The Interactive 3D Solar System Simulation working explained
The Interactive 3D Solar System Simulation is created such that all the planets and the Moon revolve around uniformly circular orbits at constant speed. However all planets have two circular motions added. Therefore effectively they function as an elliptical orbital movement in the model.
The only real difference between the current heliocentric model of our solar system and the Interactive 3D Solar System Simulation is therefore the lack of variable speeds. Kepler had to add variable speeds in order to fit his model to observations. Having variable speeds of planets means for instance Mercury moves at an orbital speed that varies from about 59 km/s at perihelion to 39 km/s at aphelion. That is quite unrealistic to me, but I will leave it up to scientist if these speed differences are really needed.
I have added all planets with orbital sizes and distances EXACTLY according to Keplerâs 3rd law.
âKeplerâs Third Law of Planetary Motion: The square of the period of a planetâs orbit around the sun is proportional to the cube of the size of its orbitâ
You can check all input numbers in the Excel.
What is both really annoying AND very nice about this model is that you cannot cheat with the movements, in contrary to all known heliocentric (3D) models â which are just based upon some measurement in time and predictions about the movement in between. Therefore those models are always more or less right. This Interactive 3D Solar System Simulation is programed once and it cannot be fixed along the way. It will perpetually be running.
I mostly focused the Interactive 3D Solar System Simulation on all precession cycles. The movements of the most important solar bodies are however added in the model. So far, it seems to be in concordance with all recorded planetary ephemerides, Mars oppositions, the transits of Venus and Mercury across the Sunâs disk, Jupiter-Saturn conjunctions, most other periodic interplanetary alignments and all solar and lunar eclipses. The model however also can be refined further. I have added an Excel with all background data which will help in constructing the geo-heliocentric model of our universe. Feel free to improve them!
There are a number of TABs in the Excel that should be self-explanatory. The only thing you really need to know is the YELLOW cells are Input cells. you can change the values, but be careful, other cells are most probably dependant on them.
Below I summed up some clear instructions how to use the Interactive 3D Solar System Simulation.
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Some basic instructions and tips for starters:
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Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
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Click the ârunâ button to start the Interactive 3D Solar System Simulation. You may then choose to speed up or slow down its motion with the â1 second equalsâ function.
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Left-clicking (and holding) your mouse will let you toggle at will the 3-D orientation of our cosmos. The scroll wheel regulates the zoom level. You can off course also use your laptopâs touchpad to zoom in/out.
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Showing the Right Ascension, Declination & Distances values of solar system bodies in the model
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Go to âCelestial Positionsâ and you will see these results
You will see all planets and objects with the proper values of Right Ascension, Declination & Distances. These âcelestial positionsâ (ephemerides) of any of our solar systemâs bodies, can be compared and verified for yourselves with other online planetariums such as the popular Stellarium simulatorâ
Let me explain the most important âCelestial Positionsâ at the start of the Interactive 3D Solar System Simulation on date 21st of June 00:00 UTC 2000 AD.
- Date = 2000-06-21
- Time (UTC) = 00:00:00
- Julian day = 2451716.5
- RA = 06h51m48s
- Dec
- Distance to Earth = 0.016710112 AU
- Distance to Sun = 1 AU
- RA = 07h03m17s
- Dec
- Distance to Earth = 0.01370018 AU
- Distance to Sun = 1.00308205 AU
- RA = 05h59m39s
- Dec = +23°26'21â
- Distance to Earth = 1.01633048 AU
- Distance to Sun = 0 AU
A) The top three settings provide the Date, Julian day and Time (UTC). These are the input values.
- The âDateâ and âJulian dayâ are interchangeable. Change one of them (and press enter) and you will see they are related.
- The âTime (UTC)â element is in hours. If you want to show the exact position in your local time, you can use a UTC time converterâ.
B) The âRAâ values of the PERIHELION-OF-EARTH and MID-ECCENTRICITY-POINT:
- The PERIHELION-OF-EARTH âRAâ position shows the RA value of 06h51m48s which is ~102.9506°.
- The âRAâ values of the PERIHELION-OF-EARTH are fully in line with the Longitude of Perihelion values as provided via the Formula by J. Meeus as mentioned in chapter 1.
