astro/lite/internal/moon.go
starainrt 3ffdbe0034
feat: 扩展天文计算能力
- 新增日食、月食、本地可见性、中心线、半影区域、SVG 图示与沙罗周期信息
- 新增行星冲合、留、方照、物理星历、视直径、相位、亮肢角、轨道节点等计算
- 新增木星伽利略卫星位置、现象与接触事件计算
- 新增恒星星表、星座判定、自行修正与观测辅助能力
- 新增 coord、formula、orbit、sundial、lite/sun、lite/moon 等扩展包
- 完善农历年号、月相英文别名、视差角、大气质量、折射、日晷与双星计算
- 增加 NASA、JPL Horizons、IMCCE 等回归测试数据与基线测试
- 重构基础算法文件组织,补充大量公开 API 注释和语义回归测试
- 更新中文和英文 README,补充示例、精度说明、SVG 配图
2026-05-01 22:38:44 +08:00

126 lines
4.8 KiB
Go

package internal
import (
"math"
. "b612.me/astro/tools"
)
type MoonState struct {
Longitude float64
Latitude float64
DistanceEarthRadii float64
RightAscension float64
Declination float64
}
func MoonGeocentric(jd float64) MoonState {
d := jd - 2451543.5
node := Limit360(125.1228 - 0.0529538083*d)
inclination := 5.1454
perigee := Limit360(318.0634 + 0.1643573223*d)
semiMajorAxis := 60.2666
eccentricity := 0.054900
meanAnomaly := Limit360(115.3654 + 13.0649929509*d)
meanLongitude := Limit360(node + perigee + meanAnomaly)
argumentLatitude := Limit360(meanLongitude - node)
sunPerigee := Limit360(282.9404 + 0.0000470935*d)
sunEccentricity := 0.016709 - 0.000000001151*d
sunMeanAnomaly := Limit360(356.0470 + 0.9856002585*d)
sunTrueLongitude, _ := orbitalLongitudeDistance(sunPerigee, sunEccentricity, 1, sunMeanAnomaly)
longitude, latitude, distance := orbitalLongitudeLatitudeDistance(node, inclination, perigee, semiMajorAxis, eccentricity, meanAnomaly)
elongation := Limit360(meanLongitude - sunTrueLongitude)
longitude += -1.274 * Sin(meanAnomaly-2*elongation)
longitude += 0.658 * Sin(2*elongation)
longitude += -0.186 * Sin(sunMeanAnomaly)
longitude += -0.059 * Sin(2*meanAnomaly-2*elongation)
longitude += -0.057 * Sin(meanAnomaly-2*elongation+sunMeanAnomaly)
longitude += 0.053 * Sin(meanAnomaly+2*elongation)
longitude += 0.046 * Sin(2*elongation-sunMeanAnomaly)
longitude += 0.041 * Sin(meanAnomaly-sunMeanAnomaly)
longitude += -0.035 * Sin(elongation)
longitude += -0.031 * Sin(meanAnomaly+sunMeanAnomaly)
longitude += -0.015 * Sin(2*argumentLatitude-2*elongation)
longitude += 0.011 * Sin(meanAnomaly-4*elongation)
latitude += -0.173 * Sin(argumentLatitude-2*elongation)
latitude += -0.055 * Sin(meanAnomaly-argumentLatitude-2*elongation)
latitude += -0.046 * Sin(meanAnomaly+argumentLatitude-2*elongation)
latitude += 0.033 * Sin(argumentLatitude+2*elongation)
latitude += 0.017 * Sin(2*meanAnomaly+argumentLatitude)
distance += -0.58 * Cos(meanAnomaly-2*elongation)
distance += -0.46 * Cos(2*elongation)
longitude = Limit360(longitude)
ra, dec := EclipticToEquatorial(jd, longitude, latitude)
return MoonState{
Longitude: longitude,
Latitude: latitude,
DistanceEarthRadii: distance,
RightAscension: ra,
Declination: dec,
}
}
func MoonTopocentric(jd, observerLon, observerLat, heightMeters float64) MoonState {
geo := MoonGeocentric(jd)
ra, dec := TopocentricRaDec(geo.RightAscension, geoDeclinationClamp(geo.Declination), observerLat, observerLon, jd, geo.DistanceEarthRadii, heightMeters)
geo.RightAscension = ra
geo.Declination = dec
return geo
}
func orbitalLongitudeLatitudeDistance(node, inclination, perigee, axis, eccentricity, meanAnomaly float64) (float64, float64, float64) {
meanAnomalyRad := meanAnomaly * math.Pi / 180.0
eccentricAnomaly := meanAnomalyRad + eccentricity*math.Sin(meanAnomalyRad)*(1+eccentricity*math.Cos(meanAnomalyRad))
for i := 0; i < 5; i++ {
eccentricAnomaly -= (eccentricAnomaly - eccentricity*math.Sin(eccentricAnomaly) - meanAnomalyRad) / (1 - eccentricity*math.Cos(eccentricAnomaly))
}
xv := axis * (math.Cos(eccentricAnomaly) - eccentricity)
yv := axis * math.Sqrt(1-eccentricity*eccentricity) * math.Sin(eccentricAnomaly)
trueAnomaly := math.Atan2(yv, xv)
radius := math.Hypot(xv, yv)
nodeRad := node * math.Pi / 180.0
inclinationRad := inclination * math.Pi / 180.0
perigeeRad := perigee * math.Pi / 180.0
xh := radius * (math.Cos(nodeRad)*math.Cos(trueAnomaly+perigeeRad) - math.Sin(nodeRad)*math.Sin(trueAnomaly+perigeeRad)*math.Cos(inclinationRad))
yh := radius * (math.Sin(nodeRad)*math.Cos(trueAnomaly+perigeeRad) + math.Cos(nodeRad)*math.Sin(trueAnomaly+perigeeRad)*math.Cos(inclinationRad))
zh := radius * math.Sin(trueAnomaly+perigeeRad) * math.Sin(inclinationRad)
longitude := math.Atan2(yh, xh) * 180.0 / math.Pi
latitude := math.Atan2(zh, math.Hypot(xh, yh)) * 180.0 / math.Pi
return Limit360(longitude), latitude, radius
}
func orbitalLongitudeDistance(perigee, eccentricity, axis, meanAnomaly float64) (float64, float64) {
meanAnomalyRad := meanAnomaly * math.Pi / 180.0
eccentricAnomaly := meanAnomalyRad + eccentricity*math.Sin(meanAnomalyRad)*(1+eccentricity*math.Cos(meanAnomalyRad))
for i := 0; i < 5; i++ {
eccentricAnomaly -= (eccentricAnomaly - eccentricity*math.Sin(eccentricAnomaly) - meanAnomalyRad) / (1 - eccentricity*math.Cos(eccentricAnomaly))
}
xv := axis * (math.Cos(eccentricAnomaly) - eccentricity)
yv := axis * math.Sqrt(1-eccentricity*eccentricity) * math.Sin(eccentricAnomaly)
trueAnomaly := math.Atan2(yv, xv) * 180.0 / math.Pi
radius := math.Hypot(xv, yv)
return Limit360(trueAnomaly + perigee), radius
}
func geoDeclinationClamp(dec float64) float64 {
if dec > 90 {
return 90
}
if dec < -90 {
return -90
}
return dec
}