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</p><h3><img src="./- Astrodienst_files/swefl300.gif" alt="Swiss Ephemeris">
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<br>Test Output </h3>
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<hr noshade="">
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<pre> <font face="courier" size="-1">
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Swetest computes a complete set of geocentric planetary positions,
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for a given date or a sequence of dates.
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Input can either be a date or an absolute julian day number.
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0:00 (midnight).
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With the proper options, swetest can be used to output a printed
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ephemeris and transfer the data into other programs like spreadsheets
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for graphical display.
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Version: 2.10.02
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Command line options:
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help commands:
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-?, -h display whole info
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-hcmd display commands
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-hplan display planet numbers
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-hform display format characters
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-hdate display input date format
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-hexamp display examples
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-glp report file location of library
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input time formats:
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-bDATE begin date; e.g. -b1.1.1992 if
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Note: the date format is day month year (European style).
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-bj... begin date as an absolute Julian day number; e.g. -bj2415020.5
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-j... same as -bj
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-tHH[:MM[:SS]] input time (as Ephemeris Time)
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-ut input date is Universal Time (UT1)
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-utHH[:MM[:SS]] input time (as Universal Time)
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-utcHH[:MM[:SS]] input time (as Universal Time Coordinated UTC)
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H,M,S can have one or two digits. Their limits are unchecked.
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output time for eclipses, occultations, risings/settings is UT by default
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-lmt output date/time is LMT (with -geopos)
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-lat output date/time is LAT (with -geopos)
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object, number of steps, step with
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-pSEQ planet sequence to be computed.
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See the letter coding below.
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-dX differential ephemeris: print differential ephemeris between
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body X and each body in list given by -p
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example: -p2 -d0 -fJl -n366 -b1.1.1992 prints the longitude
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distance between SUN (planet 0) and MERCURY (planet 2)
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for a full year starting at 1 Jan 1992.
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-dhX differential ephemeris: print differential ephemeris between
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heliocentric body X and each body in list given by -p
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example: -p8 -dh8 -ftl -n36600 -b1.1.1500 -s5 prints the longitude
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distance between geocentric and heliocentric Neptune (planet 8)
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for 500 year starting at 1 Jan 1500.
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Using this option mostly makes sense for a single planet
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to find out how much its geocentric and heliocentric positions can differ
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over extended periods of time
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-DX midpoint ephemeris, works the same way as the differential
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mode -d described above, but outputs the midpoint position.
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-nN output data for N consecutive timesteps; if no -n option
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is given, the default is 1. If the option -n without a
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number is given, the default is 20.
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-sN timestep N days, default 1. This option is only meaningful
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when combined with option -n.
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If an 'y' is appended, the time step is in years instead of days,
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for example -s10y for a time step of 10 years.
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If an 'mo' is appended, the time step is in months instead of days,
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for example -s3mo for a time step of 3 months.
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If an 'm' is appended, the time step is in minutes instead of days,
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for example -s15m for a time step of 15 minutes.
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If an 's' is appended, the time step is in seconds instead of days,
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for example -s1s for a time step of 1 second.
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output format:
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-fSEQ use SEQ as format sequence for the output columns;
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default is PLBRS.
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-head don't print the header before the planet data. This option
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is useful when you want to paste the output into a
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spreadsheet for displaying graphical ephemeris.
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+head header before every step (with -s..)
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-gPPP use PPP as gap between output columns; default is a single
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blank. -g followed by white space sets the
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gap to the TAB character; which is useful for data entry
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into spreadsheets.
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-hor list data for multiple planets 'horizontally' in same line.
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all columns of -fSEQ are repeated except time colums tTJyY.
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astrological house system:
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-house[long,lat,hsys]
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include house cusps. The longitude, latitude (degrees with
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DECIMAL fraction) and house system letter can be given, with
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commas separated, + for east and north. If none are given,
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Greenwich UK and Placidus is used: 0.00,51.50,p.