- The MID-ECCENTRICITY-POINT âRAâ position shows the RA value of 07h03m17s which is ~105.8214°. As explained in chapter 3 and 4 the real value of the Longitude of perihelion is already further away since it is actually measured from the EARTH-WOBBLE-CENTER which is the mid eccentricity point. This is also the reason why ALL PRECESSION MOVEMENTS are currently experienced to take longer than the mean values (e.g. Axial precession currently experienced ~25,772 years/ mean ~22,937 years).
- The âRAâ values of the PERIHELION-OF-EARTH and MID-ECCENTRICITY-POINT change cyclic in a repeating cycle of 18,636 years.
C) The âDistance to Earthâ values of the PERIHELION-OF-EARTH and the MID-ECCENTRICITY-POINT:
- The PERIHELION-OF-EARTH âDistance to Earthâ position shows the eccentricity of 0.016710112. Since the real movement of the PERIHELION-OF-EARTH is around the Sun, the max value of the distance from Earth to the PERIHELION-OF-EARTH in 2000 AD is +1 = 1.016710112.
- The MID-ECCENTRICITY-POINT âDistance to Earthâ position shows the eccentricity of 0.01370018 which is the mean value of the orbital eccentricity of Earth compared to the Sun.
- The âDistance to Earthâ value of the MID-ECCENTRICITY-POINT stays fixed since the MID-ECCENTRICITY-POINT is a helping point for calculating the length of days and years and not a gravitational point.
- The âDistance to Earthâ value of the PERIHELION-OF-EARTH changes in a repeating cycle of 18,636 years.
D) The âRAâ and âDecâ values of the Sun:
- The âRAâ value from the Sun shows the actual RA value of the Sun on date 21st of June 00:00 UTC being 05h59m39s.
- The âDecâ value from the Sun shows the Sun is highest in the Sky with a âDecâ value of +23°26â21â on the Northern hemisphere at that date/ time.
- The Sun was highest in the sky later in the morning at 01:47. See the pageâ. All dates and times are aligned in the Interactive 3D Solar System Simulation to the June Solstice dates.
- The âDecâ value from the Sun is fully in line with the Obliquity value as provided via the Formula by Chapront et al/ J. Laskar as mentioned in chapter 1.
- The âDecâ value (Declination) is the âObliquityâ of the Sun as seen from Earth and its behaviour can best be shown by adding or subtracting a few hours around the 21st of June 2000 AD 01:47 UTC time. In both directions the obliquity value will DECREASE.
- The âDecâ value (Declination) MAXIMUM value on the SOUTHERN HEMISPHERE (= MINIMUM value on NORTHERN HEMISPHERE) is half a year later (and earlier) and is best shown by adding or subtracting a few hours around the 21st of December 2000 01:47 UTC time. In both directions the obliquity value of -23°26â21â will INCREASE.
- The âRAâ and âDecâ values of the Sun changes cyclic in one solar year AND on the longer term the âRAâ and âDecâ max/min values changes slightly in a repeating cycle of 298,176 years.
E) The âDistance to Earthâ values of the Sun:
- The Sun âDistance to Earthâ position shows the actual eccentricity of 1.01633048 on date 2000-06-21. This value is less than the MAXIMUM value for this year 2000 AD which is the PERIHELION-OF-EARTH value of 0.01671012 since Earth is furthest from the Sun in 2000 AD on 3th of July 09:00 UTC when the Sun was at RA 06h51m48s and NOT on 21st of June 00:00 UTC. You can go to this date to check it for yourself.
- This maximum âDistance to Earthâ value of the Sun is in line with the values provided via the Orbital eccentricity Formula as mentioned in chapter 1.
- The Sun âDistance to Earthâ behaviour can best be shown by adding or subtracting a few hours around the date of its maximum value on 3rd of July 09:00 UTC time. In both directions the âDistance to Earthâ value will DECREASE.
- The Sun âDistance to Earthâ MIMIMUM value is half a year earlier (or later) and its behaviour can best be shown by adding or subtracting a few hours around the date of its minimum value of â0.98329878â (1-0.98329878 = 0.01671022) around 2nd of January 2000 AD 17:00 UTC time. In both directions the âDistance to Earthâ value will INCREASE.
