Live state
- Distance from Sun
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- Orbital speed
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- Radial velocity
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- Heliocentric x, y, z
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- Distance from Earth
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- Light travel time
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- Geocentric longitude
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Kepler's equation
M = E − e·sin E
- Mean anomaly M
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- Eccentric anomaly E
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- True anomaly ν
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- Newton iterations
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- Residual
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Orbit
- Semi-major axis a
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- Eccentricity e
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- Inclination i
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- Perihelion q
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- Aphelion Q
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- Sidereal period
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- Next perihelion
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- Kepler III: a³ / T²
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- Areal velocity (Kepler II)
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The shaded wedge is the area swept in one twelfth of the period. It stretches near perihelion and narrows near aphelion.
Rotation
- Sidereal day
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- Axial tilt
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- Spin direction
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Detected motion events
Perihelion, aphelion and retrograde stations are detected here as the simulation runs. Speed time up to see them sooner.