Equation%20summary:%20linear%20motion - PowerPoint PPT Presentation

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Equation%20summary:%20linear%20motion

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Equation summary: linear motion v = d/t p = mv a = v/t F = ma v=speed (or velocity) d=distance t=time p=momentum – PowerPoint PPT presentation

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Title: Equation%20summary:%20linear%20motion


1
Equation summary linear motion
  • v d/t
  • p mv
  • a v/t
  • F ma
  • vspeed (or velocity)
  • ddistance
  • ttime
  • pmomentum
  • mmass
  • aacceleration
  • FForce

2
Eqn summary circular motion
  • v 2pr/P
  • C 2pr
  • Lmvr
  • Fc mv2/r
  • v speed
  • r radius
  • P period
  • C circumference
  • L angular momentum
  • m mass
  • Fc Centrifugal Force

3
Eqn summary gravity
  • Fg force of gravity (weight)
  • m mass
  • g acceleration of gravity
  • d distance from mass m to M
  • G gravitation constant
  • M mass (e.g. of planet)
  • R radius (e.g. of planet)
  • W Work against gravity
  • vesc escape speed
  • Fg mg
  • Fg G Mm/d2
  • g GM/R2
  • W mgd
  • vesc Sqrt2GM/R

4
Keplers 3rd law
  • Mm combined mass
  • (in Msun)
  • a semi-major axis
  • (in au)
  • P Period
  • (in years)
  • Mm a3/P2

5
Eqn summary waves light
  • l f s
  • E h f
  • FE E/At s T4
  • lmax2.8 x 106/T
  • Waves
  • l wavelength
  • f frequency
  • s speed of wave ( c for light)
  • Photon of light
  • E Energy
  • h Plancks constant
  • FE radiative flux
  • (energy E per area A and time t)
  • T temperature (in K)
  • lmax wavelength of maximum intensity (in nm)

6
Doppler shift
  • ex1 l 500 nm lobs 550 nm
  • Dl lobs-l 50 nm
  • v (50/500) c c/10 30,000 km/s
  • Dlgt0 gt Redshift gt moving away from obs.
  • ex2 l 500 nm lobs 495 nm
  • Dl lobs-l -5 nm
  • v (-5/500) c -c/100 -3000 km/s
  • Dllt0 gt Blueshift gt moving toward obs.

7
Angle, distance, parallax, resolution
  • a 360o s/2pd
  • aarcsec sau/dpc
  • a 2.5 x 105 arcsec (l/D)
  • a angular size
  • s linear size
  • d distance
  • aarcsec parallax angle in arcsec
  • sau separation size in au
  • dpc distance in parsec (pc)
  • a diffraction limit resolution for telescope of
    diameter D and light of wavelength l

8
Dating from Radioactive Decay
  • If element x decays with half-life th, then
  • of x at time t Nx(t) Nx(t0)
    2-t/th
  • fraction of x at t fx(t) Nx(t)/Nx(t0)
    2-t/th
  • To solve for time t, take Log of both sides
  • Log(fx) - (t/th) Log(2) (t/th) Log(1/2) gt
  • t th Log(fx)/Log(1/2)

9
Luminosity magnitude
  • Luminosity L sT4 4pR2
  • or L/Lsun (T/Tsun)4 (R/Rsun)2
  • App. Brightness L/4pD2
  • Abs. Magnitude 5 - 2.5 log(L/Lsun)
  • App. Mag. Abs. Mag. 5 log(D/10pc)

10
Gravitational Escape
  • Grav. Escape energy Eg GMm/R
  • Kinetic energy Ek mV2/2
  • EkEg gt Escape speed Vesc Sqrt2GM/R
  • For Sun Vesc 600 km/s
  • Thus Vesc 600 km/s SqrtM/R
  • (where M,R in solar
    units)

11
Black Holes
  • Vesc Sqrt2GM/R
  • R 2GM/(Vesc)2
  • For black hole, Vesc c speed of light
  • RBH 2GM/c2 (a.k.a. Schwarzschild radius)
  • For object with mass of Sun, RBH 3 km
  • Thus in general, RBH 3 km (M/Msun)

12
Orbital motion
13
Galactic Rotation speed vs. mass
  • V2 M/r
  • V SqrtM/r
  • M(r) V2 r
  • V Dl

14
Hubble Law Redshfit
  • Doppler shift V c Dl/lo
  • V velocity
  • c speed of light
  • Dl l-loDoppler shift from rest wavelength lo
  • Hubbles law V Ho d
  • d distance Ho Hubbles constant

15
Drake Equation
NHP number of habitable planets in the Galaxy
flife fraction of habitable planets which
actually contain life
fciv fraction of life-planets where a
civilization has at some time arisen
fnow fraction of civilizations which exist now
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