The Circumnavigation of Mercury

Oh dear, levitation; it's time to cool the GPU.

Levitation.png
 
(0,89)

Another huge impact crater took a long time to negotiate - no skimming over the rocks, just picking your way boulder by boulder across a surface that seems, suddenly, to be very slippy.

(0,88).png
(0,89).png
 
I can't tell whether Earth has moved in the five hours fifty minutes as I travelled 4 degrees to the East and Mercury itself rotated 1.5 degrees eastwards. Maybe it's too soon to see it.

EarthObs01.png

EarthObs02.png

EarthObs03.png
 
Still at (0,91), I can convince myself that Earth has moved within that quadrilateral of distant stars. In the 9 hours since the last observation, Mercury has rotated on its axis by 2.3 degrees [ (9/24)*(360/58.6) ]. That's why Earth's altitude has risen to a shade under 10 degrees. My sextant is not the most accurate and the methodology is dubious, but I'm happy to say the Earth moved for me.

EarthObs04.png
 
(0,94), Earth altitude: 14.2 degrees.

Now I want to find the other Sol system bodies. Venus is to the North and Mars to the North-West, according to the orrery view.

(0,94).png
 
Planets.png


I made a quick scan of the sky using the ship's sysmap. None of the other major planets are currently visible. However, there's a good chance of seeing Venus and Neptune in about 50 degrees time and Jupiter after another 68 degrees of eastward travel.
 
This sequence of images shows the orbit of Earth relative to the fixed stars. This orbit defines the ecliptic plane.

Earth orbit.png


And in this image I've tried to show the tilt of the ecliptic relative to the galactic plane. To illustrate this, I've transferred the galactic plane to coincide with Earth.

Tilt of the ecliptic.png
 
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