TRACKER LAUNCH DATE ASTRONOMY SPACEX CONTROVERSY FAQ REFLECT ORBITAL
35.7°NLATITUDE
68°MAX ELEVATION
JST (UTC+9)TIMEZONE
~−4PEAK MAGNITUDE
♦ PRE-LAUNCH — NO MIRROR IN ORBIT YET
EARENDIL-1 is targeting a mid-2026 launch pending FCC approval. There is currently no space mirror in orbit. Pass predictions for Tokyo will go live on OrbitalNodes.ai from launch day — exact times, directions, and beam footprint data updated in real time.
30° 60° 90° 5km beam footprint Peak 68° SW SE TOKYO · 35.7°N · EARENDIL-1 PASS GEOMETRY 3–5 passes/week (season) mag ~−4 at peak EARENDIL-1 VIEWING CONDITIONS — TOKYO BY MONTH J BEST F M A M J J A S O BEST N D STATS 68° MAX ELEV 3–5/wk PASSES B9 BORTLE 35.7°N ★ BEST: OCT–APR Autumn and winter — clear, dry air from Siberian High ✗ AVOID: JUN–SEP Monsoon season — persistent cloud cover
PASS GEOMETRY

What to Expect in Tokyo

LATITUDE AND PASS GEOMETRY
At 35.7°N in the Northern Hemisphere, EARENDIL-1 passes are rising in the SW and crossing toward the SE. Maximum elevation up to 68°. EARENDIL-1 orbits in sun-synchronous orbit at 600–650km altitude, meaning it will pass over Tokyo multiple times per week when operational. The mirror is steerable — it will only be at full brightness during targeted commercial passes.
VIEWING WINDOW
OCT–APR offers the best conditions. Autumn (October–November) is Tokyo's best season: monsoon has cleared, humidity drops, and views to the west from higher ground are dramatic. June–September cloud cover is near-continuous. Like all satellites, EARENDIL-1 is only visible during twilight — when your sky is dark but the mirror is still in direct sunlight.
LIGHT POLLUTION BORTLE 9
Inner city — severe light pollution. EARENDIL-1 at magnitude ~−4 is bright enough to be clearly visible from central Tokyo regardless of light pollution — comparable to Venus at maximum brightness. For darker skies, Mount Takao (~50km west) or Okutama (~70km) for dark skies offers better conditions.
LOCAL CONTEXT
Tokyo at Bortle 9 is one of the most light-polluted major cities on Earth — but EARENDIL-1 at magnitude −4 is bright enough to be clearly visible even here. Like Venus in daylight, it punches through city glow. Japan's culture of astronomical interest means passes will likely be widely followed.
5KM BEAM FOOTPRINT
The 5km beam is comparable to the distance from Shinjuku to Shibuya. A targeted pass during evening peak demand could illuminate the urban canyon of central Tokyo — a commercially interesting proposition for Reflect Orbital.
OBSERVER GUIDE

What EARENDIL-1 Will Look Like from Tokyo

From Tokyo, EARENDIL-1 passes will appear as a fast-moving point of light crossing the sky in approximately 3–4 minutes. At peak brightness it will reach magnitude ~−4 — comparable to Venus at maximum and clearly visible even from the city centre. It will be one of the brightest objects in the sky during a pass.

The mirror is steerable — between targeted commercial passes, Reflect Orbital tilts it away from Earth, making it much dimmer. During an active pass you'll see a sudden brightening as the beam angle locks onto the target region, then abrupt dimming when the mirror tilts away again.

Track EARENDIL-1 from Tokyo at Launch

OrbitalNodes.ai will provide real-time pass predictions for Tokyo from the moment EARENDIL-1's orbital data is published. No app download required.

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