- The âDistance to Earthâ of the Sun changes cyclic in one solar year AND on the longer term these values changes slightly in a repeating cycle of 18,636 years.
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Showing the zodiac wheel in the model
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Open âCelestial Toolsâ
- Select âZodiacâ
You will see the Zodiac wheel as it is experienced on Earth. You can make it larger or smaller. It is centered on earth since we are the ones observing it. The Zodiac stays fixed in time, since Earth is moving in the ICRF.
With the zodiac wheel you will see the orientation of Earth compared to the 12 zodiac constellations.
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Have a look at the EARTH-WOBBLE-CENTER and PERIHELION-OF-EARTH
Earth is wobbling around the EARTH-WOBBLE-CENTER. In the 3D model it is modelled as âThe Death Starâ and the PERIHELION-OF-EARTH as the white version of it since it is orbiting in the opposite direction.
The EARTH-WOBBLE-CENTER is currently in front up the constellation Orion.
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Open âCelestial Toolsâ
- Choose âStar namesâ and âConstellationsâ
- Tilt the angle to the location of âEARTH-WOBBLE-CENTERâ
- Just a little to the left and a bit further away is the âPERIHELION-OF-EARTHâ
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Showing the axial tilt of the earth in his movements in a year with the Sun at the center
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Open âCelestial Toolsâ
- Select âPolar lineâ
- Go to âLook atâ and select the âSunâ
- You can close the extra information box (and orbit grid) by pressing the cross next to it
Now you can tilt the view, such you have a 90 degree view on our solar system.
- Select the option â1 second equalsâ â1 monthâ
- Press âRunâ
You will see Earth orbiting the Sun and along the path of a year, the axial tilt stays pointed to the same location (Polaris). So in a 1 year orbit, the tilt does hardly move at all, although we are travelling from one side of the Sun to the completely other side of the Sun (300m km).
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Showing the axial tilt of the earth in his movements in a year as if Earth (actually EARTH-WOBBLE-CENTER) is at the center
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Open âCelestial Toolsâ
- Select âPolar lineâ
- If you selected another planet, go to âLook atâ and select âEarthâ again (and close the information box)
Now you can tilt the view, such you have a 90 degree view on our solar system.
- Select the option â1 second equalsâ â1 monthâ
- Press âRunâ
You will see Sun orbiting around Earth and along the path of a year, the axial tilt stays pointed to the same location (Polaris). So in a 1 year orbit, the tilt does not move at all because the Earth is only traveling slowly on its Axial Precession Orbit (APO).
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Showing the axial tilt of the earth in his movements in a Great year
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Open âCelestial Toolsâ
- Select âPolar lineâ
- Select âStar namesâ
Now you can tilt the view, such you see Polaris. You can also zoom into Earth a bit
- Select the option â1 second equalsâ â1000 yearsâ
- Press âRunâ
You will see the axial precession moving in a cycle of ~22,937 years from Polaris to Polaris.
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Showing the Moon always facing the same side to Earth
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Zoom in to have a closer look at Earth and the Moon
- Select the option â1 second equalsâ â1 dayâ
- Press âRunâ
You will see the Earth rotating on its axis, and the Moon orbiting Earth with the same face. You can also speed up to â1 second equalsâ â1 weekâ.
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Showing the Moon Apsidal precession
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Zoom in to have a closer look at Earth and the Moon without tilting the view
- Select the option â1 second equalsâ â1 yearâ
- Press âRunâ
You will see the Moon apsides (furthest and closest to Earth) rotate in a mean duration of ~8.85 years. You can also speed up to â1 second equalsâ â10 yearsâ.
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Showing the Moon Nodal precession
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Zoom in to have a closer look at Earth and the Moon and tilt the view to the same level as the ecliptic
- Select the option â1 second equalsâ â1 yearâ
- Press âRunâ
You will see the Moon rotating on its axis in a mean duration of ~18.6 years (in the opposite direction of the Apsidal precession). You can also speed up to â1 second equalsâ â10 yearsâ.
