astro/basic/mercury.go
starainrt 34ff6a36ae
fix: 修正行星事件边界与留点计算
- 统一 UT 事件时刻与 TT 查询时刻的边界判断
- 将外行星留点搜索锚定到对应冲日周期
- 修正水星、金星合日、留、大距事件选择
- 统一七大行星视位置计算辅助逻辑
- 增加公开 Last/Next 边界和 JPL/NAOJ 基线回归测试
2026-05-22 12:24:41 +08:00

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package basic
import (
"math"
"b612.me/astro/planet"
. "b612.me/astro/tools"
)
func MercuryL(jd float64) float64 {
return planet.WherePlanet(1, 0, jd)
}
func MercuryB(jd float64) float64 {
return planet.WherePlanet(1, 1, jd)
}
func MercuryR(jd float64) float64 {
return planet.WherePlanet(1, 2, jd)
}
func AMercuryX(jd float64) float64 {
l := MercuryL(jd)
b := MercuryB(jd)
r := MercuryR(jd)
el := planet.WherePlanet(-1, 0, jd)
eb := planet.WherePlanet(-1, 1, jd)
er := planet.WherePlanet(-1, 2, jd)
x := r*Cos(b)*Cos(l) - er*Cos(eb)*Cos(el)
return x
}
func AMercuryY(jd float64) float64 {
l := MercuryL(jd)
b := MercuryB(jd)
r := MercuryR(jd)
el := planet.WherePlanet(-1, 0, jd)
eb := planet.WherePlanet(-1, 1, jd)
er := planet.WherePlanet(-1, 2, jd)
y := r*Cos(b)*Sin(l) - er*Cos(eb)*Sin(el)
return y
}
func AMercuryZ(jd float64) float64 {
//l := MercuryL(jd)
b := MercuryB(jd)
r := MercuryR(jd)
// el := planet.WherePlanet(-1, 0, jd)
eb := planet.WherePlanet(-1, 1, jd)
er := planet.WherePlanet(-1, 2, jd)
z := r*Sin(b) - er*Sin(eb)
return z
}
func AMercuryXYZ(jd float64) (float64, float64, float64) {
l := MercuryL(jd)
b := MercuryB(jd)
r := MercuryR(jd)
el := planet.WherePlanet(-1, 0, jd)
eb := planet.WherePlanet(-1, 1, jd)
er := planet.WherePlanet(-1, 2, jd)
x := r*Cos(b)*Cos(l) - er*Cos(eb)*Cos(el)
y := r*Cos(b)*Sin(l) - er*Cos(eb)*Sin(el)
z := r*Sin(b) - er*Sin(eb)
return x, y, z
}
func MercuryApparentRa(jd float64) float64 {
lo, bo := MercuryApparentLoBo(jd)
return LoToRa(jd, lo, bo)
}
func MercuryApparentDec(jd float64) float64 {
lo, bo := MercuryApparentLoBo(jd)
eps := TrueObliquity(jd)
dec := ArcSin(Sin(bo)*Cos(eps) + Cos(bo)*Sin(eps)*Sin(lo))
return dec
}
func MercuryApparentRaDec(jd float64) (float64, float64) {
lo, bo := MercuryApparentLoBo(jd)
return LoBoToRaDec(jd, lo, bo)
}
func EarthMercuryAway(jd float64) float64 {
return planetEarthAwayExplicitN(1, jd, -1)
}
func MercuryApparentLo(jd float64) float64 {
geo, _ := planetApparentGeocentricPositionN(1, jd, -1)
return geo.lo
}
func MercuryApparentBo(jd float64) float64 {
geo, _ := planetApparentGeocentricPositionN(1, jd, -1)
return geo.bo
}
func MercuryApparentLoBo(jd float64) (float64, float64) {
geo, _ := planetApparentGeocentricPositionN(1, jd, -1)
return geo.lo, geo.bo
}
func MercuryMag(jd float64) float64 {
sunDistance := MercuryR(jd)
earthDistance := EarthMercuryAway(jd)
earthSunDistance := planet.WherePlanet(-1, 2, jd)
i := (sunDistance*sunDistance + earthDistance*earthDistance - earthSunDistance*earthSunDistance) / (2 * sunDistance * earthDistance)
i = ArcCos(i)
