EXPLORER-VII
13.2 RS · v 0.31c · length 180 m

Chapter 01 · A journey through the cosmos

The universe is not the limit. It's the beginning.

Every atom in your body was forged in a star that died so you could look up. Tonight, the light that left it finally arrives.

Sgr A* · 4.3 million M☉ · Rs ≈ 12.7 million km
Distance to target: 26,000 light-years

Chapter 02

Our cosmic neighbourhood

One star. Eight worlds. Select a trajectory and fly to it.

Gyro tilt active · move cursor

Gas giant · 9.58 AU

Saturn

Surface gravity
10.44 m/s²
Orbital velocity
9.7 km/s
Mean temp
−140 °C
  • Less dense than water. In a big enough ocean, it would float.
  • Its rings span 280,000 km yet are mostly about ten metres thick.

Display notice: orbital distances and planetary sizes are normalised for display ergonomics. Real separations are far larger and not to scale. Physical metrics are published NASA values.

Chapter 03

Beyond our solar system

Three windows into the deep sky. Open the spectral inspector to read the chemistry of light that travelled for ages to reach you.

Stellar nursery · 8,500 ly · Carina

Pillars of creation

Columns of cold gas three light-years tall, sculpted by the radiation of the stars being born inside them.

Alien atmospheres · 40 ly

TRAPPIST-1e

  • Radius 0.92 R⊕
  • Orbit 6.1 days
  • Flux 0.66 S⊕
  • Zone Habitable

Telemetry · candidate signatures

H₂O ▲CH₄ ▲CO₂ ▲

Macro-galactic core · 23 Mly

Whirlpool Galaxy · M51

Grand-design spiral arms, shaped by a close pass with its companion NGC 5195.

Chapter 04

Humanity's next frontier

Seventy years from a beeping sphere to a telescope reading the dawn of time.

Active · 1977

Voyager 1 & 2

Across the interstellar boundary

Both probes have crossed the heliopause and still whisper back on less power than a refrigerator bulb.

Voyager 1
160+ AU out

Chapter 05

The unknown

Everything we can see makes up five percent of the universe. The rest is a question mark with a gravitational field.

Dark-matter halo · inferred from lensing, never seen

Visible matter 5% · Dark matter 27% · Dark energy 68%

Confirmed

Expanding universe

Galaxies recede, redshift proportional to distance (Hubble, 1929).

Unresolved

Dark energy

Roughly 68% of the cosmos pushes expansion faster. Nobody knows what it is.

Confirmed

Cosmic microwave background

The afterglow of the Big Bang, mapped to one part in 100,000.

Unresolved

Cosmic inflation

A split-second burst of expansion that explains the CMB’s smoothness. Never directly seen.

Confirmed

Gravitational waves

LIGO heard two black holes merge in 2015, ripples a thousandth the width of a proton.

Unresolved

Dark matter

About 85% of all matter. Visible only through its gravity. No particle found.

Confirmed

Worlds beyond the Sun

More than 6,000 confirmed exoplanets, many in their stars’ habitable zones.

Unresolved

The Fermi paradox

With so many worlds and so much time, where is everybody?

Schwarzschild time-dilation engine

Drag toward the horizon

t′ = t · √(1 − rs / r)

r = 1.1995 rₛ15.23 million km

Earth clock (far away)

00:00:00

Probe clock (near hole)

00:00:00
rₛ

Time dilation factor √(1 − rₛ/r)

0.4078

One hour aboard the probe equals 2.5 hours back on Earth.

Static observer model · hovering probe, black hole of 4.3 million solar masses.

Chapter 06 · The pale blue dot

One universe. Endless questions.

From here, borders vanish and the atmosphere is a film thinner than a coat of paint. Everyone you have ever loved, every war and every song, happened on this single speck. It is fragile, and it is the only home we have ever known.

Sources · Planetary fact sheets: NASA Solar System Exploration · Mission data: NASA, ESA, JPL-Caltech · Webb & Hubble observations: ESA / STScI · Renderings are procedural artistic interpretations, not photographs.

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