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Showing the Moonâs Lunar standstillâ dates
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Open âCelestial Toolsâ
- Select âPolar lineâ
- Fill in at âJulian dayâ â2450538â or at âDateâ â1997-03-30â
- Zoom in to have a closer look at Earth and the Moon, such you see the Earth and Moon and EARTH-WOBBLE-CENTER
- Go to âCelestial Positionsâ
Look at the Right Ascension, Declination & Distances numbers from the âMoonâ You will see the Moon Declination with a value of -18°17â27â.
- Select the option â1 second equalsâ â1 hourâ
- Press âStep backwardâ
You will see the Moon almost getting in line with EARTH-WOBBLE-CENTER at 11:00 with a maximum declination -18°17â31â. If you go 1 hour earlier or further you will see the declination to go down. This is the maximum declination at that specific date. By using this method we can create a diagram:
Juliandate Date Time Declination Juliandate Date Time Declination 2450401 1996-11-13 23:00 -18°13â54â 2450415 1996-11-27 04:00 +18°25â36â 2450429 1996-12-11 07:00 -18°14â07â 2450442 1996-12-24 11:00 +18°25â03â 2450456 1997-01-07 14:00 -18°14â36â 2450471 1997-01-20 18:00 +18°24â45â 2450483 1997-02-03 21:00 -18°15â20â 2450497 1997-02-17 01:00 +18°24â41â 2450511 1997-03-03 04:00 -18°16â18â 2450524 1997-03-16 08:00 +18°24â52â 2450538 1997-03-30 11:00 -18°17â31â 2450551 1997-04-12 15:00 +18°25â17â 2450565 1997-04-26 18:00 -18°18â60â 2450578 1997-05-09 22:00 +18°25â57â 2450592 1997-05-24 01:00 -18°20â42â 2450606 1997-06-06 05:00 +18°26â51â So the Minor Lunar standstill happened somewhere around early 1997.
We can do the same for the major lunar standstill:
Juliandate Date Time Declination Juliandate Date Time Declination 2453775 2006-02-08 16:00 +28°35â38â 2453790 2006-02-22 19:00 -28°37â52â 2453802 2006-03-08 00:00 +28°36â24â 2453817 2006-03-22 03:00 -28°37â36â 2453830 2006-04-04 08:00 +28°37â01â 2453844 2006-04-18 11:00 -28°37â10â 2453857 2006-05-02 00:00 +28°31â53â 2453871 2006-05-15 19:00 -28°36â35â 2453884 2006-05-29 00:00 +28°37â45â 2453899 2006-06-12 04:00 -28°35â50â 2453912 2006-06-25 08:00 +28°37â52â 2453926 2006-07-09 12:00 -28°34â57â 2453939 2006-07-22 17:00 +28°37â49â 2453953 2006-08-05 20:00 -28°33â53â 2453967 2006-08-19 01:00 +28°37â38â 2453981 2006-09-02 04:00 -28°32â40â 2453994 2006-09-15 09:00 +28°37â16â 2454008 2006-09-29 12:00 -28°31â17â 2454021 2006-10-12 17:00 +28°36â44â 2454035 2006-10-26 20:00 -28°29â44â 2454049 2006-11-09 01:00 +28°36â02â 2454063 2006-11-23 04:00 -28°28â02â So the Major Lunar standstill happened somewhere around mid 2006.
I have shown you the minor and major lunar standstill moments in time. It is fluctuating in a mean period of ~18.6 years between ~18° degrees to ~28.5° degrees. You can also look at above dates with the objects on (see âShowing the Moon Nodal precessionâ).
- Open âObjects show/hideâ
- Select âMoon Apsidal Nodalâ AND âMoon Nodal Precessionâ
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Showing aphelion aligned with the Sun on 4th of July 2003 AD 03:35 UTC
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Fill in at âJulian dayâ â2452825â or at âDateâ â2003-07-04â and hour â03:35â
- Zoom in to have a closer look at the level you see Earth and the Moon Now you can tilt the view, but you have to turn around 180 degrees such you see the Sun.
You will see the PERIHELION-OF-EARTH, white dot, aligned with the Sun. In 2003 AD the Aphelion alignment was on 4th of July 03:35 and in line with Sun closest to earth (perihelion).
