Starlight and What it Tells Us The Stars in the Sky Vary in Brightness • Distance • Size Vary in Color • Color = Temperature Star Names • • • • Proper star names mostly Arabic Greek Letters, Numbers Catalog Identifiers Faint stars usually have no name The Names of Sirius • Alpha Canis Majoris (Bayer, 1603) • 9 Canis Majoris (Flamsteed, 1725) • BD -16 1591 (Bonner Durchmusterung 18591903) • HR 2491 (Harvard Revised Catalog, 1908) • HD 48915 (Henry Draper, 1918-1924) • ADS 5423 (Aitken Double Star Catalog, 1932) • HIP 32349 (HIPPARCOS, 1997) The Heavens Are Not Changeless • The Stars Move – Most of our constellations would have been unrecognizable to Neanderthal Man • The Solar System Moves – Very few of our nearby stars would have been visible to the first humans • Stars are Born, Live and Die – Many of our brightest stars did not exist in the days of the dinosaurs Brightness of Stars • Variations in distance and intrinsic brightness • Scale based on one by Hipparcos 500 B.C. • Magnitude: Large Numbers = Fainter – One magnitude = 2.5 x – Five magnitudes = 100 x Magnitudes • • • • • • • • Planet around nearby star: Pluto: Faintest Naked-Eye Star: Big Dipper Stars: Sirius (Brightest Star) Venus Full Moon Sun 30 13 6 2 -1.6 -4 -12 -27 Absolute Magnitude • Altair and Deneb are about equally bright as seen from Earth • Altair is 16 l.y. away, Deneb 1600 • Hence Deneb must be about 10,000 times brighter Absolute Magnitude • How bright a star would be at a distance of 32.6 l.y. (10 parsecs) • Sun: 4.5 (inconspicuous naked-eye star) • Altair: 2.2 • Deneb: -7.1 (bright as crescent moon) – Note: Deneb - Altair about 10 magnitudes = 100 x 100 = 10,000 times Black-Body Radiation • Objects Emit Radiation Because They Are Hot • Why “Black”? Because None of the Radiation is Reflected from Some Other Source • The Sun Emits Black-Body Radiation, Mars Does Not • Close Example of pure Black-Body radiation: Peephole in a pottery kiln Black Body Radiation What’s The Source of the Light? Color = Temperature Why Black-Body Radiation is so Important • Color is directly related to temperature • Temperature is the only determinant of color • Energy per unit area is the same if temperature is the same – If two stars have the same color and distance, difference in brightness is due to difference in size – Dwarf and giant stars are literally dwarfs or giants Sirius and the Pup Sirius and the Pup • • • • Sirius M = -1.5; Pup M = 8.5 10 magnitude difference 100 x 100 = 10,000 times brightness distance Sirius and the Pup are same color, therefore same temperature (Pup is hotter) • Pup must have 1/10,000 the apparent area of Sirius = 1/100 the diameter Spectroscopy • Different atoms absorb or emit specific wavelengths of light • When light spread into a spectrum, the absorbed wavelengths show up as dark (missing) bands • These spectral lines are indicators of: – Chemical composition – Physical conditions Atoms and Radiation The Solar Spectrum Spectra and Spectral Lines • Continuous Spectrum: Incandescent solids or liquids (steel mill) and dense hot gases (Sun’s photosphere) • Emission Spectrum: Thin hot gases (fireworks, sodium or mercury vapor lights, Sun’s chromosphere • Absorption Spectrum: Light shining through thin gases (Sun and star light) How the Chromosphere Works Spectral Lines are Affected By: • Electrical and Magnetic Fields • Number of Electrons Atoms Have Lost (Indicates Temperature and Pressure) • Motion (Doppler Effect) • Blue-shifted if Motion Toward Observer • Red-shifted if Motion Away From Observer The Doppler Effect What the Doppler Effect Tells Us • Radial Motion • Rotation of Stars – Approaching side of star blue-shifted, receding side red-shifted • Unseen Companions (Stars or Planets) – Star oscillates around center of mass • Surface and Interior Motions – Changes in Size – Interior Oscillations Spectral Classification of Stars • W – very hot young stars expelling their outer layers • Main Sequence: O, B, A, F, G, K, M (hottest to coolest) – “Oh be a fine girl/guy, kiss me” • Subdwarfs: L, T, Y (hottest to coolest) • Chemically Peculiar Stars: C, N, R, S • White Dwarfs: D Spectral Signatures of Stars • • • • • • • O: Ionized Helium B: Neutral Helium A: Strongest Hydrogen Lines F: Ionized Calcium G: Strongest Calcium Lines + Neutral Metals K: Neutral Metals Dominate M: Titanium Oxide The Hertzsprung-Russell Diagram The Main Sequence: O • • • • • • • 30,000-60,000 K (Blue-white) Absolute Magnitude -5 1,000,000 times Sun’s Luminosity 16 times Sun’s Diameter 64 times Sun’s Mass Lifetime: Less than a million years Examples: Orion's Belt The Main Sequence: B • • • • • • • 10,000-30,000 K (Blue-white) Absolute Magnitude -3 20,000 times Sun’s Luminosity 7 times Sun’s Diameter 18 times Sun’s Mass Lifetime: 10 million years Examples: Spica The Main Sequence: A • • • • • • • Temperature: 7500-10,000 K (White) Absolute Magnitude +0.5 40 times Sun’s Luminosity 2 times Sun’s Diameter 3 times Sun’s Mass Lifetime: 600 million years Examples: Vega, Sirius The Main Sequence: F • • • • • • • Temperature: 6000-7500 K (Yellow-White) Absolute Magnitude +2.5 6 times Sun’s Luminosity 1.5 times Sun’s Diameter 1.7 times Sun’s Mass Lifetime: 2.5 billion years Examples: Procyon The Main Sequence: G • • • • • • • Temperature: 5000-6000 K (Yellow) Absolute Magnitude +5 1 times Sun’s Luminosity 1 times Sun’s Diameter 1 times Sun’s Mass Lifetime: 10 billion years Examples: Sun, Alpha Centauri A The Main Sequence: K • • • • • • • Temperature: 3500-5000 K (Orange) Absolute Magnitude +6 0.4 times Sun’s Luminosity 0.9 times Sun’s Diameter 0.8 times Sun’s Mass Lifetime: 10 billion years Examples: Alpha Centauri B The Main Sequence: M • • • • • • • • Temperature: 2000-3500 K (Red) Absolute Magnitude +10 to +15 0.04 times Sun’s Luminosity 0.5 times Sun’s Diameter 0.4 times Sun’s Mass Lifetime: 5 trillion years 75% + of all stars Examples: Barnard's Star, Proxima Centauri Sub-Dwarfs • L: 1300-2000 K, Borderline stars with alkali metals and metal hydrides • T: 700-1300 K, Substellar, methane in spectra • Y <700 K, Substellar, ammonia in spectra (predicted)