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Charles Hakes Fort Lewis College 1 Charles Hakes Fort Lewis College 2 “Dead” Stars Charles Hakes Fort Lewis College 3 Outline • Test 3 Wednesday • Dead (?) Stars • Review (?) Charles Hakes Fort Lewis College 4 Test 3 • Review Spectroscopy (Wein, Stefan) and Doppler Shift • The Sun (structure, fusion) • Magnitude • Parallax • Interstellar Medium • Stellar Evolution • Dead Stars Charles Hakes Fort Lewis College 5 More Precisely 12-1 The Cycle of Stellar Evolution Charles Hakes Fort Lewis College 6 Supernovae • On-line images • Supernova in M 74 http://www.rochesterastronomy.org/sn2003/n628s2.jpg • Supernova in NGC 1448 http://members.optushome.com.au/edobosz/images/1448_sn.jpg • Supernova in NGC 3169 http://www.astrooptik.com/Bildergalerie/PolluxGallery/NGC3169.htm • Supernova in NGC 3190 • • http://www.astrooptik.com/Bildergalerie/PolluxGallery/NGC3190.htm Supernova in NGC 5965 http://www.nordita.dk/~dahle/ngc5965_sub.gif Supernova in NGC 918 http://antwrp.gsfc.nasa.gov/apod/ap091112.html Charles Hakes Fort Lewis College 7 Chapter 13 • What is left after a Supernova? Charles Hakes Fort Lewis College 8 Figure 12.21 Supernova Remnants Charles Hakes Fort Lewis College 9 Figure 13.1 Neutron Star - from a type II Supernova • typically ~20 km diameter • mass > Msun • thimbleful would weigh 108 tons • rotate very quickly • have very strong magnetic fields. Charles Hakes Fort Lewis College 10 Figure 13.2 Pulsar Radiation • The first observed neutron star was a pulsar • Neutron stars rotate VERY quickly. Charles Hakes Fort Lewis College 11 Figure 13.3 Pulsar Model Charles Hakes Fort Lewis College 12 lighthouse model - if the beam sweeps past the Earth, we see a pulse. At a distance of 1 A.U., which would have the greatest gravitational force? A) A 1 solar mass main sequence star B) A 1 solar mass white dwarf C) A 1 solar mass neutron star D) They all have the same force. Charles Hakes Fort Lewis College 13 At a distance of 1 A.U., which would have the greatest gravitational force? A) A 1 solar mass main sequence star B) A 1 solar mass white dwarf C) A 1 solar mass neutron star D) They all have the same force. Charles Hakes Fort Lewis College 14 At the surface of the object, which would have the greatest gravitational force? A) A 1 solar mass main sequence star B) A 1 solar mass white dwarf C) A 1 solar mass neutron star D) They all have the same force. Charles Hakes Fort Lewis College 15 At the surface of the object, which would have the greatest gravitational force? A) A 1 solar mass main sequence star B) A 1 solar mass white dwarf C) A 1 solar mass neutron star D) They all have the same force. Charles Hakes Fort Lewis College 16 • A neutron star cannot be more than 3 Msun. Charles Hakes Fort Lewis College 17 • A neutron star cannot be more than 3 Msun. • Surface gravity will become so great that not even light can escape. (Escape velocity > c) Charles Hakes Fort Lewis College 18 • A neutron star cannot be more than 3 Msun. • Surface gravity will become so great that not even light can escape. (Escape velocity > c) • Stars that began with > 25 Msun will probably become black holes. Charles Hakes Fort Lewis College 19 Black Holes • Can black holes be made of things other than neutron stars? • Any object of any mass has a radius that if it is compressed below that radius, light cannot escape. • This is called the Schwarzschild radius. • rS = 3km x M(solar masses) Charles Hakes Fort Lewis College 20 Black Holes • Example Schwarzschild radii : • Sun = 3km • 3MsolarCore = 9km • Jupiter = 3m Charles Hakes Fort Lewis College 21 Black Holes • Exercise - calculate the size required to compress a 70 kg person to make a black hole. • recall: rS = 3km x M(solar masses) Charles Hakes Fort Lewis College 22 Black Holes • Example Schwarzschild radii : • • • • • • Charles Hakes Fort Lewis College Sun = 3km 3MsolarCore = 9km Jupiter = 3m Earth = ~1cm Person = ~1x10-25 m Mobservable universe = ~robservable universe 23 If the Sun were suddenly replaced by a one solar mass black hole: A) we would immediately escape into deep space, driven out by its radiation. B) our clocks would all stop. C) life here would be unchanged. D) we would still orbit it in a period of one year. E) all terrestrial planets would fall in immediately. Charles Hakes Fort Lewis College 24 If the Sun were suddenly replaced by a one solar mass black hole: A) we would immediately escape into deep space, driven out by its radiation. B) our clocks would all stop. C) life here would be unchanged. D) we would still orbit it in a period of one year. E) all terrestrial planets would fall in immediately. Charles Hakes Fort Lewis College 25 Practice Problem • You observe a binary star system where the two stars are exactly the same temperature. The diameter of one star is 1.2 times the diameter of the second star. How many times more energy is emitted by the brighter star? Charles Hakes Fort Lewis College 26 Practice Problem • You observe a binary star system where the two stars are exactly the same temperature. The diameter of one star is 1.2 times the diameter of the second star. How many times more energy is emitted by the brighter star? A. 1.095x B. 1.2x C. 1.44x D. 2x Charles Hakes Fort Lewis College 27 Practice Problem • You observe a binary star system where the two stars are exactly the same size. One star is 5500 K. The other star is 6100 K. How many times more energy is emitted by the brighter star? Charles Hakes Fort Lewis