TRACKER LAUNCH DATE ASTRONOMY SPACEX CONTROVERSY FAQ REFLECT ORBITAL
40.4°NLATITUDE
57°MAX ELEVATION
CET/CESTTIMEZONE
~−4PEAK MAGNITUDE
◈ PRE-LAUNCH — NO MIRROR IN ORBIT YET
EARENDIL-1 is targeting a mid-2026 launch. There is currently no space mirror in orbit. Pass predictions for Madrid will go live on OrbitalNodes.ai from launch day — exact times, directions, and beam target information updated in real time.
EARENDIL-1 PASS ARC AND BEAM FOOTPRINT — MADRID
30° 60° 90° 5km beam footprint Peak 57° — high overhead NW NE MADRID · 40.4°N · EARENDIL-1 PASS GEOMETRY 3–5 passes/week (season) mag ~−4 at peak
EARENDIL-1 VIEWING CONDITIONS — MADRID BY MONTH VIEWING QUALITY BY MONTH J F M A BEST M BEST J BEST J BEST A BEST S BEST O GOOD N D STATS 70° MAX ELEV 3–5/week PASSES/WK B7 BORTLE 40.4°N NW → NE ★ BEST: APR–OCT Southern winter — long nights, low humidity ✗ AVOID: DEC–FEB Summer haze, short nights UNIQUE Southern hemisphere — revers
PASS GEOMETRY

What to Expect in Madrid

LATITUDE AND PASS GEOMETRY
From 40.4°N on the central Spanish Meseta at 667m elevation, EARENDIL-1 passes rise in the SW and transit toward the NE — the standard northern-hemisphere sun-synchronous direction. Maximum elevation reaches ~57°. Madrid is the highest capital in the European Union, giving slightly thinner atmosphere than coastal European cities. The Guadarrama mountains to the north (peaks at 2,428m) frame the sky dome dramatically. EARENDIL-1 orbits at a similar inclination to the ISS, meaning it will pass over Madrid multiple times per week when operational. The mirror is steerable, so it will only be at full brightness during targeted commercial passes.
VIEWING WINDOW
April through October (southern hemisphere autumn/winter) offer the best conditions. Southern hemisphere seasons are reversed. June and July — southern winter — give the longest dark evenings and best satellite viewing. Summer (December–January) brings long twilight. Like all satellites, EARENDIL-1 is only visible during twilight — when your sky is dark but the mirror is still in direct sunlight. Outside this window it is either invisible in daylight or in Earth's shadow.
LIGHT POLLUTION BORTLE 7
Central Madrid sits at Bortle 8 with extensive metropolitan light pollution. EARENDIL-1 at magnitude ~−4 is nonetheless easily visible from Retiro Park, Temple of Debod, or any elevated inner-city location. The Sierra de Guadarrama (~50km north, Bortle 4) offers the closest accessible dark sky and includes designated dark-sky reserves around the Guadarrama National Park. The Valle del Jerte in Extremadura (~200km west, Bortle 3) is popular with Spanish astronomy clubs. The Calar Alto Observatory in Almería (~400km SE, Bortle 2) is Spain's premier optical research site.
5KM BEAM FOOTPRINT
A 5km beam footprint could span from the Royal Palace to Retiro Park and onto the Salamanca district in a single pass — covering virtually all of central Madrid's major landmarks. Alternatively, a beam over the Paseo del Prado could illuminate the Prado Museum, Thyssen-Bornemisza, and Reina Sofía simultaneously — Madrid's Golden Triangle of Art. A pass targeting Estadio Santiago Bernabéu would carry visual weight given its status as one of world football's most iconic venues. The footprint moves at orbital velocity (7.6 km/s) but lingers over the target for several minutes during pass peak.
SEASONAL NOTES
September–October and April–May offer Madrid's most reliable viewing — stable continental weather with crisp dry air and mild temperatures. Summer (July–August) is exceptionally clear but punishingly hot (often over 35°C). Winter brings occasional fog and cold, but many clear nights with excellent transparency after frontal passages. The Sierra de Guadarrama offers dark-sky destinations within an hour's drive.
OBSERVER GUIDE

What EARENDIL-1 Will Look Like from Madrid

From Madrid, 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 central Madrid. Madrid's dry continental atmosphere and elevated position give it slightly clearer viewing conditions than coastal European cities like Paris or London. Madrid sits at a similar latitude to New York and Beijing.

