monkeyball_lifecycleofastar
... gravity sucks the star inward, and not even light can escape a black hole. Some people think that a black hole can lead to another dimension or another universe, sounds cool right ? Well no its not cool because if you ever get caught in one you would be stretched out and you probably would die. ...
... gravity sucks the star inward, and not even light can escape a black hole. Some people think that a black hole can lead to another dimension or another universe, sounds cool right ? Well no its not cool because if you ever get caught in one you would be stretched out and you probably would die. ...
157a_midterm_2016
... Orbit radius 47 108 m emissivity 0.3 We are observing this system from a long distance, so we cannot resolve individual details. Plot the relative intensity that we would observe as a function of time (i.e. as a function of the planet position in its orbit) at a wavelength of 16 microns. Can we ...
... Orbit radius 47 108 m emissivity 0.3 We are observing this system from a long distance, so we cannot resolve individual details. Plot the relative intensity that we would observe as a function of time (i.e. as a function of the planet position in its orbit) at a wavelength of 16 microns. Can we ...
Lecture11
... Eventually T becomes high enough that molecular hydrogen dissociates; this absorbs some of the energy supporting the protostar, so the core begins to collapse further, until it becomes ~30% larger than the present Solar radius (but still much less massive). The protostar continues to accrete materia ...
... Eventually T becomes high enough that molecular hydrogen dissociates; this absorbs some of the energy supporting the protostar, so the core begins to collapse further, until it becomes ~30% larger than the present Solar radius (but still much less massive). The protostar continues to accrete materia ...
Sample Midterm - IUPUI Physics
... 1) A) For a brief period after the Hydrogen in a core of a star is all fused to Helium where does the energy that a star needs to survive come from (before it starts to fuse Helium) and how does that affect the size and temperature of the surface of the star? B) What is the process by which Helium ( ...
... 1) A) For a brief period after the Hydrogen in a core of a star is all fused to Helium where does the energy that a star needs to survive come from (before it starts to fuse Helium) and how does that affect the size and temperature of the surface of the star? B) What is the process by which Helium ( ...
Stars - Montville.net
... 9. When a high mass star begins to die it turns into a supergiant. 10. When a supergiant runs out of fuel it can suddenly explode. This explosion is called a super nova. ...
... 9. When a high mass star begins to die it turns into a supergiant. 10. When a supergiant runs out of fuel it can suddenly explode. This explosion is called a super nova. ...
Chapter 25 - Notes Super Size
... • Spiral galaxy that is about 100,000 _________________ across. • Out solar system is located about half-way out on one of the spiral arms. • Like many galaxies, the Milky Way has a super massive Black Hole at its _________________. Origin of _________________ • _________________ State Theory- the U ...
... • Spiral galaxy that is about 100,000 _________________ across. • Out solar system is located about half-way out on one of the spiral arms. • Like many galaxies, the Milky Way has a super massive Black Hole at its _________________. Origin of _________________ • _________________ State Theory- the U ...
Homework, August 29, 2002 AST110-6
... 3. Chapter 5, Problem 30. (20pt) Energy Level Transition. The following labeled transitions represent an electron moving between energy levels in hydrogen atom. Answer each of the following questions and explain your answer. a. Which transition could represent an atom that absorbs a photon with 10.2 ...
... 3. Chapter 5, Problem 30. (20pt) Energy Level Transition. The following labeled transitions represent an electron moving between energy levels in hydrogen atom. Answer each of the following questions and explain your answer. a. Which transition could represent an atom that absorbs a photon with 10.2 ...
Our Community`s Place Among the Stars
... http://www.youtube.com/watch?v=EO9CPO3CBF0 http://www.atomicarchive.com/Fusion/FusionMov.shtml ...
... http://www.youtube.com/watch?v=EO9CPO3CBF0 http://www.atomicarchive.com/Fusion/FusionMov.shtml ...
For stars
... • Rigel (m = 0.12) • Spica (m = +1.0) • Which looks brighter? Rigel BUT... It turns out that Spica actually gives off 1000 times more light than Rigel!! SO..If Spica is giving off more light, why would it appear dimmer in the sky here at Earth? ...
... • Rigel (m = 0.12) • Spica (m = +1.0) • Which looks brighter? Rigel BUT... It turns out that Spica actually gives off 1000 times more light than Rigel!! SO..If Spica is giving off more light, why would it appear dimmer in the sky here at Earth? ...
Astronomy Library wk 7.cwk (WP)
... higher energy levels because there are no lower energy levels available. Even at low temperatures (even absolute zero), these electrons will have considerable energy, moving about quickly. This energy and motion creates an outward pressure—electron degeneracy pressure. This electron degeneracy press ...
... higher energy levels because there are no lower energy levels available. Even at low temperatures (even absolute zero), these electrons will have considerable energy, moving about quickly. This energy and motion creates an outward pressure—electron degeneracy pressure. This electron degeneracy press ...
Apparent brightness
... Explain how stellar distances are determined. Explain how physical laws are used to estimate stellar sizes. Distinguish between luminosity and brightness and explain how stellar luminosity is determined. Explain how stars are classified according to their colors, surface temperatures and spe ...
... Explain how stellar distances are determined. Explain how physical laws are used to estimate stellar sizes. Distinguish between luminosity and brightness and explain how stellar luminosity is determined. Explain how stars are classified according to their colors, surface temperatures and spe ...
Stars and Galaxies
... 24. Astronomers use spectrographs to study the ___________________ of stars to identify properties of stars. 25. Spectrographs break ______________________ into its component colors. 26. Dark lines are in the spectrum of a star. 27. The dark lines are caused by _____________________ in the star’s at ...
... 24. Astronomers use spectrographs to study the ___________________ of stars to identify properties of stars. 25. Spectrographs break ______________________ into its component colors. 26. Dark lines are in the spectrum of a star. 27. The dark lines are caused by _____________________ in the star’s at ...
chapter9
... absorbed by interstellar clouds Red light can more easily penetrate the cloud, but is still absorbed to some extent ...
... absorbed by interstellar clouds Red light can more easily penetrate the cloud, but is still absorbed to some extent ...
The Hertzsprung – Russell Diagram
... The Hertzsprung – Russell Diagram Background Information: For astronomers, a graph that displays a star’s luminosity on the y-axis and its surface temperature on the x-axis sets up an extremely useful diagram called a Hertzsprung-Russell, or H-R Diagram. In 1910 Ejnar Hertzsprung and Henry Norris Ru ...
... The Hertzsprung – Russell Diagram Background Information: For astronomers, a graph that displays a star’s luminosity on the y-axis and its surface temperature on the x-axis sets up an extremely useful diagram called a Hertzsprung-Russell, or H-R Diagram. In 1910 Ejnar Hertzsprung and Henry Norris Ru ...