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The science
Tides. The tide-generating force from a body of mass M at distance d scales as M / d³ (the difference of gravity across Earth, not gravity itself). Moon: 7.342×10²² kg at 384,400 km; Sun: 1.989×10³° kg at 149.6 million km. Ratio Moon : Sun = (Mm/dm³)/(Ms/ds³) ≈ 2.18. Without the Moon only the solar tide remains: about 31% of today's spring range and 46% of the average range, and the 14.8-day spring/neap beat (two close frequencies, M2 12.42 h and S2 12.00 h, drifting in and out of phase) disappears.
The water level is a sum of tidal constituents h(t) = G · Σ Ai cos(ωi t + φi) with equilibrium amplitudes M2 0.244 m, S2 0.114, N2 0.047, K1 0.142, O1 0.101, P1 0.047 m (Cartwright-Doodson type values). The site gain G (resonance of the local basin) is calibrated so today's spring range matches the coast you choose. Lunar terms scale as (d0/d)³; the Moon's frequencies follow Kepler's third law (period ∝ d3/2). The 3D bulge is the equilibrium tide, exaggerated roughly a million times.
Axial tilt. The spin axis s obeys ds/dt = α (s·n)(s×n), where n is the orbit normal and α the precession constant: about 50.3 arcsec/yr today, of which the Sun gives ~15.9 and the Moon ~34.4 (so α falls to ~16 without the Moon). The orbit normal wobbles because of the planets, here as six sinusoids with the real nodal frequencies (-5.6, -7.1, -17.7, -18.9, -26.4, -3.0 arcsec/yr) and rough amplitudes. With the Moon the model reproduces the 41,000-year cycle and a ~2 degree range; without it the precession rate falls into the band of planetary frequencies and resonances stir the tilt. Published results: Laskar, Joutel and Robutel (Nature 1993) found a moonless obliquity wandering chaotically between about 0 and 85 degrees over millions of years, versus 22.1-24.5 degrees with the Moon; Lissauer, Barnes and Chambers (Icarus 2012) found much milder variations (a few tens of degrees at most) for a moonless Earth with fast rotation. This simulation is a simplified illustration, not a full N-body integration - at forcing x1 it lands nearer the milder results.
Day length. Tidal bulges are dragged ahead of the Moon, giving a torque that slows Earth's spin and pushes the Moon outwards (angular momentum is conserved): the Moon recedes 3.8 cm/yr and the day lengthens ~2.3 ms per century from tides (the net observed change is ~1.7 ms/century because post-glacial rebound partly offsets it). Solar-tide torque scales as (1/2.18)² of the lunar one, so the remainder would be small. Past day lengths come from fossil coral and bivalve growth bands (~400 days per year about 400 Myr ago).
Night sky. Moon illuminance follows E = 10-0.4(m + 14.18) lux with m = -12.74 + 0.026|α| + 4×10-9α4 (α = phase angle in degrees; Krisciunas and Schaefer 1991 type formula), reduced by atmospheric extinction (airmass). Full Moon at the zenith ≈ 0.25 lux; a moonless clear night (starlight plus airglow) ≈ 0.002 lux, about 100 times darker. The Moon's angular diameter (0.52 degrees mean) is almost equal to the Sun's (0.53), which is why total eclipses exist; without the Moon there would be no lunar and no total solar eclipses.
What is simplified or dramatised. Sudden disappearance is a thought experiment. Screen brightness at night is boosted, like dark-adapted eyes; the lux numbers are the real values. Space view distances are compressed unless "True scale" is on; the Sun is drawn not to scale. Continents are procedurally generated (not real geography). The "close Moon" preset (tide force 100x, ~83,000 km) is indicative only; the equilibrium tide model is not valid at that strength. The ocean response after the Moon vanishes is modelled as a simple exponential decay. "Moon twice as far" is hypothetical: at 3.8 cm/yr recession this would take far longer than the Sun's lifetime.
Sources: Laskar et al. 1993, Nature 361, 615 and 361, 608; Lissauer et al. 2012, Icarus 217, 77; Stephenson, Morrison and Hohenkerk 2016 (length of day); Williams 2000 (palaeorotation); Doodson/Cartwright tidal potential amplitudes; Krisciunas and Schaefer 1991 (lunar brightness).