Name - MIT
									
... A) The rate that visible light from the Sun is being absorbed by the Earth’s atmosphere B) The rate that hydrogen is being fused into helium in the Sun C) The rate that gamma rays are hitting the Earth’s atmosphere D) The rate that white dwarfs are being formed in the galaxy E) The rate that stars f ...
                        	... A) The rate that visible light from the Sun is being absorbed by the Earth’s atmosphere B) The rate that hydrogen is being fused into helium in the Sun C) The rate that gamma rays are hitting the Earth’s atmosphere D) The rate that white dwarfs are being formed in the galaxy E) The rate that stars f ...
									Name
									
... A) The rate that visible light from the Sun is being absorbed by the Earth’s atmosphere B) The rate that hydrogen is being fused into helium in the Sun C) The rate that gamma rays are hitting the Earth’s atmosphere D) The rate that white dwarfs are being formed in the galaxy E) The rate that stars f ...
                        	... A) The rate that visible light from the Sun is being absorbed by the Earth’s atmosphere B) The rate that hydrogen is being fused into helium in the Sun C) The rate that gamma rays are hitting the Earth’s atmosphere D) The rate that white dwarfs are being formed in the galaxy E) The rate that stars f ...
									Name - MIT
									
... A) The rate that visible light from the Sun is being absorbed by the Earth’s atmosphere B) The rate that hydrogen is being fused into helium in the Sun C) The rate that gamma rays are hitting the Earth’s atmosphere D) The rate that white dwarfs are being formed in the galaxy E) The rate that stars f ...
                        	... A) The rate that visible light from the Sun is being absorbed by the Earth’s atmosphere B) The rate that hydrogen is being fused into helium in the Sun C) The rate that gamma rays are hitting the Earth’s atmosphere D) The rate that white dwarfs are being formed in the galaxy E) The rate that stars f ...
									Stellar Evolution
									
... around a white dwarf heats up to ~ 1 million oK, in which wavelength band do you expect that it radiates the most strongly? ...
                        	... around a white dwarf heats up to ~ 1 million oK, in which wavelength band do you expect that it radiates the most strongly? ...
									ppt
									
... Therefore stars have an extremely large gravitational attraction that keeps their plasma held together. As gravity acts equally in all directions the plasma that forms the star is moulded into a sphere. But there must be some force keeping the star from collapsing in on itself. Because stars are so ...
                        	... Therefore stars have an extremely large gravitational attraction that keeps their plasma held together. As gravity acts equally in all directions the plasma that forms the star is moulded into a sphere. But there must be some force keeping the star from collapsing in on itself. Because stars are so ...
									15 - Edmodo
									
... The purpose of this activity will be to use the star chart (Page 551 of your textbook) to determine the location and appearance of well known stars, constellations, and asterisms visible in the ...
                        	... The purpose of this activity will be to use the star chart (Page 551 of your textbook) to determine the location and appearance of well known stars, constellations, and asterisms visible in the ...
									Name
									
... C) The rate that hydrogen is being fused into helium in the Sun D) The rate that white dwarfs are being formed in the galaxy E) The rate that stars form in the galaxy 10) A K5 star and a B2 star both have an apparent magnitude of +0.5 in the visible wavelength region. Both stars are 144 light years ...
                        	... C) The rate that hydrogen is being fused into helium in the Sun D) The rate that white dwarfs are being formed in the galaxy E) The rate that stars form in the galaxy 10) A K5 star and a B2 star both have an apparent magnitude of +0.5 in the visible wavelength region. Both stars are 144 light years ...
									PDF - Interactive Stars
									
... May 16th to May 31 If you were born between these dates, your guiding star is Mirfak, a yellow supergiant, marking the hero's side. It is said to give courage and success through perseverance. Nearby, lies Algol, the Demon Star that marks the head of the petrifying gorgon that Perseus overcame. The ...
                        	... May 16th to May 31 If you were born between these dates, your guiding star is Mirfak, a yellow supergiant, marking the hero's side. It is said to give courage and success through perseverance. Nearby, lies Algol, the Demon Star that marks the head of the petrifying gorgon that Perseus overcame. The ...
									Galaxy Far Far Away ppt
									
... Nucleus is the most mysterious part Evidence of a Supermassive Black Hole in Saggitarius: ...
                        	... Nucleus is the most mysterious part Evidence of a Supermassive Black Hole in Saggitarius: ...
									The Heliocentric Model of the Solar System
									
... • Just one of eight planets circling around the Sun who, in turn , is located in one arm of our galaxy and rotates around the galactic center • Our Sun is one (the closest to us) of about 200 Billion (200.000.000.000) Stars that make up our Galaxy, the Milky Way • The Sun is about 100 times large ...
                        	... • Just one of eight planets circling around the Sun who, in turn , is located in one arm of our galaxy and rotates around the galactic center • Our Sun is one (the closest to us) of about 200 Billion (200.000.000.000) Stars that make up our Galaxy, the Milky Way • The Sun is about 100 times large ...
									Lecture Summary (11/22)
									
