15760 Albion

15760 Albion is a fascinating asteroid in our Solar System that has captured the attention of astronomers and space enthusiasts alike. With a 15760 Albion radius of 60 km, making it 106.2× 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 6.55e+9 km (43.766 AU) from the Sun, 15760 Albion occupies a significant place in the Solar System's architecture. As an asteroid, 15760 Albion represents the remnants of the early Solar System, providing valuable insights into the formation and evolution of our cosmic neighborhood.

The 15760 Albion physical characteristics reveal a world of remarkable dimensions and properties. The 15760 Albion radius measures 60 km, making it 106.2× smaller than Earth's size. The 15760 Albion mass of 9.00e+17 kg represents 6635555.6× smaller than Earth's mass, giving this world substantial gravitational influence.

The 15760 Albion orbit reveals fascinating details about its journey around the Sun and its relationship to other Solar System objects. The 15760 Albion orbit has a semimajor axis of 6.55e+9 km (43.766 AU), placing it 43.8× Earth's distance from the Sun. At its closest approach (perihelion), 15760 Albion comes within 6.12e+9 km of the Sun, while at its farthest point (aphelion), it reaches 6.98e+9 km, creating a 13.1% variation in solar distance. The 15760 Albion orbit is nearly circular with an eccentricity of 0.066 (4.0× Earth's orbital eccentricity), resulting in relatively stable solar heating throughout its year. The 15760 Albion orbit takes 1.22 days to complete (298.4× smaller than Earth's orbital period), defining the length of its year. The orbital inclination of 2.195° indicates how much the 15760 Albion orbit is tilted relative to the Solar System's ecliptic plane. This low inclination means 15760 Albion follows a path very close to the plane where most planets orbit, suggesting a stable formation history.

The 15760 Albion rotation and axial orientation provide crucial insights into its daily and seasonal cycles, as well as its orbital dynamics. The 15760 Albion axial tilt of 0° determines the intensity and nature of seasonal variations. With minimal axial tilt, 15760 Albion experiences virtually no seasonal changes, maintaining relatively constant temperatures throughout its year. The orbital orientation parameters reveal additional details about 15760 Albion'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 15760 Albion temperature and atmospheric conditions are fundamental to understanding its habitability and environmental characteristics. The 15760 Albion average temperature of 0.0 K (-273.1 °C) (-459.7°F) provides the baseline for understanding its climate. These extremely cold temperatures make 15760 Albion 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), 15760 Albion presents a dramatically different thermal environment. Being farther from the Sun than Earth, 15760 Albion receives less solar radiation, resulting in cooler conditions.

The 15760 Albion escape velocity and shape characteristics reveal important details about its gravitational field and rotational dynamics. The 15760 Albion 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 15760 Albion to retain a substantial atmosphere. The 15760 Albion 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.