mag := -0.42 + 5*math.Log10(sunDistance*earthDistance) + 0.0380*i - 0.000273*i*i + 0.000002*i*i*i
return FloatRound(mag, 2)
}
func MercuryHeight(jde, lon, lat, timezone float64) float64 {
// 转换为世界时
utcJde := jde - timezone/24.0
// 计算视恒星时
ra, dec := MercuryApparentRaDec(TD2UT(utcJde, true))
st := Limit360(ApparentSiderealTime(utcJde)*15 + lon)
// 计算时角
hourAngle := Limit360(st - ra)
// 高度角、时角与天球座标三角转换公式
// sin(h)=sin(lat)*sin(dec)+cos(dec)*cos(lat)*cos(hourAngle)
sinHeight := Sin(lat)*Sin(dec) + Cos(dec)*Cos(lat)*Cos(hourAngle)
return ArcSin(sinHeight)
}
func MercuryAzimuth(jde, lon, lat, timezone float64) float64 {
// 转换为世界时
utcJde := jde - timezone/24.0
// 计算视恒星时
ra, dec := MercuryApparentRaDec(TD2UT(utcJde, true))
st := Limit360(ApparentSiderealTime(utcJde)*15 + lon)
// 计算时角
hourAngle := Limit360(st - ra)
// 三角转换公式
tanAzimuth := Sin(hourAngle) / (Cos(hourAngle)*Sin(lat) - Tan(dec)*Cos(lat))
azimuth := ArcTan(tanAzimuth)
if azimuth < 0 {
if hourAngle/15 < 12 {
return azimuth + 360
}
return azimuth + 180
}
if hourAngle/15 < 12 {
return azimuth + 180
}
return azimuth
}
func MercuryHourAngle(jd, lon, timezone float64) float64 {
siderealLongitude := Limit360(ApparentSiderealTime(jd-timezone/24)*15 + lon)
hourAngle := siderealLongitude - MercuryApparentRa(TD2UT(jd-timezone/24.0, true))
if hourAngle < 0 {
hourAngle += 360
}
return hourAngle
}
func MercuryCulminationTime(jde, lon, timezone float64) float64 {
//jde 世界时,非力学时,当地时区 0时无需转换力学时
//ra,dec 瞬时天球座标非J2000等时间天球坐标
jde = math.Floor(jde) + 0.5
estimateJD := jde + Limit360(360-MercuryHourAngle(jde, lon, timezone))/15.0/24.0*0.99726851851851851851
normalizedHourAngle := func(jde, lon, timezone float64) float64 {
currentHourAngle := MercuryHourAngle(jde, lon, timezone)
if currentHourAngle < 180 {
currentHourAngle += 360
}
return currentHourAngle
}
for {
prevJD := estimateJD
hourAngleDelta := normalizedHourAngle(prevJD, lon, timezone) - 360
hourAngleSlope := (normalizedHourAngle(prevJD+0.000005, lon, timezone) - normalizedHourAngle(prevJD-0.000005, lon, timezone)) / 0.00001
estimateJD = prevJD - hourAngleDelta/hourAngleSlope
if math.Abs(estimateJD-prevJD) <= 0.00001 {
break
}
}
return estimateJD
}
func MercuryRiseTime(jd, lon, lat, timezone, aeroCorrection, observerHeight float64) (float64, error) {
return mercuryRiseDown(jd, lon, lat, timezone, aeroCorrection, observerHeight, true)
}
func MercurySetTime(jd, lon, lat, timezone, aeroCorrection, observerHeight float64) (float64, error) {
return mercuryRiseDown(jd, lon, lat, timezone, aeroCorrection, observerHeight, false)
}
func mercuryRiseDown(jd, lon, lat, timezone, aeroCorrection, observerHeight float64, isRise bool) (float64, error) {
return planetRiseDown(jd, lon, lat, timezone, aeroCorrection, observerHeight, isRise, MercuryCulminationTime, MercuryHeight, MercuryApparentDec)
}