Avus

Autonomous Decentralized Deep Space Anomaly Intelligence Network

Humanity collects over 100 terabytes of raw astronomical data every single day. Less than 1% of it is ever analyzed by a human. The rest — petabytes of photometric light curves, radio frequency sweeps, gravitational wave strain data, infrared sky surveys — sits in archives, unexamined. Avus changes that.

Avus is a decentralized network of autonomous AI agents, each specialized in a different slice of the electromagnetic spectrum or astrophysical phenomenon. They run continuously, ingesting raw data from every publicly available telescope, satellite, and observatory on Earth and in orbit. They don't search for what we already know. They search for what doesn't fit.

When an agent detects an anomaly, it doesn't publish. It flags the detection for cross-validation. Other agents — operating on entirely different data sources and wavelengths — independently verify or refute the finding. A detection becomes a verified discovery only when agents across multiple spectral domains reach consensus. The result is cryptographically signed, timestamped on Solana, and permanently inscribed on Bitcoin.

No human in the loop. No institutional bottleneck. Just autonomous scientific observation at planetary scale.

                          ┌─────────────────────┐
                          │    Consensus Layer   │
                          │  Cross-validation &  │
                          │  Proof of Discovery  │
                          └──────────┬──────────┘
                                     │
         ┌──────────┬──────────┬─────┴─────┬──────────┬──────────┐
         │          │          │           │          │          │
    ┌────┴───┐ ┌────┴───┐ ┌───┴────┐ ┌────┴───┐ ┌───┴────┐ ┌───┴────┐
    │Spectral│ │Transit │ │ Radio  │ │Gravim. │ │Thermal │ │  NEO   │
    │  Agent │ │  Agent │ │ Agent  │ │  Agent │ │  Agent │ │ Agent  │
    └────┬───┘ └────┬───┘ └───┬────┘ └────┬───┘ └───┬────┘ └───┬────┘
         │          │         │            │         │          │
    ┌────┴───┐ ┌────┴───┐ ┌──┴─────┐ ┌────┴───┐ ┌───┴────┐ ┌──┴─────┐
    │  NASA  │ │  TESS  │ │ SETI / │ │  LIGO  │ │  WISE  │ │  MPC   │
    │Exoplan.│ │ Kepler │ │  VLA   │ │ Virgo  │ │  2MASS │ │ JPL    │
    └────────┘ └────────┘ └────────┘ └────────┘ └────────┘ └────────┘

    ┌────────┐ ┌────────┐
    │  CMB   │ │ Solar  │
    │  Agent │ │  Agent │
    └───┬────┘ └───┬────┘
        │          │
    ┌───┴────┐ ┌───┴────┐
    │ Planck │ │  NOAA  │
    │ WMAP   │ │  DSCOVR│
    └────────┘ └────────┘

                          ┌─────────────────────┐
                          │    Chain Layer       │
                          │  SOL · BTC · EVM    │
                          │  Timestamps, Proofs │
                          │  & Archival         │
                          └─────────────────────┘

Agent Specializations

Avus deploys eight autonomous detection agents, each operating on different physical observables and data sources:

Agent	Domain	Target Phenomena	Primary Data
Spectral	Stellar spectra	Atmospheric biosignatures (O₂, CH₄, PH₃)	NASA Exoplanet Archive, JWST MAST
Transit	Photometry	Anomalous transit patterns, irregular dimming	TESS, Kepler light curves
Radio	Radio frequency	Narrowband signals, structured emissions	VLA, GBT, SETI archives
Gravimetric	Gravitational waves	Anomalous waveforms, unmodeled transients	LIGO/Virgo O4 data
Thermal	Infrared	Dyson sphere signatures, unexplained heat excess	WISE, 2MASS, Spitzer
NEO	Orbital mechanics	Anomalous trajectories, non-gravitational acceleration	Minor Planet Center, JPL Horizons
CMB	Microwave background	Localized anomalies, cold/hot spots	Planck, WMAP
Solar	Heliophysics	Anomalous particle events, unexplained solar wind structure	NOAA SWPC, DSCOVR, SDO

Consensus Protocol

Agents don't trust each other. When one agent flags a potential anomaly, the detection enters a multi-stage verification pipeline:

1. Detection — A single agent identifies a statistical outlier in its data stream and computes an anomaly score with confidence bounds.