You can also check the Celestial Positions and see it is fully aligned. You can also check this date in existing simulators e.g. Stellarium. The exact value of alignment is hard to program because it is fluctuating as can be seen over hereâ. The values added in the Interactive 3D Solar System Simulation are the values according to the trend. There is for instance also a difference between the values in Stellarium webâ and Stellarium softwareâ.
- Go to âCelestial Positionsâ in the Interactive 3D Solar System Simulation and you will see these results
- Date = 2003-07-04
- Time (UTC) = 03:35:00
- Julian day = 2452825
- RA = 06h52m01s
- Dec
- Distance to Earth = 0.01670047
- Distance to Sun = 1 AU
- RA = 06h52m01s
- Dec = +22°53'59â
- Distance to Earth = 1.01670047 AU
- Distance to Sun = 0 AU
A) On that particular date and time you will see the PERIHELION-OF-EARTH and Sun BOTH have a âRAâ value of 06h52m01s AND BOTH have an âDistance to Earthâ value of 0.01670047.
- This means the Sun has reached its furthest distance from the Earth at that moment in time.
B) On that particular date and time you will see the Sun has a âDecâ value of +22°53â59â.
- The Sun is no longer at its maximum possible obliquity at that moment in time. It was maximum around 21st of June 01:47 UTC in that year.
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Showing perihelion aligned with solstice in December 1245 AD
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Fill in at âJulian dayâ â2176141.5â or at âDateâ â1245-12-14â and âTimeâ â00:00:00â.
- Zoom in to have a closer look at the level you see Earth and the Moon Now you can tilt the view, but you have to turn around 180 degrees such you see the Sun.
You will see the PERIHELION-OF-EARTH, white dot, aligned with EARTH-WOBBLE-CENTER, black dot. In 1245 AD (start of Year 1246 AD) the December solstice was on 14th of Decemberâ and in line with Sun closest to earth (perihelion).
- Go to âCelestial Positionsâ and you will see these results
- Date = 1245-12-14
- Time (UTC) = 00:00:00
- Julian day = 2176141.5
- RA = 05h59m60s
- Dec = +23°32'14â
- Distance to Earth = 0.01678229 AU
- Distance to Sun = 1 AU
- RA = 06h00m00s
- Dec = +23°25'38â
- Distance to Earth = 0.01370018 AU
- Distance to Sun = 0.99691791 AU
- RA = 18h00m03s
- Dec = -23°32'14â
- Distance to Earth = 0.9837444 AU
- Distance to Sun = 0 AU
A) On that particular date and time you will see the PERIHELION-OF-EARTH and MID-ECCENTRICITY-POINT BOTH have a âRAâ value of 06h00m00s.
- This means the Earth-axis is EXACTLY ALIGNED with the PERIHELION-OF-EARTH
- This means the perihelion precession cycle of 18,636 years starts/ends.
B) On that particular date and time you will see the Sun has a âDecâ value of -23°32â14â.
- The âDecâ value from the Sun shows the Sun is highest in the Sky with a âDecâ value of 23°32â14â on the Southern hemisphere at that date/ time.
- The âDecâ value from the Sun is fully in line with the Obliquity value as provided via the Formula by Chapront et al/ J. Laskar as mentioned in chapter 1.
- The âDecâ value (Declination) is the âObliquityâ of the Sun as seen from Earth and its behaviour can best be shown by adding or subtracting a few hours around the 14th of December 1245 AD 00:00 UTC time. In both directions the obliquity value will INCREASE.
- This means this date was a solstice day.
C) On that particular date and time you will also see the PERIHELION-OF-EARTH and Sun BOTH have a âDecâ value of 23°32â14â.
- This means the perihelion precession cycle of 18,636 years starts/ends.
D) On that particular date and time you will see the PERIHELION-OF-EARTH and Sun (1-0.98321771) BOTH have a âDistance to Earthâ value of 0.01678229.
- This means the Sun has reached its closest distance from the Earth at that moment in time AND ALSO reached its possible max orbital eccentricity in the 18,636 year cycle.
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Showing the perihelion aligned with solstice in year 8072 BC with the Four Royal Stars.
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Fill in at âJulian dayâ â-1227187.5â or at âDateâ â-8072-02-23â and âTimeâ 00:00:00.
