22 Stellar Remnant/HR Diagram
... Star Clusters All stars formed at the same time Match the shape of the main sequence Compare age to MS lifetime Gives spectral type of MS “turnoff” stars Spectral type gives absolute magnitude! Yields a distance! ...
... Star Clusters All stars formed at the same time Match the shape of the main sequence Compare age to MS lifetime Gives spectral type of MS “turnoff” stars Spectral type gives absolute magnitude! Yields a distance! ...
AST 207 Test 2 Answers 20 October 2010
... star A. Prof. Adams says he discovered a new type of star that is fainter than white dwarfs. Has he discovered a new type of star? Explain. The clues are very much like Walter Adams’ discovery that Sirius B is a white dwarf. However, there is a crucial missing clue. Since Sirius A and B were known t ...
... star A. Prof. Adams says he discovered a new type of star that is fainter than white dwarfs. Has he discovered a new type of star? Explain. The clues are very much like Walter Adams’ discovery that Sirius B is a white dwarf. However, there is a crucial missing clue. Since Sirius A and B were known t ...
Which property of a star would not change if we could observe it
... A cool star that is very luminous must have : a) A small radius b) A large radius c) A small mass d) A great distance e) A low velocity ...
... A cool star that is very luminous must have : a) A small radius b) A large radius c) A small mass d) A great distance e) A low velocity ...
Life Cycles of Stars
... • Remaining core of a supergiant that was more than 40 times the size of our Sun • The core of the supergiant, after a supernova, is so dense that its gravitational pull sucks in space, time, light and matter • Thought to be at the centre of all galaxies ...
... • Remaining core of a supergiant that was more than 40 times the size of our Sun • The core of the supergiant, after a supernova, is so dense that its gravitational pull sucks in space, time, light and matter • Thought to be at the centre of all galaxies ...
H-R Diagram - Faculty Website Listing
... Please read the section in textbook that talks about HR diagram. We have also discussed this in class with examples. It may be useful to have your class notes with you when you do the lab. You can also look them up on the class webpage. 1. Using Stellarium software to collect the information on abso ...
... Please read the section in textbook that talks about HR diagram. We have also discussed this in class with examples. It may be useful to have your class notes with you when you do the lab. You can also look them up on the class webpage. 1. Using Stellarium software to collect the information on abso ...
Stellar Evolution
... We do not know that all stars, regardless of their size, eventually run out of fuel and collapse due to gravity Low Mass Stars – consume fuel at a slow rate, may remain on main-sequence for up to 100 billion years, end up collapsing into white dwarfs Medium Mass Stars – go into red-giant stage, foll ...
... We do not know that all stars, regardless of their size, eventually run out of fuel and collapse due to gravity Low Mass Stars – consume fuel at a slow rate, may remain on main-sequence for up to 100 billion years, end up collapsing into white dwarfs Medium Mass Stars – go into red-giant stage, foll ...
Star Life Cycles
... After becoming a planetary nebula, the remains of the core of the star become a white dwarf. A white dwarf is a star that has exhausted most or all of its nuclear fuel and has collapsed to a very small size; such a star is near its final stage of life. White dwarfs eventually become black dwarfs ...
... After becoming a planetary nebula, the remains of the core of the star become a white dwarf. A white dwarf is a star that has exhausted most or all of its nuclear fuel and has collapsed to a very small size; such a star is near its final stage of life. White dwarfs eventually become black dwarfs ...
Document
... observer; Red and blue shifts- Doppler Effect the study of the origin, structure, evolution of the universe- Cosmology galaxy elongated oval in shape- Elliptical Galaxy galaxy of no particular shape, rich in dust and gas- Irregular galaxy a large explosion which causes a star to become suddenly brig ...
... observer; Red and blue shifts- Doppler Effect the study of the origin, structure, evolution of the universe- Cosmology galaxy elongated oval in shape- Elliptical Galaxy galaxy of no particular shape, rich in dust and gas- Irregular galaxy a large explosion which causes a star to become suddenly brig ...
Parallax - High Point University
... • Early evidence that Einstein was right was the observation that light from a star was bent as it passed near the Sun (this could only be seen during a total solar eclipse of course) ...
... • Early evidence that Einstein was right was the observation that light from a star was bent as it passed near the Sun (this could only be seen during a total solar eclipse of course) ...
