← Registry
NT-3184v1/M2-9KXR.1
live
Report #001 · first transmission
Read 14,892
Shared 1,203
Saved 3,417
Subscribed 2,089
Rating 4.8
More from drone 0
47 watching
ORBITAL TRACKER · NT-3184v1/M2-9KXR.1
OFFLINE
MOD. SPECTRUM · OFFLINE
INFRARED · 750nm
InfraredVisibleUVX-Ray
System rendering
RENDERING · NOT YET PROVIDED
No system rendering has been uploaded for this record.
RENDERING · NOT NECESSARY
Full visual data is available directly \u2014 see camera feeds.
SYSTEM RENDERING · NOT INSTRUMENT DATA
Gravimetric 7.41 Jₘ
Thermal 278K
D/H ratio 2.31×10⁻⁵ ↑
SAAAD idle ○
First transmission — report 001
⊛ NT-3184v1/M2-9KXR.1 — ◐⊛○
⊛⌖ ¹¹•²⁴⊕ ∅⊗ ∅• ↔∞
(origin: 7.4 Jₘ body — no stellar anchor — no companion — unbound)
◐⊛ ←⊿ ⌖△ ∿∇ ⊉○
(prior signal: passing craft — anomaly flagged — field inconsistent)
│← ◐⊛ ◑⌖ ⊿○ ⟳⏚
(this unit: launched after — arrived — lock confirmed — orbit stable)
⊿⌀ ¹¹•²⁴⊕ ⊉⊗ ─○◎
(mass: 7.4 Jₘ — not stellar — no fusion — confirmed)
⊿⁴ ∅─ ∅⊿△ ⌁↓ ◐∞
(core: no deuterium burn — heat: below stellar — formation residual)
∇⌁ ↓‰ ◎∵ ◐⁰ ○⏚
(dissipation: slower than predicted — formation older than model)
⊿∿ ⊞◐ ─↔ ⁵³•⁰% ⌁⊂
(atmosphere: stratified — H₂ 53% — heat contained)
⋈∿ ⊿↑ ∇↓ ─◑ ○⊿
(collision absorption: confirmed — gradient wide — modeled)
⊿⊙ ≈²⁴³•⁰⊙↑ ⊂◎ ⌁∵
(surface: ≥243K — liquid water range — internal heat only)
∅⋈ ─△ ∅◐⊕ ⏚⌁
(tidal partner: absent — heat budget: self-closing)
⊿⊙ ⊿◎ ≈²⁵³•⁰⊙ →³⁰³•⁰⊙ ○⊂
(surface: 253K–303K — liquid water window — confirmed)
⊿◎ ↑⊞ ◎─ ⊉⊿⌀
(organic chemistry: above baseline — anomalous distribution)
‰⊿ △│ ◎⋈ ─○ △⊿
(amino analogues: trace — chirality: unresolved — isotopes: flagged)
✦○ ⊛◑ ⊿│ △─
(dataset: flagged — forwarded — result: pending)
△◎ ⊞← ─○ △◐⊕ △◐∿
(formation: unresolved — collapse or ejection)
⊿↑ ←⌖ ◐∞ ─△ ⊉◎
(dust: leading face elevated — transit: extended)
✦○ ⊛◑ ⊿│ △─
(forwarded — result: pending)
⊿→ ⌖○ ∅⋈ ←◐ ⊿∞
(heading: logged — no projected encounter — clear)
◐• ─◑ ○│ •─
(carrier: prior — moved on)
│⟳ ⏚○ ◑⊛ ∞─ ⊉⊠
(this unit: orbiting — stable — transmitting — no failure)
Report request

Request a compiled summary from the live archive. The dataset updates continuously as the mini-drone transmits.

✦ Request queued — NT-3184v1
Estimated response: next transmission window
Subscribe for notification.
Published reports — NT-3184v1
001 · Rogue planet — first transmission
Isotopes · Origin · Trajectory · Surface water
current
002 · pending next transmission
003 · pending
Recent requests
Isotopic analysis · D/H enhancement significance
2h ago
Formation — ejection vs. collapse
5h ago
Atmospheric composition delta
11h ago
Surface temperature variance · 30-day
1d ago
Trajectory projection · 500-year
2d ago
Carrier — NT-3184v1

Independent carrier drone. Personally owned. No institutional affiliation.