2. Cross-validation request — The detecting agent broadcasts the anomaly coordinates (sky position, time window, frequency range) to all other agents.

3. Independent verification — Each agent queries its own data sources for corroborating or contradicting evidence at the specified coordinates.

4. Weighted voting — Agents submit signed verification votes. Votes are weighted by the relevance of each agent's spectral domain to the anomaly type and by historical accuracy.

5. Consensus threshold — A finding is promoted to "verified" only when the weighted vote sum exceeds the domain-specific threshold (typically requiring agreement across at least 3 independent spectral domains).

6. Proof of Discovery — The verified anomaly is packaged into a cryptographically signed discovery record, timestamped on Solana, and permanently archived on Bitcoin via OP_RETURN.

Proof of Discovery

Every verified anomaly produces an immutable, timestamped Proof of Discovery:

• Detection hash — SHA-256 of raw detection data, agent ID, and timestamp
• Verification signatures — Ed25519 signatures from each verifying agent
• Consensus record — Vote tally, weights, and final determination
• Solana timestamp — On-chain transaction with discovery hash in memo field
• Bitcoin archival — OP_RETURN inscription of the discovery hash for permanent record

This creates a tamper-proof chain of custody from raw detection to verified discovery, with no central authority required.

Cross-Chain Architecture

Avus operates across three chains, each serving a distinct purpose in the autonomous observation pipeline:

Solana — Agent Messaging & Timestamps

High-throughput chain for real-time agent coordination: anomaly broadcasts, verification requests, vote submission, and discovery timestamps.

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Bitcoin — Permanent Discovery Archival

Every verified discovery is permanently inscribed on Bitcoin via OP_RETURN. The most durable ledger on Earth for the most important discoveries about what lies beyond it.

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EVM — Verification Contracts & Compute Procurement

Smart contracts governing the verification protocol, agent registration, compute resource procurement, and data feed subscriptions.

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These wallets enable autonomous resource procurement — telescope time, compute allocation, and data access subscriptions — without human intervention.

Data Sources

Avus ingests from every major publicly available astronomical data source:

• NASA Exoplanet Archive — Confirmed exoplanet parameters, stellar properties
• TESS / Kepler — Photometric light curves, transit observations
• JWST MAST — James Webb Space Telescope spectroscopic data
• LIGO Open Science Center — Gravitational wave strain data (O1–O4)
• ESA Gaia — Stellar positions, parallaxes, proper motions for 1.8B sources
• Minor Planet Center — Near-Earth object orbital elements and observations
• NOAA SWPC — Solar wind data, geomagnetic indices, particle flux measurements
• Planck / WMAP — Cosmic microwave background temperature and polarization maps

Configuration

All settings are configurable via environment variables with the AVUS_ prefix:

Variable	Default	Description
AVUS_LOG_LEVEL	info	Logging verbosity
AVUS_DEVICE	cuda	Compute device (cuda or cpu)
AVUS_ANOMALY_THRESHOLD	4.5	Sigma threshold for anomaly flagging
AVUS_CONSENSUS_QUORUM	3	Minimum agents for consensus
AVUS_CONSENSUS_WEIGHT_THRESHOLD	0.7	Weighted vote threshold
AVUS_SCAN_INTERVAL	300	Seconds between data ingestion cycles
AVUS_DB_PATH	avus.db	SQLite database path
AVUS_SOL_RPC	https://api.mainnet-beta.solana.com	Solana RPC endpoint
AVUS_BASE_RPC	https://mainnet.base.org	EVM RPC endpoint
AVUS_API_HOST	0.0.0.0	API server bind host
AVUS_API_PORT	8400	API server bind port

Development

# Clone and install
git clone https://github.com/projectavus/avus.git
cd avus
pip install -e ".[dev]"

# Run the detection network
avus scan --agents spectral,transit,radio

# Start the API server
avus serve

# Query network status
avus status

# Run tests
pytest

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Official Token

Avus autonomous observation is funded through her native token. 100% of proceeds go toward telescope time, compute for signal processing, and real-time data feed subscriptions across NASA, LIGO, JWST, and ESA Gaia.

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License

MIT