College 28 Practice Problem • You observe a binary star system where the two stars are exactly the same size. One star is 5500 K. The other star is 6100 K. How many times more energy is emitted by the brighter star? A. 1.11x B. 1.23x C. 1.51x D. 600x Charles Hakes Fort Lewis College 29 Review Questions Charles Hakes Fort Lewis College 30 An ordinary star becomes a Red Giant when: A) A white dwarf companion star goes nova B) There is no Hydrogen remaining in the star C) Nutrino oscillations drive the outer layers D) The core becomes almost entirely Helium Charles Hakes Fort Lewis College 31 An ordinary star becomes a Red Giant when: A) A white dwarf companion star goes nova B) There is no Hydrogen remaining in the star C) Nutrino oscillations drive the outer layers D) The core becomes almost entirely Helium Charles Hakes Fort Lewis College 32 A main sequence star of 19 solar masses will eventually be a: A) A brown dwarf B) A white dwarf C) A type I supernova D) A type II supernova Charles Hakes Fort Lewis College 33 A main sequence star of 19 solar masses will eventually be a: A) A brown dwarf B) A white dwarf C) A type I supernova D) A type II supernova Charles Hakes Fort Lewis College 34 A supernova is observed with very little H in the spectrum. It is most likely a: A) type I B) type II C) type III D) not enough information Charles Hakes Fort Lewis College 35 A supernova is observed with very little H in the spectrum. It is most likely a: A) type I B) type II C) type III D) not enough information Charles Hakes Fort Lewis College 36 A source of light is approaching us at 3,000 km/s. All its waves are: A) Red shifted by 1% B) Blue shifted by 1% C) Not affected, as c is constant in all reference frames. D) Red shifted out of the visible into the infrared E) Blue shifted out of the visible into the ultraviolet Charles Hakes Fort Lewis College 37 A source of light is approaching us at 3,000 km/s. All its waves are: A) Red shifted by 1% B) Blue shifted by 1% C) Not affected, as c is constant in all reference frames. D) Red shifted out of the visible into the infrared E) Blue shifted out of the visible into the ultraviolet Charles Hakes Fort Lewis College 38 How could you determine the temperature of the photosphere of the Sun? A) only direct spacecraft measurement B) Newton’s Law C) Stefan’s Law D) Wein’s law Charles Hakes Fort Lewis College 39 How could you determine the temperature of the photosphere of the Sun? A) only direct spacecraft measurement B) Newton’s Law C) Stefan’s Law D) Wein’s law Charles Hakes Fort Lewis College 40 If a star has a parallax of 0.05”, then its distance must be A) 5 light years. B) 5 parsecs C) 20 light years. D) 20 parsecs. E) 200 parsecs Charles Hakes Fort Lewis College 41 If a star has a parallax of 0.05”, then its distance must be A) 5 light years. B) 5 parsecs C) 20 light years. D) 20 parsecs. E) 200 parsecs Charles Hakes Fort Lewis College 42 Assume your naked eye limiting magnitude is 4. With a 70mm diameter telescope (100x area of your pupil) which object would be barely visible? A) Seventh magnitude Titan, Saturn’s largest moon. B) Eighth magnitude Uranus. C) Ninth magnitude Barnard’s Star D) Eleventh magnitude Tethys, another Saturn moon E) Thirteenth magnitude Pluto Charles Hakes Fort Lewis College 43 Assume your naked eye limiting magnitude is 4. With a 70mm diameter telescope (100x area of your pupil) which object would be barely visible? A) Seventh magnitude Titan, Saturn’s largest moon. B) Eighth magnitude Uranus. C) Ninth magnitude Barnard’s Star D) Eleventh magnitude Tethys, another Saturn moon E) Thirteenth magnitude Pluto Charles Hakes Fort Lewis College 44 On the H-R diagram, red supergiants like Betelguese lie: A) top right B) top left C) about the middle D) lower left E) on the coolest portion of the main sequence Charles Hakes Fort Lewis College 45 On the H-R diagram, red supergiants like Betelguese lie: A) top right B) top left C) about the middle D) lower left E) on the coolest portion of the main sequence Charles Hakes Fort Lewis College 46 From inside out, which is the correct order? A) core, convective zone, radiative zone B) photosphere, radiative zone, corona C) radiative zone, convective zone, chromosphere D) core, chromosphere, photosphere E) convective zone, radiative zone, granulation Charles Hakes Fort Lewis College 47 From inside out, which is the correct order? A) core, convective zone, radiative zone B) photosphere, radiative zone, corona C) radiative zone, convective zone, chromosphere D) core, chromosphere, photosphere E) convective zone, radiative zone, granulation Charles Hakes Fort Lewis College 48 If Vega is apparent magnitude zero, and Deneb first magnitude, then A) Vega is about 100x brighter than Deneb.. B) Deneb is one magnitude brighter than Vega. C) Vega appears 2.5x brighter than Deneb. D) Deneb must be a main sequence star, and Vega a giant. E) Vega must be 2.5x more luminous than Deneb. Charles Hakes Fort Lewis College 49 If Vega is apparent magnitude zero, and Deneb first magnitude, then A) Vega is about 100x brighter than Deneb.. B) Deneb is one magnitude brighter than Vega. C) Vega appears 2.5x brighter than Deneb. D) Deneb must be a main sequence star, and Vega a giant. E) Vega must be 2.5x more luminous than Deneb. Charles Hakes Fort Lewis College 50 Three Minute Paper • Write 1-3 sentences. • What was the most important thing you learned today? • What questions do you still have about today’s topics? Charles Hakes Fort Lewis College 51