... The electrons and protons are forced together by gravity giving neutrons. Meanwhile the outer regions of the star fall in as well, encounter this dense rigid core and recoil outward with tremendous release of energy the supernova explosion. The radio waves of pulsars are produced by fast moving elec ...
                        	... The electrons and protons are forced together by gravity giving neutrons. Meanwhile the outer regions of the star fall in as well, encounter this dense rigid core and recoil outward with tremendous release of energy the supernova explosion. The radio waves of pulsars are produced by fast moving elec ...
									Page 1 of 4 Name PSCI 1055 Test #4 (Form B) Spring 2008 Buckley
									
... brightness on the H-R diagram? ...
                        	... brightness on the H-R diagram? ...
									(HR) Diagrams
									
... Absolute visual magnitude relates to how bright the star really is, not just how bright it appears to be as seen from Earth. Remember that the SMALLER the MV number, the MORE LUMINOUS the star is, in absolute terms. A star with MV = –5.0 is MUCH more luminous than an MV = 1.0 star. To put it another ...
                        	... Absolute visual magnitude relates to how bright the star really is, not just how bright it appears to be as seen from Earth. Remember that the SMALLER the MV number, the MORE LUMINOUS the star is, in absolute terms. A star with MV = –5.0 is MUCH more luminous than an MV = 1.0 star. To put it another ...
									Quiz Chapter 10 Answers
									
... Quiz Chapter 10 Answers 10-1. Protostars are not seen in visible light telescopes because: a) they don’t emit any radiation b) they are surrounded by clouds of gas and dust X c) they only emit infrared radiation d) they are all moving away from Earth so fast that their visible light is Doppler shift ...
                        	... Quiz Chapter 10 Answers 10-1. Protostars are not seen in visible light telescopes because: a) they don’t emit any radiation b) they are surrounded by clouds of gas and dust X c) they only emit infrared radiation d) they are all moving away from Earth so fast that their visible light is Doppler shift ...
									Stars - Trimble County Schools
									
... • Apparent shift in position caused by motion of observer • Change in position of Earth as it orbits – Closer stars have larger change in parallax – Farther stars have smaller change in parallax ...
                        	... • Apparent shift in position caused by motion of observer • Change in position of Earth as it orbits – Closer stars have larger change in parallax – Farther stars have smaller change in parallax ...
									Study Guide for 3RD Astronomy Exam
									
... Solve problems relating to the relative brightness or luminosity of two stars given their m or M values. Determine the hottest and coolest stars from a list of stars with their spectral types. Interpret the luminosity class of a star by naming the luminosity class and identifying if the star is in t ...
                        	... Solve problems relating to the relative brightness or luminosity of two stars given their m or M values. Determine the hottest and coolest stars from a list of stars with their spectral types. Interpret the luminosity class of a star by naming the luminosity class and identifying if the star is in t ...
									File - Awakening in Grade 6
									
...  What is the Zodiac? Earth orbits our Sun once each year. Viewed from Earth, our Sun appears to trace a circular path. This path defines a plane called the plane of the ecliptic (or just the ecliptic). The zodiac is the group (or “belt”) of constellations that fall along the plane of the ecliptic. ...
                        	...  What is the Zodiac? Earth orbits our Sun once each year. Viewed from Earth, our Sun appears to trace a circular path. This path defines a plane called the plane of the ecliptic (or just the ecliptic). The zodiac is the group (or “belt”) of constellations that fall along the plane of the ecliptic. ...
									February 16
									
... Discussion But, what if there is a lot of dust between us and the object we are observing. That would make the object appear fainter and we would be misled into thinking the object was much farther away than it really is. How can astronomers determine if dust is making things fainter? ...
                        	... Discussion But, what if there is a lot of dust between us and the object we are observing. That would make the object appear fainter and we would be misled into thinking the object was much farther away than it really is. How can astronomers determine if dust is making things fainter? ...
									Death of massive stars
									
... known in the Western tradition as Taurus the Bull. – The star quickly became so bright that it was visible in the daytime. – After a month, it slowly faded, taking almost two years to vanish from sight. ...
                        	... known in the Western tradition as Taurus the Bull. – The star quickly became so bright that it was visible in the daytime. – After a month, it slowly faded, taking almost two years to vanish from sight. ...
									Galaxy
									
... star it is called an eclipsing star  Astronomers know there are actually 2 stars by looking at the effects of gravity  Our solar system is not the only solar system with planets revolving around a star  In 2000, astronomers discovered a solar system about 10.5 light-years away with planets simila ...
                        	... star it is called an eclipsing star  Astronomers know there are actually 2 stars by looking at the effects of gravity  Our solar system is not the only solar system with planets revolving around a star  In 2000, astronomers discovered a solar system about 10.5 light-years away with planets simila ...
									The Sun and Beyond - Valhalla High School
									
...  Science tries to answer them all  What is the fate of our universe? Will it continue to expand or undergo the Big ...
                        	...  Science tries to answer them all  What is the fate of our universe? Will it continue to expand or undergo the Big ...
Perseus (constellation)
                        Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.