(HR) Diagrams
... show how a star such as the sun (a G2 star while it is on the main sequence) evolves through the following stages: a. protostar (which may have formed in a Bok globule) to main sequence star b. main sequence star to red giant to helium flash c. ejecting a planetary nebula (which exposes an interior ...
... show how a star such as the sun (a G2 star while it is on the main sequence) evolves through the following stages: a. protostar (which may have formed in a Bok globule) to main sequence star b. main sequence star to red giant to helium flash c. ejecting a planetary nebula (which exposes an interior ...
Homework #2
... How does that luminosity compare to the heat flux diffusing out from the interior of the hot core of the earth, 4.5 ×1020 erg s−1 ? 6) a) Star A and Star B both have the same luminosity. If Star A has a higher surface temperature than Star B, how do the radii of both stars compare to each other? No ...
... How does that luminosity compare to the heat flux diffusing out from the interior of the hot core of the earth, 4.5 ×1020 erg s−1 ? 6) a) Star A and Star B both have the same luminosity. If Star A has a higher surface temperature than Star B, how do the radii of both stars compare to each other? No ...
Finding Constellations From Orion
... The second constellation that El Nath belongs to is Taurus (TOR-us), the Bull. Taurus is easily located by following a line from Betelgeuse through Orion’s head. This takes you to the eye of the Bull, Aldebaran (al-DEB-a-ron), the 14th brightest star. The Hyades, a V-shaped cluster of bout 200 stars ...
... The second constellation that El Nath belongs to is Taurus (TOR-us), the Bull. Taurus is easily located by following a line from Betelgeuse through Orion’s head. This takes you to the eye of the Bull, Aldebaran (al-DEB-a-ron), the 14th brightest star. The Hyades, a V-shaped cluster of bout 200 stars ...
Astronomy.Practice.Quiz3
... 13. After the red giant phase, the next phase for a medium mass star is: a. nova b. planetary nebula c. white dwarf 14. This is how bright a star appears on Earth. a. apparent magnitude b. absolute magnitude ...
... 13. After the red giant phase, the next phase for a medium mass star is: a. nova b. planetary nebula c. white dwarf 14. This is how bright a star appears on Earth. a. apparent magnitude b. absolute magnitude ...
galaxies and stars - Valhalla High School
... universe formed in an enormous explosion about 10 to 15 billion years ago. • The universe has been expanding ever since. ...
... universe formed in an enormous explosion about 10 to 15 billion years ago. • The universe has been expanding ever since. ...
here - University of Toronto Astronomy
... pressure and magnetic support push outwards. The balance between pressure and gravity is called hydrostatic equilibrium. Wien’s Law: W= 0.00290/T, where W is the wavelength at which the maximum amount of radiation comes from a body of temperature T. The law has implications for the prediction of inf ...
... pressure and magnetic support push outwards. The balance between pressure and gravity is called hydrostatic equilibrium. Wien’s Law: W= 0.00290/T, where W is the wavelength at which the maximum amount of radiation comes from a body of temperature T. The law has implications for the prediction of inf ...
Section 25.2 Stellar Evolution
... remain in the stable main-sequence stage until they consume all their hydrogen fuel and collapse into a white dwarf. Death of Medium-Mass Stars Stars with masses similar to the sun evolve in essentially the same way as lowmass stars. During their collapse from red giants to white dwarfs, medium- ...
... remain in the stable main-sequence stage until they consume all their hydrogen fuel and collapse into a white dwarf. Death of Medium-Mass Stars Stars with masses similar to the sun evolve in essentially the same way as lowmass stars. During their collapse from red giants to white dwarfs, medium- ...
Reach_for_the_stars_final_questions.doc
... 1. What is the Sun’s spectral class? (1 pt) ________________________________________________________ 2. What is the Sun’s absolute magnitude? (1 pt) _________________________________________________ 3. At what distance are apparent and absolute magnitude the same? (1 pt) __________________ 4. What d ...
... 1. What is the Sun’s spectral class? (1 pt) ________________________________________________________ 2. What is the Sun’s absolute magnitude? (1 pt) _________________________________________________ 3. At what distance are apparent and absolute magnitude the same? (1 pt) __________________ 4. What d ...
Star - Uplift Education
... • If two stars have the same absolute magnitude but different apparent magnitude they would have the same brightness if they were both at distance of 10 pc from Earth, so we conclude they have the same luminosity, but are at different distances from Earth !!!!!!!!!!!!!! • Every one step in absolute ...
... • If two stars have the same absolute magnitude but different apparent magnitude they would have the same brightness if they were both at distance of 10 pc from Earth, so we conclude they have the same luminosity, but are at different distances from Earth !!!!!!!!!!!!!! • Every one step in absolute ...
The Sun and Stardust
... How are other elements made? Massive stars burn their hydrogen (and helium and carbon-nitrogen-oxygen) very quickly. At the end of their life heavier (metals) are formed such as vanadium, chromium, manganese, iron, cobalt, and nickel etc. Then massive stars (about ten times more massive than the Su ...
... How are other elements made? Massive stars burn their hydrogen (and helium and carbon-nitrogen-oxygen) very quickly. At the end of their life heavier (metals) are formed such as vanadium, chromium, manganese, iron, cobalt, and nickel etc. Then massive stars (about ten times more massive than the Su ...
