Star Life Cycle Powerpoin
... • The massive outer layers of the star again rush into the core and rebound, generating staggering amounts of energy. ...
... • The massive outer layers of the star again rush into the core and rebound, generating staggering amounts of energy. ...
View Presentation Slides
... Stars have “life cycles”. They are “born” and they “die” but are not alive like us. Stars like the Sun “die” by “puffing” off their outer layers of gas and dust. This process creates a beautiful variety of NEBULAE in the Milky Way GALAXY. ...
... Stars have “life cycles”. They are “born” and they “die” but are not alive like us. Stars like the Sun “die” by “puffing” off their outer layers of gas and dust. This process creates a beautiful variety of NEBULAE in the Milky Way GALAXY. ...
File - Adopt A Constellation
... • Constellations - A pattern or group of stars in the sky that humans observe in a pattern and give a name. • People of ancient time saw the constellations as character or animals in the sky. They made up stories to explain how the object, animal, or character came into the night sky • Earth rotate ...
... • Constellations - A pattern or group of stars in the sky that humans observe in a pattern and give a name. • People of ancient time saw the constellations as character or animals in the sky. They made up stories to explain how the object, animal, or character came into the night sky • Earth rotate ...
(AU): Average distance from Earth to Sun
... turn to gas when heated by the sun • Heating by sun forms a tail, which is blown away from sun by solar ...
... turn to gas when heated by the sun • Heating by sun forms a tail, which is blown away from sun by solar ...
Chapter 28 – Stars and Galaxies
... supernova blackhole or neutron star c. our sun will swell into a red giant, then its outer layers will get blown away and only an earth-sized fiery hot carbon-oxygen core will remain (white dwarf) D. Remnants of Massive Stars 1 Massive star goes supernova, the core that is left behind is so massiv ...
... supernova blackhole or neutron star c. our sun will swell into a red giant, then its outer layers will get blown away and only an earth-sized fiery hot carbon-oxygen core will remain (white dwarf) D. Remnants of Massive Stars 1 Massive star goes supernova, the core that is left behind is so massiv ...
NIE10x301Sponsor Thank You (Page 1)
... featureless balls of stars flattened to various degrees, but they cover an enormous range of sizes, from dwarfs to titanic giants formed from galaxy mergers with over a trillion stars! Galaxies are typically spread throughout the universe in groups and clusters. Our own neck of the woods in the cosm ...
... featureless balls of stars flattened to various degrees, but they cover an enormous range of sizes, from dwarfs to titanic giants formed from galaxy mergers with over a trillion stars! Galaxies are typically spread throughout the universe in groups and clusters. Our own neck of the woods in the cosm ...
December 1, 2011 - Perry Local Schools
... Sometimes the labels are a little different: The vertical position represents the star's luminosity. This could be the luminosity in watts. More commonly it is in units of the Sun's luminosity. In either case, a ``ratio scale'' is used. Absolute magnitude is also com ...
... Sometimes the labels are a little different: The vertical position represents the star's luminosity. This could be the luminosity in watts. More commonly it is in units of the Sun's luminosity. In either case, a ``ratio scale'' is used. Absolute magnitude is also com ...
Stars Powerpoint
... Just one teaspoon of a neutron star would have the mass of over 5 x 1012 kilograms. ...
... Just one teaspoon of a neutron star would have the mass of over 5 x 1012 kilograms. ...
Homework #3
... a) Assuming uniform density, how does the average density of a star vary with mass on the main sequence? If the mass is halved, does the density go up or down and by what factor? b) Assuming hydrostatic equilibrium continuing to assume constant density and the dominance of ideal gas pressure, how do ...
... a) Assuming uniform density, how does the average density of a star vary with mass on the main sequence? If the mass is halved, does the density go up or down and by what factor? b) Assuming hydrostatic equilibrium continuing to assume constant density and the dominance of ideal gas pressure, how do ...
StarType
... þ Lõõ °TÐÿÿÿÿÿÿÿÿ÷& à=Ð/Ð8Types of Stars When you look at the stars you’ll notice that some are white, some are yellow, and some are red. Stars are classified according to their colors, ranging from electric blue for the hottest stars to dull red for the coolest stars. Early spectrometers identified ...
... þ Lõõ °TÐÿÿÿÿÿÿÿÿ÷& à=Ð/Ð8Types of Stars When you look at the stars you’ll notice that some are white, some are yellow, and some are red. Stars are classified according to their colors, ranging from electric blue for the hottest stars to dull red for the coolest stars. Early spectrometers identified ...
Life in the Universe
... to considering extrasolar planets with habitable surfaces. So far all detected extrasolar planets (except maybe one or two) are gaseous giants and are unlikely to have surface life. ...
... to considering extrasolar planets with habitable surfaces. So far all detected extrasolar planets (except maybe one or two) are gaseous giants and are unlikely to have surface life. ...
How many planets are there in the galaxy?
... massive they are. In the case of the transit method, planets are detected when they pass directly in front of their star, causing it to dim. Here, size and mass are estimated based on the level of dimming. In the course of its mission, the Kepler mission has observed about 150,000 stars, which durin ...
... massive they are. In the case of the transit method, planets are detected when they pass directly in front of their star, causing it to dim. Here, size and mass are estimated based on the level of dimming. In the course of its mission, the Kepler mission has observed about 150,000 stars, which durin ...
Galactic Address/Stars/Constellations
... • Milky Way Galaxy • Local Group • Virgo Supercluster • Universe ...
... • Milky Way Galaxy • Local Group • Virgo Supercluster • Universe ...
The Hertzsprung-Russell Diagram
... sequence K5 stars radiate the same amount of energy from each square meter. So, in order for the K5 giant to be more luminous, it must have more square meters; i.e, it must have a larger surface area, thus a larger radius. 5. The B0 I star is farthest away, as it is the most luminous among the star ...
... sequence K5 stars radiate the same amount of energy from each square meter. So, in order for the K5 giant to be more luminous, it must have more square meters; i.e, it must have a larger surface area, thus a larger radius. 5. The B0 I star is farthest away, as it is the most luminous among the star ...
astronomy - sfox4science
... Our solar system is a just a small speck within the Milky Way Galaxy. The Milky Way Galaxy is a spiral galaxy. The Milky Way Galaxy has a diameter of about 100,000 light years, with the sun being located about 30,000 light-years from the center of the galaxy. 11. What type of galaxy is the Milky Wa ...
... Our solar system is a just a small speck within the Milky Way Galaxy. The Milky Way Galaxy is a spiral galaxy. The Milky Way Galaxy has a diameter of about 100,000 light years, with the sun being located about 30,000 light-years from the center of the galaxy. 11. What type of galaxy is the Milky Wa ...
Star Types
... sun, an O star, a white dwarf, or a red giant? Which of these star is the hottest? What are Sun-like stars (0.4 Msun < M < 8 Msun) in common? What about red dwarfs (0.08 Msun < M < 0.4 Msun) ? Where do stars spend most of their time? ...
... sun, an O star, a white dwarf, or a red giant? Which of these star is the hottest? What are Sun-like stars (0.4 Msun < M < 8 Msun) in common? What about red dwarfs (0.08 Msun < M < 0.4 Msun) ? Where do stars spend most of their time? ...