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The output lists 12 house cusps, Asc, MC, ARMC, Vertex,
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Equatorial Ascendant, co-Ascendant as defined by Walter Koch,
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co-Ascendant as defined by Michael Munkasey, and Polar Ascendant.
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Houses can only be computed if option -ut is given.
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A equal
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B Alcabitius
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C Campanus
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D equal / MC
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E equal = A
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F Carter poli-equatorial
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G 36 Gauquelin sectors
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H horizon / azimuth
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I Sunshine
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i Sunshine alternative
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K Koch
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L Pullen S-delta
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M Morinus
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N Whole sign, Aries = 1st house
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O Porphyry
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P Placidus
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Q Pullen S-ratio
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R Regiomontanus
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S Sripati
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T Polich/Page ("topocentric")
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U Krusinski-Pisa-Goelzer
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V equal Vehlow
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W equal, whole sign
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X axial rotation system/ Meridian houses
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Y APC houses
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The use of lower case letters is deprecated. They will have a
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different meaning in future releases of Swiss Ephemeris.
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-hsy[hsys]
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house system to be used (for house positions of planets)
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for long, lat, hsys, see -house
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The use of lower case letters is deprecated. They will have a
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different meaning in future releases of Swiss Ephemeris.
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-geopos[long,lat,elev]
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Geographic position. Can be used for azimuth and altitude
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or house cusps calculations.
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The longitude, latitude (degrees with DECIMAL fraction)
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and elevation (meters) can be given, with
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commas separated, + for east and north. If none are given,
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Greenwich is used: 0,51.5,0.
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For topocentric planet positions please user the parameter -topo
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sidereal astrology:
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-ay.. ayanamsha, with number of method, e.g. ay0 for Fagan/Bradley
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-sid.. sidereal, with number of method (see below)
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-sidt0.. dito, but planets are projected on the ecliptic plane of the
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reference date of the ayanamsha (more info in general documentation
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www.astro.com/swisseph/swisseph.htm)
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-sidsp.. dito, but planets are projected on the solar system plane.
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(see www.astro.com/swisseph/swisseph.htm)
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-sidudef[jd,ay0,...] sidereal, with user defined ayanamsha;
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jd=julian day number in TT/ET
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ay0=initial value of ayanamsha,
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...=optional parameters, comma-sparated:
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'jdisut': ayanamsha reference date is UT
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'eclt0': project on ecliptic of reference date (like -sidt0..)
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'ssyplane': project on solar system plane (like -sidsp..)
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e.g. '-sidudef2452163.8333333,25.0,jdisut': ayanamsha is 25.0° on JD 2452163.8333333 UT
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number of ayanamsha method:
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0 for Fagan/Bradley
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1 for Lahiri
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2 for De Luce
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3 for Raman
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4 for Usha/Shashi
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5 for Krishnamurti
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6 for Djwhal Khul
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7 for Yukteshwar
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8 for J.N. Bhasin
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9 for Babylonian/Kugler 1
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10 for Babylonian/Kugler 2
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11 for Babylonian/Kugler 3
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12 for Babylonian/Huber
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13 for Babylonian/Eta Piscium
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14 for Babylonian/Aldebaran = 15 Tau
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15 for Hipparchos
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16 for Sassanian
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17 for Galact. Center = 0 Sag
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18 for J2000
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19 for J1900
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20 for B1950
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21 for Suryasiddhanta
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22 for Suryasiddhanta, mean Sun
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23 for Aryabhata
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24 for Aryabhata, mean Sun
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25 for SS Revati
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26 for SS Citra
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27 for True Citra
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28 for True Revati
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29 for True Pushya (PVRN Rao)
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30 for Galactic (Gil Brand)
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31 for Galactic Equator (IAU1958)
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32 for Galactic Equator
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33 for Galactic Equator mid-Mula
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34 for Skydram (Mardyks)
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35 for True Mula (Chandra Hari)
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36 Dhruva/Gal.Center/Mula (Wilhelm)
