Aegaeon

Aegaeon is a fascinating moon in our Solar System that has captured the attention of astronomers and space enthusiasts alike. With a Aegaeon radius of 0.5 km, making it 12742.0× smaller than Earth's size, this celestial body presents unique characteristics that distinguish it from other objects in our cosmic neighborhood. Positioned at an average distance of 167,500 km (0.001 AU) from the Sun, Aegaeon occupies a significant place in the Solar System's architecture. As a moon, Aegaeon demonstrates the incredible diversity of natural satellites that orbit larger celestial bodies throughout our Solar System.

The Aegaeon physical characteristics reveal a world of remarkable dimensions and properties. The Aegaeon radius measures 0.5 km, making it 12742.0× smaller than Earth's size. The Aegaeon mass of 1.00e+11 kg represents 59720000000000.0× smaller than Earth's mass, giving this world substantial gravitational influence.

The Aegaeon orbit reveals fascinating details about its journey around the Sun and its relationship to other Solar System objects. The Aegaeon orbit has a semimajor axis of 167,500 km (0.001 AU), placing it 893.1× smaller than Earth's distance from the Sun. The Aegaeon orbit is nearly circular with an eccentricity of 0 (83.5× smaller than Earth's orbital eccentricity), resulting in relatively stable solar heating throughout its year. The Aegaeon orbit takes 0.00 hours to complete (39057115.7× smaller than Earth's orbital period), defining the length of its year. The orbital inclination of 0.001° indicates how much the Aegaeon orbit is tilted relative to the Solar System's ecliptic plane. This low inclination means Aegaeon follows a path very close to the plane where most planets orbit, suggesting a stable formation history.

The Aegaeon rotation and axial orientation provide crucial insights into its daily and seasonal cycles, as well as its orbital dynamics. The Aegaeon rotation period of 0.01 hours (4389.4× smaller than Earth's rotation period) determines the length of its day. This extremely fast rotation creates intense centrifugal forces and may contribute to the planet's flattened shape. The Aegaeon axial tilt of 0° determines the intensity and nature of seasonal variations. With minimal axial tilt, Aegaeon experiences virtually no seasonal changes, maintaining relatively constant temperatures throughout its year. The orbital orientation parameters reveal additional details about Aegaeon's position in space. The mean anomaly of 0° indicates the planet's current position in its orbit relative to its perihelion. The argument of periapsis of 0° shows how the orbit's orientation changes over time due to gravitational perturbations. The longitude of ascending node of 0° defines the reference point where the orbit crosses the ecliptic plane.

The Aegaeon temperature and atmospheric conditions are fundamental to understanding its habitability and environmental characteristics. The Aegaeon average temperature of 0.0 K (-273.1 °C) (-459.7°F) provides the baseline for understanding its climate. These extremely cold temperatures make Aegaeon inhospitable to life as we know it, with any atmosphere likely frozen solid on the surface. Compared to Earth's average temperature of 15°C (59°F), Aegaeon presents a dramatically different thermal environment. Being closer to the Sun than Earth, Aegaeon receives more intense solar radiation, contributing to its temperature profile.

The Aegaeon escape velocity and shape characteristics reveal important details about its gravitational field and rotational dynamics. The Aegaeon escape velocity of 0 m/s determines how easily objects can break free from its gravitational pull. This relatively low escape velocity means that gases and light molecules can easily escape into space, making it difficult for Aegaeon to retain a substantial atmosphere. The Aegaeon flattening of 0.0000% indicates how much the planet's rotation affects its shape. This minimal flattening suggests a nearly spherical shape, indicating either slow rotation or a very rigid internal structure.