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Life Cycle of a Star worksheet
... _____ The star begins to run out of fuel and expands into a red giant or red super giant. _____ Stars start out as diffused clouds of gas and dust drifting through space. A single one of these clouds is called a nebula _____ What happens next depends on the mass of the star. _____ Heat and pressure ...
... _____ The star begins to run out of fuel and expands into a red giant or red super giant. _____ Stars start out as diffused clouds of gas and dust drifting through space. A single one of these clouds is called a nebula _____ What happens next depends on the mass of the star. _____ Heat and pressure ...
31-2 - Fremont Peak Observatory
... a last attempt to balance gravity and nuclear fusion. For a time this works, but eventually the outer layers become detached and drift away. The remainder then collapses into a white dwarf. Planetary nebula are rich in Oxygen and Carbon since these elements are created in the end stages of the life ...
... a last attempt to balance gravity and nuclear fusion. For a time this works, but eventually the outer layers become detached and drift away. The remainder then collapses into a white dwarf. Planetary nebula are rich in Oxygen and Carbon since these elements are created in the end stages of the life ...
life cycle of stars notes
... Then the HELIUM RUNS OUT – Take 2 Core collapses again – becomes hotter & denser ...
... Then the HELIUM RUNS OUT – Take 2 Core collapses again – becomes hotter & denser ...
Pretty Pictures of the Cosmos
... planetary nebula, the gases of which composed the outer layers of a Sun-like star only 10,000 years ago. The inner filaments visible are being ejected by strong wind of particles from the central star. The outer disk contains unusual light-year long orange filaments. The Eskimo Nebula lies about 500 ...
... planetary nebula, the gases of which composed the outer layers of a Sun-like star only 10,000 years ago. The inner filaments visible are being ejected by strong wind of particles from the central star. The outer disk contains unusual light-year long orange filaments. The Eskimo Nebula lies about 500 ...
Document
... flood of ultraviolet light emitted by four bright stars, collectively called the Trapezium. ...
... flood of ultraviolet light emitted by four bright stars, collectively called the Trapezium. ...
The Superhero's Universe: Observing the Cosmos with X-ray Vision and Beyond
... Do You See What I See? Crab Nebula ...
... Do You See What I See? Crab Nebula ...
main sequence star
... • Small mass stars will collapse into white dwarfs after being red giants. • The outer gases are lost, which allows us to see the core of the star. The white dwarf is very dense and hot. The emit (release) less light than they did when they were stars. • As these white dwarfs cool they become fainte ...
... • Small mass stars will collapse into white dwarfs after being red giants. • The outer gases are lost, which allows us to see the core of the star. The white dwarf is very dense and hot. The emit (release) less light than they did when they were stars. • As these white dwarfs cool they become fainte ...
Astro vol.6 issue 1 - Global Friendship Through Space Education
... Nebula is a Latin word. It means a cloud between stars formed by dust, hydrogen, helium and other gasses. This particular nebula is located in the Monoceros constellation. It was discovered on December 26, 1785 by William Herschel, a German-born British astronomer (1738 – 1822). The Cone Nebula is s ...
... Nebula is a Latin word. It means a cloud between stars formed by dust, hydrogen, helium and other gasses. This particular nebula is located in the Monoceros constellation. It was discovered on December 26, 1785 by William Herschel, a German-born British astronomer (1738 – 1822). The Cone Nebula is s ...
RFS_multiple_choice_Dec8_Key
... hence occulted by the moon at some time or the other. D. All of them lie in the Milky Way band of the sky (the galactic equator) 3. On July 4, 1054, Chinese astronomers (and possibly Native Americans) recorded a supernova explosion taking place in the constellation Taurusso bright that it was even v ...
... hence occulted by the moon at some time or the other. D. All of them lie in the Milky Way band of the sky (the galactic equator) 3. On July 4, 1054, Chinese astronomers (and possibly Native Americans) recorded a supernova explosion taking place in the constellation Taurusso bright that it was even v ...
The solar system
... the extra material was being pulled towards the center. • The temperature at the center became so great that nuclear fusion occurred. • The explosion created a new star (our sun) which swept away all of the left over material that was in the solar nebula ...
... the extra material was being pulled towards the center. • The temperature at the center became so great that nuclear fusion occurred. • The explosion created a new star (our sun) which swept away all of the left over material that was in the solar nebula ...
The HR Diagram and Stars Worksheet
... 2. Use your book to add the following information to the H-R diagram. a. Page 622 – Add the Spectral Class below the temperatures. b. Page 626 – Use colored pencils to add and label the band that represents Main Sequence stars. c. Page 626 – Use colored pencils to label the following areas: Blue Gia ...
... 2. Use your book to add the following information to the H-R diagram. a. Page 622 – Add the Spectral Class below the temperatures. b. Page 626 – Use colored pencils to add and label the band that represents Main Sequence stars. c. Page 626 – Use colored pencils to label the following areas: Blue Gia ...
Star Life Cycle - GSHS Mrs. Francomb
... Pumbaa: Oh. Gee. I always thought that they were balls of gas burning billions of miles away. Timon: Pumbaa, wit' you, everything's gas. ...
... Pumbaa: Oh. Gee. I always thought that they were balls of gas burning billions of miles away. Timon: Pumbaa, wit' you, everything's gas. ...
THE LIFE CYCLE OF A STAR
... This is the explosive death of a star, and often results in the star obtaining the brightness of 100 million suns for a short time. There are two general types of Supernova:Type I - These occur in binary star systems in which gas from one star falls on to a white dwarf, causing it to explode. Type I ...
