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Here you have Astronomy formulas on: constants and conversion factors, angle and distances, properties of light, Doppler effect, optics and so on.
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I. CONSTANTS AND CONVERSION FACTORS
speed of light c = 299792 km/s,
Planck constant h = 6. 62607 × 10 −^34 kg m^2 /s
Boltzmann constant k = 1. 3806503 × 10 −^23 J/K
Stefan-Boltzmann constant σ = 5. 6704 × 10 −^8 W m−^2 K−^1
Rydberg constant R = 1. 097 × 107 m−^1
Mass of the proton mp = 1. 007276 u = 1. 67262158 × 10 −^27 kg
Mass of the electron me = 0. 0005486 u = 9. 10938188 × 10 −^31 kg
Mass of the Hydrogen atom (with electron) mH = 1. 007825 u = 1. 67353322 × 10 −^27 kg
Mass of the Helium atom (with 2 electrons) MHe = 4. 002677 u = 6. 6466032 × 10 −^27 kg
1 eV = 1. 60218 × 10 −^19 J
II. ANGLES AND DISTANCES
Conversion between radians, arcmin, and arcseconds
1 rad = 57. 2958 deg = 3437. 75 ′^ = 206265′′
Small angle α distance d -size D relation
D = d × α(radians) = d × α(arcsec)/ 206265
III. PROPERTIES OF LIGHT, BLACK BODY RADIATION
Relation between wavelength λ , frequency f of light and energy Ef of photons
f λ = c, Ef = hf = hc λ Blackbody radiation: wavelength λmax of the peak of Planck curve (Wien’s Law) and total energy flux
F through the surface of the blackbody of temperature T (Stefan-Boltzmann Law) (temperature always
in Kelvin)
λmax = 0. 0029
T m,^ F^ =^ σT^
4
Total Luminosity L of a spherical black body (a star) of radius R and temperature T
L = 4πR^2 F = 4πσR^2 T 4
IV. STRUCTURE OF ATOMS, ATOMIC SPECTRUM OF HYDROGEN
Energy levels of Hydrogen atom and energy of transitions between the levels
En = − 13.^6 eV n^2
, En − EN = 13. 6 eV
n^2
)
Wavelength of the photon emitted or absorbed during atomic transition 1 λ =^ R
n^2
)
V. DOPPLER EFFECT
Wavelength shift ∆λ of the photon that has wavelength in the laboratory λ if the light source and the
observer moves with relative velocity v
∆λ λ
= v c
v = c · ∆λ λ
Relative velocity v is considered positive if the distance between the light source and the observer increases.
VI. OPTICS AND TELESCOPES
Angular resolution diffraction limit αDif f of a telescope with aperture DA observing at wavelength λ
αDif f (radians) = 1. 22
λ DA^ ,^ αDif f^ (arcsec) = 250000^
λ DA
VII. BRIGHTNESS OF STARS
Inverse square law linking brightness b to luminosity L and distance d of the source (star).
b = L 4 πd^2
, b^1 b 2
1 L 2
) ( (^) d 2 d 1
) 2