wk9 (part 1)
... C. Protons and electrons formed stable hydrogen atoms for the first time at this epoch, and the matter in the Universe became mostly transparent to radiation D. This epoch was immediately followed by Inflation ...
... C. Protons and electrons formed stable hydrogen atoms for the first time at this epoch, and the matter in the Universe became mostly transparent to radiation D. This epoch was immediately followed by Inflation ...
Ch.10 Stellar old age
... • H fusion is faster because C, N and O act as catalysts • Same net result: 4 H become 1 He. • No total gain or loss of C, N, O Question: How does energy produced by CNO cycle compare to PP chain? ...
... • H fusion is faster because C, N and O act as catalysts • Same net result: 4 H become 1 He. • No total gain or loss of C, N, O Question: How does energy produced by CNO cycle compare to PP chain? ...
Lectures 10 & 11 powerpoint (stellar formation) [movie below]
... Fusion into Heavier Elements Fusion into elements heavier than C, O: ...
... Fusion into Heavier Elements Fusion into elements heavier than C, O: ...
Lec 25.2- STELLAR EVOLUTION SUMMARY
... Gravity is a key to star evolution. You may recall that according to Newton's law of gravity, all bodies, from the largest objects to the smallest particles in the universe, attract each other. Thus, the gas and dust particles of the vast interstellar' clouds exert gravity upon one another. Eventual ...
... Gravity is a key to star evolution. You may recall that according to Newton's law of gravity, all bodies, from the largest objects to the smallest particles in the universe, attract each other. Thus, the gas and dust particles of the vast interstellar' clouds exert gravity upon one another. Eventual ...
Astronomy Chap 1
... sunburns. What is the critical angle? 6. Review the Solar Motion Demonstrator Activities. Chapter 2: The Nighttime Sky 1. How would you describe the motion of the stars visible at night? 2. How would the motion of stars change if viewed from the equator, Michigan, the North Pole? Draw a picture for ...
... sunburns. What is the critical angle? 6. Review the Solar Motion Demonstrator Activities. Chapter 2: The Nighttime Sky 1. How would you describe the motion of the stars visible at night? 2. How would the motion of stars change if viewed from the equator, Michigan, the North Pole? Draw a picture for ...
Structure of the Sun, our nearest star
... o Tremendous amounts of energy flung into space, including high-energy particles and electromagnetic radiation o When the radiation and particles reach the Earth's magnetic field, they interact with it to produce auroras o Solar flares can also disrupt communications, satellites, navigation systems ...
... o Tremendous amounts of energy flung into space, including high-energy particles and electromagnetic radiation o When the radiation and particles reach the Earth's magnetic field, they interact with it to produce auroras o Solar flares can also disrupt communications, satellites, navigation systems ...
Life cycle of Stars Notes
... • The spherical surface is known as the event horizon. • Astronomers believe black holes exist because they bend the fabric of space. ...
... • The spherical surface is known as the event horizon. • Astronomers believe black holes exist because they bend the fabric of space. ...
File
... supergiant. When the star stops expanding because it can no longer create enough energy to support its own mass, it collapses completely and makes a giant explosion. A supernova is brighter than all the stars in the galaxy combined! The energy created by the explosion can travel at a speed of a thou ...
... supergiant. When the star stops expanding because it can no longer create enough energy to support its own mass, it collapses completely and makes a giant explosion. A supernova is brighter than all the stars in the galaxy combined! The energy created by the explosion can travel at a speed of a thou ...
The formation of stars and planets
... Strömgren sphere Effect of extinction: Inside sphere: virtually complete ionization. Recombination rate per volume element is: N H2 (H 0 ,T) ...
... Strömgren sphere Effect of extinction: Inside sphere: virtually complete ionization. Recombination rate per volume element is: N H2 (H 0 ,T) ...
solutions - Las Cumbres Observatory
... 1. It is 197 parsecs (640 light years) away, but how many magnitudes brighter than the Sun would it look if both stars were 10 parsecs (32.6 light years) away? Using absolute magnitude: MBetelgeuse = MSun - 2.5log10(LBetelgeuse/LSun) MBetelgeuse = 4.74 - 2.5log10(149,245.07 LSun/LSu ...
... 1. It is 197 parsecs (640 light years) away, but how many magnitudes brighter than the Sun would it look if both stars were 10 parsecs (32.6 light years) away? Using absolute magnitude: MBetelgeuse = MSun - 2.5log10(LBetelgeuse/LSun) MBetelgeuse = 4.74 - 2.5log10(149,245.07 LSun/LSu ...
doc - EU-HOU
... and the Commission cannot be held responsible for any use which may be made of the information contained therein. ...
... and the Commission cannot be held responsible for any use which may be made of the information contained therein. ...
Distance measurement in astronomy
... Cepheid variables are one particular type of variable star (one whose brightness changes with time) called after delta Cephei, the first star of this type to be observed. The variation in brightness of this star was discovered by John Goodricke in 1784. Goodricke lived in York and was a promising yo ...
... Cepheid variables are one particular type of variable star (one whose brightness changes with time) called after delta Cephei, the first star of this type to be observed. The variation in brightness of this star was discovered by John Goodricke in 1784. Goodricke lived in York and was a promising yo ...
STARS
... • The absence of pressure causes a neutron star or a black hole. • The explosion can be bright enough to see during the day! ...
... • The absence of pressure causes a neutron star or a black hole. • The explosion can be bright enough to see during the day! ...