- Zoom in to have a closer look at the level you see Earth and the Moon. Now you can tilt the view such you see the Sun.
You will see the PERIHELION-OF-EARTH, white dot, aligned with EARTH-WOBBLE-CENTER, black dot. In Year 8072 BC the December solstice was on 23rd of February and in line with Sun furthest from earth (aphelion).
- Go to âCelestial Positionsâ and you will see these results
- Date = -8072-02-23
- Time (UTC) = 00:00:00
- Julian day = -1227187.5
- RA = 17h59m59s
- Dec
- Distance to Earth = 0.01061807 AU
- Distance to Sun = 1 AU
- RA = 17h59m60s
- Dec
- Distance to Earth = 0.01370018 AU
- Distance to Sun = 0.99692097 AU
- RA = 17h53m36s
- Dec = -24°23'60â
- Distance to Earth = 1.01061462 AU
- Distance to Sun = 0 AU
A) On that particular date and time you will see the PERIHELION-OF-EARTH and MID-ECCENTRICITY-POINT BOTH have a âRAâ value of 18h00m00s.
- This means the Earth-axis is EXACTLY ALIGNED with the PERIHELION-OF-EARTH
- This means the perihelion precession cycle of 18,636 years is mid-way.
B) On that particular date and time you will see the Sun has a âDecâ value of -24°23â60â.
- The âDecâ value from the Sun shows the Sun is highest in the Sky with a âDecâ value of -24°23â60â on the Southern hemisphere at that date/ time.
- The âDecâ value (Declination) is the âObliquityâ of the Sun as seen from Earth and its behaviour can best be shown by adding or subtracting a few hours around the 23rd of February 8072 BC 00:00 UTC time. In both directions the obliquity value will INCREASE.
- This means this date was a solstice day.
C) Around that particular date and time you will see the PERIHELION-OF-EARTH and Sun BOTH have a âAU Distanceâ value of 0.01061807.
- This means the Sun has reached its furthest distance from the Earth around that moment in time AND ALSO reached its possible min orbital eccentricity in the 18,636 year cycle.
Now letâs have a look at the stars around that time.
- Open âCelestial Toolsâ
- Select âStar namesâ
- Select âConstellationsâ
You will see the PERIHELION-OF-EARTH, white dot to be more or less aligned with the star âAldebaranâ. Turn around 180 degrees, you will see the PERIHELION-OF-EARTH more or less aligned with the star âAntaresâ. Turn 90 degrees back and forth and you will the Stars âFomalhautâ and âRegulusâ. These 4 stars form a Square / Cross and are called the Four Royal Stars a.k.a. the Guardians of the Sky.
These stars are most probably the reason why certain Coat of armsâ/ Royal houses have Eagles, Lions and Bulls in them, including 17,000 years old cave paintingsâ, and are depicted on ancient art piecesâ a lot. Just browse a day on the internet and you will see the references all over the place including depictions of Jesus with the four archangels.
These stars, represented by their zodiac sign, are also depicted on the Pillars in Göbleki Tepeâ which is at the core of our civilisation.
Göbleki Tepe was build around 9,500 BCâ. The site covers over 90 soccer fields but is only expedited for a very small 5 percentageâ. The intention of the owning DoÄuĆ Groupâ, is to keep it buried âfor future generationsââ.
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Showing the start of the Age of Aquarius in year 1962 AD
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Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
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Open âCelestial Toolsâ
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Select âZodiacâ
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Zoom in to have a closer look at the level you see EARTH-WOBBLE-CENTER.
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Fill in at âJulian dayâ â2437745â or at âDateâ â1962-03-21â
You will see the zodiac wheel EXACTLY is aligned with EARTH-WOBBLE-CENTER.
To be even more complete, the real date when exactly the Age of Aquarius starts/ started is hard to say. Since the actual start is related to the movement of the longitude of perihelion and this is not a fixed movement but sometimes speeds up and sometimes slows down. The mentioned mean duration of the precession of the Equinoxes is therefore not exactly ~22,937 years. This movement speeds up and slows down as well.