... This is the explosive death of a star, and often results in the star obtaining the brightness of 100 million suns for a short time. There are two general types of Supernova:Type I - These occur in binary star systems in which gas from one star falls on to a white dwarf, causing it to explode. Type I ...
20.1 A Solar System is Born
... 3. Planetesimals begin to form within the swirling disk. 4. As the largest planetesimals grown in size, their gravity attracts more gas and dust. 5. Smaller planetesimals collide with the larger ones, and planets begin to grow 6. A star is born, and the remaining gas and dust are blown out of the ne ...
... 3. Planetesimals begin to form within the swirling disk. 4. As the largest planetesimals grown in size, their gravity attracts more gas and dust. 5. Smaller planetesimals collide with the larger ones, and planets begin to grow 6. A star is born, and the remaining gas and dust are blown out of the ne ...
proposed october viewing list
... OBJECT DESCRIPTIONS M11 Known as the Wild Duck cluster, this open cluster in the constellation Scutum, (SKEW-tum) is seen best with the 4” refractor at low magnification. It contains more than 2900 stars and is estimated to be about 250 million years old. M11 is receding from us at a speed of 27 km ...
... OBJECT DESCRIPTIONS M11 Known as the Wild Duck cluster, this open cluster in the constellation Scutum, (SKEW-tum) is seen best with the 4” refractor at low magnification. It contains more than 2900 stars and is estimated to be about 250 million years old. M11 is receding from us at a speed of 27 km ...
bYTEBoss lesson 3 life of star
... The end of the life cycle of really massive stars is different to that of massive stars. After a really massive red giant collapses in a supernova explosion, it leaves a star so dense that not even light can escape its gravitational pull. This is called a black hole! Some scientists believe that the ...
... The end of the life cycle of really massive stars is different to that of massive stars. After a really massive red giant collapses in a supernova explosion, it leaves a star so dense that not even light can escape its gravitational pull. This is called a black hole! Some scientists believe that the ...
Slide 1
... No matter the size of the star or whether it dies quietly or in a supernova, all stars will form a planetary nebula. The nebula is made out of the gases that got blown from the star. It may look like it expands slowly, but these gases move out at an average of 30 miles/second. Most of this is hydrog ...
... No matter the size of the star or whether it dies quietly or in a supernova, all stars will form a planetary nebula. The nebula is made out of the gases that got blown from the star. It may look like it expands slowly, but these gases move out at an average of 30 miles/second. Most of this is hydrog ...
Stars - Mc Guckin Science
... – Smaller stars will live on for billions of years because they burn their fuel much more slowly ...
... – Smaller stars will live on for billions of years because they burn their fuel much more slowly ...
The Pulsar “Lighthouse”
... • Outer layers of star gradually contract onto core which becomes too massive to be held up by degenerate electron pressure • e- + p Î n • Sudden core collapse: 104 km Î 20 km • Then core rebounds • Outer layers fall in, then get hit by rebounding core. ...
... • Outer layers of star gradually contract onto core which becomes too massive to be held up by degenerate electron pressure • e- + p Î n • Sudden core collapse: 104 km Î 20 km • Then core rebounds • Outer layers fall in, then get hit by rebounding core. ...
ES High mass star life cycle plus black holes
... What is the life cycle of a low mass star (5 stages)? What is the life cycle of a high mass star? What is the heaviest element forms in the center of a high mass star? Why is supernova crucial to our existence? Where is calcium formed in the life a high mass star? What is a supernova? What are the 2 ...
... What is the life cycle of a low mass star (5 stages)? What is the life cycle of a high mass star? What is the heaviest element forms in the center of a high mass star? Why is supernova crucial to our existence? Where is calcium formed in the life a high mass star? What is a supernova? What are the 2 ...
Crab Nebula
![](https://en.wikipedia.org/wiki/Special:FilePath/Crab_Nebula.jpg?width=300)
The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus. It is not, as its name might suggest, in Cancer. The now-current name is due to William Parsons, 3rd Earl of Rosse, who observed the object in 1840 using a 36-inch telescope and produced a drawing that looked somewhat like a crab. Corresponding to a bright supernova recorded by Chinese astronomers in 1054, the nebula was observed later by English astronomer John Bevis in 1731. The nebula was the first astronomical object identified with a historical supernova explosion.At an apparent magnitude of 8.4, comparable to that of Saturn's moon Titan, it is not visible to the naked eye but can be made out using binoculars under favourable conditions. The nebula lies in the Perseus Arm of the Milky Way galaxy, at a distance of about 2.0 kiloparsecs (6,500 ly) from Earth. It has a diameter of 3.4 parsecs (11 ly), corresponding to an apparent diameter of some 7 arcminutes, and is expanding at a rate of about 1,500 kilometres per second (930 mi/s), or 0.5% c.At the center of the nebula lies the Crab Pulsar, a neutron star 28–30 kilometres (17–19 mi) across with a spin rate of 30.2 times per second, which emits pulses of radiation from gamma rays to radio waves. At X-ray and gamma ray energies above 30 keV, the Crab is generally the strongest persistent source in the sky, with measured flux extending to above 10 TeV. The nebula's radiation allows for the detailed studying of celestial bodies that occult it. In the 1950s and 1960s, the Sun's corona was mapped from observations of the Crab's radio waves passing through it, and in 2003, the thickness of the atmosphere of Saturn's moon Titan was measured as it blocked out X-rays from the nebula.