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37 Aryabhata 522
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38 Babylonian/Britton
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39 Vedic/Sheoran
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40 Cochrane (Gal.Center = 0 Cap)
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41 Galactic Equator (Fiorenza)
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42 Vettius Valens
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43 Lahiri 1940
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44 Lahiri VP285 (1980)
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45 Krishnamurti VP291
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46 Lahiri ICRC
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ephemeris specifications:
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-edirPATH change the directory of the ephemeris files
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-eswe swiss ephemeris
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-ejpl jpl ephemeris (DE431), or with ephemeris file name
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-ejplde200.eph
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-emos moshier ephemeris
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-true true positions
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-noaberr no aberration
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-nodefl no gravitational light deflection
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-noaberr -nodefl astrometric positions
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-j2000 no precession (i.e. J2000 positions)
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-icrs ICRS (use Internat. Celestial Reference System)
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-nonut no nutation
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-speed calculate high precision speed
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-speed3 'low' precision speed from 3 positions
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do not use this option. -speed parameter
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is faster and more precise
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-iXX force iflag to value XX
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-testaa96 test example in AA 96, B37,
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i.e. venus, j2450442.5, DE200.
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attention: use precession IAU1976
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and nutation 1980 (s. swephlib.h)
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-testaa95
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-testaa97
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-roundsec round to seconds
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-roundmin round to minutes
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-ep use extra precision in output for some data
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-dms use dms instead of fractions, at some places
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-lim print ephemeris file range
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observer position:
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-hel compute heliocentric positions
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-bary compute barycentric positions (bar. earth instead of node)
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-topo[long,lat,elev]
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topocentric positions. The longitude, latitude (degrees with
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DECIMAL fraction) and elevation (meters) can be given, with
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commas separated, + for east and north. If none are given,
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Greenwich is used 0.00,51.50,0
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-pc... compute planetocentric positions
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to specify the central body, use the internal object number
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of Swiss Ephemeris, e.g. 3 for Venus, 4 for Mars,
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-pc3 Venus-centric
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-pc4 Mars-centric
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-pc5 Jupiter-centric (barycenter)
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-pc9599 Jupiter-centric (center of body)
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-pc9699 Saturn-centric (center of body)
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For asteroids use MPC number + 10000, e.g.
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-pc10433 Eros-centric (Eros = 433 + 10000)
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orbital elements:
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-orbel compute osculating orbital elements relative to the
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mean ecliptic J2000. (Note, all values, including time of
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pericenter vary considerably depending on the date for which the
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osculating ellipse is calculated
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special events:
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-solecl solar eclipse
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output 1st line:
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eclipse date,
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time of maximum (UT):
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geocentric angle between centre of Sun and Moon reaches minimum.
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core shadow width (negative with total eclipses),
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eclipse magnitudes:
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1. NASA method (= 2. with partial ecl. and
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ratio lunar/solar diameter with total and annular ecl.)
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2. fraction of solar diameter covered by moon;
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if the value is > 1, it means that Moon covers more than
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just the solar disk
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3. fraction of solar disc covered by moon (obscuration)
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with total and annular eclipses it is the ratio of
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the sizes of the solar disk and the lunar disk.
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Saros series and eclipse number
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Julian day number (6-digit fraction) of maximum
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output 2nd line:
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start and end times for partial and total phases
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delta t in sec
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output 3rd line:
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geographical longitude and latitude of maximum eclipse,
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totality duration at that geographical position,
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output with -local, see below.
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-occult occultation of planet or star by the moon. Use -p to
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specify planet (-pf -xfAldebaran for stars)
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output format same as with -solecl, with the following differences:
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Magnitude is defined like no. 2. with solar eclipses.
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There are no saros series.