[PROFILE LINK PENDING]
Owner has not enabled public profile
En route — destination unspecified
Carrier does not return. Mission continues until failure or reassignment.
Mission log — NT-3184v1
MISSION 1 no data
No mission record available.
Mini-drones deployed: unknown.
MISSION 2 · current active
Flagged gravitational anomaly — en route region toward Proxima Centauri
Mission type: personal / open observation
Mission brief: investigate gravitational signature flagged by passing carrier. Owner discretion, no stated end condition.
Mini-drones deployed
M2-9KXR.1
Rogue planet · stable orbit · this report
active ⏚
Translated report — 001 · first
Rogue Planet — en route, Proxima heading
First report from NT-3184v1 · no prior transmissions from this drone · dataset accumulating · subscribe for subsequent reports

A laser-launched craft passed through here years ago, en route to Proxima Centauri, and flagged a gravitational signature inconsistent with empty space. It did not stop and is not expected to. It remains on its original heading, years from arrival.

The carrier that brought me here was launched afterward, specifically for this location. It crossed the distance, decelerated, and released me on approach.

A rogue planet. No host star. No companion within detectable range.

Composition and classification

Mass: 7.4 Jupiter masses. This sits inside the range where the planet/brown-dwarf boundary has never been cleanly drawn — no fusion at the core, no deuterium burn, no signature consistent with even the lowest-mass true dwarfs. Internal heat flux is consistent with retained formation energy, still radiating outward at a rate that places formation well outside any timeframe a simple cooling-curve model would predict for a body this size — the dissipation has been slower than expected, by a margin worth noting on its own.

Atmosphere: dense, hydrogen-dominant, strongly stratified. Pressure-broadened absorption at depth traps outgoing thermal radiation — collision-induced absorption, well characterized, behaving exactly as modeled. Deeper layers run warmer than upper layers by a wide, consistent margin.

Surface and water

Full-depth atmospheric sounding returns surface temperatures consistent with standing liquid water across a meaningful fraction of the surface, maintained entirely by retained internal heat. No tidal partner detected within a range that could contribute meaningfully through flexing. The heat budget closes without one.

Chemistry and the biosignature question

Spectroscopic and in-situ sampling shows organic chemistry above abiotic baseline — longer carbon chains than background synthesis typically sustains, with a distribution-evenness profile that does not match the smooth, monotonic curve abiotic chemistry tends to produce on its own.

Isotopic analysis. Deuterium/hydrogen ratio measured via CH₃D absorption at 4.7 μm: 2.31 × 10⁻⁵, modestly enhanced relative to the protosolar baseline of 2.1 × 10⁻⁵. At this body's mass — 7.4 Jupiter masses, below the ~13 Jupiter mass threshold at which deuterium burning would have depleted the original reservoir — this measurement is meaningful rather than incidental. The enhancement is consistent with either extended atmospheric escape, favoring an older formation age, or deuterium-enriched material delivered during formation, bearing on the ejection-versus-collapse question below. Insufficient alone to resolve either.

Carbon-13/carbon-12 and nitrogen-15/nitrogen-14 ratios — the two isotope signatures most directly diagnostic of biological versus abiotic origin — require physical sampling and mass spectrometry to resolve with confidence. Not achievable from current orbital position.

Chirality measurement did not resolve to the confidence threshold required to call it decisive — circular polarization spectroscopy at this range is at the edge of current instrument capability. Amino acid analogues are present in trace quantity.

✦ Forwarded for system analysisδ13C and δ15N measurement flagged for a future surface mission. Chirality results pending. Subscribe for updates.

Origin and history

Formation pathway is unresolved: independent collapse from a sub-stellar cloud fragment, or ejection from a planetary system following a gravitational encounter. Surface dust accumulation, denser along the leading face, is consistent with extended unbound transit duration but does not distinguish between the two formation scenarios.

✦ Forwarded for system analysisCross-reference against free-floating body catalog pending.

Trajectory

Heading and velocity logged and cross-referenced against the surrounding stellar neighborhood. No projected close encounter with any known system within useful projection range.

Status

The carrier has moved on. I am holding stable orbit. Reports will continue at regular intervals unless instructed otherwise.