astro-0.4.1.0: src/Data/Astro/Moon.hs
{-|
Module: Data.Astro.Moon
Description: Calculation characteristics of the Moon
Copyright: Alexander Ignatyev, 2016
Calculation characteristics of the Moon.
= Example
@
import Data.Astro.Time.JulianDate
import Data.Astro.Coordinate
import Data.Astro.Types
import Data.Astro.Effects
import Data.Astro.CelestialObject.RiseSet
import Data.Astro.Moon
ro :: GeographicCoordinates
ro = GeoC (fromDMS 51 28 40) (-(fromDMS 0 0 5))
dt :: LocalCivilTime
dt = lctFromYMDHMS (DH 1) 2017 6 25 10 29 0
today :: LocalCivilDate
today = lcdFromYMD (DH 1) 2017 6 25
jd :: JulianDate
jd = lctUniversalTime dt
-- distance from the Earth to the Moon in kilometres
mdu :: MoonDistanceUnits
mdu = moonDistance1 j2010MoonDetails jd
-- MDU 0.9550170577020396
distance :: Double
distance = mduToKm mdu
-- 367109.51199772174
-- Angular Size
angularSize :: DecimalDegrees
angularSize = moonAngularSize mdu
-- DD 0.5425033990980761
-- The Moon's coordinates
position :: JulianDate -> EquatorialCoordinates1
position = moonPosition1 j2010MoonDetails
ec1 :: EquatorialCoordinates1
ec1 = position jd
-- EC1 {e1Declination = DD 18.706180658927323, e1RightAscension = DH 7.56710547682055}
hc :: HorizonCoordinates
hc = ec1ToHC ro jd ec1
-- HC {hAltitude = DD 34.57694951316064, hAzimuth = DD 103.91119101451832}
-- Rise and Set
riseSet :: RiseSetMB
riseSet = riseAndSet2 0.000001 position ro verticalShift today
-- RiseSet
-- (Just (2017-06-25 06:22:51.4858 +1.0,DD 57.81458864497365))
-- (Just (2017-06-25 22:28:20.3023 +1.0,DD 300.4168238905249))
-- Phase
phase :: Double
phase = moonPhase j2010MoonDetails jd
-- 2.4716141948212922e-2
sunEC1 :: EquatorialCoordinates1
sunEC1 = sunPosition2 jd
-- EC1 {e1Declination = DD 23.37339098989099, e1RightAscension = DH 6.29262026252748}
limbAngle :: DecimalDegrees
limbAngle = moonBrightLimbPositionAngle ec1 sunEC1
-- DD 287.9869373767473
@
-}
module Data.Astro.Moon
(
moonPosition1
, moonDistance1
, moonAngularSize
, moonHorizontalParallax
, moonPhase
, moonBrightLimbPositionAngle
)
where
import qualified Data.Astro.Utils as U
import Data.Astro.Types (DecimalDegrees(..), toRadians, fromRadians)
import Data.Astro.Time.JulianDate (JulianDate(..), numberOfDays)
import Data.Astro.Coordinate (EquatorialCoordinates1(..), EclipticCoordinates(..), eclipticToEquatorial)
import Data.Astro.Planet (planetBrightLimbPositionAngle)
import Data.Astro.Sun (sunDetails, sunMeanAnomaly2, sunEclipticLongitude2)
import Data.Astro.Moon.MoonDetails (MoonDetails(..), MoonDistanceUnits(..), j2010MoonDetails)
-- | Reduce the value to the range [0, 360)
reduceDegrees :: DecimalDegrees -> DecimalDegrees
reduceDegrees = U.reduceToZeroRange 360
-- | Calculate Equatorial Coordinates of the Moon with the given MoonDetails and at the given JulianDate.
-- It is recommended to use 'j2010MoonDetails' as a first parameter.
moonPosition1 :: MoonDetails -> JulianDate -> EquatorialCoordinates1
moonPosition1 md ut =
let sd = sunDetails ut
lambdaS = sunEclipticLongitude2 sd
ms = sunMeanAnomaly2 sd
mmq = meanMoonQuantities md ut
MQ lm'' _ nm' = correctedMoonQuantities lambdaS ms mmq
a = toRadians $ lm''-nm'
i = toRadians $ mdI md
y = (sin a) * (cos i)
x = cos a
at = reduceDegrees $ fromRadians $ atan2 y x
lambdaM = at + nm'
betaM = fromRadians $ asin $ (sin a) * (sin i)
in eclipticToEquatorial (EcC betaM lambdaM) ut
-- | Calculates the Moon's Distance at the given julian date.