The “Big Bang” Theory
... • Matter started to “clump” back together • This was due to gravity • The galaxies, stars and planets formed from these clumps of dust and gas • There are billions of galaxies in the universe and each galaxy consists of billions of stars ...
... • Matter started to “clump” back together • This was due to gravity • The galaxies, stars and planets formed from these clumps of dust and gas • There are billions of galaxies in the universe and each galaxy consists of billions of stars ...
Astronomy Universe2
... What is a Main Sequence Star? • The H-R diagram represents a pattern that was discovered that allows stars to be compared by brightness and color. • The majority of stars are found in a band stretching diagonally across the diagram called the “Main Sequence”. • Stars start out in the Main Sequence ...
... What is a Main Sequence Star? • The H-R diagram represents a pattern that was discovered that allows stars to be compared by brightness and color. • The majority of stars are found in a band stretching diagonally across the diagram called the “Main Sequence”. • Stars start out in the Main Sequence ...
ASTRONOMY WEBQUEST…… EXPLORE THE UNIVERSE
... Universe - http://starchild.gsfc.nasa.gov/docs/StarChild/universe_level2/universe.html Using the website find the following box and Click on the topics to find your answers: The Milky Way ...
... Universe - http://starchild.gsfc.nasa.gov/docs/StarChild/universe_level2/universe.html Using the website find the following box and Click on the topics to find your answers: The Milky Way ...
Measuring stars Part I
... If p is in arcsec and d is in parsecs A star with a parallax of 1 arcsec is 1 parsec distant ...
... If p is in arcsec and d is in parsecs A star with a parallax of 1 arcsec is 1 parsec distant ...
Pretest
... measures how far light travels through space in one year. 12. The distance that a star so far away would appear to move when seen from opposite sides of Earth’s orbit would be too small to measure accurately. 13. A star is born when nuclear fusion begins. 14. Most star formation takes place in the s ...
... measures how far light travels through space in one year. 12. The distance that a star so far away would appear to move when seen from opposite sides of Earth’s orbit would be too small to measure accurately. 13. A star is born when nuclear fusion begins. 14. Most star formation takes place in the s ...
Earth Science – Quiz 2
... a. that stars are stationary. b. the apparent displacement of background stars as the earth orbits the sun. c. our solar system location in the Milky Way. d. that most stars belong to the main sequence group of stars. 4. Which of the following astronomers invented and used the telescope to view the ...
... a. that stars are stationary. b. the apparent displacement of background stars as the earth orbits the sun. c. our solar system location in the Milky Way. d. that most stars belong to the main sequence group of stars. 4. Which of the following astronomers invented and used the telescope to view the ...
Binary Star Systems Discussion Points 1. What characteristic of a
... 19. The V809 Cyg pair takes 213 years to orbit one another. The V986 Sgr pair orbits one another in only 10.3 days. What does this mean about the distances between the stars within each pair? ...
... 19. The V809 Cyg pair takes 213 years to orbit one another. The V986 Sgr pair orbits one another in only 10.3 days. What does this mean about the distances between the stars within each pair? ...
Lives of stars
... initiate a second stage of thermonuclear fusion 19-4 How H-R diagrams for star clusters reveal the later stages in the evolution of stars 19-5 The two kinds of stellar populations and their significance ...
... initiate a second stage of thermonuclear fusion 19-4 How H-R diagrams for star clusters reveal the later stages in the evolution of stars 19-5 The two kinds of stellar populations and their significance ...
Life Cycle of a Star
... Step Five Stars bigger than our sun will collapse so quickly they explode into a __________________. The core that is leftover after a supernova may form a ______________ star. If the leftover core was above a certain mass, it will continue to collapse in on itself and form a _______ _________. Its ...
... Step Five Stars bigger than our sun will collapse so quickly they explode into a __________________. The core that is leftover after a supernova may form a ______________ star. If the leftover core was above a certain mass, it will continue to collapse in on itself and form a _______ _________. Its ...
HR Diagram - Geneva 304
... a. optical doubles b. double star / binary star c. spectroscopic binary 43. How could you recognize an eclipsing binary? 44. About what percent of all stars are members of a double star system? 45. What is a variable star? 46. Of what spectral type are Mira variables, and how big are they relative t ...
... a. optical doubles b. double star / binary star c. spectroscopic binary 43. How could you recognize an eclipsing binary? 44. About what percent of all stars are members of a double star system? 45. What is a variable star? 46. Of what spectral type are Mira variables, and how big are they relative t ...
How to Find the North Star ppt
... Dipper as shown, toward the Little Dipper. The North Star is located at the end of the handle of the Little Dipper. The Polestar is the brightest of the Little Dipper stars. ...
... Dipper as shown, toward the Little Dipper. The North Star is located at the end of the handle of the Little Dipper. The Polestar is the brightest of the Little Dipper stars. ...
il 3 ~ )
... (c) Estimate the surface area of your body (in m2). You are welcome to make any reasonable assumptions and approximations, but be sure to state what they are! (d) Assuming your body radiates like a blackbody (OK within a factor of 2-3), estjmate the total power L radiated by your body in Watts. How ...
... (c) Estimate the surface area of your body (in m2). You are welcome to make any reasonable assumptions and approximations, but be sure to state what they are! (d) Assuming your body radiates like a blackbody (OK within a factor of 2-3), estjmate the total power L radiated by your body in Watts. How ...
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.