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Dreamers and Builders.
A Mission to Venus.
We are NEPHELIS.

AETHER is a crowd-funded aerostat probe to Venus, floating where temperature and pressure are Earth-like (50–55 km) to stream back images and data for 30–90 days.

The Mission: Project AETHER

Project AETHER will send Cloudseeker, a miniprobe, to Venus's atmosphere. It unlocks energy and resources for floating habitats, extending human life, consciousness and AI to another world.

Targeting 50–55 km altitude—Earth-like conditions—Cloudseeker validates habitation models, resource extraction and astrobiology. Launch: 2027.

Be part of humanity's backup plan. Venus ensures life thrives across the solar system.

Venus offers abundant solar power, CO₂ for fuel, nitrogen for breathable air. Join us!

Future VenusExpress concepts with advanced propulsion could cut travel time to 30–45 days (vs. today’s 3–6 months).

Technology: Cloudseeker

  • Acid-Resistant Aerostat: Fluoropolymer balloon; floats at 50–55 km.
  • Integrated Sensor Suite: imagery + mass spectrometry + aerosol/bio-sensors.
  • 3U CubeSat Relay: high-bandwidth data relay in Venus orbit.
  • AI-Optimized Navigation: autonomous ops in dynamic atmosphere.
Cloudseeker Probe

Astrophysics & Trajectory

Transfer & Timing

  • Profile: Earth→Venus Hohmann-like transfer (outreach model)
  • Time of Flight: ~146 days
  • LEO→TVI ΔvDelta-v: A measure of the impulse required to perform a maneuver. The 'change in velocity'.: ~3.5 km/s (purchased)
  • Onboard Δv: 150–200 m/s (TCMs/margin)
  • Arrival: v∞Hyperbolic excess velocity: the velocity of a spacecraft in excess of the escape velocity of a celestial body. ~2.7 km/s; entry ~10.7 km/s; deploy balloon ~55 km

Trajectory Mini-Planner

Phase:
TOF: 146.0 d
Δv est.: 3.50 km/s

Atmosphere Model

Comms/Day Estimator

Rocket Equation

The Tsiolkovsky rocket equation calculates the propellant needed for a given change in velocity (Δv), based on engine efficiency (Isp) and mass.

Compute Propellant

Mission Diagrams

Venus Orbit & Entry

Venus Atmosphere 3U CubeSat Relay Atmospheric Entry (~10.7 km/s) Balloon deploy ~55 km

Venus Cloud Layers

Altitude 70 km 60 km 50 km 45 km Upper Haze (H₂SO₄) Middle Cloud Lower Cloud Cloudseeker Habitable Zone: 50–55 km

Why Venus? The Smart Bet

With Earth-like gravity and a temperate, 1-bar pressure layer at 50–55 km altitude, Venus isn't just a potential habitat—it's the most practical and resource-rich destination for off-world colonization in our solar system.

Venus complements Mars. At the right altitude, it offers near‑Earth pressure/temperature and abundant solar energy—balanced against acid clouds and power/radiation trade‑offs.

Aspect Venus (Cloud Tops) Mars (Surface)
Travel Time ~5 months (current) | 30-45 days (future concept) ~6-9 months (current)
Gravity 0.904 g (~90% Earth) 0.38 g (~38% Earth)
Habitable Zone Conditions ~30–70 °C; 0.5–1 bar pressure ~-60 °C; ~0.006 bar pressure (requires pressure suits/domes)
Solar Energy ~2601 W/m² (1.9x Earth), reduced in clouds ~590 W/m² (0.43x Earth)
Resources 96.5% CO₂, 3.5% N₂, trace SO₂ CO₂ atmosphere, polar water ice
Key Challenges Sulfuric acid clouds, material degradation Cosmic radiation, dust storms, low gravity

Mission Timeline

Venus Today: Daily Fact

Loading today's fascinating fact about Venus...

Funding

Raised: $0 / Target: $500,000

ETCH YOUR LEGACY ON A PANEL

From a personal message ($100) to a corporate logo ($10k), your support will be physically integrated into the Cloudseeker probe, orbiting Venus for decades to come.

427 of 500 panels left

IMMORTALIZE YOUR DNA ON VENUS

For a $500 contribution, send us a hair or nail sample. We'll seal it in an inert time capsule aboard the probe, making your biological signature part of an eternal cosmic journey.

Vendors & Partners

Launch via SpaceX rideshare program. Testing: Acid chamber at TBD facility (e.g., Glenn Research Center analogs); thermal-vac at commercial labs.

Frequently Asked Questions

Is this a real mission?

Nephelis Industries and Project AETHER are a rral mission, designed to inspire and build a first step to Venus exploration.

Why not Mars?

While Mars gets a lot of attention, Venus's upper atmosphere offers Earth-like pressure and temperature, plus better protection from solar radiation, making it a compelling alternative for floating habitats.