The Sun
... • Places where the sun’s magnetic field is concentrated and inhibits the normal convective flow of hot material from below. So the material sits on the surface and cools off as it radiates to the sky. • Charged particles in a magnetic field feel a force sideways to their motion, binding the gas to t ...
... • Places where the sun’s magnetic field is concentrated and inhibits the normal convective flow of hot material from below. So the material sits on the surface and cools off as it radiates to the sky. • Charged particles in a magnetic field feel a force sideways to their motion, binding the gas to t ...
Name Period ______ Astronomy Unit Study Guide 1. _____
... 16. What is the reason for Earth’s seasons? How long does it take the Earth to orbit the sun once? 17. Define: ...
... 16. What is the reason for Earth’s seasons? How long does it take the Earth to orbit the sun once? 17. Define: ...
STARS and GALAXIES
... • A large ball of gas held together by gravity that produces tremendous amounts of heat and light. • Some stars are very old and the size of planets or moons, and some no longer emit radiation (no light). ...
... • A large ball of gas held together by gravity that produces tremendous amounts of heat and light. • Some stars are very old and the size of planets or moons, and some no longer emit radiation (no light). ...
Sun
... up and rises to the surface. Photosphere – (circle of light) This is the outer visible of the sun. It contains many ...
... up and rises to the surface. Photosphere – (circle of light) This is the outer visible of the sun. It contains many ...
Stars - Independence High School
... • Fission- Separation of large nucleus into smaller nuclei • The Sun uses fusion to combine Hydrogen into Helium ...
... • Fission- Separation of large nucleus into smaller nuclei • The Sun uses fusion to combine Hydrogen into Helium ...
THE SUN - Halton District School Board
... own gravity is balanced by the nuclear explosions at its core. ...
... own gravity is balanced by the nuclear explosions at its core. ...
The Sun*s
... each time, until the core temperature cannot rise any higher. At this point, the star “dies”. ...
... each time, until the core temperature cannot rise any higher. At this point, the star “dies”. ...
Solar System
... THE SUN • Photosphere- the brightest part of the sun • Chromosphere- gives off faint red light and cannot be seen • Corona- halo that surrounds the sun ...
... THE SUN • Photosphere- the brightest part of the sun • Chromosphere- gives off faint red light and cannot be seen • Corona- halo that surrounds the sun ...
Document
... • Sound waves cross the the solar interior and reflect off of the surface (photosphere). ...
... • Sound waves cross the the solar interior and reflect off of the surface (photosphere). ...
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... • In addition to the p-p cycle, there is the CNO Cycle, in which the C, N, O, nuclei catalyze the burning of H into He • The rates of TNR are usually very steep functions of temperature, due to high potential barriers • Generally, more massive stars achieve higher Tc , and can synthesize elements ...
... • In addition to the p-p cycle, there is the CNO Cycle, in which the C, N, O, nuclei catalyze the burning of H into He • The rates of TNR are usually very steep functions of temperature, due to high potential barriers • Generally, more massive stars achieve higher Tc , and can synthesize elements ...
Homework Solutions: Chapter 7, The Sun
... A: The spectral emission lines of the corona are strongly broadened in wavelength, indicating extremely high temperature. Furthermore in the corona’s spectrum we find emission lines of highly ionized gases which also give us more evidence that corona has a very high temperature. RQ: 7-13 Q: Why does ...
... A: The spectral emission lines of the corona are strongly broadened in wavelength, indicating extremely high temperature. Furthermore in the corona’s spectrum we find emission lines of highly ionized gases which also give us more evidence that corona has a very high temperature. RQ: 7-13 Q: Why does ...
The Sun: Home Star
... • Key to solar-stellar connection • Close-up model for other stars • Local “lab” for testing ideas about the physics of stars • Energy source for most life on earth ...
... • Key to solar-stellar connection • Close-up model for other stars • Local “lab” for testing ideas about the physics of stars • Energy source for most life on earth ...
STARS In your textbook, read about the properties of the Sun and
... 6. Stars on the main sequence produce energy by fusing hydrogen into----' 7. As a contracts, its rotation forces it into a disk shape with a hot condensed object at the center, which will become a new stsr. 8. During a the entire portion of the star is blown off in a massive explosion! What are Gala ...
... 6. Stars on the main sequence produce energy by fusing hydrogen into----' 7. As a contracts, its rotation forces it into a disk shape with a hot condensed object at the center, which will become a new stsr. 8. During a the entire portion of the star is blown off in a massive explosion! What are Gala ...
Notes 14-2
... The Sun is a Star • Star made of hydrogen and helium • located at the center of the solar system and is also the largest object • Has a strong gravitational pull which holds planets in orbit • 4.6 billion years old ...
... The Sun is a Star • Star made of hydrogen and helium • located at the center of the solar system and is also the largest object • Has a strong gravitational pull which holds planets in orbit • 4.6 billion years old ...
Astronomy II (ASTR1020) — Exam 1 Test No. 1D
... 4. Which of the following best describes a photon’s journey inside the Sun? a) Travels in a straight line at the speed of 2.997925 × 105 km/s. b) Travels in a curved path following the Sun’s magnetic field. c) Travels in a zig-zag (random walk) type of path. d) Photons do not exist inside the Sun. e ...
... 4. Which of the following best describes a photon’s journey inside the Sun? a) Travels in a straight line at the speed of 2.997925 × 105 km/s. b) Travels in a curved path following the Sun’s magnetic field. c) Travels in a zig-zag (random walk) type of path. d) Photons do not exist inside the Sun. e ...
A Red Giant - Cloudfront.net
... Stars with masses similar to our Sun fuse at a rate that allows them to “live” as mainsequence stars for about 10 billion years. Then they run out of Hydrogen in their core Hydrostatic Equilibrium is lost… They Shrink a bit And begin to fuse Hydrogen into Helium in a shell outside the core. ...
... Stars with masses similar to our Sun fuse at a rate that allows them to “live” as mainsequence stars for about 10 billion years. Then they run out of Hydrogen in their core Hydrostatic Equilibrium is lost… They Shrink a bit And begin to fuse Hydrogen into Helium in a shell outside the core. ...
We Are All Star Dust - High School of Language and Innovation
... Inside the Sun, Temperatures are so High… • Nuclear Fusion occurs ...
... Inside the Sun, Temperatures are so High… • Nuclear Fusion occurs ...