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9 Stars … how I wonder what you are.. 9 Goals Stars are Suns. Are they: –Near? Far? –Brighter? Dimmer? –Hotter? Cooler? –Heavier? Lighter? –Larger? Smaller?

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Presentation on theme: "9 Stars … how I wonder what you are.. 9 Goals Stars are Suns. Are they: –Near? Far? –Brighter? Dimmer? –Hotter? Cooler? –Heavier? Lighter? –Larger? Smaller?"— Presentation transcript:

1 9 Stars … how I wonder what you are.

2 9 Goals Stars are Suns. Are they: –Near? Far? –Brighter? Dimmer? –Hotter? Cooler? –Heavier? Lighter? –Larger? Smaller? What categories can we place them in?

3 9 Angular Size Linear size = how big something really is –Meters, inches, light years, feet Angular size = how big something looks –Degrees, arcminutes, arcseconds, milliarcseconds Circle = 360 degrees 1 degree = 60 arcmin 1 arcmin = 60 arcsec 1 arcsec = 1000 mas

4 9

5 9 Distance One proof of a heliocentric Universe is stellar parallax. –Tycho Brahe saw no parallax. –Copernicus: stars too far away. Nearest star: Proxima Centauri Parallax angle = 0.76 arcsec –Tycho’s precision = 1 arcmin

6 9 The Parsec What is the distance of an object with a parallax angle of 1 arcsec? Distance = 206,265 AU This distance is 1 parsec (pc) 1 pc = 206,265 AU = 3.3 ly 1 lightyear = distance light travels in one year.

7 9 Concept Test If Star A has a parallax of 2 arcseconds, and Star B has a parallax of 0.25 arcseconds: a.Star A is closer to us than Star B. Both are farther from us than 1 pc. b.Star A is closer to us than Star B. Both are closer to us than 1 pc. c.Star A is closer to us than 1 pc. Star B is farther than 1 pc. d.Star B is closer to us than 1 pc. Star A is farther than 1 pc. e.Star B is closer to us than Star A. Both are farther away than 1 pc.

8 9 Distances Closest star: Proxima Centauri parallax = 0.76 arcsec Distance = 1.3 pc or 4.3 lightyears

9 9 Terms Brightness = How intense is the light I see from where I am. –Magnitude is numerical term for this. Luminosity = how much light is the thing really giving off.

10 9 Magnitude Scale The SMALLER the number the BRIGHTER the star! –Every difference of 1 magnitude = 2.5x brighter or dimmer. –Difference of 2 magnitudes = 2.5x2.5 = 6.3x brighter or dimmer

11 9 Magnitude vs. Brightness Mag. Difference Factors of 2.5Brightness Diff = = 2.5 X = 2.5 X 2.5 X = 2.5 X 2.5 X 2.5 X = 2.5 X 2.5 X 2.5 X 2.5 X = 2.5 X 2.5 X 2.5 X 2.5 X 2.5 X

12 9 Star light, star bright Sirius is magnitude -1.5 Polaris is magnitude 2.5 Is Sirius really more luminous than Polaris? No, Sirius is just closer.

13 9 Apparent and Absolute Apparent Magnitude = brightness (magnitude) of a star as seen from Earth.  m –Depends on star’s total energy radiated (Luminosity) and distance Absolute Magnitude = brightness (magnitude) of a star as seen from a distance of 10 pc.  M –Only depends on a star’s luminosity

14 9 Concept Test Polaris has a an apparent magnitude of 2.5. It’s absolute magnitude is 3.1. Polaris is: a.Closer to us than 10pc. b.Farther from us than 10 pc. c.Exactly 10 pc away. d.Can’t know without the parallax angle. e.None of these is correct.

15 9 Concept Test Polaris has a parallax angle of 0.01 arcsconds. Polaris is therefore: a.Closer to us than 1pc. b.Farther from us than 1pc. c.Exactly 1pc away.