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-lunecl lunar eclipse
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output 1st line:
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eclipse date,
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time of maximum (UT),
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eclipse magnitudes: umbral and penumbral
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method as method 2 with solar eclipses
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Saros series and eclipse number
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Julian day number (6-digit fraction) of maximum
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output 2nd line:
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6 contacts for start and end of penumbral, partial, and
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total phase
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delta t in sec
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output 3rd line:
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geographic position where the Moon is in zenith at maximum eclipse
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-local only with -solecl or -occult, if the next event of this
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kind is wanted for a given geogr. position.
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Use -geopos[long,lat,elev] to specify that position.
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If -local is not set, the program
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searches for the next event anywhere on earth.
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output 1st line:
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eclipse date,
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time of maximum,
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eclipse magnitudes, as with global solar eclipse function
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(with occultations: only diameter method, see solar eclipses, method 2)
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Saros series and eclipse number (with solar eclipses only)
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Julian day number (6-digit fraction) of maximum
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output 2nd line:
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local eclipse duration for totality (zero with partial occultations)
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local four contacts,
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delta t in sec
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Occultations with the remark "(daytime)" cannot be observed because
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they are taking place by daylight. Occultations with the remark
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"(sunrise)" or "(sunset)" can be observed only partly because part
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of them takes place in daylight.
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-hev[type] heliacal events,
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type 1 = heliacal rising
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type 2 = heliacal setting
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type 3 = evening first
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type 4 = morning last
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type 0 or missing = all four events are listed.
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-rise rising and setting of a planet or star.
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Use -geopos[long,lat,elev] to specify geographical position.
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-metr southern and northern meridian transit of a planet of star
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Use -geopos[long,lat,elev] to specify geographical position.
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specifications for eclipses:
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-total total eclipse (only with -solecl, -lunecl)
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-partial partial eclipse (only with -solecl, -lunecl)
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-annular annular eclipse (only with -solecl)
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-anntot annular-total (hybrid) eclipse (only with -solecl)
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-penumbral penumbral lunar eclipse (only with -lunecl)
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-central central eclipse (only with -solecl, nonlocal)
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-noncentral non-central eclipse (only with -solecl, nonlocal)
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specifications for risings and settings:
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-norefrac neglect refraction (with option -rise)
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-disccenter find rise of disc center (with option -rise)
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-discbottom find rise of disc bottom (with option -rise)
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-hindu hindu version of sunrise (with option -rise)
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specifications for heliacal events:
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-at[press,temp,rhum,visr]:
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pressure in hPa
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temperature in degrees Celsius
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relative humidity in %
