Ammoniac Atmosphere: Difference between revisions
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Cdjensen94 (talk | contribs) (Created page with "{{DISPLAYTITLE:Ammoniac Atmosphere}} {{Atmosphere | name = Ammoniac Atmosphere | image = Ammoniac_Sky.png | universe = Continuum Universes | type = Cryogenic Jovian Atmosphere | classification = Ammonia-Hydrogen Gas System | contents = NH₃ 60%, H₂ 25%, He 10%, CH₄ 5% | pressure = 12–40 atm | temperature = 110–180 K | molar_mass = ≈17 g/mol | compounds = Ammonia, Hydrogen, Methane, Helium | ef...") |
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The '''Ammoniac Atmosphere''' defines the frigid gas envelopes of outer-Continuum worlds — immense, swirling chemistries of hydrogen and ammonia wrapped in perpetual twilight. | The '''Ammoniac Atmosphere''' defines the frigid gas envelopes of outer-Continuum worlds — immense, swirling chemistries of hydrogen and ammonia wrapped in perpetual twilight. | ||
It is the | It is the '''archetype of Jovian cold worlds''', where heat is a memory, color comes from chemistry, and clouds build mountains that float. | ||
== Composition and Structure == | == Composition and Structure == | ||
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The result is a stratified, layered gas ocean — each tier a different phase of ammonia and water ice suspended in supercritical hydrogen. | The result is a stratified, layered gas ocean — each tier a different phase of ammonia and water ice suspended in supercritical hydrogen. | ||
| | {| class="wikitable" style="width:100%; text-align:center;" | ||
|- | ! Layer | ||
| | ! Primary Composition | ||
| | ! Approx. Temp. (K) | ||
| | ! Notes | ||
|- | |||
| '''Upper Stratosphere''' | |||
| NH₃ vapor, H₂, He | |||
| 110–130 | |||
| Pale blue, semi-transparent; violent winds. | |||
|- | |||
| '''Middle Troposphere''' | |||
| NH₃–H₂O clouds | |||
| 130–150 | |||
| Thick storm belts; ammonia snow. | |||
|- | |||
| '''Deep Mantle''' | |||
| Supercritical H₂, NH₃, CH₄ | |||
| 150–180 | |||
| Luminous lightning discharges; ionized gas layer. | |||
|} | |||
== Environmental Characteristics == | == Environmental Characteristics == | ||
* | * '''Pressure:''' 12–40 atm — increasing exponentially with depth. | ||
* | * '''Temperature:''' 110–180 K — stable across the troposphere. | ||
* | * '''Visuals:''' Blue-gray with violet undertones; constant banded cloud motion. | ||
* | * '''Acoustics:''' Deep resonant thunder; infrasonic wavelengths dominate. | ||
* | * '''Aroma:''' Sharp and alkaline — detectable even through vacuum-rated filters. | ||
== Atmospheric Phenomena == | == Atmospheric Phenomena == | ||
* | * '''Ammonia Snow:''' Microscopic NH₃ crystals fall from mid-cloud decks, evaporating before surface impact. | ||
* | * '''Electro-Ammonic Storms:''' High-pressure lightning arcs between layers, forming kilometer-wide plasma curtains. | ||
* | * '''Floating Icebergs:''' Buoyant clumps of ammonia-water ice drift through mid-atmosphere, acting as seeds for cloud vortices. | ||
* | * '''Acoustic Rings:''' Standing wave patterns circling entire planets; believed to modulate magnetic fields. | ||
== Biochemical Potential == | == Biochemical Potential == | ||
While hostile to standard biology, Ammoniac environments support theoretical | While hostile to standard biology, Ammoniac environments support theoretical '''chemoautotrophic life''' utilizing the “hydronitric cycle.” | ||
In this cycle, organisms synthesize energy by converting NH₃ and H₂ into amino analogs under high pressure, producing faint infrared bioluminescence. | In this cycle, organisms synthesize energy by converting NH₃ and H₂ into amino analogs under high pressure, producing faint infrared bioluminescence. | ||
Speculative forms — nicknamed *drifters* — are vast, translucent sacs kilometers wide, feeding on storm energy. | Speculative forms — nicknamed *drifters* — are vast, translucent sacs kilometers wide, feeding on storm energy. | ||
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== Thermal and Reflective Properties == | == Thermal and Reflective Properties == | ||
Ammoniac worlds reflect ~60% of incoming light due to their dense clouds, making them bright to telescopes but dim in infrared. | Ammoniac worlds reflect ~60% of incoming light due to their dense clouds, making them bright to telescopes but dim in infrared. | ||
The [[Grand Archive Division of Exoatmospherics]] notes that their refractive spectra are stable enough to serve as | The [[Grand Archive Division of Exoatmospherics]] notes that their refractive spectra are stable enough to serve as '''galactic calibration standards''' for optical sensors. | ||
== Research and Cultural Notes == | == Research and Cultural Notes == | ||