16 9 Concept Test Polaris has a parallax angle of 0.01 arcsconds. Polaris is therefore: a.1pc. b.10pc. c.100pc. d.1000pc. e.None of the above.

17 9 example Our Sun: –m = -26.8, –distance = 4.8 x pc So: M = 4.8 Polaris: –m = 2.5, –distance = ~100 pc So: M = -3.1 Polaris is 1500 times more luminous than the Sun!

18 9 Concept Test The most likely absolute magnitudes (M) for each is: a.A = 2.5, B = -2.5, C = 2.5 b.A = 2.5, B = 2.5, C = -2.5 c.A = -2.5, B = 2.5, C = 2.5 d.A = 2.5, B = 2.5, C = 2.5 e.None of the above. StarDistancemM A5 pc1.0 B10 pc2.5 C20 pc

19 9 A Spectrum A spectrum = the amount of light given off by an object at a range of wavelengths. Emission lines Absorption lines Continuum

20 9 Three Reasons All objects do one or more: 1.Reflect light because of color or smoothness (same as scatter) 2.Emit light because of their temperature (thermal radiation) 3.Emit or absorb light because of their composition (spectral lines) A person, house, or the Moon: reflects visible light, and because each is warm, emits infrared light.

21 9 Concept Question A red chair appear red because: a.it emits red light. b.it transmits red light. c.it absorbs red light. d.it reflects red light. e.all of the above

22 9 Temperature and Light Warm objects emit light. –Thermal radiation

23 9 Stellar Temperatures How hot are stars? Thermal radiation and temperature. Different stars have different colors, different stars are temperatures. Different temp, different trace compositions Stellar Spectra Hot Cool

24 9 Spectral Classification

25 9 Stellar Masses How massive are stars? Kepler’s Laws – devised for the planets. Apply to any object that orbits another object. Kepler’s Third Law relates: – Period: “how long it takes to orbit something” –Semimajor axis: “how far you are away from that something” –Mass: “how much gravity is pulling you around in orbit” Where M is the Total Mass. Can calculate the mass of stars this way.

26 9 Binary Stars Most stars in the sky are in multiple systems. Binaries, triplets, quadruplets, etc…. –Sirius –Alcor and Mizar –Tatooine The Sun is in the minority by being single.

27 arcsec

28 9 Stellar Masses How massive are stars? Most stars have masses calculated this way. Find: –The more massive the star, the more luminous it is. –The more massive the star, the hotter it is.

29 9 Stellar Radii How big are stars? We see stars have different luminosities and different temperatures. Stars have different sizes. If you know: –Distance –Angular size Learn real size. 50 mas

30 9 Betelgeuse Angular size = 50 mas Parallax = 7.6 mas = arcsec Apparent mag = 0.6 Distance = 1/parallax = 132 pc True size = distance * angular size = 1400 R sol –Model solar system: 97 yards in radius. Absolute Mag = m – 5log(d/10pc) = -5 –Our sun M ~5, Betelgeuse = 10,000x luminosity

31 9 Angular versus Linear Supergiants, Giants and Dwarfs

32 9 H-R Diagram Can order the stars by: –Temperature (or spectral type) –Luminosity (or absolute magnitude). And see where other qualities fall: –Mass –Radius

33 9

34 9 Luminosity Class The roman numerals. Stars at same temp can have different luminosities. Corresponds to different classes: MS, giant, supergiant. V III I

35 9 Concept Test Which star is: 1.Hottest? 2.Coolest? 3.Faintest as seen from Earth? 4.Most luminous? Of Main Seq. Stars? 1.Most massive? 2.Most like the Sun? StarSpec Type mM AF0 V0.0 BG2 V CK5 III DF7 I-5.0 EK3 V5.06.5

36 9 The Main Sequence Stars characterized by what holds them up. 90% held up by heat of Hydrogen fusion? 4H  He + Energy


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