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visual range, interpreted as follows:
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> 1 : meteorological range in km
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1>visr>0 : total atmospheric coefficient (ktot)
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= 0 : calculated from press, temp, rhum
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Default values are -at1013.25,15,40,0
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-obs[age,SN] age of observer and Snellen ratio
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Default values are -obs36,1
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-opt[age,SN,binocular,magn,diam,transm]
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age and SN as with -obs
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0 monocular or 1 binocular
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telescope magnification
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optical aperture in mm
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optical transmission
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Default values: -opt36,1,1,1,0,0 (naked eye)
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backward search:
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-bwd
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Planet selection letters:
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planetary lists:
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d (default) main factors 0123456789mtABCcg
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p main factors as above, plus main asteroids DEFGHI
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h ficticious factors J..X
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a all factors
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(the letters above can only appear as a single letter)
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single body numbers/letters:
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|
0 Sun (character zero)
|
|
1 Moon (character 1)
|
|
2 Mercury
|
|
3 Venus
|
|
4 Mars
|
|
5 Jupiter
|
|
6 Saturn
|
|
7 Uranus
|
|
8 Neptune
|
|
9 Pluto
|
|
m mean lunar node
|
|
t true lunar node
|
|
n nutation
|
|
o obliquity of ecliptic
|
|
q delta t
|
|
y time equation
|
|
b ayanamsha
|
|
A mean lunar apogee (Lilith, Black Moon)
|
|
B osculating lunar apogee
|
|
c intp. lunar apogee
|
|
g intp. lunar perigee
|
|
C Earth (in heliocentric or barycentric calculation)
|
|
For planets Jupiter to Pluto the center of body (COB) can be
|
|
calculated using the additional parameter -cob
|
|
dwarf planets, plutoids
|
|
F Ceres
|
|
9 Pluto
|
|
s -xs136199 Eris
|
|
s -xs136472 Makemake
|
|
s -xs136108 Haumea
|
|
some minor planets:
|
|
D Chiron
|
|
E Pholus
|
|
G Pallas
|
|
H Juno
|
|
I Vesta
|
|
s minor planet, with MPC number given in -xs
|
|
some planetary moons and center of body of a planet:
|
|
v with moon number given in -xv:
|
|
v -xv9501 Io/Jupiter:
|
|
v -xv9599 Jupiter, center of body (COB):
|
|
v -xv94.. Mars moons:
|
|
v -xv95.. Jupiter moons and COB:
|
|
v -xv96.. Saturn moons and COB:
|
|
v -xv97.. Uranus moons and COB:
|
|
v -xv98.. Neptune moons and COB:
|
|
v -xv99.. Pluto moons and COB:
|
|
The numbers of the moons are given here:
|
|
https://www.astro.com/ftp/swisseph/ephe/sat/plmolist.txt
|
|
fixed stars:
|
|
f fixed star, with name or number given in -xf option
|
|
f -xfSirius Sirius
|
|
fictitious objects:
|
|
J Cupido
|
|
K Hades
|
|
L Zeus
|
|
M Kronos
|
|
N Apollon
|
|
O Admetos
|
|
P Vulkanus
|
|
Q Poseidon
|
|
R Isis (Sevin)
|
|
S Nibiru (Sitchin)
|
|
T Harrington
|
|
U Leverrier's Neptune
|
|
V Adams' Neptune
|
|
W Lowell's Pluto
|
|
X Pickering's Pluto
|
|
Y Vulcan
|
|
Z White Moon
|
|
w Waldemath's dark Moon
|
|
z hypothetical body, with number given in -xz
|
|
sidereal time:
|
|
x sidereal time
|
|
e print a line of labels
|
|
|
|
|
|
Output format SEQ letters:
|
|
In the standard setting five columns of coordinates are printed with
|
|
the default format PLBRS. You can change the default by providing an
|
|
option like -fCCCC where CCCC is your sequence of columns.
|
|
The coding of the sequence is like this:
|
|
y year
|
|
Y year.fraction_of_year
|
|
p planet index
|
|
P planet name
|
|
J absolute juldate
|
|
T date formatted like 23.02.1992
|
|
t date formatted like 920223 for 1992 february 23
|
|
L longitude in degree ddd mm'ss"
|
|
l longitude decimal
|
|
Z longitude ddsignmm'ss"
|
|
S speed in longitude in degree ddd:mm:ss per day
|
|
SS speed for all values specified in fmt
|
|
s speed longitude decimal (degrees/day)
|
|
ss speed for all values specified in fmt
|
|
B latitude degree
|
|
b latitude decimal
|
|
R distance decimal in AU
|
|
r distance decimal in AU, Moon in seconds parallax
|
|
W distance decimal in light years
|
|
w distance decimal in km
|
|
q relative distance (1000=nearest, 0=furthest)
|
|
A right ascension in hh:mm:ss
|
|
a right ascension hours decimal
|
|
m Meridian distance
|
|
z Zenith distance
|
|
D declination degree
|
|
d declination decimal
|
|
I azimuth degree
|
|
i azimuth decimal
|
|
H altitude degree
|
|
h altitude decimal
|
|
K altitude (with refraction) degree
|
|
k altitude (with refraction) decimal
|
|
G house position in degrees
|
|
g house position in degrees decimal
|
|
j house number 1.0 - 12.99999
|
|
X x-, y-, and z-coordinates ecliptical
|
|
x x-, y-, and z-coordinates equatorial
|
|
U unit vector ecliptical
|
|
u unit vector equatorial
|
|
Q l, b, r, dl, db, dr, a, d, da, dd
|
|
n nodes (mean): ascending/descending (Me - Ne); longitude decimal
|
|
N nodes (osculating): ascending/descending, longitude; decimal
|
|
f apsides (mean): perihelion, aphelion, second focal point; longitude dec.