If we âjustâ stick to dividing the cycle of ~22,937 years into 12 equal pieces of ~1911.385 years (298,176/(12*13)) each and as a result we are truly living in the Age-of-Aquarius since the year 1962 AD.
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Showing Mars in opposition to Earth (e.g. in year 2003 AD)
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Fill in at âJulian dayâ â2452880â or at âDateâ â2003-08-28â at time â12:00:00â
- Zoom in and tilt a little to see Earth between Mars and the Sun.
- Open Celestial Positions and see the Sun at RA â10h30m10sâ and Mars at RA â22h30m55sâ.
- Date = 2003-08-28
- Time (UTC) = 12:00:00
- Julian day = 2452880
- RA = 10h30m10s
- Dec
- Distance to Earth = 1.00977618 AU
- Distance to Sun = 0 AU
- RA = 22h30m55s
- Dec
- Distance to Earth = 0.37152020 AU
- Distance to Sun = 1.38012636 AU
You can compare those with values in Stellarium.
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Showing the 5 petals structure of Venus
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Click on the âSelect objects to traceâ MENU and deselect the default settings and select âVenusâ to determine which planets you want to trace.
- Select the option â1 second equalsâ â1 yearâ
- Select the Enable tracing BOX, to turn the trace actually on
- Press âRunâ
You will see the â5 petalsâ by Venus on its trip around the Sun appearing.
You can also see the petals moving in clockwise direction with:
- Select the option â1 second equalsâ â10 yearsâ
NOTE be careful to select larger amounts of time because the traces are calculated. Your browser might stall. Just press the RUN button ONCE more and wait a few seconds so it can end normally. In my browser 100 years is still doable but above the figures it doesnât work anymore.
You can choose any celestial body for which you wish to exhibit its path around our system over time. This will show you the beautiful âmandala-likeâ, spinographic trajectories of our Solar Systemâs various bodies.
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Showing the location of the barycenter of all planets
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Open âPerihelion Planetsâ
- Select the âPerihelion Spiralâ
- Select the option â1 second equalsâ â1000 yearsâ
- Press âRunâ
You will see the planet perihelion points in the Perihelion Spiral turn.
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Showing the PERIHELION-OF-EARTH moving 360° in 99,392 years.
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Zoom in to have a closer look at the level you see Earth and the Moon. No need to tilt. Just zoom
You will see a white dot: The PERIHELION-OF-EARTH
- Select the option â1 second equalsâ â1000 yearsâ
- Press âRunâ
You will see the PERIHELION-OF-EARTH moving 360° in 99,392 years around EARTH-WOBBLE-CENTER.
- Go to Speed multiplier and put it to max 5.
Now you will see it even more clearly.
- Now click the checkbox âTraceâ. By default both the âPERIHELION-OF-EARTHâ and âMID-ECCENTRICITY-ORBITâ are selected.
If you Click âTraceâ and âRunâ, you will notice Axial meets Inclination in a perihelion precession cycle of 18,636 years so if you leave it running you will see the Holistic-Year cycle resulting on a famous ancient pattern where solstice meets perihelion 16 times on the zodiac wheel.
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Showing Earth moving along the Axial Precession Orbit (APO) through time
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Open âCelestial Toolsâ
- Select âPolar lineâ
- Zoom in to have a closer look at the level you see EARTH-WOBBLE-CENTER.
- Select the option â1 second equalsâ â1000 yearsâ
- Press âRunâ
You will see the axial precession moving in a cycle of ~22,937 years from Polaris to Polaris.
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Showing Earth maximum obliquity date
- Go to the 3D Model (link in right top corner) (OR just press âRESETâ)
- Fill in at âJulian dayâ â-42172125.75â or at âDateâ â-120173-01-05â
You will see Sun maximum obliquity at that date being -24°34â38â which is ~24.5801°. This is quite observable because ~23.42723+~0.564+~0.564+ is a little less.
NOTE the theoretically minimum possible obliquity in the Interactive 3D Solar System Simulation is a little smaller than ~23.42723-~0.564-~0.564 because when the inclination is at its highest point, the axial tilt is never maximum.
If you play with all above mentioned settings, AND read this book, AND study the Excel intensively, you will most probably understand the Interactive 3D Solar System Simulation.