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this is the formula sheet we were given to print for our finals
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Astro 122 – Astronomy of Stars and Galaxies–Formula Sheet 1
P 2 = a^3 (around Sun) Perihelion=a(1 − e) Aphelion=a(1 + e) e = c/a c = f λ E = hf (Emitted) Flux=σT 4 (Received) Flux= (^4) πdL 2 L = 4πR^2 σT 4 λmax = (^) T^2 [.K^9 ] mm =^2. T^9 × [K^10 ] 6 nm d[parsecs]= (^) p[arcsec]^1 vrad/c = (λshif t − λrest)/λrest P 2 = (^) G(M^4 π 12 +aM^32 ) E = mc^2 Mbalance = 18M √(T 3 /n) (n in cm−^3 ) LObs = LLocal ∗ √ 1 − (v/c)^2 MObs = Mrest/√ 1 − (v/c)^2 RS = 2GMBH /c^2 ∆x∆p > h tBH = 10, 240 π^2 G^2 M 3 /(hc^4 ) Mr = rv^2 /G
v = c ∗ z v = H 0 ∗ d 1 + z = λobs/λrest = TCM B,then/TCM B,now vH =(140 m/s)√T Constants: AU=1. 496 × 1011 m light-year (ly)=9. 46 × 1015 m parsec (pc)=3. 09 × 1016 m=3.26 ly c = 3. 00 × 108 m/s G = 6. 67 × 10 −^11 m^3 /kg/s^2 h = 6. 63 × 10 −^34 J s σ = 5. 67 × 10 −^8 W/m^2 /K^4 mp = 1. 67 × 10 −^27 kg MSun = 2. 0 × 1030 kg RSun = 6. 96 × 105 km LSun = 3. 8 × 1026 W REarth = 6. 38 × 103 km year=3. 15 × 107 s H 0 =22 km/s/Mly