-- Returns distance to the Moon
-- moonDistance1 :: JulianDate -> MoonDistanceUnits
-- you can use 'mduToKm' (defined in "Data.Astro.Moon.MoonDetails") to convert result to kilometers
moonDistance1 :: MoonDetails -> JulianDate -> MoonDistanceUnits
moonDistance1 md ut =
let sd = sunDetails ut
lambdaS = sunEclipticLongitude2 sd
ms = sunMeanAnomaly2 sd
mmq = meanMoonQuantities md ut
cmq = correctedMoonQuantities lambdaS ms mmq
mm' = toRadians $ mqAnomaly cmq
ec = toRadians $ centreEquation mm'
e = mdE md
in MDU $ (1 - e*e)/(1+e*(cos(mm'+ec)))
-- | Calculate the Moon's angular size at the given distance.
moonAngularSize :: MoonDistanceUnits -> DecimalDegrees
moonAngularSize (MDU p) = (mdBigTheta j2010MoonDetails) / (DD p)
-- | Calculates the Moon's horizontal parallax at the given distance.
moonHorizontalParallax :: MoonDistanceUnits -> DecimalDegrees
moonHorizontalParallax (MDU p) = (mdPi j2010MoonDetails) / (DD p)
-- | Calculates the Moon's phase (the area of the visible segment expressed as a fraction of the whole disk)
-- at the given universal time.
moonPhase :: MoonDetails -> JulianDate -> Double
moonPhase md ut =
let sd = sunDetails ut
lambdaS = sunEclipticLongitude2 sd
ms = sunMeanAnomaly2 sd
mmq = meanMoonQuantities md ut
MQ ml _ _ = correctedMoonQuantities lambdaS ms mmq
d = toRadians $ ml - lambdaS
f = 0.5 * (1 - cos d)
in f
-- | Calculate the Moon's position-angle of the bright limb.
-- It takes the Moon's coordinates and the Sun's coordinates.
-- Position-angle is the angle of the midpoint of the illuminated limb
-- measured eastwards from the north point of the disk.
moonBrightLimbPositionAngle :: EquatorialCoordinates1 -> EquatorialCoordinates1 -> DecimalDegrees
moonBrightLimbPositionAngle = planetBrightLimbPositionAngle
-- | The Moon's quantities
-- Used to store intermidiate results
data MoonQuantities = MQ {
mqLongitude :: DecimalDegrees -- ^ the Moon's longitude
, mqAnomaly :: DecimalDegrees -- ^ the Moon's anomaly
, mqAscendingNode :: DecimalDegrees -- ^ the Moon's ascending node's longitude
}
-- | Calculates the Moon's mean quantities on the given date.
-- It takes the Moon's orbita details and julian date
meanMoonQuantities :: MoonDetails -> JulianDate -> MoonQuantities
meanMoonQuantities md ut =
let d = DD $ numberOfDays (mdEpoch md) ut
lm = reduceDegrees $ (mdL md) + 13.1763966*d -- Moon's mean longitude
mm = reduceDegrees $ lm - 0.1114041*d - (mdP md) -- Moon's mean anomaly
nm = reduceDegrees $ (mdN md) - 0.0529539*d -- ascending node's mean longitude
in MQ lm mm nm
-- | Calculates correction for the equation of the centre
-- It takes the Moon's corrected anomaly in radians
centreEquation :: Double -> DecimalDegrees
centreEquation mm = DD $ 6.2886 * (sin mm)
-- | Calculates the Moon's corrected longitude, anomaly and asceding node's longitude
-- It takes the Sun's longitude, the Sun's mean anomaly and the Moon's mean quantities
correctedMoonQuantities :: DecimalDegrees -> DecimalDegrees -> MoonQuantities -> MoonQuantities
correctedMoonQuantities lambdaS ms (MQ lm mm nm) =
let ms' = toRadians ms
c = lm - lambdaS
ev = DD $ 1.2739 * (sin $ toRadians $ 2*c - mm) -- correction for evection
ae = DD $ 0.1858 * (sin ms') -- correction for annual equation
a3 = DD $ 0.37 * (sin ms') -- third correction
mm' = mm + (ev - ae - a3) -- Moon's corrected anomaly
mm'' = toRadians mm'
ec = centreEquation mm'' -- correction for the equation of the centre
a4 = DD $ 0.214 * (sin $ 2*mm'') -- fourth correction term
lm' = lm + (ev + ec -ae + a4) -- Moon's corrected longitude
v = DD $ 0.6583 * (sin $ toRadians $ 2*(lm' - lambdaS))-- correction for variation
lm'' = lm' + v -- Moon's true orbital longitude
nm' = nm - (DD $ 0.16 * (sin ms')) -- ascending node's corrected longitude
in MQ lm'' mm' nm'