|
|
F apsides (osc.): perihelion, aphelion, second focal point; longitude dec.
|
|
+ phase angle
|
|
- phase
|
|
* elongation
|
|
/ apparent diameter of disc (without refraction)
|
|
= magnitude
|
|
v (reserved)
|
|
V (reserved)
|
|
|
|
Date entry:
|
|
In the interactive mode, when you are asked for a start date,
|
|
you can enter data in one of the following formats:
|
|
|
|
1.2.1991 three integers separated by a nondigit character for
|
|
day month year. Dates are interpreted as Gregorian
|
|
after 4.10.1582 and as Julian Calendar before.
|
|
Time is always set to midnight (0 h).
|
|
If the three letters jul are appended to the date,
|
|
the Julian calendar is used even after 1582.
|
|
If the four letters greg are appended to the date,
|
|
the Gregorian calendar is used even before 1582.
|
|
|
|
j2400123.67 the letter j followed by a real number, for
|
|
the absolute Julian daynumber of the start date.
|
|
Fraction .5 indicates midnight, fraction .0
|
|
indicates noon, other times of the day can be
|
|
chosen accordingly.
|
|
|
|
<return> repeat the last entry
|
|
|
|
. stop the program
|
|
|
|
+20 advance the date by 20 days
|
|
|
|
-10 go back in time 10 days
|
|
|
|
|
|
Examples:
|
|
|
|
swetest -p2 -b1.12.1900 -n15 -s2
|
|
ephemeris of Mercury (-p2) starting on 1 Dec 1900,
|
|
15 positions (-n15) in two-day steps (-s2)
|
|
|
|
swetest -p2 -b1.12.1900 -n15 -s2 -fTZ -roundsec -g, -head
|
|
same, but output format = date and zodiacal position (-fTZ),
|
|
separated by comma (-g,) and rounded to seconds (-roundsec),
|
|
without header (-head).
|
|
|
|
swetest -ps -xs433 -b1.12.1900
|
|
position of asteroid 433 Eros (-ps -xs433)
|
|
|
|
swetest -pf -xfAldebaran -b1.1.2000
|
|
position of fixed star Aldebaran
|
|
|
|
swetest -p1 -d0 -b1.12.1900 -n10 -fPTl -head
|
|
angular distance of moon (-p1) from sun (-d0) for 10
|
|
consecutive days (-n10).
|
|
|
|
swetest -p6 -DD -b1.12.1900 -n100 -s5 -fPTZ -head -roundmin
|
|
Midpoints between Saturn (-p6) and Chiron (-DD) for 100
|
|
consecutive steps (-n100) with 5-day steps (-s5) with
|
|
longitude in degree-sign format (-f..Z) rounded to minutes (-roundmin)
|
|
|
|
swetest -b5.1.2002 -p -house12.05,49.50,K -ut12:30
|
|
Koch houses for a location in Germany at a given date and time
|
|
|
|
swetest -b1.1.2016 -g -fTlbR -p0123456789Dmte -hor -n366 -roundsec
|
|
tabular ephemeris (all planets Sun - Pluto, Chiron, mean node, true node)
|
|
in one horizontal row, tab-separated, for 366 days. For each planet
|
|
list longitude, latitude and geocentric distance.
|
|
|
|
</return></font>
|
|
</pre>
|
|
<p>
|
|
</p></td></tr></tbody></table>
|
|
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