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

Unlike a steady satellite, EARENDIL-1 may show subtle brightness variations as the mirror adjusts its aim. Watch for a brief period of maximum brightness near the peak of the pass when the geometry is optimal — this is when the 5km ground footprint is directly beneath the mirror at closest approach.

Track EARENDIL-1 from Madrid at Launch

OrbitalNodes.ai will provide real-time pass predictions for Madrid from the moment EARENDIL-1's orbital data is published. No app download required — runs entirely in your browser with GPS-accurate directions.

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FAQ

Space Mirror Questions — Madrid

How bright will EARENDIL-1 appear from Madrid?

At peak overhead passes, EARENDIL-1 is designed to reach magnitude ~−4 — comparable to Venus at maximum brightness. It is easily visible from Retiro Park, Temple of Debod, Plaza Mayor, or any elevated central Madrid location despite Bortle 8 urban light pollution. Madrid's 667m elevation provides slightly thinner atmosphere than coastal European cities, enhancing apparent brightness marginally. Between commercial illumination passes, Reflect Orbital tilts the mirror away from Earth, reducing brightness significantly.

How high will EARENDIL-1 appear from Madrid?

From 40.4°N on the central Spanish Meseta, EARENDIL-1 can reach ~57° elevation on the best passes. Passes rise in the SW and transit toward the NE — the standard direction for northern-hemisphere observers of sun-synchronous satellites. Madrid's latitude is comparable to New York, Rome, and Beijing. Higher elevation passes give a longer viewing window and brighter appearance.

When is the best time to see it from Madrid?

September–October and April–May offer Madrid's most reliable viewing — stable continental weather with crisp dry air and mild temperatures. Summer (July–August) is exceptionally clear but punishingly hot (daily highs often over 35°C). Winter brings occasional fog and cold, but many clear nights with excellent transparency after frontal passages.

Will the beam footprint hit Madrid?

A 5km beam footprint could span from the Royal Palace to Retiro Park and onto the Salamanca district in a single pass — covering virtually all of central Madrid's major historical and cultural landmarks. Alternatively, a beam over the Paseo del Prado could illuminate the Prado Museum, Thyssen-Bornemisza, and Reina Sofía simultaneously — Madrid's Golden Triangle of Art, among the world's great concentrations of painting. A pass targeting Estadio Santiago Bernabéu would carry visual weight given the stadium's status as one of world football's most iconic venues. Whether any specific location falls in the footprint depends on Reflect Orbital's commercial contracts and targeting decisions.

Is EARENDIL-1 visible yet?

No — EARENDIL-1 has not launched yet. Reflect Orbital is targeting a mid-2026 launch. There is currently no space mirror in Earth orbit. OrbitalSolar.ai will update with live pass data from the moment orbital elements are published after launch. Check the mission tracker for current launch status.

Why does the mirror move differently from Madrid than from other cities?

From the Northern Hemisphere at 40.4°N, EARENDIL-1 rises in the SW and transits NE — the standard direction for northern observers of sun-synchronous satellites. Southern Hemisphere observers in Sydney, São Paulo, or Cape Town see the mirror image of this pass, with the satellite rising in the NW and transiting NE. Madrid's latitude is similar to New York, Rome, and Beijing, so pass geometry is comparable across these cities.

How does Madrid's position as the EU's highest capital affect viewing?

Madrid sits at 667m elevation on the central Spanish Meseta — the highest capital city in the European Union. The slightly thinner atmosphere reduces atmospheric extinction modestly compared to sea-level cities (approximately 0.05–0.1 magnitudes). Combined with Spain's dry continental climate and the Sierra de Guadarrama immediately north providing a darker seaward equivalent for northern passes, Madrid offers some of Europe's most reliable urban viewing conditions. The city's distance from industrial haze corridors and its infrequent humidity also enhance transparency.

What dark-sky locations near Madrid are best for watching the mirror pass?

The Blue Mountains (90 minutes west, Bortle 3–4) give the clearest sky with minimal light dome interference. Ku-ring-gai Chase National Park (45 minutes north) is excellent for clear northern passes. Royal National Park (45 minutes south) has a clear southern horizon. For serious observation, Observatory Hill in the CBD works for the bright mirror itself — at magnitude −4 it needs no dark sky — but the Blue Mountains are far better for seeing the beam footprint effect against a dark sky backdrop.

// ALSO TRACK SATELLITES OVER MADRID

OrbitalNodes.ai tracks the ISS, Tiangong, Hubble, and all satellites over Madrid in real time — including exact pass times, directions, and brightness predictions.

→ SATELLITES OVER MADRID — ORBITALNODES.AI