Things to Memorize (March 2010) Constants and Units Velocity of light c=2.998 x 105 km s-1 c=2.998 x 108 m s-1 Grav. Constant G=6.67 x 10-11 m3 kg-1 s-2 Mass H atom mH=1.67 x 10-27 kg h=Planck’s Const 6.626 x 10-34 joule sec Energy = h x frequency (for light) = hc/ο¬ 1 AU = 1.5 x 108 km = 1.5 x 1011 m Parsec = 206265 AU = 3.26 light years Light year = 6.3 x 104 AU =0.307 pc = 9.5 x 1012 km 1 sidereal year =365.25 days = 3.16 x 107 s 7 (about π x 10 seconds in a year!) Astronomical unit Earth mass Earth radius Orbital velocity 6 x 1024 kg 6378 km 30 km s-1 Parallax Parallax μ (in arc sec) = 1/distance (in pc) (parallax is sometimes measured in milliarcseconds or 10-3 arcsec) Orbits P2 = k a3 (P=period, a=semi major axis) P2 = 4 π2a3/G(m1+m2) Using solar masses, years, and AU: P2 = a3/(m1+m2) m1/m2 = v2/v1 = a2/a1 = α2/α (m is mass, a is separation = a1+a2, α is angular sep) Orbital velocity (km s-1) v = 2 π r / P (r = radius of orbit) For visual binaries: - For systemic velocity, average max and min velocity of an individual star π π Newton’s law of gravity: πΉ = πΊ π1 2 2 G=6.67x10-11m3s-2kg-1, r in meters, m in kg, F in Newtons Circular Velocity Vc=√ Sun's mass 2 x 1030 kg = 2 x 1033 g Sun's radius R = 7 x 105 km Sun's luminosity L = 3.9 x 1026 Watts Sun's temperature T = 5800 K Sun's abs. magnitude MV = 4.83 Sun's app. Magnitude mV = -26 Sun’s flux as seen from earth: 1380 W/m2 Angular measures 360 degrees = 24 hours = 2π radians 1 radian ~ 57 degrees = 206265 arc sec 1 degree = 60' = 3600" 1 hour = 15 degrees Equations Circumference of a circle = 2ο°r Area of a circle = ο°r2 Surface area of sphere 4 π r2 Volume of sphere (4/3) π r3 Magnitudes M1-M2 = -2.5 log10 (L1/L2) or, Luminosity = 85.5 x (0.398)M (if given apparent magnitude, use flux as seen from earth for L1, L2) m-M = 5 log10(d) - 5 = 5 log10(d/10pc) (d is distance in parsecs) πΊπ π M=mass of central body, r is radius (in meters) but only if object’s mass ≈0. Misc: ac = vt2 = rω2 ; F = mobjv2 / r = mobj r ω2 Eccentricity b2 = a2(1-e2) (a and b are semi-major and semi-minor axes) e = focal length/a aphelion, apogee, apastron are farthest points perihelion, perigee, periastron are nearest Kepler's Laws 1. A planet orbits the sun in an ellipse with the sun at one focus of the ellipse 2. A line connecting a planet to the Sun sweeps out equal areas in equal time intervals 3. Using years, AU, and solar mass P2 = a3 otherwise, P2 = 4ο°2a3/G(m1+m2) Energy Wien's Law: λmax T = 0.29 cm K (λ=wavelength of peak flux) Flux = σ T4 (σ = Stefan-Boltzman constant = 5.67 x 10-8 watts m-2K-4, T=temp in K) Luminosity = 4πr2 σ T4 (r in meters) σ=7.12 x 10-17 solar radii-2 k-4 LSun 10 Å per nm Flux at distance d = L / (4 * π * d2) Periods of variable stars RR Lyrae stars - 0.5 - 3 days Cepheids = a few to 10s of days Long period variables - hundreds of days Magnitudes of variable stars and Red Giants RR Lyrae stars MV = ~0.75 Cepheids - Depends on period MV=-2.76(log10 (P) - 1.0) - 4.16 Supernovae (Ia) - MV about -19.5 Supernovae (II) – Mv less, very roughly -15 or -16 Brightest red giants: Mv = -3 Extragalactic stuff Age of Universe: 13.7 x 109 years Hubble constant: 70 km s-1 Mpc-1 Mass-Luminosity Relationship (M/Msun)4 =( L/Lsun) Ages M(in solar mass)/L(in Solar Lums) * 12 x 109 = main sequence lifetime in years =(1/M in solar masses)2.5 x 1010 Lifetime of red giants is 1/10 of giant’s main sequence liftime. Doppler Shift Δλ/λ=v/c (Positive for motion away from the observer, i.e. Positive is increasing separation) ο λ = obs – actual Redshift = z = v/c 1 + z = λobsv/λemit Hα is at 656.281 nm. Chandrasekhar limit = 1.4 MSun (electron pressure cannot support more mass than this - no white dwarfs bigger than 1.4 MSun - become neutron stars) Neutron star limit: about 3.6 solar masses; become black holes Misc. factoids: Distance of Jupiter - about 5 AU Distance of Pluto - about 40 AU Size of Milky Way – about 30 Kpc diam, about 100,000 LY Distance to Galactic Center ~ 26,000 LY The Solar system is on MWG’s Orion spur Distance to Andromeda ~ 2.6 million LY Size of Observable Universe Radius =13.7 billion LY Vrot MWG = 220 km/s Black holes: Schwarzschild radius=2Gm/c2 M − σ relation: log(M/Msun)=8.12 + αlog(σ/200km/s-1) α=4.2 (some sources give 5) σ is stellar velocity dispersion mcenteral black hole = .005mgalaxy (also works for black holes in the center of globular clusters) Temperature α 1/mass Spectral Types Class Temp. O B A F G 35,000K 20,000K 10,000K 7,000K 5,900K K 5,200K M 3,700K Lines B-V (approx.) -0.24 -0.16 0.00 +0.42 +0.65 He H, He H H, Ca, Fe Metals, weak H More +1.54 metals Molecules +1.85 Luminosity Classes (for solar temp) I Supergiant 104 Solar lum II Bright Giant 103 Solar lum III Giant 102 solar lum IV Subgiant 10 solar lum V Main Sequence 1 solar lum Telescopes πΏπΊπ π· 2 Light Gathering Power (LGP): πΏπΊππ΄ = (π·π΄ ) π΅ π΅ where D is diameter 11.6 Resolving power πΌ = π· where D is diameter in cm, gives power in arcseconds πΉ Magnification π = πΉπ where FO, E is the focal πΈ length of the objective and eyepiece, respectively Equations for Galaxies Tully-Fisher relation: For Sa, ππ΅ = − 9.95log ππππ₯ + 3.15 For Sb, ππ΅ = − 10.2log ππππ₯ + 2.71 For Sc, ππ΅ = −11.0 log ππππ₯ + 3.31 Spirals: log(πππππ’π ππ πππ) = −.249ππ΅ − 4 Ellipticals: log π = −.1ππ΅ + .2 Virial Theorem: π‘ππ‘ππ πππ π = 2 ππ£ 2 πΊ −2 ∑ πΎπΈ = ∑ ππΈ ππ