Conclusions of Ygrodrill’s immersion into the spheres of exoplanet A0–1.
As part of the Spiral mission to study the composition of the atmospheric spheres A3–2, to perform a gravitational deceleration maneuver, we also came so close to the exoplanet A0–1 for the first time.
During the maneuver, 5 years after the discovery of this cosmic giant, its first near-planetary image was taken. Then the device for vertical immersion into the layers of the exoplanet “Ygrodrill” was undocked. The following photograph was also taken before entering the steam environment.
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To study the conditions on A0 - 1, ygrodrill was droped vertically
to the core. Due to the boiling nucleus, a dynamic equilibrium between
the liquid and the gas phases, which will lead to the formation of
bubbles and steam pockets inside the liquid. The behavior of
these bubbles under high gravity differs from standard conditions,
possibly less and more short-lived due to higher pressure.During the study of the data, it was found that the core of the exoplanet, being metallic, is extremely hot. This heat creates a steep temperature gradient from the core outward. The pressure is also extremely high due to the gravitational forces of A0–1, which would compress both the metal core and the overlying water. The high temperature and pressure causes significant interactions between the water layer and the metal core. Water reacts with the metal, forming oxides and other compounds. Water is subjected to high temperatures and pressures, causing it to exist in a supercritical state. Supercritical water behaves neither strictly as a liquid nor as a gas and has unique properties that affect its ability to conduct heat and dissolve materials, which weakened the defense and interrupted the introduction into deeper layers. Moving outward, the pressure decreases, and water transitions through different phases. At certain layers, water exists as high-pressure ice VII, which forms under extreme pressures. Due to the heat from the core being intense, the surface is covered by superheated steam. In the vapor layer, convective movements are also significant, with hot vapor rising and cooler vapor sinking, contributing to a dynamic atmosphere.
Because the metal core is molten and convecting, it is generating a magnetic field through the dynamo effect. The presence of a water layer influences the characteristics of this magnetic field, depending on interaction with the conductive properties of water and steam at different phases.
Later, in the secondary study of materials, a valuable image was found with immersion of Ygrodrill, which opened the approval of data as the density and humidity of the atmosphere, temperature profile, and the rate of fall.
On the basis of the length and density of the pyroculus trace, information on the density and humidity of the atmosphere at different heights was revealed, which is important for modeling climatic and meteorological processes.
Analysis of changes in the length of the trace with height gave information about the temperature of the atmosphere and chemical properties at different levels of atmospheric layers, which is important for studying processes and climatic models A0–1.
Also, the length of the trace helped to determine how quickly the Ygrodrill lost the height in the atmosphere of the exoplanets. This is important for calculating and adjusting the descent trajectory in subsequent missions.
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Upon secondary examination of the data received from Stellarship, an
unexpected image was discovered! It captures Ygrodrill's descent into
the atmosphere of A0 - 1, taken on the route to the exoplanet A3 - 2.
This stunning image offers new insights by the measurement of the length
of pyrokumulus trace with a free fall provided important information for
various aspects of planetological studies of A0 - 1. These data helped to
improve the understanding of atmospheric conditions as a density,
temperature profile and chemical properties of atmospheric layers. As well
as measurements of the rate of fall, optimization of the trajectory and
technology of future immersions.
Overall the metal core of an exoplanet covered by water and vapor creates a fascinating environment with complex interactions between heat, pressure, and phase changes. High-pressure water ice, supercritical water, and dynamic convective currents all play roles in shaping the A0–1’s characteristics. The exact physical space and structure depend s on the specific parameters of temperature, pressure, and composition, leading to a unique planetary system.
NFTs via: https://foundation.app/@eminmathers/NOVAIII/5
NOVA III project via: https://www.eminmathers.me/nova3
The article is supplemented: June 1st, 2024