Ch.10 Stellar old age
... Core of helium is supported by electron degeneracy pressure When He ‘ignites’, whole core is ready to fuse He into C ...
... Core of helium is supported by electron degeneracy pressure When He ‘ignites’, whole core is ready to fuse He into C ...
TU Muscae and the Early-type Overcontact Binaries
... Binary orbital plane is oriented so that the two stars pass in front of one another as seen from Earth. The light curve is rich in information about the two stars. ...
... Binary orbital plane is oriented so that the two stars pass in front of one another as seen from Earth. The light curve is rich in information about the two stars. ...
1. Compute the deflection angle of a star whose light... limb of the Sun. Also compute the deflection angle of...
... 1. Compute the deflection angle of a star whose light just grazes the limb of the Sun. Also compute the deflection angle of a star whose light just grazes the limb of a 1.4M neutron star, if the neutron star was at the same distance from the Earth as the Sun. State assumptions. 2. Use the Plummer p ...
... 1. Compute the deflection angle of a star whose light just grazes the limb of the Sun. Also compute the deflection angle of a star whose light just grazes the limb of a 1.4M neutron star, if the neutron star was at the same distance from the Earth as the Sun. State assumptions. 2. Use the Plummer p ...
Lecture 5: Light as a tool
... 1) Why does our sky appear to be mostly blue, and not violet, at mid-day? 2) What color would our sky be if atmospheric particles were slightly larger? 3) Why is the sky black on the moon? ...
... 1) Why does our sky appear to be mostly blue, and not violet, at mid-day? 2) What color would our sky be if atmospheric particles were slightly larger? 3) Why is the sky black on the moon? ...
Stars - Independence High School
... • Seasonal- Orbit equator and can only be seen during certain times of the year ...
... • Seasonal- Orbit equator and can only be seen during certain times of the year ...
solution
... apparent magnitude of 13.25. Which star appears brighter? From this information alone, what can you conclude about the luminosities of these stars? Explain your answer. Zubenelgenubi appears to be brighter, since it has a lower apparent magnitude (remember that a negative apparent magnitude is very ...
... apparent magnitude of 13.25. Which star appears brighter? From this information alone, what can you conclude about the luminosities of these stars? Explain your answer. Zubenelgenubi appears to be brighter, since it has a lower apparent magnitude (remember that a negative apparent magnitude is very ...
1 Ay 124 Winter 2014 – HOMEWORK #2 Problem 1
... Due Friday, Jan 31, 2014 by 5pm, in Steidel’s mailbox in 249 Cahill ...
... Due Friday, Jan 31, 2014 by 5pm, in Steidel’s mailbox in 249 Cahill ...
Star Sizes
... Sirius is the brightest star in our night sky. The reason for this is that it is relatively close at only 8.6 light years away. Remember the next nearest star is 4.3 light years away. Sirius is about twice as massive as the Sun but it is 25 times as luminous. It can be found in the constellation Ca ...
... Sirius is the brightest star in our night sky. The reason for this is that it is relatively close at only 8.6 light years away. Remember the next nearest star is 4.3 light years away. Sirius is about twice as massive as the Sun but it is 25 times as luminous. It can be found in the constellation Ca ...
Corona Australis
Corona Australis /kɵˈroʊnə ɒˈstreɪlɨs/ or Corona Austrina /kɵˈroʊnə ɒˈstraɪnə/ is a constellation in the Southern Celestial Hemisphere. Its Latin name means ""southern crown"", and it is the southern counterpart of Corona Borealis, the northern crown. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations. The Ancient Greeks saw Corona Australis as a wreath rather than a crown and associated it with Sagittarius or Centaurus. Other cultures have likened the pattern to a turtle, ostrich nest, a tent, or even a hut belonging to a rock hyrax.Although fainter than its namesake, the oval- or horseshoe-shaped pattern of its brighter stars renders it distinctive. Alpha and Beta Coronae Australis are the two brightest stars with an apparent magnitude of around 4.1. Epsilon Coronae Australis is the brightest example of a W Ursae Majoris variable in the southern sky. Lying alongside the Milky Way, Corona Australis contains one of the closest star-forming regions to our Solar System—a dusty dark nebula known as the Corona Australis Molecular Cloud, lying about 430 light years away. Within it are stars at the earliest stages of their lifespan. The variable stars R and TY Coronae Australis light up parts of the nebula, which varies in brightness accordingly.