Dia

Dia is a fascinating moon in our Solar System that has captured the attention of astronomers and space enthusiasts alike. With a Dia radius of 2 km, making it 3185.5× 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 1.21e+7 km (0.081 AU) from the Sun, Dia occupies a significant place in the Solar System's architecture. As a moon, Dia demonstrates the incredible diversity of natural satellites that orbit larger celestial bodies throughout our Solar System.

The Dia physical characteristics reveal a world of remarkable dimensions and properties. The Dia radius measures 2 km, making it 3185.5× smaller than Earth's size. The Dia mass of 9.00e+13 kg represents 66355555555.6× smaller than Earth's mass, giving this world substantial gravitational influence.

The Dia orbit reveals fascinating details about its journey around the Sun and its relationship to other Solar System objects. The Dia orbit has a semimajor axis of 1.21e+7 km (0.081 AU), placing it 12.3× smaller than Earth's distance from the Sun. The Dia orbit is moderately elliptical with an eccentricity of 0.211 (12.6× Earth's orbital eccentricity), creating noticeable seasonal variations in solar radiation. The Dia orbit takes 0.08 hours to complete (109958.7× smaller than Earth's orbital period), defining the length of its year. The orbital inclination of 28.23° indicates how much the Dia orbit is tilted relative to the Solar System's ecliptic plane. This moderate inclination indicates a typical orbital evolution for objects in this region of the Solar System.

The Dia rotation and axial orientation provide crucial insights into its daily and seasonal cycles, as well as its orbital dynamics. The Dia axial tilt of 0° determines the intensity and nature of seasonal variations. With minimal axial tilt, Dia experiences virtually no seasonal changes, maintaining relatively constant temperatures throughout its year. The orbital orientation parameters reveal additional details about Dia'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 Dia temperature and atmospheric conditions are fundamental to understanding its habitability and environmental characteristics. The Dia average temperature of 0.0 K (-273.1 °C) (-459.7°F) provides the baseline for understanding its climate. These extremely cold temperatures make Dia 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), Dia presents a dramatically different thermal environment. Being closer to the Sun than Earth, Dia receives more intense solar radiation, contributing to its temperature profile. The elliptical orbit creates significant temperature variations throughout the year, with extreme seasonal changes.

The Dia escape velocity and shape characteristics reveal important details about its gravitational field and rotational dynamics. The Dia 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 Dia to retain a substantial atmosphere. The Dia 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.