look, , the more: a circumference drawn around at that distance would be smaller than 2 and the area at that distance would be less than 4 2 . Ultimately w ...
... The 3-sphere, k 1 , is a very serious candidate for the geometry of space in our universe, and it would mean that the further away you look, , the more: a circumference drawn around at that distance would be smaller than 2 and the area at that distance would be less than 4 2 . Ultimately w ...
How long does it take sunlight to reach the Earth?
... Earth. The Sun is more than 8 light-minutes away. If the Sun suddenly disappeared from the Universe (not that this could actually happen, don't And so, if the light from the nearest star (Alpha Centauri) takes more than 4 years to reach us, panic), it would take a little more than 8 minutes before y ...
... Earth. The Sun is more than 8 light-minutes away. If the Sun suddenly disappeared from the Universe (not that this could actually happen, don't And so, if the light from the nearest star (Alpha Centauri) takes more than 4 years to reach us, panic), it would take a little more than 8 minutes before y ...
the universe
... observations to develop a theory called the Big Bang. The theory states that about 13,700 million years ago all the matter in the universe was concentrated into a single incredibly tiny point. This began to enlarge rapidly in a hot explosion, and it is still expanding today. Gravity is slowing down ...
... observations to develop a theory called the Big Bang. The theory states that about 13,700 million years ago all the matter in the universe was concentrated into a single incredibly tiny point. This began to enlarge rapidly in a hot explosion, and it is still expanding today. Gravity is slowing down ...
Instructions - Chandra X
... At this scale, the farthest distance humans have traveled is from the salt-grain Earth to the dust-speck Moon half an inch away. NASA is working to send astronauts to Mars, another 30 feet (or 10 meters) away at this scale. THE REALM OF OUR SOLAR SYSTEM. What is the farthest distance a NASA spacecra ...
... At this scale, the farthest distance humans have traveled is from the salt-grain Earth to the dust-speck Moon half an inch away. NASA is working to send astronauts to Mars, another 30 feet (or 10 meters) away at this scale. THE REALM OF OUR SOLAR SYSTEM. What is the farthest distance a NASA spacecra ...
the universe
... observations to develop a theory called the Big Bang. The theory states that about 13,700 million years ago all the matter in the universe was concentrated into a single incredibly tiny point. This began to enlarge rapidly in a hot explosion, and it is still expanding today. Gravity is slowing down ...
... observations to develop a theory called the Big Bang. The theory states that about 13,700 million years ago all the matter in the universe was concentrated into a single incredibly tiny point. This began to enlarge rapidly in a hot explosion, and it is still expanding today. Gravity is slowing down ...
Astronomy
... Have no definite shape Contain bright, young stars If it does not shape like a spiral or elliptical galaxy, it is classified as an irregular galaxy ...
... Have no definite shape Contain bright, young stars If it does not shape like a spiral or elliptical galaxy, it is classified as an irregular galaxy ...
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.